Pith. sign in

REVIEW 2 major objections 4 minor 2 cited by

The Polarisation Sky Survey of the Universe's Magnetism (POSSUM): Science Goals and Survey Description

T0 review · 2 major / 4 minor · reviewed 2026-08-15 · deepseek-v4-flash

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗ Review JSON

Pith's one-line read POSSUM will chart half the sky's magnetism through a grid of up to one million Faraday rotation measures of background galaxies.

desk verdict Solid, honest survey description with one internal inconsistency: the abstract and §8 claim a survey-wide median RM uncertainty of ~1 rad m^-2, which the paper's own §3.3 numbers do not support. read the letter →

arxiv 2505.08272 v1 pith:QCE745HI submitted 2025-05-13 astro-ph.GA

B.M. Gaensler , G.H. Heald , N.M. McClure-Griffiths , C.S. Anderson , C.L. Van Eck , J.L. West , A.J.M. Thomson , J.P. Leahy
show 52 more authors
L. Rudnick Y.K. Ma Takuya Akahori G. Gürkan T.L. Landecker S.A. Mao S.P. O'Sullivan W. Raja X. Sun T. Vernstrom Lerato Baidoo Ettore Carretti A.R. Taylor A.G. Willis Erik Osinga J.D. Livingston E.L. Alexander David Alonso-López A.D. Amaral T. An Andrea Bracco S. Bradbury Marcus Brüggen Chakali Eswaraiah Torsten En{ss}lin T.J. Galvin Marijke Haverkorn A.M. Hopkins Sebastian Hutschenreuter Shinsuke Ideguchi S. Jaswanth S. Lyla Jung J.F. Kaczmarek Roland Kothes Sanja Lazarević Denis Leahy Francesca Loi Joshua R. Marvil Ray Norris Ayush Pandhi Jason M. Price C.J. Riseley P. Ryder Amit Seta Vasundhara Shaw A.X. Shen C. Sobey J. Stil Chiara Stuardi Gupta Upasana Shannon Vanderwoude Velibor Velović
This is my paper · ORCID
classification astro-ph.GA
keywords FaradayrotationmeasureRMgridradiopolarimetrycosmicmagneticfieldsASKAPintergalacticGalacticinterstellarmediumpolarisationsurvey
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper describes POSSUM, a radio-polarisation survey that aims to measure Faraday rotation toward as many as one million compact extragalactic sources across 20,630 square degrees, half of the celestial sphere. At a projected density of 30 to 50 rotation measures per square degree and a median uncertainty near $1\ \mathrm{rad\,m^{-2}}$, the survey would be the densest and most precise RM grid ever built, tens of times denser than the largest existing catalogue. Alongside the grid it will deliver polarisation spectra, Faraday-depth cubes, and maps of diffuse Galactic emission. If these projections hold, POSSUM would turn magnetic fields from the Milky Way's gas to galaxy clusters and the cosmic web into a routinely measurable quantity rather than a poorly mapped curiosity.

What carries the argument

The load-bearing object is the Faraday rotation measure grid: an ensemble of background polarised radio sources whose polarisation angles are rotated by foreground magnetised plasma according to $\mathrm{RM} = 0.812 \int n_e B_{\parallel}\, dl$ in $\mathrm{rad\,m^{-2}}$. Each source is a line of sight through the magneto-ionic medium, so a dense grid turns a source catalogue into a tomographic tracer of magnetic fields along every sight line. The paper's pipelines convert measured polarisation spectra $P(\lambda^2)$ into Faraday dispersion functions using RM synthesis, and run this transformation both per detected source (the 1D pipeline) and pixel-by-pixel over full Stokes cubes (the 3D pipeline). The expected density and precision rest on scaling the pilot survey's measured counts to the full 853-field tiling, using an $8\sigma$ polarised-intensity detection threshold of $144\ \mu\mathrm{Jy\,beam^{-1}}$.

What would settle it

In the first public data release, count polarised sources with signal-to-noise ratio above 8 within the 98 scheduling blocks that received the double leakage correction and within the Galactic-plane fields with bright diffuse emission; if their density falls below 30 per square degree there, the stated grid density and the projected total of 620,000 to 1,030,000 RMs cannot be met even if the rest of the survey performs as piloted.

Watch

Extended reading notes

Core claim

The central claim is that the survey's observing design—a 30-square-degree instantaneous field of view, full-Stokes spectra across 800–1088 MHz, and long-track synthesis observations—will produce a catalogue of up to one million linearly polarised background radio galaxies, with 30–50 rotation measures per square degree and a median RM uncertainty of roughly $1\ \mathrm{rad\,m^{-2}}$. Every source in the commensal total-intensity catalogue will carry measured polarisation spectra and a Faraday dispersion function, whether or not it is detected in polarisation. The rotation-measure spread function in band 1 has FWHM $58\ \mathrm{rad\,m^{-2}}$, giving RM errors near $3\ \mathrm{rad\,m^{-2}}$ at the detection limit and means and medians of 2.1 and 1.6 $\mathrm{rad\,m^{-2}}$ over the detected population; combining bands tightens the median to about $1\ \mathrm{rad\,m^{-2}}$. The paper argues this grid, together with resolved polarisation maps of more than a hundred radio galaxies and all-sky diffuse emission maps, will enable the first systematic measurements of magnetic fields in the intergalactic medium, cluster and group outskirts, galaxy halos, and the multiphase Milky Way.

Load-bearing premise

The million-source projection assumes the polarised-source density measured in the pilot survey—42 per square degree in an extragalactic field and 20 per square degree in a Galactic-plane field—holds across the entire 20,630-square-degree footprint, including regions of bright diffuse emission and the roughly 10 percent of observations that received an erroneous double leakage correction.

Editorial extensions

If this is right

  • The RM grid will contain roughly 35 times more sources per square degree than the NVSS catalogue, with about ten times smaller median RM uncertainty, making coherent magnetic structures visible at arcminute scales where previous surveys showed noise.
  • Cluster and group science will shift from individual targets to ensembles: over a dozen clusters with 100+ sight lines inside the virial radius and at least a hundred more with 50+ sight lines, enabling RM stacking in bins of mass and redshift.
  • For the Milky Way, the dense grid supports an all-sky Faraday rotation map at sub-degree resolution, allowing direct tests of disk dynamo models and reconstruction of the halo magnetic field geometry.
  • Polarisation spectra for roughly $10^5$ blazars and resolved RM maps of hundreds to thousands of radio galaxies will let population studies separate intrinsic AGN magneto-ionic structure from environmental Faraday rotation.
  • Combining band-1 with band-2 data cuts the rotation-measure spread-function width from 58 to 36 $\mathrm{rad\,m^{-2}}$ and pushes the median uncertainty to about 1 $\mathrm{rad\,m^{-2}}$, improving precision without losing the 800–1088 MHz source density.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the pilot density holds only in clean extragalactic fields and not in bright diffuse regions, the final catalogue may contain roughly 600,000–800,000 RMs rather than the advertised 'up to one million'; the paper's own range of $6.2$–$10.3 \times 10^5$ already brackets this uncertainty.
  • The 98 scheduling blocks that received the erroneous double leakage correction form a natural reproducibility experiment: comparing re-reduced leakage-corrected products with the archived versions would directly test whether the double correction introduced residuals larger than the claimed $1\ \mathrm{rad\,m^{-2}}$ median error.
  • Pairing each RM with a redshift from the commensurate continuum survey would convert the statistical grid into a three-dimensional magnetic-field map of the intervening medium, since RM alone yields only the line-of-sight integral of electron density times field strength.
  • A testable extension the paper points toward but does not promise: merge POSSUM's diffuse polarisation maps with single-dish data to separate emission from Faraday rotation along the line of sight, which would let the survey constrain the 3D structure of the magnetised interstellar medium.
Share X Bluesky LinkedIn Reddit HN

Signed reviews

No signed human review yet.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

2 major / 4 minor

Summary. This paper presents the survey design, science goals, data products, and expected performance of POSSUM, an ASKAP polarisation survey covering 20,630 deg^2 (50% of the sky) in band 1 (800-1088 MHz) with an ancillary band-2 component (1296-1440 MHz) over 15,470 deg^2. The central claims are that POSSUM will deliver an RM grid of up to one million compact extragalactic sources at a density of 30-50 RMs per square degree, with a median RM uncertainty of about 1 rad m^-2, 20 arcsecond resolution, and about 18 microJy/beam sensitivity in Stokes Q and U. The paper describes the observational setup, the pilot-survey basis for the expected yield, the calibration and processing pipelines, the public data products, and the complementarity with other radio and multi-wavelength surveys, including future SKA work.

Significance. If the stated performance is achieved, POSSUM will be a transformative resource for cosmic magnetism studies: it will increase the extragalactic RM grid density by roughly an order of magnitude over NVSS, improve per-source RM precision by a similar factor, and open the under-explored southern sky to RM-grid science across the IGM, clusters, galaxy halos, the Milky Way ISM, and AGN. A particular strength of the paper is that the headline yield and precision numbers are grounded in the POSSUM pilot survey (Vanderwoude et al. 2024) rather than asserted from simulations alone, and the paper is transparent about several caveats, including the double-leakage correction affecting 98 scheduling blocks and the lack of single-dish short-spacing data for diffuse emission. The survey description is detailed enough to be useful to future users of the dataset, and the comparison table with other polarisation surveys is a valuable reference. My main reservation is an internal inconsistency in the headline RM-precision claim, which is consequential for one of the stated science drivers.

major comments (2)
  1. [Abstract, §3.3, Table 1, §8] The abstract, Section 1, and Section 8 state that POSSUM will achieve a survey-wide median RM uncertainty of about 1 rad m^-2, but this is contradicted by the numbers in Section 3.3 and Table 1. Section 3.3 reports a median RM uncertainty of 1.6 rad m^-2 for band-1-only data and about 1 rad m^-2 only for areas with both band-1 and band-2 coverage; Table 1 gives the dual-band overlap as 36.75% of the survey area, so roughly 63% of the survey will have only band-1 precision. A properly weighted survey-wide median therefore lies between 1.0 and 1.6 rad m^-2 and cannot be quoted as about 1. This matters because Section 2.3.1 identifies delta RM <~ 1 rad m^-2 as the precision needed to detect halo fields around external edge-on spirals; the unqualified wording overstates the capability available over most of the survey. Please quote band-dependent medians or a properly weighted survey-wide median, and qualify the Section 2.3.1 science forecast accordingly.
  2. [§3.3, Fig. 2, §5.1] The headline yield of 30-50 RMs per square degree and the corresponding (6.2-10.3) x 10^5 RM total are extrapolated from a single extragalactic pilot field (42 RMs deg^-2) and a single Galactic-plane pilot field (20 RMs deg^-2). The Galactic-plane value is a factor of about two lower than the extragalactic value, and the survey deliberately includes the Galactic plane (Figure 2) as well as 98 scheduling blocks affected by the double leakage correction (Section 5.1). I do not regard the pilot measurements as circular or invalid, but the extrapolation is the principal uncertainty in the central yield claim. Please state the pilot coverage explicitly in Section 3.3, quantify the systematic uncertainty in the yield estimate, or present the yield as an environment-dependent estimate (e.g., applying the Galactic-plane density separately to the plane region).
minor comments (4)
  1. [§7.2.3] The heading 'Low-freqeuncy surveys' contains a typo; it should read 'Low-frequency surveys'.
  2. [§7.2.4] The heading 'Galactic Plane Purveys' contains a typo; it should read 'Galactic Plane Surveys'.
  3. [§5.1] The double-leakage caveat for the 98 affected scheduling blocks is appropriately disclosed, but the effect on the expected RM grid density for those 10% of survey fields is not quantified; a sentence estimating the impact on source yield or RM precision would help readers assess the overall survey forecast.
  4. [Table 1] Table 1 is dense and very informative, but the distinction between the phi_max and phi_max-scale columns could be made more explicit in the caption; currently the footnote defines the quantities but the physical difference is not described.

Circularity Check

0 steps flagged · score 0.0 of 10

No circular reasoning: the survey yield and RM precision claims are empirical extrapolations from the independent POSSUM pilot survey, not from the science goals they support.

full rationale

The paper's central quantitative claims—RM grid density, total yield, and RM uncertainty—are not derived from the science goals or from the survey's own conclusions. Section 3.3 states that the 30–50 RMs deg^-2 projection is based on previous polarisation studies and is now supported by the POSSUM pilot survey (Vanderwoude et al. 2024), which measured 42 RMs deg^-2 in an extragalactic field and 20 RMs deg^-2 in a Galactic-plane field. The RM precision values (median 1.6 rad m^-2 in band 1, ≈1 rad m^-2 in dual-band areas) are likewise presented as measured properties of the pilot survey's detected source population. These are empirical inputs, not quantities defined by POSSUM's science objectives, so there is no self-definitional or fitted-input-called-prediction circularity. The paper also cites earlier POSSUM-related work for context and for the pilot measurements, but these citations are not used as the sole justification of the target result; the pilot data are external, falsifiable observations. The only substantive weakness is internal rather than circular: the abstract and Section 8 state a survey-wide median RM uncertainty of ~1 rad m^-2, while Section 3.3 reports 1.6 rad m^-2 for band-1-only coverage and ≈1 rad m^-2 only where dual-band data exist, so the survey-wide median should be a weighted intermediate value. That is a support/consistency gap, not a circular derivation, and it does not affect the yield estimates. No circular step is present under the required standards.

Assumptions & free parameters 0 free parameters · 3 assumptions · 0 invented entities

No free parameters are fitted in this descriptive paper; survey parameters are design choices or measurements from the pilot survey. The axioms are standard physics and instrumentation assumptions that underlie the interpretation of the planned data. No new entities are postulated.

assumptions (3)
  • domain assumption Faraday rotation, RM = 0.81 * integral(n_e * B_parallel * dl), can be used to infer line-of-sight magnetic fields from polarized radio sources.
    This is the foundational relation used throughout Section 2 to interpret RM grids. It is standard astrophysics and not derived in this paper.
  • domain assumption RM synthesis and broadband spectropolarimetric techniques can reliably recover Faraday rotation from the observed polarized spectra.
    Section 4.4 uses RM-Tools and RM synthesis to produce Faraday dispersion functions and RMs. The reliability of these methods is assumed from prior literature.
  • domain assumption ASKAP polarimetric calibration maintains the stated purity (leakage around 0.2 percent across the field, on-axis corrected to better than 0.1 percent) over the full survey.
    Section 3.1 and 5.1 describe the calibration approach and note that 98 scheduling blocks were affected by a double leakage correction, implying this assumption is not yet fully satisfied for about 10 percent of the survey area.

how reviews work

0 comments
Cite this review

Pith. "Pith review of The Polarisation Sky Survey of the Universe's Magnetism (POSSUM): Science Goals and Survey Description." pith.science (2026). https://pith.science/paper/QCE745HI

@misc{pith2026250508272,
  author       = {Pith},
  title        = {Pith review of: The Polarisation Sky Survey of the Universe's Magnetism (POSSUM): Science Goals and Survey Description},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/QCE745HI}},
  note         = {Machine review of arXiv:2505.08272}
}
abstract

The Australian SKA Pathfinder (ASKAP) offers powerful new capabilities for studying the polarised and magnetised Universe at radio wavelengths. In this paper, we introduce the Polarisation Sky Survey of the Universe's Magnetism (POSSUM), a groundbreaking survey with three primary objectives: (1) to create a comprehensive Faraday rotation measure (RM) grid of up to one million compact extragalactic sources across the southern ~50 per cent of the sky (20,630 deg$^2$); (2) to map the intrinsic polarisation and RM properties of a wide range of discrete extragalactic and Galactic objects over the same area; and (3) to contribute interferometric data with excellent surface brightness sensitivity, which can be combined with single-dish data to study the diffuse Galactic interstellar medium. Observations for the full POSSUM survey commenced in May 2023 and are expected to conclude by mid-2028. POSSUM will achieve an RM grid density of around 30-50 RMs per square degree with a median measurement uncertainty of ~1 rad m$^{-2}$. The survey operates primarily over a frequency range of 800-1088 MHz, with an angular resolution of 20'' and a typical RMS sensitivity in Stokes $Q$ or $U$ of 18 $\mu$Jy beam$^{-1}$. Additionally, the survey will be supplemented by similar observations covering 1296-1440 MHz over 38 per cent of the sky. POSSUM will enable the discovery and detailed investigation of magnetised phenomena in a wide range of cosmic environments, as well as the interplay between these components. This paper reviews the current science case developed by the POSSUM Collaboration and provides an overview of POSSUM's observations, data processing, outputs, and its complementarity with other radio and multi-wavelength surveys, including future work with the SKA. [Abstract abridged]

Figures

Figures reproduced from arXiv: 2505.08272 by the authors.

Figure 1
Figure 1. Comparison of NVSS (left; Taylor et al., 2009) and POSSUM (right) Band 1 RMs within the Fornax cluster’s virial radius (grey dashed circle), showcasing POSSUM’s transformative capability to probe magnetised gas in clusters, groups, and many other ∼degree-scale extragalactic objects. The background is a Digitized Sky Survey optical image (greyscale). Solid circles indicate the position, magnitude, and sign of RMs mea… view at source ↗
Figure 2
Figure 2. Planned sky coverage of POSSUM. The coverage of the band 1 (800–1088 MHz) component, commensal with the EMU survey, is shaded purple, and the band 2 (1296–1440 MHz) component, commensal with the WALLABY survey, is shaded green. (Regions covered by both components appear dark green.) The location of the Galactic Centre is marked by the cyan cross. The background greyscale map in the top panel is the reprocessed Hasla… view at source ↗
Figure 4
Figure 4. [PITH_FULL_IMAGE:figures/full_fig_p011_4.png] view at source ↗
Figures from the paper (7 more)
Figure 4
Figure 4. Figure 4: Comparison of POSSUM’s performance with other surveys listed in [PITH_FULL_IMAGE:figures/full_fig_p014_4.png]
Figure 3
Figure 3. Figure 3: The expected percentage of polarised sources for Stokes I fluxes above various thresholds (top) and percentage of polarised sources for var￾ious polarised fractions (bottom) computed using the Vanderwoude et al. (2024) prototype POSSUM catalogues. pertain to polarisati…
Figure 5
Figure 5. Figure 5: An illustration of the dramatic improvement in RM grid density and precision between the NVSS (top; Taylor et al., 2009) and POSSUM (bottom) band 1 surveys, focusing on mid-northern Galactic latitudes where the surveys currently overlap. POSSUM provides approximately 3…
Figure 6
Figure 6. Figure 6: Similar to the bottom panel of [PITH_FULL_IMAGE:figures/full_fig_p020_6.png]
Figure 7
Figure 7. Figure 7: POSSUM band 1 images of selected radio galaxies, illustrating POSSUM’s remarkable combination of resolution and sensitivity to large-scale emission. Each row features a different object, decreasing in angular size from top to bottom. POSSUM is expected to map the polar…
Figure 8
Figure 8. Figure 8: Part of a field centred at (ℓ, b) = (49.75◦, −29.5◦), demonstrating POSSUM’s excellent sensitivity to Galactic ISM emission structures. The top left panel shows the all-sky Wilkinson Microwave Anisotropy Probe (WMAP; Bennett et al., 2003) linearly polarised intensity i…
Figure 9
Figure 9. Figure 9: Comparison of NVSS (Condon et al., 1998) and ASKAP EMU/POSSUM maps in a typical extragalactic field. The top left panel shows the NVSS Stokes I map, while the top right panel presents the corresponding NVSS linearly polarised intensity. The bottom left panel displays t…

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A Catalog of Galactic Supernova Remnants and Supernova Remnant Candidates from the EMU/POSSUM Radio Sky Surveys. I

    astro-ph.GA 2025-07 conditional novelty 6.0 of 10

    ASKAP EMU/POSSUM data yield 6 newly confirmed supernova remnants, 37 new candidates, and updated classifications for 46 previously identified radio candidates in a quarter of the Galactic plane.

  2. A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity

    astro-ph.GA 2025-06 conditional novelty 6.0 of 10

    Faraday complexity in 191 background radio sources is dominated by sub-2.5-arcsecond magneto-ionic structures in the Milky Way, likely linked to anisotropic turbulent magnetic fields.

Reference graph

Works this paper leans on

249 extracted references · 22 canonical work pages · cited by 2 Pith papers

  1. [1]

    write newline

    " write newline "" before.all 'output.state := FUNCTION fin.entry write newline FUNCTION new.block output.state before.all = 'skip after.block 'output.state := if FUNCTION new.sentence output.state after.block = 'skip output.state before.all = 'skip after.sentence 'output.state := if if FUNCTION not #0 #1 if FUNCTION and 'skip pop #0 if FUNCTION or pop #1...

  2. [2]

    W., 2024, [ ] 10.1093/mnras/stad3967 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.528..937A 528, 937

    Achikanath Chirakkara R., Seta A., Federrath C., Kunz M. W., 2024, [ ] 10.1093/mnras/stad3967 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.528..937A 528, 937

    doi:10.1093/mnras/stad3967 2024

  3. [3]

    Adams E. A. K., et al., 2022, [ ] 10.1051/0004-6361/202244007 , https://ui.adsabs.harvard.edu/abs/2022A&A...667A..38A 667, A38

    doi:10.1051/0004-6361/202244007 2022

  4. [4]

    Adebahr B., et al., 2022, [ ] 10.1051/0004-6361/202243201 , https://ui.adsabs.harvard.edu/abs/2022A&A...663A.103A 663, A103

    doi:10.1051/0004-6361/202243201 2022

  5. [5]

    Ahumada R., et al., 2020, [ ] 10.3847/1538-4365/ab929e , https://ui.adsabs.harvard.edu/abs/2020ApJS..249....3A 249, 3

    doi:10.3847/1538-4365/ab929e 2020

  6. [6]

    M., Ryu D., 2014, [ ] 10.1088/0004-637X/790/2/123 , https://ui.adsabs.harvard.edu/abs/2014ApJ...790..123A 790, 123

    Akahori T., Gaensler B. M., Ryu D., 2014, [ ] 10.1088/0004-637X/790/2/123 , https://ui.adsabs.harvard.edu/abs/2014ApJ...790..123A 790, 123

    doi:10.1088/0004-637x/790/2/123 2014

  7. [7]

    R., et al., 2022, [ ] 10.1017/pasa.2022.3 , https://ui.adsabs.harvard.edu/abs/2022PASA...39...10A 39, e010

    Allison J. R., et al., 2022, [ ] 10.1017/pasa.2022.3 , https://ui.adsabs.harvard.edu/abs/2022PASA...39...10A 39, e010

    doi:10.1017/pasa.2022.3 2022

  8. [8]

    Alonso D., 2025, Shapley, in preparation

    2025

Show all 249 references
  1. [9]

    D., Vernstrom T., Gaensler B

    Amaral A. D., Vernstrom T., Gaensler B. M., 2021, [ ] 10.1093/mnras/stab564 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.503.2913A 503, 2913

    2021 doi

  2. [10]

    Anderson C., 2016, PhD thesis, The University of Sydney

    2016

  3. [11]

    S., Gaensler B

    Anderson C. S., Gaensler B. M., Feain I. J., Franzen T. M. O., 2015, [ ] 10.1088/0004-637X/815/1/49 , http://adsabs.harvard.edu/abs/2015ApJ...815...49A 815, 49

    2015 doi

  4. [12]

    S., Gaensler B

    Anderson C. S., Gaensler B. M., Feain I. J., 2016, [ ] 10.3847/0004-637X/825/1/59 , http://adsabs.harvard.edu/abs/2016ApJ...825...59A 825, 59

    2016 doi

  5. [13]

    Anderson C., et al., 2018a, [Galaxies] 10.3390/galaxies6040127 , https://ui.adsabs.harvard.edu/abs/2018Galax...6..127A 6, 127

    doi

  6. [14]

    S., Gaensler B

    Anderson C. S., Gaensler B. M., Heald G. H., O'Sullivan S. P., Kaczmarek J. F., Feain I. J., 2018b, [ ] 10.3847/1538-4357/aaaec0 , http://adsabs.harvard.edu/abs/2018ApJ...855...41A 855, 41

    doi

  7. [15]

    S., O'Sullivan S

    Anderson C. S., O'Sullivan S. P., Heald G. H., Hodgson T., Pasetto A., Gaensler B. M., 2019, [ ] 10.1093/mnras/stz377 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.485.3600A 485, 3600

    2019 doi

  8. [16]

    S., et al., 2021, [ ] 10.1017/pasa.2021.4 , https://ui.adsabs.harvard.edu/abs/2021PASA...38...20A 38, e020

    Anderson C. S., et al., 2021, [ ] 10.1017/pasa.2021.4 , https://ui.adsabs.harvard.edu/abs/2021PASA...38...20A 38, e020

    2021 doi

  9. [17]

    S., et al., 2022, [ ] 10.3847/1538-4357/ac7ec0 , https://ui.adsabs.harvard.edu/abs/2022ApJ...937...45A 937, 45

    Anderson C. S., et al., 2022, [ ] 10.3847/1538-4357/ac7ec0 , https://ui.adsabs.harvard.edu/abs/2022ApJ...937...45A 937, 45

    2022 doi

  10. [19]

    S., et al., 2024b, [ ] 10.1093/mnras/stae1954 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.533.4068A 533, 4068

    Anderson C. S., et al., 2024b, [ ] 10.1093/mnras/stae1954 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.533.4068A 533, 4068

    doi

  11. [20]

    K., O'Sullivan S

    Banfield J. K., O'Sullivan S. P., Wieringa M. H., Emonts B. H. C., 2019, [ ] 10.1093/mnras/sty3108 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.5250B 482, 5250

    2019 doi

  12. [21]

    J., et al., 2019, [ ] 10.1093/mnras/stz1814 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.3003B 488, 3003

    Barnes D. J., et al., 2019, [ ] 10.1093/mnras/stz1814 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.3003B 488, 3003

    2019 doi

  13. [22]

    A., Kepley A

    Basu A., Mao S. A., Kepley A. A., Robishaw T., Zweibel E. G., Gallagher John. S. I., 2017, [ ] 10.1093/mnras/stw2369 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.464.1003B 464, 1003

    2017 doi

  14. [23]

    A., Fletcher A., Kanekar N., Shukurov A., Schnitzeler D., Vacca V., Junklewitz H., 2018, [ ] 10.1093/mnras/sty766 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.2528B 477, 2528

    Basu A., Mao S. A., Fletcher A., Kanekar N., Shukurov A., Schnitzeler D., Vacca V., Junklewitz H., 2018, [ ] 10.1093/mnras/sty766 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.2528B 477, 2528

    2018 doi

  15. [24]

    J., Urakawa Y., 2021, [ ] 10.1103/PhysRevLett.126.191102 , https://ui.adsabs.harvard.edu/abs/2021PhRvL.126s1102B 126, 191102

    Basu A., Goswami J., Schwarz D. J., Urakawa Y., 2021, [ ] 10.1103/PhysRevLett.126.191102 , https://ui.adsabs.harvard.edu/abs/2021PhRvL.126s1102B 126, 191102

    2021 doi

  16. [25]

    Beck R., 2015, [ ] 10.1007/s00159-015-0084-4 , https://ui.adsabs.harvard.edu/abs/2015A&ARv..24....4B 24, 4

    2015 doi

  17. [26]

    M., 2004, [ ] 10.1016/j.newar.2004.09.013 , https://ui.adsabs.harvard.edu/abs/2004NewAR..48.1289B 48, 1289

    Beck R., Gaensler B. M., 2004, [ ] 10.1016/j.newar.2004.09.013 , https://ui.adsabs.harvard.edu/abs/2004NewAR..48.1289B 48, 1289

    2004 doi

  18. [27]

    D., Gilmore G., eds, Planets, Stars and Stellar Systems

    Beck R., Wielebinski R., 2013, in Oswalt T. D., Gilmore G., eds, Planets, Stars and Stellar Systems. Volume 5: Galactic Structure and Stellar Populations. p. 641, 10.1007/978-94-007-5612-0_13

    2013 doi

  19. [28]

    arXiv:1302.5663v11

    Beck R., Wielebinski R., 2023, https://arxiv.org/abs/1302.5663v11 p. arXiv:1302.5663v11

    2023 arXiv

  20. [29]

    L., et al., 2003, [ ] 10.1086/345346 , https://ui.adsabs.harvard.edu/abs/2003ApJ...583....1B 583, 1

    Bennett C. L., et al., 2003, [ ] 10.1086/345346 , https://ui.adsabs.harvard.edu/abs/2003ApJ...583....1B 583, 1

    2003 doi

  21. [30]

    L., Miniati F., Lilly S

    Bernet M. L., Miniati F., Lilly S. J., 2012, [ ] 10.1088/0004-637X/761/2/144 , https://ui.adsabs.harvard.edu/abs/2012ApJ...761..144B 761, 144

    2012 doi

  22. [31]

    K., Hill A

    Betti S. K., Hill A. S., Mao S. A., Gaensler B. M., Lockman F. J., McClure-Griffiths N. M., Benjamin R. A., 2019, [ ] 10.3847/1538-4357/aaf886 , https://ui.adsabs.harvard.edu/abs/2019ApJ...871..215B 871, 215

    2019 doi

  23. [32]

    Beuther H., et al., 2016, [ ] 10.1051/0004-6361/201629143 , https://ui.adsabs.harvard.edu/abs/2016A&A...595A..32B 595, A32

    2016 doi

  24. [33]

    V., Cameron R

    Bicknell G. V., Cameron R. A., Gingold R. A., 1990, [ ] 10.1086/168928 , http://adsabs.harvard.edu/abs/1990ApJ...357..373B 357, 373

    1990 doi

  25. [34]

    B \"o ckmann K., et al., 2023, [ ] 10.1051/0004-6361/202346777 , https://ui.adsabs.harvard.edu/abs/2023A&A...678A..56B 678, A56

    2023 doi

  26. [35]

    B., 2010, [ ] 10.1051/0004-6361/200913696 , https://ui.adsabs.harvard.edu/abs/2010A&A...513A..30B 513, A30

    Bonafede A., Feretti L., Murgia M., Govoni F., Giovannini G., Dallacasa D., Dolag K., Taylor G. B., 2010, [ ] 10.1051/0004-6361/200913696 , https://ui.adsabs.harvard.edu/abs/2010A&A...513A..30B 513, A30

    2010 doi

  27. [36]

    Bonafede A., Vazza F., Br \"u ggen M., Murgia M., Govoni F., Feretti L., Giovannini G., Ogrean G., 2013, [ ] 10.1093/mnras/stt960 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.433.3208B 433, 3208

    2013 doi

  28. [37]

    L., 2019, [ ] 10.1093/mnras/sty2603 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.482....2B 482, 2

    Bonaldi A., Bonato M., Galluzzi V., Harrison I., Massardi M., Kay S., De Zotti G., Brown M. L., 2019, [ ] 10.1093/mnras/sty2603 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.482....2B 482, 2

    2019 doi

  29. [38]

    A., de Bruyn A

    Brentjens M. A., de Bruyn A. G., 2005, [ ] 10.1051/0004-6361:20052990 , https://ui.adsabs.harvard.edu/abs/2005A&A...441.1217B 441, 1217

    2005 doi

  30. [39]

    C., Taylor A

    Brown J. C., Taylor A. R., 2001, [ ] 10.1086/338358 , https://ui.adsabs.harvard.edu/abs/2001ApJ...563L..31B 563, L31

    2001 doi

  31. [40]

    C., Taylor A

    Brown J. C., Taylor A. R., Jackel B. J., 2003, [ ] 10.1086/346082 , https://ui.adsabs.harvard.edu/abs/2003ApJS..145..213B 145, 213

    2003 doi

  32. [41]

    C., Haverkorn M., Gaensler B

    Brown J. C., Haverkorn M., Gaensler B. M., Taylor A. R., Bizunok N. S., McClure-Griffiths N. M., Dickey J. M., Green A. J., 2007, [ ] 10.1086/518499 , https://ui.adsabs.harvard.edu/abs/2007ApJ...663..258B 663, 258

    2007 doi

  33. [42]

    J., 1966, [ ] 10.1093/mnras/133.1.67 , https://ui.adsabs.harvard.edu/abs/1966MNRAS.133...67B 133, 67

    Burn B. J., 1966, [ ] 10.1093/mnras/133.1.67 , https://ui.adsabs.harvard.edu/abs/1966MNRAS.133...67B 133, 67

    1966 doi

  34. [43]

    R., Roukema B

    Calabretta M. R., Roukema B. F., 2007, [ ] 10.1111/j.1365-2966.2007.12297.x , https://ui.adsabs.harvard.edu/abs/2007MNRAS.381..865C 381, 865

    2007

  35. [44]

    L., Rawlings S., 2004, [ ] 10.1016/j.newar.2004.09.001 , http://adsabs.harvard.edu/abs/2004NewAR..48..979C 48, 979

    Carilli C. L., Rawlings S., 2004, [ ] 10.1016/j.newar.2004.09.001 , http://adsabs.harvard.edu/abs/2004NewAR..48..979C 48, 979

    2004 doi

  36. [45]

    L., Perley R

    Carilli C. L., Perley R. A., Dreher J. H., 1988, [ ] 10.1086/185315 , http://adsabs.harvard.edu/abs/1988ApJ...334L..73C 334, L73

    1988 doi

  37. [46]

    Carretti E., et al., 2019, [ ] 10.1093/mnras/stz806 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.489.2330C 489, 2330

    2019 doi

  38. [48]

    Carretti E., et al., 2022b, [ ] 10.1093/mnras/stac384 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.512..945C 512, 945

    doi

  39. [49]

    P., Vacca V., Vazza F., Gheller C., Vernstrom T., Bonafede A., 2023, [ ] 10.1093/mnras/stac2966 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.2273C 518, 2273

    Carretti E., O'Sullivan S. P., Vacca V., Vazza F., Gheller C., Vernstrom T., Bonafede A., 2023, [ ] 10.1093/mnras/stac2966 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.2273C 518, 2273

    2023 doi

  40. [50]

    Carretti E., et al., 2025, [ ] 10.1051/0004-6361/202451333 , https://ui.adsabs.harvard.edu/abs/2025A&A...693A.208C 693, A208

    2025 doi

  41. [51]

    Cen R., 2024, [Proceedings of the National Academy of Science] 10.1073/pnas.2402435121 , https://ui.adsabs.harvard.edu/abs/2024PNAS..12102435C 121, e2402435121

    2024 doi

  42. [52]

    P., 1999, [ ] 10.1086/306949 , http://adsabs.harvard.edu/abs/1999ApJ...514....1C 514, 1

    Cen R., Ostriker J. P., 1999, [ ] 10.1086/306949 , http://adsabs.harvard.edu/abs/1999ApJ...514....1C 514, 1

    1999 doi

  43. [53]

    Commonwealth Scientific and Industrial Research Organisation, https://www.atnf.csiro.au/projects/askap/ACES-memos

    Chippendale A., Anderson C., 2019, 019, On-Dish Calibration of XY Phase for ASKAP’s Phased Array Feeds, https://www.atnf.csiro.au/projects/askap/ACES-memos . Commonwealth Scientific and Industrial Research Organisation, https://www.atnf.csiro.au/projects/askap/ACES-memos

    2019

  44. [54]

    E., Peek J

    Clark S. E., Peek J. E. G., Putman M. E., 2014, [ ] 10.1088/0004-637X/789/1/82 , https://ui.adsabs.harvard.edu/abs/2014ApJ...789...82C 789, 82

    2014 doi

  45. [55]

    J., Cotton W

    Condon J. J., Cotton W. D., Greisen E. W., Yin Q. F., Perley R. A., Taylor G. B., Broderick J. J., 1998, [ ] 10.1086/300337 , https://ui.adsabs.harvard.edu/abs/1998AJ....115.1693C 115, 1693

    1998 doi

  46. [56]

    G., Haves P., Kronberg P

    Conway R. G., Haves P., Kronberg P. P., Stannard D., Vallee J. P., Wardle J. F. C., 1974, [ ] 10.1093/mnras/168.1.137 , http://adsabs.harvard.edu/abs/1974MNRAS.168..137C 168

    1974 doi

  47. [57]

    G., Birch P., Davis R

    Conway R. G., Birch P., Davis R. J., Jones L. R., Kerr A. J., Stannard D., 1983, [ ] 10.1093/mnras/202.3.813 , https://ui.adsabs.harvard.edu/abs/1983MNRAS.202..813C 202, 813

    1983 doi

  48. [58]

    Cooper B. F. C., Price R. M., 1962, [ ] 10.1038/1951084a0 , https://ui.adsabs.harvard.edu/abs/1962Natur.195.1084C 195, 1084

    1962 doi

  49. [59]

    H., Spangler S

    Costa A. H., Spangler S. R., 2018, [ ] 10.3847/1538-4357/aada06 , https://ui.adsabs.harvard.edu/abs/2018ApJ...865...65C 865, 65

    2018 doi

  50. [60]

    J., 2021, [ ] 10.1093/mnras/stab1865 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.1548C 506, 1548

    Curran S. J., 2021, [ ] 10.1093/mnras/stab1865 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.1548C 506, 1548

    2021 doi

  51. [61]

    arXiv:2403.00909

    Di Mascolo L., et al., 2024, [arXiv e-prints] 10.48550/arXiv.2403.00909 , https://ui.adsabs.harvard.edu/abs/2024arXiv240300909D p. arXiv:2403.00909

    2024 doi arXiv

  52. [62]

    M., et al., 2013, [ ] 10.1017/pasa.2012.003 , https://ui.adsabs.harvard.edu/abs/2013PASA...30....3D 30, e003

    Dickey J. M., et al., 2013, [ ] 10.1017/pasa.2012.003 , https://ui.adsabs.harvard.edu/abs/2013PASA...30....3D 30, e003

    2013 doi

  53. [63]

    M., et al., 2022, [ ] 10.3847/1538-4357/ac94ce , https://ui.adsabs.harvard.edu/abs/2022ApJ...940...75D 940, 75

    Dickey J. M., et al., 2022, [ ] 10.3847/1538-4357/ac94ce , https://ui.adsabs.harvard.edu/abs/2022ApJ...940...75D 940, 75

    2022 doi

  54. [64]

    Donnert J., Vazza F., Br \"u ggen M., ZuHone J., 2018, [ ] 10.1007/s11214-018-0556-8 , https://ui.adsabs.harvard.edu/abs/2018SSRv..214..122D 214, 122

    2018 doi

  55. [65]

    P., et al., 2022, [ ] 10.1093/mnras/stac472 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.513..439D 513, 439

    Driver S. P., et al., 2022, [ ] 10.1093/mnras/stac472 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.513..439D 513, 439

    2022 doi

  56. [66]

    T., Chy \.z y K

    Drzazga R. T., Chy \.z y K. T., Jurusik W., Wi \'o rkiewicz K., 2011, [ ] 10.1051/0004-6361/201016092 , https://ui.adsabs.harvard.edu/abs/2011A&A...533A..22D 533, A22

    2011 doi

  57. [67]

    Erceg A., et al., 2022, [ ] 10.1051/0004-6361/202142244 , https://ui.adsabs.harvard.edu/abs/2022A&A...663A...7E 663, A7

    2022 doi

  58. [68]

    D., 2024a, [ ] 10.1051/0004-6361/202348586 , https://ui.adsabs.harvard.edu/abs/2024A&A...687A..23E 687, A23

    Erceg A., Jeli \'c V., Haverkorn M., Bracco A., Ceraj L., Turi \'c L., Soler J. D., 2024a, [ ] 10.1051/0004-6361/202348586 , https://ui.adsabs.harvard.edu/abs/2024A&A...687A..23E 687, A23

    doi

  59. [69]

    W., Tasse C., 2024b, [ ] 10.1051/0004-6361/202450082 , https://ui.adsabs.harvard.edu/abs/2024A&A...688A.200E 688, A200

    Erceg A., Jeli \'c V., Haverkorn M., Gajovi \'c L., Hardcastle M., Shimwell T. W., Tasse C., 2024b, [ ] 10.1051/0004-6361/202450082 , https://ui.adsabs.harvard.edu/abs/2024A&A...688A.200E 688, A200

    doi

  60. [70]

    S., O'Sullivan S

    Farnes J. S., O'Sullivan S. P., Corrigan M. E., Gaensler B. M., 2014, [ ] 10.1088/0004-637X/795/1/63 , https://ui.adsabs.harvard.edu/abs/2014ApJ...795...63F 795, 63

    2014 doi

  61. [71]

    J., et al., 2009, [ ] 10.1088/0004-637X/707/1/114 , http://adsabs.harvard.edu/abs/2009ApJ...707..114F 707, 114

    Feain I. J., et al., 2009, [ ] 10.1088/0004-637X/707/1/114 , http://adsabs.harvard.edu/abs/2009ApJ...707..114F 707, 114

    2009 doi

  62. [72]

    Feretti L., Johnston-Hollitt M., 2004, [ ] 10.1016/j.newar.2004.09.035 , https://ui.adsabs.harvard.edu/abs/2004NewAR..48.1145F 48, 1145

    2004 doi

  63. [73]

    Fernique P., et al., 2017, HiPS - Hierarchical Progressive Survey Version 1.0 , IVOA Recommendation 19 May 2017 ( @eprint arXiv 1708.09704 ), 10.5479/ADS/bib/2017ivoa.spec.0519F

    2017 arXiv

  64. [74]

    Ferri \`e re K., Terral P., 2014, [ ] 10.1051/0004-6361/201322966 , https://ui.adsabs.harvard.edu/abs/2014A&A...561A.100F 561, A100

    2014 doi

  65. [75]

    L., Jaffe T

    Ferri \`e re K., West J. L., Jaffe T. R., 2021, [ ] 10.1093/mnras/stab1641 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.507.4968F 507, 4968

    2021 doi

  66. [76]

    Floyd D. J. E., Perlman E., Leahy J. P., Beswick R. J., Jackson N. J., Sparks W. B., Axon D. J., O'Dea C. P., 2006, [ ] 10.1086/499295 , https://ui.adsabs.harvard.edu/abs/2006ApJ...639...23F 639, 23

    2006 doi

  67. [77]

    B., Ebneter K

    Fomalont E. B., Ebneter K. A., van Breugel W. J. M., Ekers R. D., 1989, [ ] 10.1086/185568 , https://ui.adsabs.harvard.edu/abs/1989ApJ...346L..17F 346, L17

    1989 doi

  68. [78]

    M., Dickey J

    Gaensler B. M., Dickey J. M., McClure-Griffiths N. M., Green A. J., Wieringa M. H., Haynes R. F., 2001, [ ] 10.1086/319468 , https://ui.adsabs.harvard.edu/abs/2001ApJ...549..959G 549, 959

    2001 doi

  69. [79]

    M., Beck R., Feretti L., 2004, [ ] 10.1016/j.newar.2004.09.003 , https://ui.adsabs.harvard.edu/abs/2004NewAR..48.1003G 48, 1003

    Gaensler B. M., Beck R., Feretti L., 2004, [ ] 10.1016/j.newar.2004.09.003 , https://ui.adsabs.harvard.edu/abs/2004NewAR..48.1003G 48, 1003

    2004 doi

  70. [80]

    M., Haverkorn M., Staveley-Smith L., Dickey J

    Gaensler B. M., Haverkorn M., Staveley-Smith L., Dickey J. M., McClure-Griffiths N. M., Dickel J. R., Wolleben M., 2005, [Science] 10.1126/science.1108832 , https://ui.adsabs.harvard.edu/abs/2005Sci...307.1610G 307, 1610

    2005 doi

  71. [81]

    M., Landecker T

    Gaensler B. M., Landecker T. L., Taylor A. R., POSSUM Collaboration 2010, in American Astronomical Society Meeting Abstracts \#215. p. 515

    2010

  72. [82]

    M., et al., 2011, [ ] 10.1038/nature10446 , https://ui.adsabs.harvard.edu/abs/2011Natur.478..214G 478, 214

    Gaensler B. M., et al., 2011, [ ] 10.1038/nature10446 , https://ui.adsabs.harvard.edu/abs/2011Natur.478..214G 478, 214

    2011 doi

  73. [83]

    F., Whiteoak J

    Gardner F. F., Whiteoak J. B., 1966, [ ] 10.1146/annurev.aa.04.090166.001333 , http://adsabs.harvard.edu/abs/1966ARA

    1966

  74. [84]

    T., Leahy J

    Garrington S. T., Leahy J. P., Conway R. G., Laing R. A., 1988, [ ] 10.1038/331147a0 , https://ui.adsabs.harvard.edu/abs/1988Natur.331..147G 331, 147

    1988 doi

  75. [85]

    A., Shukurov A., Fletcher A., Sarson G

    Gent F. A., Shukurov A., Fletcher A., Sarson G. R., Mantere M. J., 2013, [ ] 10.1093/mnras/stt560 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.432.1396G 432, 1396

    2013 doi

  76. [86]

    A., Mac Low M.-M., K \"a pyl \"a M

    Gent F. A., Mac Low M.-M., K \"a pyl \"a M. J., Singh N. K., 2021, [ ] 10.3847/2041-8213/abed59 , https://ui.adsabs.harvard.edu/abs/2021ApJ...910L..15G 910, L15

    2021 doi

  77. [87]

    M., Hivon E., Banday A

    G \'o rski K. M., Hivon E., Banday A. J., Wandelt B. D., Hansen F. K., Reinecke M., Bartelmann M., 2005, [ ] 10.1086/427976 , https://ui.adsabs.harvard.edu/abs/2005ApJ...622..759G 622, 759

    2005 doi

  78. [88]

    Gr nnow A., Tepper-Garc \' a T., Bland-Hawthorn J., 2018, [ ] 10.3847/1538-4357/aada0e , https://ui.adsabs.harvard.edu/abs/2018ApJ...865...64G 865, 64

    2018 doi

  79. [89]

    A., Murgia M., Govoni F., Gregorini L., Parma P., 2010, [ ] 10.1051/0004-6361/200913872 , http://adsabs.harvard.edu/abs/2010A

    Guidetti D., Laing R. A., Murgia M., Govoni F., Gregorini L., Parma P., 2010, [ ] 10.1051/0004-6361/200913872 , http://adsabs.harvard.edu/abs/2010A

    2010 doi

  80. [92]

    J., Saikia D

    Gupta N., Salter C. J., Saikia D. J., Ghosh T., Jeyakumar S., 2006, [ ] 10.1111/j.1365-2966.2006.11064.x , https://ui.adsabs.harvard.edu/abs/2006MNRAS.373..972G 373, 972

    2006

  81. [94]

    Gupta N., et al., 2024, [ ] 10.1017/pasa.2024.25 , https://ui.adsabs.harvard.edu/abs/2024PASA...41...27G 41, e027

    2024 doi

  82. [95]

    M., Heesen V., 2019, [ ] 10.1093/mnras/stz2033 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.4220H 488, 4220

    Hackstein S., Br \"u ggen M., Vazza F., Gaensler B. M., Heesen V., 2019, [ ] 10.1093/mnras/stz2033 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.4220H 488, 4220

    2019 doi

  83. [96]

    J., Krause M

    Hardcastle M. J., Krause M. G. H., 2014, [ ] 10.1093/mnras/stu1229 , https://ui.adsabs.harvard.edu/abs/2014MNRAS.443.1482H 443, 1482

    2014 doi

  84. [98]

    M., Kothes R., Townsend R., Heald G

    Harvey-Smith L., Gaensler B. M., Kothes R., Townsend R., Heald G. H., Ng C. Y., Green A. J., 2010, [ ] 10.1088/0004-637X/712/2/1157 , https://ui.adsabs.harvard.edu/abs/2010ApJ...712.1157H 712, 1157

    2010 doi

  85. [99]

    J., Gaensler B

    Harvey-Smith L., Madsen G. J., Gaensler B. M., 2011, [ ] 10.1088/0004-637X/736/2/83 , https://ui.adsabs.harvard.edu/abs/2011ApJ...736...83H 736, 83

    2011 doi

  86. [100]

    Haslam C. G. T., Salter C. J., Stoffel H., Wilson W. E., 1982, , https://ui.adsabs.harvard.edu/abs/1982A&AS...47....1H 47, 1

    1982

  87. [101]

    M., Melioli C., eds, Astrophysics and Space Science Library Vol

    Haverkorn M., 2015, in Lazarian A., de Gouveia Dal Pino E. M., Melioli C., eds, Astrophysics and Space Science Library Vol. 407, Magnetic Fields in Diffuse Media. p. 483 ( @eprint arXiv 1406.0283 ), 10.1007/978-3-662-44625-6\_17

    2015 arXiv

  88. [102]

    Heald G., Braun R., Edmonds R., 2009, [ ] 10.1051/0004-6361/200912240 , https://ui.adsabs.harvard.edu/abs/2009A&A...503..409H 503, 409

    2009 doi

  89. [103]

    Heald G., et al., 2020, [Galaxies] 10.3390/galaxies8030053 , https://ui.adsabs.harvard.edu/abs/2020Galax...8...53H 8, 53

    2020 doi

  90. [104]

    Heesen V., et al., 2023, [ ] 10.1051/0004-6361/202346008 , https://ui.adsabs.harvard.edu/abs/2023A&A...670L..23H 670, L23

    2023 doi

  91. [105]

    W., et al., 2021, [ ] 10.1017/pasa.2021.1 , https://ui.adsabs.harvard.edu/abs/2021PASA...38....9H 38, e009

    Hotan A. W., et al., 2021, [ ] 10.1017/pasa.2021.1 , https://ui.adsabs.harvard.edu/abs/2021PASA...38....9H 38, e009

    2021 doi

  92. [106]

    L., Aller M

    Hovatta T., Lister M. L., Aller M. F., Aller H. D., Homan D. C., Kovalev Y. Y., Pushkarev A. B., Savolainen T., 2012, [ ] 10.1088/0004-6256/144/4/105 , https://ui.adsabs.harvard.edu/abs/2012AJ....144..105H 144, 105

    2012 doi

  93. [107]

    Hurley-Walker N., et al., 2022, [ ] 10.1017/pasa.2022.17 , https://ui.adsabs.harvard.edu/abs/2022PASA...39...35H 39, e035

    2022 doi

  94. [108]

    Hutschenreuter S., et al., 2022, [ ] 10.1051/0004-6361/202140486 , https://ui.adsabs.harvard.edu/abs/2022A&A...657A..43H 657, A43

    2022 doi

  95. [109]

    T., Ophel M., 2020, in Ballester P., Ibsen J., Solar M., Shortridge K., eds, Astronomical Society of the Pacific Conference Series Vol

    Huynh M., Dempsey J., Whiting M. T., Ophel M., 2020, in Ballester P., Ibsen J., Solar M., Shortridge K., eds, Astronomical Society of the Pacific Conference Series Vol. 522, Astronomical Data Analysis Software and Systems XXVII. p. 263

    2020

  96. [110]

    Johnston-Hollitt M., et al., 2015, in Advancing Astrophysics with the Square Kilometre Array (AASKA14). p. 92 ( @eprint arXiv 1506.00808 ), 10.22323/1.215.0092

    2015 arXiv

  97. [111]

    E., et al., 2018, [ ] 10.1093/mnras/sty1956 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.3224J 480, 3224

    Jones M. E., et al., 2018, [ ] 10.1093/mnras/sty1956 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.3224J 480, 3224

    2018 doi

  98. [112]

    L., McClure-Griffiths N

    Jung S. L., McClure-Griffiths N. M., Hill A. S., 2021, [ ] 10.1093/mnras/stab2773 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.508.3921J 508, 3921

    2021 doi

  99. [113]

    L., McClure-Griffiths N

    Jung S. L., McClure-Griffiths N. M., Pakmor R., Ma Y. K., Hill A. S., Van Eck C. L., Anderson C. S., 2023, [ ] 10.1093/mnras/stad2811 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.526..836J 526, 836

    2023 doi

  100. [114]

    L., et al., 2024, [ ] 10.1093/mnras/stae2245 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.534.2938J 534, 2938

    Jung S. L., et al., 2024, [ ] 10.1093/mnras/stae2245 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.534.2938J 534, 2938

    2024 doi

  101. [115]

    F., Purcell C

    Kaczmarek J. F., Purcell C. R., Gaensler B. M., McClure-Griffiths N. M., Stevens J., 2017, [ ] 10.1093/mnras/stx206 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.467.1776K 467, 1776

    2017 doi

  102. [116]

    L., et al., 2019, [ ] 10.3847/1538-4357/ab397f , https://ui.adsabs.harvard.edu/abs/2019ApJ...884...96K 884, 96

    Kaplan D. L., et al., 2019, [ ] 10.3847/1538-4357/ab397f , https://ui.adsabs.harvard.edu/abs/2019ApJ...884...96K 884, 96

    2019 doi

  103. [117]

    Kierdorf M., et al., 2020, [ ] 10.1051/0004-6361/202037847 , https://ui.adsabs.harvard.edu/abs/2020A&A...642A.118K 642, A118

    2020 doi

  104. [118]

    S., Lilly S

    Kim K. S., Lilly S. J., Miniati F., Bernet M. L., Beck R., O'Sullivan S. P., Gaensler B. M., 2016, [ ] 10.3847/0004-637X/829/2/133 , http://adsabs.harvard.edu/abs/2016ApJ...829..133K 829, 133

    2016 doi

  105. [119]

    P., Curiel S., Emonts B

    Knuettel S., O'Sullivan S. P., Curiel S., Emonts B. H. C., 2019, [ ] 10.1093/mnras/sty3018 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.4606K 482, 4606

    2019 doi

  106. [120]

    S., et al., 2020, [ ] 10.1007/s10509-020-03831-4 , https://ui.adsabs.harvard.edu/abs/2020Ap&SS.365..118K 365, 118

    Koribalski B. S., et al., 2020, [ ] 10.1007/s10509-020-03831-4 , https://ui.adsabs.harvard.edu/abs/2020Ap&SS.365..118K 365, 118

    2020 doi

  107. [121]

    A., Riley J., 2009, [ ] 10.1111/j.1365-2966.2009.15489.x , https://ui.adsabs.harvard.edu/abs/2009MNRAS.400..646K 400, 646

    Krause M., Alexander P., Bolton R., Geisb \"u sch J., Green D. A., Riley J., 2009, [ ] 10.1111/j.1365-2966.2009.15489.x , https://ui.adsabs.harvard.edu/abs/2009MNRAS.400..646K 400, 646

    2009

  108. [122]

    Krause M., et al., 2020, [ ] 10.1051/0004-6361/202037780 , https://ui.adsabs.harvard.edu/abs/2020A&A...639A.112K 639, A112

    2020 doi

  109. [123]

    P., 2016, Cosmic Magnetic Fields

    Kronberg P. P., 2016, Cosmic Magnetic Fields . Cambridge University Press

    2016

  110. [124]

    P., Perry J

    Kronberg P. P., Perry J. J., Zukowski E. L. H., 1990, [ ] 10.1086/185731 , https://ui.adsabs.harvard.edu/abs/1990ApJ...355L..31K 355, L31

    1990 doi

  111. [125]

    W., Jones T

    Kunz M. W., Jones T. W., Zhuravleva I., 2022, in , Handbook of X-ray and Gamma-ray Astrophysics. Springer, p. 56, 10.1007/978-981-16-4544-0_125-1

    2022 doi

  112. [126]

    Lacy M., et al., 2020, [ ] 10.1088/1538-3873/ab63eb , https://ui.adsabs.harvard.edu/abs/2020PASP..132c5001L 132, 035001

    2020 doi

  113. [127]

    S., Carretti E., Gaensler B

    Lamee M., Rudnick L., Farnes J. S., Carretti E., Gaensler B. M., Haverkorn M., Poppi S., 2016, [ ] 10.3847/0004-637X/829/1/5 , https://ui.adsabs.harvard.edu/abs/2016ApJ...829....5L 829, 5

    2016 doi

  114. [128]

    X., 2020, [ ] 10.1093/mnras/staa1750 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3142L 496, 3142

    Lan T.-W., Prochaska J. X., 2020, [ ] 10.1093/mnras/staa1750 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3142L 496, 3142

    2020 doi

  115. [129]

    Lenc E., et al., 2016, [ ] 10.3847/0004-637X/830/1/38 , 830, 38

    2016 doi

  116. [130]

    L., Homan D

    Lister M. L., Homan D. C., 2005, [ ] 10.1086/432969 , https://ui.adsabs.harvard.edu/abs/2005AJ....130.1389L 130, 1389

    2005 doi

  117. [131]

    L., Aller M

    Lister M. L., Aller M. F., Aller H. D., Hodge M. A., Homan D. C., Kovalev Y. Y., Pushkarev A. B., Savolainen T., 2018, [ ] 10.3847/1538-4365/aa9c44 , https://ui.adsabs.harvard.edu/abs/2018ApJS..234...12L 234, 12

    2018 doi

  118. [132]

    D., McClure-Griffiths N

    Livingston J. D., McClure-Griffiths N. M., Gaensler B. M., Seta A., Alger M. J., 2021, [ ] 10.1093/mnras/stab253 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.3814L 502, 3814

    2021 doi

  119. [133]

    Loi F., Murgia M., Govoni F., Vacca V., Prandoni I., Bonafede A., Feretti L., 2019, [ ] 10.1093/mnras/stz350 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.485.5285L 485, 5285

    2019 doi

  120. [134]

    Loi F., Serra P., Murgia M., Govoni F., Vacca V., Maccagni F., Kleiner D., Kamphuis P., 2025, [ ] 10.1051/0004-6361/202451711 , https://ui.adsabs.harvard.edu/abs/2025A&A...694A.125L 694, A125

    2025 doi

  121. [135]

    A., 2021, [Universe] 10.3390/universe7050139 , https://ui.adsabs.harvard.edu/abs/2021Univ....7..139L 7, 139

    Lovisari L., Ettori S., Gaspari M., Giles P. A., 2021, [Universe] 10.3390/universe7050139 , https://ui.adsabs.harvard.edu/abs/2021Univ....7..139L 7, 139

    2021 doi

  122. [136]

    K., Mao S

    Ma Y. K., Mao S. A., Stil J., Basu A., West J., Heiles C., Hill A. S., Betti S. K., 2019a, [ ] 10.1093/mnras/stz1325 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.487.3432M 487, 3432

    doi

  123. [137]

    K., Mao S

    Ma Y. K., Mao S. A., Stil J., Basu A., West J., Heiles C., Hill A. S., Betti S. K., 2019b, [ ] 10.1093/mnras/stz1328 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.487.3454M 487, 3454

    doi

  124. [138]

    K., Mao S

    Ma Y. K., Mao S. A., Ordog A., Brown J. C., 2020, [ ] 10.1093/mnras/staa2105 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.497.3097M 497, 3097

    2020 doi

  125. [139]

    K., et al., 2023, [ ] 10.1093/mnras/stad462 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.521...60M 521, 60

    Ma Y. K., et al., 2023, [ ] 10.1093/mnras/stad462 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.521...60M 521, 60

    2023 doi

  126. [140]

    E., Kudoh T., Akahori T., Sofue Y., Matsumoto R., 2013, [ ] 10.1088/0004-637X/764/1/81 , https://ui.adsabs.harvard.edu/abs/2013ApJ...764...81M 764, 81

    Machida M., Nakamura K. E., Kudoh T., Akahori T., Sofue Y., Matsumoto R., 2013, [ ] 10.1088/0004-637X/764/1/81 , https://ui.adsabs.harvard.edu/abs/2013ApJ...764...81M 764, 81

    2013 doi

  127. [141]

    D., Feain I., Johnston-Hollitt M., 2012, [ ] 10.1088/0004-637X/750/2/139 , http://adsabs.harvard.edu/abs/2012ApJ...750..139M 750, 139

    Macquart J.-P., Ekers R. D., Feain I., Johnston-Hollitt M., 2012, [ ] 10.1088/0004-637X/750/2/139 , http://adsabs.harvard.edu/abs/2012ApJ...750..139M 750, 139

    2012 doi

  128. [142]

    P., et al., 2020, [ ] 10.1038/s41586-020-2300-2 , https://ui.adsabs.harvard.edu/abs/2020Natur.581..391M 581, 391

    Macquart J. P., et al., 2020, [ ] 10.1038/s41586-020-2300-2 , https://ui.adsabs.harvard.edu/abs/2020Natur.581..391M 581, 391

    2020 doi

  129. [143]

    K., et al., 2022, [ ] 10.1093/mnras/stab3041 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.1690M 509, 1690

    Mahony E. K., et al., 2022, [ ] 10.1093/mnras/stab3041 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.1690M 509, 1690

    2022 doi

  130. [144]

    R., 2020, [ ] 10.3847/1538-4357/ab6bd5 , https://ui.adsabs.harvard.edu/abs/2020ApJ...890..132M 890, 132

    Malik S., Chand H., Seshadri T. R., 2020, [ ] 10.3847/1538-4357/ab6bd5 , https://ui.adsabs.harvard.edu/abs/2020ApJ...890..132M 890, 132

    2020 doi

  131. [145]

    A., et al., 2012, [ ] 10.1088/0004-637X/759/1/25 , https://ui.adsabs.harvard.edu/abs/2012ApJ...759...25M 759, 25

    Mao S. A., et al., 2012, [ ] 10.1088/0004-637X/759/1/25 , https://ui.adsabs.harvard.edu/abs/2012ApJ...759...25M 759, 25

    2012 doi

  132. [146]

    M., Dickey J

    McClure-Griffiths N. M., Dickey J. M., Gaensler B. M., Green A. J., Haverkorn M., 2006, [ ] 10.1086/508706 , https://ui.adsabs.harvard.edu/abs/2006ApJ...652.1339M 652, 1339

    2006 doi

  133. [147]

    McConnell D., et al., 2020, [ ] 10.1017/pasa.2020.41 , https://ui.adsabs.harvard.edu/abs/2020PASA...37...48M 37, e048

    2020 doi

  134. [148]

    F., Ostriker J

    McKee C. F., Ostriker J. P., 1977, [ ] 10.1086/155667 , https://ui.adsabs.harvard.edu/abs/1977ApJ...218..148M 218, 148

    1977 doi

  135. [149]

    Medlock I., Nagai D., Singh P., Oppenheimer B., Angl \'e s-Alc \'a zar D., Villaescusa-Navarro F., 2024, [ ] 10.3847/1538-4357/ad3070 , https://ui.adsabs.harvard.edu/abs/2024ApJ...967...32M 967, 32

    2024 doi

  136. [150]

    Mocz P., Burkhart B., 2018, [ ] 10.1093/mnras/sty1976 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.480.3916M 480, 3916

    2018 doi

  137. [151]

    Morganti R., Oosterloo T., 2018, [ ] 10.1007/s00159-018-0109-x , https://ui.adsabs.harvard.edu/abs/2018A&ARv..26....4M 26, 4

    2018 doi

  138. [152]

    Moss D., Shukurov A., 1996, [ ] 10.1093/mnras/279.1.229 , https://ui.adsabs.harvard.edu/abs/1996MNRAS.279..229M 279, 229

    1996 doi

  139. [154]

    Murphy T., et al., 2013b, [ ] 10.1017/pasa.2012.006 , https://ui.adsabs.harvard.edu/abs/2013PASA...30....6M 30, e006

    2012 doi

  140. [155]

    P., et al., 2011, [ ] 10.1071/AS11021 , https://ui.adsabs.harvard.edu/abs/2011PASA...28..215N 28, 215

    Norris R. P., et al., 2011, [ ] 10.1071/AS11021 , https://ui.adsabs.harvard.edu/abs/2011PASA...28..215N 28, 215

    2011 doi

  141. [156]

    P., et al., 2021a, [ ] 10.1017/pasa.2020.52 , https://ui.adsabs.harvard.edu/abs/2021PASA...38....3N 38, e003

    Norris R. P., et al., 2021a, [ ] 10.1017/pasa.2020.52 , https://ui.adsabs.harvard.edu/abs/2021PASA...38....3N 38, e003

    2020 doi

  142. [157]

    P., et al., 2021b, [ ] 10.1017/pasa.2021.42 , https://ui.adsabs.harvard.edu/abs/2021PASA...38...46N 38, e046

    Norris R. P., et al., 2021b, [ ] 10.1017/pasa.2021.42 , https://ui.adsabs.harvard.edu/abs/2021PASA...38...46N 38, e046

    2021 doi

  143. [158]

    P., et al., 2012, [ ] 10.1111/j.1365-2966.2012.20554.x , http://adsabs.harvard.edu/abs/2012MNRAS.421.3300O 421, 3300

    O'Sullivan S. P., et al., 2012, [ ] 10.1111/j.1365-2966.2012.20554.x , http://adsabs.harvard.edu/abs/2012MNRAS.421.3300O 421, 3300

    2012

  144. [159]

    P., et al., 2013, [ ] 10.1088/0004-637X/764/2/162 , https://ui.adsabs.harvard.edu/abs/2013ApJ...764..162O 764, 162

    O'Sullivan S. P., et al., 2013, [ ] 10.1088/0004-637X/764/2/162 , https://ui.adsabs.harvard.edu/abs/2013ApJ...764..162O 764, 162

    2013 doi

  145. [160]

    P., Purcell C

    O'Sullivan S. P., Purcell C. R., Anderson C. S., Farnes J. S., Sun X. H., Gaensler B. M., 2017, [ ] 10.1093/mnras/stx1133 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.4034O 469, 4034

    2017 doi

  146. [161]

    P., Lenc E., Anderson C

    O'Sullivan S. P., Lenc E., Anderson C. S., Gaensler B. M., Murphy T., 2018, [ ] 10.1093/mnras/sty171 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.475.4263O 475, 4263

    2018 doi

  147. [162]

    P., et al., 2020, [ ] 10.1093/mnras/staa1395 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.495.2607O 495, 2607

    O'Sullivan S. P., et al., 2020, [ ] 10.1093/mnras/staa1395 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.495.2607O 495, 2607

    2020 doi

  148. [163]

    P., et al., 2023, [ ] 10.1093/mnras/stac3820 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.5723O 519, 5723

    O'Sullivan S. P., et al., 2023, [ ] 10.1093/mnras/stac3820 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.5723O 519, 5723

    2023 doi

  149. [164]

    D., Babul A., Bah \'e Y., Butsky I

    Oppenheimer B. D., Babul A., Bah \'e Y., Butsky I. S., McCarthy I. G., 2021, [Universe] 10.3390/universe7070209 , https://ui.adsabs.harvard.edu/abs/2021Univ....7..209O 7, 209

    2021 doi

  150. [165]

    Oppermann N., et al., 2012, [ ] 10.1051/0004-6361/201118526 , https://ui.adsabs.harvard.edu/abs/2012A&A...542A..93O 542, A93

    2012 doi

  151. [166]

    Osinga E., et al., 2025, [ ] 10.1051/0004-6361/202451885 , https://ui.adsabs.harvard.edu/abs/2025A&A...694A..44O 694, A44

    2025 doi

  152. [167]

    V., et al., 2023, [ ] 10.1093/mnras/stad1900 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.524.1291P 524, 1291

    Padmanabh P. V., et al., 2023, [ ] 10.1093/mnras/stad1900 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.524.1291P 524, 1291

    2023 doi

  153. [168]

    L., Gaensler B

    Pandhi A., Hutschenreuter S., West J. L., Gaensler B. M., Stock A., 2022, [ ] 10.1093/mnras/stac2314 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.516.4739P 516, 4739

    2022 doi

  154. [169]

    Parimbelli G., Branchini E., Viel M., Villaescusa-Navarro F., ZuHone J., 2023, [ ] 10.1093/mnras/stad1495 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.523.2263P 523, 2263

    2023 doi

  155. [170]

    Pasetto A., Carrasco-Gonz \'a lez C., O'Sullivan S., Basu A., Bruni G., Kraus A., Curiel S., Mack K.-H., 2018, [ ] 10.1051/0004-6361/201731804 , https://ui.adsabs.harvard.edu/abs/2018A&A...613A..74P 613, A74

    2018 doi

  156. [171]

    Piccirilli G., Migliaccio M., Branchini E., Dolfi A., 2023, [ ] 10.1051/0004-6361/202244799 , https://ui.adsabs.harvard.edu/abs/2023A&A...671A..42P 671, A42

    2023 doi

  157. [172]

    V., O'Sullivan S

    Pignataro G. V., O'Sullivan S. P., Bonafede A., Bernardi G., Vazza F., Carretti E., 2025, [arXiv e-prints] 10.48550/arXiv.2503.08765 , https://ui.adsabs.harvard.edu/abs/2025arXiv250308765P p. arXiv:2503.08765

    2025 doi arXiv

  158. [173]

    M., et al., 2022, [ ] 10.1017/pasa.2021.59 , https://ui.adsabs.harvard.edu/abs/2022PASA...39....5P 39, e005

    Pingel N. M., et al., 2022, [ ] 10.1017/pasa.2021.59 , https://ui.adsabs.harvard.edu/abs/2022PASA...39....5P 39, e005

    2022 doi

  159. [174]

    P., et al., 2022, [ ] 10.1093/mnras/stac1805 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.515..256P 515, 256

    Pomakov V. P., et al., 2022, [ ] 10.1093/mnras/stac1805 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.515..256P 515, 256

    2022 doi

  160. [175]

    Pritchard J., et al., 2021, [ ] 10.1093/mnras/stab299 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.5438P 502, 5438

    2021 doi

  161. [176]

    R., Van Eck C

    Purcell C. R., Van Eck C. L., West J., Sun X. H., Gaensler B. M., 2020, RM-Tools: Rotation measure (RM) synthesis and Stokes QU-fitting , Astrophysics Source Code Library, record ascl:2005.003

    2020

  162. [177]

    A., Deane R., Sridhar S

    Ranchod S., Mao S. A., Deane R., Sridhar S. S., Damas-Segovia A., Livingston J. D., Ma Y. K., 2024, [ ] 10.1051/0004-6361/202348993 , https://ui.adsabs.harvard.edu/abs/2024A&A...686A.104R 686, A104

    2024 doi

  163. [178]

    Raycheva N., et al., 2025, [ ] 10.1051/0004-6361/202449556 , https://ui.adsabs.harvard.edu/abs/2025A&A...695A.101R 695, A101

    2025 doi

  164. [179]

    J., 2006, [Astronomische Nachrichten] 10.1002/asna.200610540 , https://ui.adsabs.harvard.edu/abs/2006AN....327..395R 327, 395

    Rees M. J., 2006, [Astronomische Nachrichten] 10.1002/asna.200610540 , https://ui.adsabs.harvard.edu/abs/2006AN....327..395R 327, 395

    2006 doi

  165. [180]

    S., Pellegrini E

    Reissl S., Brauer R., Klessen R. S., Pellegrini E. W., 2019, [ ] 10.3847/1538-4357/ab3664 , https://ui.adsabs.harvard.edu/abs/2019ApJ...885...15R 885, 15

    2019 doi

  166. [181]

    J., Bigot-Sazy M

    Remazeilles M., Dickinson C., Banday A. J., Bigot-Sazy M. A., Ghosh T., 2015, [ ] 10.1093/mnras/stv1274 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.451.4311R 451, 4311

    2015 doi

  167. [182]

    Rincon F., 2019, [Journal of Plasma Physics] 10.1017/S0022377819000539 , https://ui.adsabs.harvard.edu/abs/2019JPlPh..85d2001R 85, 205850401

    2019 doi

  168. [183]

    J., et al., 2018, [ ] 10.1017/pasa.2018.39 , https://ui.adsabs.harvard.edu/abs/2018PASA...35...43R 35, e043

    Riseley C. J., et al., 2018, [ ] 10.1017/pasa.2018.39 , https://ui.adsabs.harvard.edu/abs/2018PASA...35...43R 35, e043

    2018 doi

  169. [184]

    J., et al., 2020, [ ] 10.1017/pasa.2020.20 , https://ui.adsabs.harvard.edu/abs/2020PASA...37...29R 37, e029

    Riseley C. J., et al., 2020, [ ] 10.1017/pasa.2020.20 , https://ui.adsabs.harvard.edu/abs/2020PASA...37...29R 37, e029

    2020 doi

  170. [185]

    A., et al., 2023, [ ] 10.1093/mnras/stac3439 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.3383R 519, 3383

    Rubi \ n o-Mart \' n J. A., et al., 2023, [ ] 10.1093/mnras/stac3439 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.3383R 519, 3383

    2023 doi

  171. [186]

    arXiv:1901.09448

    Rudnick L., 2019, arXiv e-prints, https://ui.adsabs.harvard.edu/abs/2019arXiv190109448R p. arXiv:1901.09448

    2019 arXiv

  172. [187]

    D., 2023, [ ] 10.1093/mnras/stad1090 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.522.1464R 522, 1464

    Rudnick L., Cotton W. D., 2023, [ ] 10.1093/mnras/stad1090 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.522.1464R 522, 1464

    2023 doi

  173. [188]

    N., 2014a, [ ] 10.1088/0004-637X/785/1/45 , https://ui.adsabs.harvard.edu/abs/2014ApJ...785...45R 785, 45

    Rudnick L., Owen F. N., 2014a, [ ] 10.1088/0004-637X/785/1/45 , https://ui.adsabs.harvard.edu/abs/2014ApJ...785...45R 785, 45

    doi

  174. [189]

    N., 2014b, [ ] 10.1088/0004-637X/786/2/160 , https://ui.adsabs.harvard.edu/abs/2014ApJ...786..160R 786, 160

    Rudnick L., Owen F. N., 2014b, [ ] 10.1088/0004-637X/786/2/160 , https://ui.adsabs.harvard.edu/abs/2014ApJ...786..160R 786, 160

    doi

  175. [190]

    D., Pasetto A., Alexander E

    Rudnick L., Anderson C., Cotton W. D., Pasetto A., Alexander E. L., Tahani M., 2024, [ ] 10.1093/mnras/stae2225 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.535.2115R 535, 2115

    2024 doi

  176. [191]

    Ruszkowski M., Pfrommer C., 2023, [ ] 10.1007/s00159-023-00149-2 , https://ui.adsabs.harvard.edu/abs/2023A&ARv..31....4R 31, 4

    2023 doi

  177. [192]

    Schnitzeler D. H. F. M., 2010, [ ] 10.1111/j.1745-3933.2010.00957.x , http://adsabs.harvard.edu/abs/2010MNRAS.409L..99S 409, L99

    2010

  178. [193]

    Sebokolodi M. L. L., Perley R., Eilek J., Carilli C., Smirnov O., Laing R., Greisen E. W., Wise M., 2020, [ ] 10.3847/1538-4357/abb80e , https://ui.adsabs.harvard.edu/abs/2020ApJ...903...36S 903, 36

    2020 doi

  179. [194]

    Seta A., Federrath C., 2021a, [Physical Review Fluids] 10.1103/PhysRevFluids.6.103701 , https://ui.adsabs.harvard.edu/abs/2021PhRvF...6j3701S 6, 103701

    doi

  180. [195]

    Seta A., Federrath C., 2021b, [ ] 10.1093/mnras/stab128 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.2220S 502, 2220

    doi

  181. [196]

    Seta A., Federrath C., 2022, [ ] 10.1093/mnras/stac1400 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.514..957S 514, 957

    2022 doi

  182. [197]

    J., Shukurov A., Wood T

    Seta A., Bushby P. J., Shukurov A., Wood T. S., 2020, [Physical Review Fluids] 10.1103/PhysRevFluids.5.043702 , https://ui.adsabs.harvard.edu/abs/2020PhRvF...5d3702S 5, 043702

    2020 doi

  183. [198]

    Seta A., Rodrigues L. F. S., Federrath C., Hales C. A., 2021, [ ] 10.3847/1538-4357/abd2bb , https://ui.adsabs.harvard.edu/abs/2021ApJ...907....2S 907, 2

    2021 doi

  184. [199]

    D., McClure-Griffiths N

    Seta A., Federrath C., Livingston J. D., McClure-Griffiths N. M., 2023, [ ] 10.1093/mnras/stac2972 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518..919S 518, 919

    2023 doi

  185. [200]

    Shah H., Seta A., 2021, [ ] 10.1093/mnras/stab2500 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.508.1371S 508, 1371

    2021 doi

  186. [201]

    Shanahan R., et al., 2019, [ ] 10.3847/2041-8213/ab58d4 , https://ui.adsabs.harvard.edu/abs/2019ApJ...887L...7S 887, L7

    2019 doi

  187. [202]

    Shanahan R., et al., 2022, [ ] 10.3847/1538-4357/ac96f0 , https://ui.adsabs.harvard.edu/abs/2022ApJ...939...92S 939, 92

    2022 doi

  188. [203]

    W., et al., 2017, [ ] 10.1051/0004-6361/201629313 , https://ui.adsabs.harvard.edu/abs/2017A&A...598A.104S 598, A104

    Shimwell T. W., et al., 2017, [ ] 10.1051/0004-6361/201629313 , https://ui.adsabs.harvard.edu/abs/2017A&A...598A.104S 598, A104

    2017 doi

  189. [204]

    W., et al., 2019, [ ] 10.1051/0004-6361/201833559 , https://ui.adsabs.harvard.edu/abs/2019A&A...622A...1S 622, A1

    Shimwell T. W., et al., 2019, [ ] 10.1051/0004-6361/201833559 , https://ui.adsabs.harvard.edu/abs/2019A&A...622A...1S 622, A1

    2019 doi

  190. [205]

    W., et al., 2022, [ ] 10.1051/0004-6361/202142484 , https://ui.adsabs.harvard.edu/abs/2022A&A...659A...1S 659, A1

    Shimwell T. W., et al., 2022, [ ] 10.1051/0004-6361/202142484 , https://ui.adsabs.harvard.edu/abs/2022A&A...659A...1S 659, A1

    2022 doi

  191. [206]

    Shukurov A., Rodrigues L. F. S., Bushby P. J., Hollins J., Rachen J. P., 2019, [ ] 10.1051/0004-6361/201834642 , https://ui.adsabs.harvard.edu/abs/2019A&A...623A.113S 623, A113

    2019 doi

  192. [207]

    M., Smith B

    Shull J. M., Smith B. D., Danforth C. W., 2012, [ ] 10.1088/0004-637X/759/1/23 , https://ui.adsabs.harvard.edu/abs/2012ApJ...759...23S 759, 23

    2012 doi

  193. [208]

    P., 1979, [ ] 10.1038/279115a0 , https://ui.adsabs.harvard.edu/abs/1979Natur.279..115S 279, 115

    Simard-Normandin M., Kronberg P. P., 1979, [ ] 10.1038/279115a0 , https://ui.adsabs.harvard.edu/abs/1979Natur.279..115S 279, 115

    1979 doi

  194. [209]

    I., 1965, , https://ui.adsabs.harvard.edu/abs/1965AZh....42..689S 42, 689

    Slysh V. I., 1965, , https://ui.adsabs.harvard.edu/abs/1965AZh....42..689S 42, 689

    1965

  195. [210]

    Smith M. W. L., et al., 2017, [ ] 10.3847/1538-4365/aa9b35 , https://ui.adsabs.harvard.edu/abs/2017ApJS..233...26S 233, 26

    2017 doi

  196. [211]

    D., Bykov A

    Sokoloff D. D., Bykov A. A., Shukurov A., Berkhuijsen E. M., Beck R., Poezd A. D., 1998, [ ] 10.1046/j.1365-8711.1998.01782.x , https://ui.adsabs.harvard.edu/abs/1998MNRAS.299..189S 299, 189

    1998

  197. [212]

    R., 2021, [Research Notes of the American Astronomical Society] 10.3847/2515-5172/abdc2d , https://ui.adsabs.harvard.edu/abs/2021RNAAS...5...12S 5, 12

    Spangler S. R., 2021, [Research Notes of the American Astronomical Society] 10.3847/2515-5172/abdc2d , https://ui.adsabs.harvard.edu/abs/2021RNAAS...5...12S 5, 12

    2021 doi

  198. [213]

    E., Dolag K., Beck R., Donnert J., 2010, [ ] 10.1111/j.1365-2966.2010.17166.x , https://ui.adsabs.harvard.edu/abs/2010MNRAS.408..684S 408, 684

    Stasyszyn F., Nuza S. E., Dolag K., Beck R., Donnert J., 2010, [ ] 10.1111/j.1365-2966.2010.17166.x , https://ui.adsabs.harvard.edu/abs/2010MNRAS.408..684S 408, 684

    2010

  199. [214]

    P., Dolag K., Lesch H., Burkert A., 2022, [ ] 10.3847/1538-4357/ac2ffd , https://ui.adsabs.harvard.edu/abs/2022ApJ...924...26S 924, 26

    Steinwandel U. P., Dolag K., Lesch H., Burkert A., 2022, [ ] 10.3847/1538-4357/ac2ffd , https://ui.adsabs.harvard.edu/abs/2022ApJ...924...26S 924, 26

    2022 doi

  200. [215]

    M., Keller B

    Stil J. M., Keller B. W., George S. J., Taylor A. R., 2014, [ ] 10.1088/0004-637X/787/2/99 , https://ui.adsabs.harvard.edu/abs/2014ApJ...787...99S 787, 99

    2014 doi

  201. [216]

    G., 1973, , https://ui.adsabs.harvard.edu/abs/1973A&A....25..303S 25, 303

    Strom R. G., 1973, , https://ui.adsabs.harvard.edu/abs/1973A&A....25..303S 25, 303

    1973

  202. [217]

    G., Jaegers W

    Strom R. G., Jaegers W. J., 1988, , https://ui.adsabs.harvard.edu/abs/1988A&A...194...79S 194, 79

    1988

  203. [218]

    Stuardi C., et al., 2019, [ ] 10.1093/mnras/stz2408 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.489.3905S 489, 3905

    2019 doi

  204. [219]

    Stuardi C., et al., 2020, [ ] 10.1051/0004-6361/202037635 , https://ui.adsabs.harvard.edu/abs/2020A&A...638A..48S 638, A48

    2020 doi

  205. [220]

    J., de Gasperin F., 2021, [ ] 10.1093/mnras/stab218 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.2518S 502, 2518

    Stuardi C., Bonafede A., Lovisari L., Dom \' nguez-Fern \'a ndez P., Vazza F., Br \"u ggen M., van Weeren R. J., de Gasperin F., 2021, [ ] 10.1093/mnras/stab218 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.2518S 502, 2518

    2021 doi

  206. [221]

    J., Vazza F., 2022, [ ] 10.1051/0004-6361/202244179 , https://ui.adsabs.harvard.edu/abs/2022A&A...666A...8S 666, A8

    Stuardi C., Bonafede A., Rajpurohit K., Br \"u ggen M., de Gasperin F., Hoang D., van Weeren R. J., Vazza F., 2022, [ ] 10.1051/0004-6361/202244179 , https://ui.adsabs.harvard.edu/abs/2022A&A...666A...8S 666, A8

    2022 doi

  207. [222]

    Subramanian K., 2016, [Reports on Progress in Physics] 10.1088/0034-4885/79/7/076901 , https://ui.adsabs.harvard.edu/abs/2016RPPh...79g6901S 79, 076901

    2016 doi

  208. [223]

    H., et al., 2015, [ ] 10.1088/0004-6256/149/2/60 , http://adsabs.harvard.edu/abs/2015AJ....149...60S 149, 60

    Sun X. H., et al., 2015, [ ] 10.1088/0004-6256/149/2/60 , http://adsabs.harvard.edu/abs/2015AJ....149...60S 149, 60

    2015 doi

  209. [224]

    Sun X., et al., 2025, [ ] 10.1051/0004-6361/202453326 , https://ui.adsabs.harvard.edu/abs/2025A&A...694A.169S 694, A169

    2025 doi

  210. [225]

    C., Kainulainen J., 2018, [ ] 10.1051/0004-6361/201732219 , https://ui.adsabs.harvard.edu/abs/2018A&A...614A.100T 614, A100

    Tahani M., Plume R., Brown J. C., Kainulainen J., 2018, [ ] 10.1051/0004-6361/201732219 , https://ui.adsabs.harvard.edu/abs/2018A&A...614A.100T 614, A100

    2018 doi

  211. [226]

    R., Stil J

    Taylor A. R., Stil J. M., Sunstrum C., 2009, [ ] 10.1088/0004-637X/702/2/1230 , https://ui.adsabs.harvard.edu/abs/2009ApJ...702.1230T 702, 1230

    2009 doi

  212. [227]

    R., et al., 2024, [ ] 10.1093/mnras/stae169 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.528.2511T 528, 2511

    Taylor A. R., et al., 2024, [ ] 10.1093/mnras/stae169 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.528.2511T 528, 2511

    2024 doi

  213. [228]

    Thomson A. J. M., et al., 2019, [ ] 10.1093/mnras/stz1438 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.487.4751T 487, 4751

    2019 doi

  214. [229]

    Thomson A. J. M., et al., 2023, [ ] 10.1017/pasa.2023.38 , https://ui.adsabs.harvard.edu/abs/2023PASA...40...40T 40, e040

    2023 doi

  215. [230]

    C., 1991, [ ] 10.1093/mnras/250.4.726 , https://ui.adsabs.harvard.edu/abs/1991MNRAS.250..726T 250, 726

    Tribble P. C., 1991, [ ] 10.1093/mnras/250.4.726 , https://ui.adsabs.harvard.edu/abs/1991MNRAS.250..726T 250, 726

    1991 doi

  216. [231]

    L., et al., 2011, [ ] 10.1088/0004-637X/728/2/97 , https://ui.adsabs.harvard.edu/abs/2011ApJ...728...97V 728, 97

    Van Eck C. L., et al., 2011, [ ] 10.1088/0004-637X/728/2/97 , https://ui.adsabs.harvard.edu/abs/2011ApJ...728...97V 728, 97

    2011 doi

  217. [232]

    L., et al., 2017, [ ] 10.1051/0004-6361/201629707 , https://ui.adsabs.harvard.edu/abs/2017A&A...597A..98V 597, A98

    Van Eck C. L., et al., 2017, [ ] 10.1051/0004-6361/201629707 , https://ui.adsabs.harvard.edu/abs/2017A&A...597A..98V 597, A98

    2017 doi

  218. [233]

    L., et al., 2019, [ ] 10.1051/0004-6361/201834777 , https://ui.adsabs.harvard.edu/abs/2019A&A...623A..71V 623, A71

    Van Eck C. L., et al., 2019, [ ] 10.1051/0004-6361/201834777 , https://ui.adsabs.harvard.edu/abs/2019A&A...623A..71V 623, A71

    2019 doi

  219. [234]

    L., et al., 2023, [ ] 10.3847/1538-4365/acda24 , https://ui.adsabs.harvard.edu/abs/2023ApJS..267...28V 267, 28

    Van Eck C. L., et al., 2023, [ ] 10.3847/1538-4365/acda24 , https://ui.adsabs.harvard.edu/abs/2023ApJS..267...28V 267, 28

    2023 doi

  220. [235]

    Vanderwoude S., et al., 2024, [ ] 10.3847/1538-3881/ad2fc8 , https://ui.adsabs.harvard.edu/abs/2024AJ....167..226V 167, 226

    2024 doi

  221. [236]

    M., 2017, [Classical and Quantum Gravity] 10.1088/1361-6382/aa8e60 , https://ui.adsabs.harvard.edu/abs/2017CQGra..34w4001V 34, 234001

    Vazza F., Br \"u ggen M., Gheller C., Hackstein S., Wittor D., Hinz P. M., 2017, [Classical and Quantum Gravity] 10.1088/1361-6382/aa8e60 , https://ui.adsabs.harvard.edu/abs/2017CQGra..34w4001V 34, 234001

    2017 doi

  222. [237]

    Vazza F., Wittor D., Brunetti G., Br \"u ggen M., 2021, [ ] 10.1051/0004-6361/202140513 , https://ui.adsabs.harvard.edu/abs/2021A&A...653A..23V 653, A23

    2021 doi

  223. [238]

    M., Rudnick L., Andernach H., 2019, [ ] 10.3847/1538-4357/ab1f83 , https://ui.adsabs.harvard.edu/abs/2019ApJ...878...92V 878, 92

    Vernstrom T., Gaensler B. M., Rudnick L., Andernach H., 2019, [ ] 10.3847/1538-4357/ab1f83 , https://ui.adsabs.harvard.edu/abs/2019ApJ...878...92V 878, 92

    2019 doi

  224. [239]

    Voronkov M., 2020, in European Physical Journal Web of Conferences. p. 01038, 10.1051/epjconf/202024501038

    2020

  225. [240]

    S., En lin T

    Waelkens A., Jaffe T., Reinecke M., Kitaura F. S., En lin T. A., 2009, [ ] 10.1051/0004-6361:200810564 , https://ui.adsabs.harvard.edu/abs/2009A&A...495..697W 495, 697

    2009 doi

  226. [241]

    J., et al., 2024, [ ] 10.3847/1538-4357/ad4f8c , https://ui.adsabs.harvard.edu/abs/2024ApJ...970...92W 970, 92

    Weatherhead K. J., et al., 2024, [ ] 10.3847/1538-4357/ad4f8c , https://ui.adsabs.harvard.edu/abs/2024ApJ...970...92W 970, 92

    2024 doi

  227. [242]

    L., Safi-Harb S., Ferrand G., 2017, [ ] 10.1051/0004-6361/201628079 , https://ui.adsabs.harvard.edu/abs/2017A&A...597A.121W 597, A121

    West J. L., Safi-Harb S., Ferrand G., 2017, [ ] 10.1051/0004-6361/201628079 , https://ui.adsabs.harvard.edu/abs/2017A&A...597A.121W 597, A121

    2017 doi

  228. [243]

    L., Brouw W

    Westerhout G., Seeger C. L., Brouw W. N., Tinbergen J., 1962, , https://ui.adsabs.harvard.edu/abs/1962BAN....16..187W 16, 187

    1962

  229. [244]

    Whiting M., Humphreys B., 2012, [ ] 10.1071/AS12028 , https://ui.adsabs.harvard.edu/abs/2012PASA...29..371W 29, 371

    2012 doi

  230. [245]

    M., 2002, [Reviews of Modern Physics] 10.1103/RevModPhys.74.775 , https://ui.adsabs.harvard.edu/abs/2002RvMP...74..775W 74, 775

    Widrow L. M., 2002, [Reviews of Modern Physics] 10.1103/RevModPhys.74.775 , https://ui.adsabs.harvard.edu/abs/2002RvMP...74..775W 74, 775

    2002 doi

  231. [246]

    R., 1962, [ ] 10.1038/195982a0 , https://ui.adsabs.harvard.edu/abs/1962Natur.195..982W 195, 982

    Wielebinski R., Shakeshaft J. R., 1962, [ ] 10.1038/195982a0 , https://ui.adsabs.harvard.edu/abs/1962Natur.195..982W 195, 982

    1962 doi

  232. [247]

    H., de Bruyn A

    Wieringa M. H., de Bruyn A. G., Jansen D., Brouw W. N., Katgert P., 1993, , https://ui.adsabs.harvard.edu/abs/1993A&A...268..215W 268, 215

    1993

  233. [248]

    L., et al., 2019, [ ] 10.1051/0004-6361/201833564 , https://ui.adsabs.harvard.edu/abs/2019A&A...622A...2W 622, A2

    Williams W. L., et al., 2019, [ ] 10.1051/0004-6361/201833564 , https://ui.adsabs.harvard.edu/abs/2019A&A...622A...2W 622, A2

    2019 doi

  234. [249]

    E., et al., 2011, [ ] 10.1111/j.1365-2966.2011.19054.x , https://ui.adsabs.harvard.edu/abs/2011MNRAS.416..832W 416, 832

    Wilson W. E., et al., 2011, [ ] 10.1111/j.1365-2966.2011.19054.x , https://ui.adsabs.harvard.edu/abs/2011MNRAS.416..832W 416, 832

    2011

  235. [250]

    Wolleben M., et al., 2019, [ ] 10.3847/1538-3881/ab22b0 , https://ui.adsabs.harvard.edu/abs/2019AJ....158...44W 158, 44

    2019 doi

  236. [251]

    Wolleben M., et al., 2021, [ ] 10.3847/1538-3881/abf7c1 , https://ui.adsabs.harvard.edu/abs/2021AJ....162...35W 162, 35

    2021 doi

  237. [252]

    Zhang X., et al., 2024, [ ] 10.1051/0004-6361/202450933 , https://ui.adsabs.harvard.edu/abs/2024A&A...691A.234Z 691, A234

    2024 doi

  238. [253]

    Zhu G., M \'e nard B., 2013, [ ] 10.1088/0004-637X/770/2/130 , https://ui.adsabs.harvard.edu/abs/2013ApJ...770..130Z 770, 130

    2013 doi

  239. [254]

    Zic A., et al., 2019, [ ] 10.1093/mnras/stz1684 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488..559Z 488, 559

    2019 doi

  240. [255]

    A., et al., 2022, [ ] 10.1051/0004-6361/202141739 , https://ui.adsabs.harvard.edu/abs/2022A&A...658A.146V 658, A146

    van Cappellen W. A., et al., 2022, [ ] 10.1051/0004-6361/202141739 , https://ui.adsabs.harvard.edu/abs/2022A&A...658A.146V 658, A146

    2022 doi

  241. [256]

    van Weeren R. J., de Gasperin F., Akamatsu H., Br \"u ggen M., Feretti L., Kang H., Stroe A., Zandanel F., 2019, [ ] 10.1007/s11214-019-0584-z , https://ui.adsabs.harvard.edu/abs/2019SSRv..215...16V 215, 16

    2019 doi

Pith tools

Reviewed August 15, 2026 · model on record in the stance chip above.