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arxiv: 2606.26355 · v1 · pith:AGARAT7Gnew · submitted 2026-06-24 · 🌌 astro-ph.GA

Probing the Nature of Lyman Continuum Emitting and Low-metallicity Galaxies Using the SKA

Omkar Bait , Daniel Schaerer , Mark Sargent This is my paper

Pith reviewed 2026-06-26 01:14 UTC · model grok-4.3

classification 🌌 astro-ph.GA
keywords Lyman continuum emittersSKAradio continuumcosmic reionizationlow-metallicity galaxiesstar formation rateLyC escape fraction
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The pith

SKA-Mid surveys can assemble samples of 10-100 Lyman continuum emitter candidates per square degree at redshifts 1-3.

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

The paper presents number density predictions for Lyman continuum emitting galaxies at z approximately 1 to 3 based on radio continuum properties. These predictions indicate that SKA-Mid observations can detect enough candidates across a star formation rate range of 1 to 100 solar masses per year to support a dedicated large program. The work builds on links seen in low-redshift systems between radio spectral index, escape of ionizing photons, metallicity, and star formation density. If correct, this approach would enable studies of the feedback processes that allow Lyman continuum photons to escape in low-mass, metal-poor galaxies.

Core claim

Targeted mid-frequency observations with SKA precursors have revealed connections between radio continuum spectral index, LyC escape fraction, ionization conditions, metallicity, and SFR surface density in low-redshift LCEs, along with deviations from the standard radio-SFR relation. The higher sensitivity of SKA Array Assemblies in Bands 1-5 will allow systematic studies of fainter LCEs and low-mass metal-poor galaxies at higher redshifts. Number density predictions show SKA-Mid surveys can yield samples of roughly 10-100 candidates per square degree over SFR 1-100 solar masses per year at z~1-3, making a dedicated SKA Large Programme feasible. With the full SKA in synergy with JWST, multi-

What carries the argument

Number density predictions for LCE candidates at z~1-3 derived by extrapolating radio continuum spectral index and escape fraction relations observed in low-redshift systems.

If this is right

  • SKA-Mid can target LCE candidates over a star-formation rate range of 1-100 solar masses per year at z~1-3.
  • A dedicated SKA Large Programme becomes scientifically feasible with samples of 10-100 candidates per square degree.
  • Full SKA observations combined with JWST data can separate thermal and non-thermal radio components in these galaxies.
  • Constraints on cosmic-ray energy spectra will inform feedback processes that control LyC photon escape.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • If the predictions hold, radio observations could help identify which low-mass galaxies contributed most to cosmic reionization.
  • The approach opens a path to test whether extreme ionization conditions in metal-poor systems are tied to specific radio signatures across cosmic time.
  • Actual SKA detections would provide a direct check on whether the low-redshift scaling relations extend to the faint end of the luminosity function.

Load-bearing premise

The observed links between radio continuum properties and LyC escape in nearby galaxies also apply to fainter systems at redshifts 1 to 3.

What would settle it

SKA-Mid observations of candidate LCEs at z~1-3 that find either far fewer than 10 per square degree or no correlation between radio spectral index and LyC escape fraction would falsify the prediction.

Figures

Figures reproduced from arXiv: 2606.26355 by Daniel Schaerer, Mark Sargent, Omkar Bait.

Figure 1
Figure 1. Figure 1: Relation between the Lyman continuum escape fraction ( 𝑓 LyC esc ) and the integrated radio spectral index measured between the S (3 GHz) and C (6 GHz) bands. Galaxies with direct LyC observations from the LzLCS survey are plotted in gray points where the 𝑓 LyC esc is derived using a UV-fit method (Flury et al., 2022a), with non-detections represented as 1𝜎 upper limits. The blue hexagons represent xSFGs f… view at source ↗
Figure 2
Figure 2. Figure 2: The expected radio flux density at SKA-Mid Band 2 (left-panel) and Band 5a (right-panel) vs the dust-corrected H𝛽 flux density. We show the relation from Eq. 4 for different values of fth 𝜈 in coloured solid lines. The dashed horizontal lines shows the 5𝜎 limit on the sensitivity of the two SKA-Mid bands assuming 1 hr on-source integration (see [PITH_FULL_IMAGE:figures/full_fig_p009_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: Predicted radio spectral luminosity function of H𝛼 emitters and EELGs at 𝜈 = 1.31 GHz (SKA￾Mid Band 2) for 𝑧 = 0.5, 1.0, 2.0, and 3.0, derived by applying Eq. 4 to two H𝛼 luminosity functions. Solid blue line shows the Schechter LF of Saito et al. (2020) for the general H𝛼-emitting galaxy population (0.3 < 𝑧 < 2.5); dashed red line shows the power-law LF of Maseda et al. (2018) for extreme EELGs with EW𝐻 𝛼… view at source ↗
Figure 4
Figure 4. Figure 4: Predicted surface number density (top) and required survey sky area (bottom) of H𝛼-emitting LCE candidates and EELG as a function of radio flux density 𝑆𝜈 at 1.31 GHz (SKA-Mid Band 2). Data points show predictions for four redshifts (𝑧 ∼ 0.5: diamonds; 𝑧 ∼ 1: triangles; 𝑧 ∼ 2: circles; 𝑧 ∼ 3: squares) and two SFR bins (blue: 1–10 𝑀⊙ yr−1 ; orange: 10–100 𝑀⊙ yr−1 ), with horizontal error bars spanning the r… view at source ↗
read the original abstract

The sources responsible for cosmic reionization remain a key open question in observational cosmology. Recent JWST results increasingly suggest that low-mass star-forming galaxies (e.g., compact starbursts and strong emission-line systems) dominated the ionizing photon budget. The physical mechanisms driving Lyman continuum (LyC) photon escape, including supernova, radiative, and cosmic-ray feedback, and the origin of extreme ionization conditions, remain poorly understood. Radio continuum (RC) emission, a well-established star-formation tracer in normal galaxies, is not yet well characterized in such extreme systems, which exhibit high star-formation rate densities, young stellar populations, low metallicity, and hard ionizing spectra. Targeted mid-frequency ($1-15$,GHz) observations with SKA precursors have begun probing low-redshift LyC emitters (LCEs), revealing links between RC spectral index, LyC escape fraction, ionization conditions, metallicity, and SFR surface density, alongwith deviations from the canonical RC$-$SFR relation. The higher sensitivity of the SKA Array Assemblies across Bands $\sim 1-5$ will enable systematic studies of fainter LCEs and low-mass, metal-poor galaxies. We present number density predictions for LCE candidates at $z \sim 1$-$3$, showing that SKA-Mid surveys can assemble samples of $\sim10-100$ candidates per square degree over a star-formation rate range of $1-100$,$M_{\odot}$yr$^{-1}$, making a dedicated SKA Large Programme scientifically feasible. With the full SKA, in synergy with JWST and next generation telescopes, multi-wavelength analyses will robustly constrain the thermal and non-thermal RC components and cosmic-ray energy spectra, providing critical insights into the feedback processes governing LyC escape and star formation in the early universe.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript claims that correlations between radio continuum spectral index, LyC escape fraction, ionization conditions, metallicity, and SFR surface density observed in low-redshift LCEs with SKA precursors can be used to predict number densities of LCE candidates at z∼1-3. It concludes that SKA-Mid surveys can assemble samples of ∼10-100 candidates per square degree over SFR 1-100 M⊙ yr⁻¹, rendering a dedicated SKA Large Programme feasible, with further synergies possible using the full SKA and JWST to constrain thermal/non-thermal RC components and cosmic-ray spectra.

Significance. If the low-z correlations prove redshift-invariant and applicable to fainter high-z systems, the number-density forecasts would provide a practical justification for allocating SKA time to study feedback mechanisms governing LyC escape in the reionization-era galaxy population, complementing JWST observations. The work identifies a potentially high-impact use case for SKA-Mid Bands 1-5 but does not supply independent validation of the extrapolation.

major comments (2)
  1. [Abstract] Abstract: The central number-density prediction (∼10-100 candidates deg⁻²) is stated without any derivation, scaling relations, input assumptions, model equations, or error analysis, so it is impossible to determine whether the quoted range is supported by the underlying low-z data or extrapolations.
  2. [Abstract] Abstract: The feasibility conclusion rests on the untested assumption that the RC-LyC, RC-metallicity, and RC-Σ_SFR relations observed at low redshift remain valid for the fainter, higher-redshift (z∼1-3) population; no high-z calibration data, simulation suite, or redshift-invariance test is presented to support this extrapolation.
minor comments (2)
  1. Text contains typographical issues including 'alongwith' (should be 'along with'), '1-15,GHz' (comma instead of space or en-dash), and '1-100,M⊙yr−1' (inconsistent spacing and punctuation around units).
  2. [Abstract] The abstract refers to 'SKA Array Assemblies across Bands ∼1-5' without defining the exact frequency coverage or array configuration assumed for the sensitivity calculations.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their constructive comments. We address the two major comments on the abstract below and indicate where revisions will be made to improve clarity without altering the core content of the work.

read point-by-point responses

  1. Referee: [Abstract] Abstract: The central number-density prediction (∼10-100 candidates deg⁻²) is stated without any derivation, scaling relations, input assumptions, model equations, or error analysis, so it is impossible to determine whether the quoted range is supported by the underlying low-z data or extrapolations.

    Authors: The number-density forecast is derived in the main text from the low-z RC-LyC, RC-metallicity and RC-Σ_SFR correlations measured with SKA precursors, combined with the observed SFR function at z∼1-3 and standard assumptions on spectral index and luminosity. To address the concern that this is not evident from the abstract alone, we will revise the abstract to include a concise clause referencing the extrapolation method (e.g., “based on low-z SKA-precursor correlations extrapolated via the SFR density evolution”). This change will make the supporting data and assumptions traceable from the abstract. revision: yes

  2. Referee: [Abstract] Abstract: The feasibility conclusion rests on the untested assumption that the RC-LyC, RC-metallicity, and RC-Σ_SFR relations observed at low redshift remain valid for the fainter, higher-redshift (z∼1-3) population; no high-z calibration data, simulation suite, or redshift-invariance test is presented to support this extrapolation.

    Authors: We agree that the relations are extrapolated from low-redshift observations and that the manuscript contains no independent high-z calibration or simulation test of redshift invariance; such data are not yet available at the necessary sensitivities. The paper frames the result explicitly as a prediction intended to motivate future SKA observations that can test the assumption. We will revise the abstract to state the extrapolation assumption more explicitly, thereby clarifying the basis and limitations of the feasibility claim. revision: partial

Circularity Check

0 steps flagged

No significant circularity detected

full rationale

The paper's central claim consists of number density forecasts for LCE candidates at z~1-3 derived from observed correlations (RC spectral index vs. LyC escape, metallicity, Σ_SFR) reported in prior SKA-precursor work at low redshift. No equations, self-citations, or derivations are exhibited in the provided text that reduce these forecasts to the input relations by construction, rename a fitted parameter as a prediction, or import uniqueness via author-overlapping citations. The forecasts are presented as extrapolations that remain externally falsifiable with SKA-Mid data, rendering the derivation chain self-contained against independent benchmarks.

Axiom & Free-Parameter Ledger

1 free parameters · 1 axioms · 0 invented entities

Based solely on the abstract, the central predictions rest on the assumption that observed correlations from SKA precursors can be scaled to new regimes; no explicit free parameters, new entities, or additional axioms are detailed in the provided text.

free parameters (1)
  • Scaling factors for RC-SFR relations in extreme galaxies
    The 10-100 candidates per square degree forecast necessarily depends on how precursor-observed deviations from the canonical RC-SFR relation are extrapolated to fainter SFRs and higher redshifts.
axioms (1)
  • domain assumption Radio continuum emission remains a usable star-formation tracer in low-metallicity, high star-formation-density systems despite known deviations from canonical relations.
    This premise underpins the discussion of characterizing RC emission in LCEs and low-metallicity galaxies.

pith-pipeline@v0.9.1-grok · 5874 in / 1504 out tokens · 38566 ms · 2026-06-26T01:14:00.932334+00:00 · methodology

discussion (0)

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Reference graph

Works this paper leans on

279 extracted references · 253 canonical work pages · 84 internal anchors

  1. [2]

    , keywords =

    Physical properties of extreme emission-line galaxies at z 4─9 from the JWST CEERS survey. , keywords =. doi:10.1051/0004-6361/202449904 , archivePrefix =. 2403.05362 , primaryClass =

    work page doi:10.1051/0004-6361/202449904

  2. [5]

    , keywords =

    Spectroscopy from Photometry: A Population of Extreme Emission Line Galaxies at 1.7 z 6.7 Selected with JWST Medium Band Filters. , keywords =. doi:10.3847/2041-8213/ad01c0 , archivePrefix =. 2304.11181 , primaryClass =

    work page doi:10.3847/2041-8213/ad01c0 2041

  3. [6]

    , keywords =

    The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope. , keywords =. doi:10.3847/1538-4357/ac4973 , archivePrefix =. 2110.01829 , primaryClass =

    work page doi:10.3847/1538-4357/ac4973

  4. [7]

    arXiv e-prints , keywords =

    Science with the Ultraviolet Explorer (UVEX). arXiv e-prints , keywords =. doi:10.48550/arXiv.2111.15608 , archivePrefix =. 2111.15608 , primaryClass =

    work page doi:10.48550/arxiv.2111.15608

  5. [8]

    The AstroSat UV Deep Field South. II. A Diverse Set of Lyman-continuum Leakers at z 1. , keywords =. doi:10.3847/1538-4357/adc10e , archivePrefix =. 2410.09515 , primaryClass =

    work page doi:10.3847/1538-4357/adc10e

  6. [9]

    Nature Astronomy , keywords =

    AstroSat detection of Lyman continuum emission from a z = 1.42 galaxy. Nature Astronomy , keywords =. doi:10.1038/s41550-020-1173-5 , archivePrefix =. 2008.11394 , primaryClass =

    work page doi:10.1038/s41550-020-1173-5 2008

  7. [10]

    , keywords =

    Diverse properties of Ly emission in low-redshift compact star-forming galaxies with extremely high [O III]/[O II] ratios. , keywords =. doi:10.1093/mnras/stz3041 , archivePrefix =. 1910.12773 , primaryClass =

    work page doi:10.1093/mnras/stz3041 1910

  8. [11]

    2026 ,publisher =

    Isabella Prandoni and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  9. [12]

    The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy

    The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy. , keywords =. doi:10.3847/1538-4357/aaa76e , archivePrefix =. 1608.01674 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aaa76e

  10. [13]

    , keywords =

    The synthetic Emission Line COSMOS catalogue: H and [O II] galaxy luminosity functions and counts at 0.3 < z < 2.5. , keywords =. doi:10.1093/mnras/staa727 , archivePrefix =. 2003.06394 , primaryClass =

    work page doi:10.1093/mnras/staa727 2003

  11. [17]

    , keywords =

    Emission-line Wings Driven by Lyman Continuum in the Green Pea Analog Mrk 71. , keywords =. doi:10.3847/2041-8213/ac2c09 , archivePrefix =. 2109.14691 , primaryClass =

    work page doi:10.3847/2041-8213/ac2c09 2041

  12. [19]

    Extreme Feedback and the Epoch of Reionization: Clues in the Local Universe

    Extreme Feedback and the Epoch of Reionization: Clues in the Local Universe. , keywords =. doi:10.1088/0004-637X/730/1/5 , archivePrefix =. 1101.4219 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/730/1/5

  13. [20]

    Advancing Astrophysics with the Square Kilometre Array (AASKA14) , year = 2015, month = apr, eid =

    The Cosmic Dawn and Epoch of Reionisation with SKA. Advancing Astrophysics with the Square Kilometre Array (AASKA14) , year = 2015, month = apr, eid =. doi:10.22323/1.215.0001 , archivePrefix =. 1505.07568 , primaryClass =

    work page doi:10.22323/1.215.0001 2015

  14. [21]

    Green Pea Galaxies and cohorts: Luminous Compact Emission-Line Galaxies in the Sloan Digital Sky Survey

    Green Pea Galaxies and Cohorts: Luminous Compact Emission-line Galaxies in the Sloan Digital Sky Survey. , keywords =. doi:10.1088/0004-637X/728/2/161 , archivePrefix =. 1012.5639 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/728/2/161

  15. [23]

    SBS 0335-052E+W: deep VLT/FORS+UVES spectroscopy of the pair of the lowest-metallicity blue compact dwarf galaxies

    SBS 0335-052E+W: deep VLT/FORS+UVES spectroscopy of the pair of the lowest-metallicity blue compact dwarf galaxies. , keywords =. doi:10.1051/0004-6361/200911965 , archivePrefix =. 0907.2116 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/200911965

  16. [24]

    , keywords =

    H I observations and star formation in the blue compact galaxy I ZW 18. , keywords =

  17. [26]

    New candidates for extremely metal-poor emission-line galaxies in the SDSS/BOSS DR10

    New candidates for extremely metal-poor emission-line galaxies in the SDSS/BOSS DR10. , keywords =. doi:10.1051/0004-6361/201525697 , archivePrefix =. 1505.03701 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201525697

  18. [27]

    Study of galaxies in the Lynx-Cancer void. II. Element abundances. Astrophysical Bulletin , keywords =. doi:10.1134/S1990341311030011 , archivePrefix =. 1108.4850 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1134/s1990341311030011

  19. [28]

    Hunting for extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey: MMT and 3.5m APO observations

    Hunting for extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey: MMT and 3.5 m APO observations. , keywords =. doi:10.1051/0004-6361/201219733 , archivePrefix =. 1207.5971 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201219733

  20. [29]

    MMT observations of new extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey

    MMT Observations of New Extremely Metal-poor Emission-Line Galaxies in the Sloan Digital Sky Survey. , keywords =. doi:10.1086/519922 , archivePrefix =. 0704.3842 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/519922

  21. [31]

    The Physics of the Far-infrared-Radio Correlation. I. Calorimetry, Conspiracy, and Implications. , keywords =. doi:10.1088/0004-637X/717/1/1 , archivePrefix =. 0907.4161 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/717/1/1

  22. [32]

    Magnetic Fields in Starburst Galaxies and The Origin of the FIR-Radio Correlation

    Magnetic Fields in Starburst Galaxies and the Origin of the FIR-Radio Correlation. , keywords =. doi:10.1086/504035 , archivePrefix =. astro-ph/0601626 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/504035

  23. [33]

    arXiv e-prints , keywords =

    The Radio Spectral Energy Distribution and Star Formation Calibration in MIGHTEE-COSMOS Highly Star-Forming Galaxies at 1.5 < z < 3.5. arXiv e-prints , keywords =. doi:10.48550/arXiv.2506.16275 , archivePrefix =. 2506.16275 , primaryClass =

    work page doi:10.48550/arxiv.2506.16275

  24. [34]

    Mr-Moose: An advanced SED-fitting tool for heterogeneous multi-wavelength datasets

    MR-MOOSE: an advanced SED-fitting tool for heterogeneous multi-wavelength data sets. , keywords =. doi:10.1093/mnras/sty831 , archivePrefix =. 1804.01748 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/sty831

  25. [35]

    emcee: The MCMC Hammer

    emcee: The MCMC Hammer. , keywords =. doi:10.1086/670067 , archivePrefix =. 1202.3665 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/670067

  26. [36]

    SEDfit: Software for Spectral Energy Distribution Fitting of Photometric Data

    SEDfit: Software for Spectral Energy Distribution Fitting of Photometric Data. , keywords =. doi:10.1086/668636 , archivePrefix =. 1210.0285 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/668636

  27. [37]

    CIGALE: a python Code Investigating GALaxy Emission

    CIGALE: a python Code Investigating GALaxy Emission. , keywords =. doi:10.1051/0004-6361/201834156 , archivePrefix =. 1811.03094 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201834156

  28. [38]

    The Far-Infrared--Radio Correlation at High Redshifts: Physical Considerations and Prospects for the Square Kilometer Array

    The Far-Infrared-Radio Correlation at High Redshifts: Physical Considerations and Prospects for the Square Kilometer Array. , keywords =. doi:10.1088/0004-637X/706/1/482 , archivePrefix =. 0910.0011 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/706/1/482

  29. [39]

    , keywords =

    Blueberry galaxies up to 200 Mpc and their optical and infrared properties. , keywords =. doi:10.1051/0004-6361/202449766 , archivePrefix =. 2405.03391 , primaryClass =

    work page doi:10.1051/0004-6361/202449766

  30. [40]

    Star Formation in Galaxies Along the Hubble Sequence

    Star Formation in Galaxies Along the Hubble Sequence. , keywords =. doi:10.1146/annurev.astro.36.1.189 , archivePrefix =. astro-ph/9807187 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1146/annurev.astro.36.1.189

  31. [42]

    , keywords =

    LBT observations of compact star-forming galaxies with extremely high [O III]/[O II] flux ratios: He I emission-line ratios as diagnostics of Lyman continuum leakage. , keywords =. doi:10.1093/mnras/stx1629 , archivePrefix =. 1706.08769 , primaryClass =

    work page doi:10.1093/mnras/stx1629

  32. [43]

    Essential Radio Astronomy

  33. [44]

    arXiv e-prints , keywords =

    The Low-Redshift Lyman Continuum Survey: The Roles of Stellar Feedback and ISM Geometry in LyC Escape. arXiv e-prints , keywords =. doi:10.48550/arXiv.2409.12118 , archivePrefix =. 2409.12118 , primaryClass =

    work page doi:10.48550/arxiv.2409.12118

  34. [45]

    arXiv e-prints , keywords =

    Low-Frequency Turnover Star Forming Galaxies I: Radio Continuum Observations and Global Properties. arXiv e-prints , keywords =. doi:10.48550/arXiv.2412.03143 , archivePrefix =. 2412.03143 , primaryClass =

    work page doi:10.48550/arxiv.2412.03143

  35. [46]

    , keywords =

    The metal-poor HII galaxy SBS 0335-052 and the primordial helium abundance. , keywords =

  36. [47]

    A., Clayton, G

    The Relationship between Infrared, Optical, and Ultraviolet Extinction. , keywords =. doi:10.1086/167900 , adsurl =

    work page doi:10.1086/167900

  37. [48]

    , keywords =

    The efficiency of ionizing photon production and the radiation energy balance in compact star-forming galaxies. , keywords =. doi:10.1093/mnras/stx347 , archivePrefix =. 1702.02420 , primaryClass =

    work page doi:10.1093/mnras/stx347

  38. [49]

    , keywords =

    Rejuvenating Star Formation Activity in an Early-type Dwarf Galaxy, LEDA 1915372, with Accreted H I Gas. , keywords =. doi:10.3847/2041-8213/acdef1 , archivePrefix =. 2306.14456 , primaryClass =

    work page doi:10.3847/2041-8213/acdef1 2041

  39. [50]

    PyBDSF: Python Blob Detection and Source Finder

  40. [51]

    The LOFAR Two-metre Sky Survey. I. Survey description and preliminary data release. , keywords =. doi:10.1051/0004-6361/201629313 , archivePrefix =. 1611.02700 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201629313

  41. [52]

    The LOFAR Two-metre Sky Survey. V. Second data release. , keywords =. doi:10.1051/0004-6361/202142484 , archivePrefix =. 2202.11733 , primaryClass =

    work page doi:10.1051/0004-6361/202142484

  42. [53]

    Using Lyman-alpha to detect galaxies that leak Lyman continuum

    Using Lyman- to detect galaxies that leak Lyman continuum. , keywords =. doi:10.1051/0004-6361/201423978 , archivePrefix =. 1404.2958 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201423978

  43. [54]

    , keywords =

    The Mass-Metallicity Relation at z ≃ 8: Direct-method Metallicity Constraints and Near-future Prospects. , keywords =. doi:10.3847/1538-4357/abb943 , archivePrefix =. 2006.02447 , primaryClass =

    work page doi:10.3847/1538-4357/abb943 2006

  44. [56]

    , keywords =

    JADES: The production and escape of ionizing photons from faint Lyman-alpha emitters in the epoch of reionization. , keywords =. doi:10.1051/0004-6361/202347132 , archivePrefix =. 2306.04536 , primaryClass =

    work page doi:10.1051/0004-6361/202347132

  45. [57]

    arXiv e-prints , keywords =

    Ionising properties of galaxies in JADES for a stellar mass complete sample: resolving the cosmic ionising photon budget crisis at the Epoch of Reionisation. arXiv e-prints , keywords =. doi:10.48550/arXiv.2409.01286 , archivePrefix =. 2409.01286 , primaryClass =

    work page doi:10.48550/arxiv.2409.01286

  46. [58]

    , keywords =

    The ionizing photon production efficiency at z 6 for Lyman-alpha emitters using JEMS and MUSE. , keywords =. doi:10.1093/mnras/stad1749 , archivePrefix =. 2303.07931 , primaryClass =

    work page doi:10.1093/mnras/stad1749

  47. [59]

    , keywords =

    Evolution of the Mass-Metallicity Relation from Redshift z 8 to the Local Universe. , keywords =. doi:10.3847/1538-4357/acdbc1 , archivePrefix =. 2212.02491 , primaryClass =

    work page doi:10.3847/1538-4357/acdbc1

  48. [60]

    , keywords =

    Metal-poor star formation at z > 6 with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scales. , keywords =. doi:10.1093/mnras/stae682 , archivePrefix =. 2401.08764 , primaryClass =

    work page doi:10.1093/mnras/stae682

  49. [61]

    , keywords =

    CEERS Spectroscopic Confirmation of NIRCam-selected z 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of Their Properties. , keywords =. doi:10.3847/2041-8213/acd2d9 , archivePrefix =. 2301.09482 , primaryClass =

    work page doi:10.3847/2041-8213/acd2d9 2041

  50. [62]

    , keywords =

    A JWST/NIRCam study of key contributors to reionization: the star-forming and ionizing properties of UV-faint z 7-8 galaxies. , keywords =. doi:10.1093/mnras/stad1919 , archivePrefix =. 2208.14999 , primaryClass =

    work page doi:10.1093/mnras/stad1919

  51. [63]

    Science , keywords =

    A magnified compact galaxy at redshift 9.51 with strong nebular emission lines. Science , keywords =. doi:10.1126/science.adf5307 , archivePrefix =. 2210.15699 , primaryClass =

    work page doi:10.1126/science.adf5307

  52. [64]

    , keywords =

    New insight on the nature of cosmic reionizers from the CEERS survey. , keywords =. doi:10.1051/0004-6361/202347884 , archivePrefix =. 2309.02219 , primaryClass =

    work page doi:10.1051/0004-6361/202347884

  53. [65]

    , keywords =

    JWST/NIRSpec spectroscopy of z = 7-9 star-forming galaxies with CEERS: new insight into bright Ly emitters in ionized bubbles. , keywords =. doi:10.1093/mnras/stad2763 , archivePrefix =. 2301.07072 , primaryClass =

    work page doi:10.1093/mnras/stad2763

  54. [66]

    Are Ultra-faint Galaxies at z=6-8 Responsible for Cosmic Reionization ? Combined Constraints from the Hubble Frontier Fields Clusters and Parallels

    Are Ultra-faint Galaxies at z = 6-8 Responsible for Cosmic Reionization? Combined Constraints from the Hubble Frontier Fields Clusters and Parallels. , keywords =. doi:10.1088/0004-637X/814/1/69 , archivePrefix =. 1509.06764 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/814/1/69

  55. [67]

    Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and Hubble Space Telescope

    Cosmic Reionization and Early Star-forming Galaxies: A Joint Analysis of New Constraints from Planck and the Hubble Space Telescope. , keywords =. doi:10.1088/2041-8205/802/2/L19 , archivePrefix =. 1502.02024 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/2041-8205/802/2/l19 2041

  56. [68]

    , keywords =

    Radio-only and Radio-to-far-ultraviolet Spectral Energy Distribution Modeling of 14 ULIRGs: Insights into the Global Properties of Infrared Bright Galaxies. , keywords =. doi:10.3847/1538-4357/ad2c93 , archivePrefix =. 2402.10786 , primaryClass =

    work page doi:10.3847/1538-4357/ad2c93

  57. [69]

    Signatures of the Youngest Starbursts: Optically-thick Thermal Bremsstrahlung Radio Sources in Henize 2-10

    Signatures of the Youngest Starbursts: Optically Thick Thermal Bremsstrahlung Radio Sources in Henize 2-10. , keywords =. doi:10.1086/308075 , archivePrefix =. astro-ph/9907233 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/308075

  58. [70]

    The Spectral Energy Distributions of Infant Super Star Clusters in Henize 2-10 from 7mm to 6cm

    The Spectral Energy Distributions of Infant Super-Star Clusters in Henize 2-10 from 7 Millimeters to 6 Centimeters. , keywords =. doi:10.1086/378585 , archivePrefix =. astro-ph/0308303 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/378585

  59. [71]

    , keywords =

    H I content of selected mid-infrared bright, starburst blue compact dwarf galaxies. , keywords =. doi:10.1093/mnras/stad3018 , archivePrefix =. 2310.02202 , primaryClass =

    work page doi:10.1093/mnras/stad3018

  60. [72]

    arXiv e-prints , keywords =

    FAST H I 21 cm study of blueberry galaxies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2411.13527 , archivePrefix =. 2411.13527 , primaryClass =

    work page doi:10.48550/arxiv.2411.13527

  61. [73]

    A radio continuum survey of Shapley-Ames galaxies at 2.8cm. II. Separation of thermal and non-thermal radio emission. , keywords =

  62. [74]

    Galaxies , keywords =

    The Interstellar Medium of Dwarf Galaxies. Galaxies , keywords =. doi:10.3390/galaxies10010011 , archivePrefix =. 2202.08231 , primaryClass =

    work page doi:10.3390/galaxies10010011

  63. [75]

    arXiv e-prints , keywords =

    The Effect of Radiation and Supernovae Feedback on LyC Escape in Local Star-forming Galaxies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2409.05180 , archivePrefix =. 2409.05180 , primaryClass =

    work page doi:10.48550/arxiv.2409.05180

  64. [76]

    arXiv e-prints , keywords =

    Primordial Rotating Disk Composed of 15 Dense Star-Forming Clumps at Cosmic Dawn. arXiv e-prints , keywords =. doi:10.48550/arXiv.2402.18543 , archivePrefix =. 2402.18543 , primaryClass =

    work page doi:10.48550/arxiv.2402.18543

  65. [77]

    arXiv e-prints , keywords =

    Anatomy of a z=6 Lyman-\ \ emitter down to parsec scales: extreme UV slopes, metal-poor regions and possibly leaking star clusters. arXiv e-prints , keywords =. doi:10.48550/arXiv.2407.20331 , archivePrefix =. 2407.20331 , primaryClass =

    work page doi:10.48550/arxiv.2407.20331

  66. [78]

    D., Vanzella, E., et al

    Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang. , keywords =. doi:10.1038/s41586-024-07703-7 , archivePrefix =. 2401.03224 , primaryClass =

    work page doi:10.1038/s41586-024-07703-7

  67. [79]

    , keywords =

    JWST/NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc. , keywords =. doi:10.3847/1538-4357/acb59a , archivePrefix =. 2211.09839 , primaryClass =

    work page doi:10.3847/1538-4357/acb59a

  68. [80]

    , keywords =

    The Atomic Gas Mass of Green Pea Galaxies. , keywords =. doi:10.3847/2041-8213/abfb76 , archivePrefix =. 2105.12756 , primaryClass =

    work page doi:10.3847/2041-8213/abfb76 2041

  69. [81]

    Stellar Feedback in Molecular Clouds and its Influence on the Mass Function of Young Star Clusters

    Stellar Feedback in Molecular Clouds and its Influence on the Mass Function of Young Star Clusters. , keywords =. doi:10.1088/2041-8205/710/2/L142 , archivePrefix =. 0910.2238 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/2041-8205/710/2/l142 2041

  70. [82]

    , keywords =

    The Morphologies and Physical Properties of Ultracompact H II Regions. , keywords =. doi:10.1086/191329 , adsurl =

    work page doi:10.1086/191329

  71. [83]

    , keywords =

    A population of hypercompact H II regions identified from young H II regions. , keywords =. doi:10.1051/0004-6361/202038608 , archivePrefix =. 2011.07620 , primaryClass =

    work page doi:10.1051/0004-6361/202038608 2011

  72. [84]

    , keywords =

    SCOTCH - search for clandestine optically thick compact H II regions: II. , keywords =. doi:10.1093/mnras/stae1910 , archivePrefix =. 2408.07273 , primaryClass =

    work page doi:10.1093/mnras/stae1910

  73. [85]

    arXiv e-prints , keywords =

    Bursts of star formation and radiation-driven outflows produce efficient LyC leakage from dense compact star clusters. arXiv e-prints , keywords =. doi:10.48550/arXiv.2408.14591 , archivePrefix =. 2408.14591 , primaryClass =

    work page doi:10.48550/arxiv.2408.14591

  74. [86]

    arXiv e-prints , keywords =

    Witnessing an extreme, highly efficient galaxy formation mode with resolved Ly and LyC emission. arXiv e-prints , keywords =. doi:10.48550/arXiv.2407.18804 , archivePrefix =. 2407.18804 , primaryClass =

    work page doi:10.48550/arxiv.2407.18804

  75. [87]

    , keywords =

    Observational signatures of forming young massive clusters: continuum emission from dense H II regions. , keywords =. doi:10.1093/mnras/stad3297 , archivePrefix =. 2305.19432 , primaryClass =

    work page doi:10.1093/mnras/stad3297

  76. [88]

    On the Lack of Correlation Between [OIII]/[OII] and Lyman-Continuum Escape Fraction

    On the lack of correlation between [O III]/[O II] and Lyman continuum escape fraction. , keywords =. doi:10.1093/mnras/sty3320 , archivePrefix =. 1812.04129 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/sty3320

  77. [89]

    , keywords =

    New methods for identifying Lyman continuum leakers and reionization-epoch analogues. , keywords =. doi:10.1093/mnras/staa2355 , archivePrefix =. 2005.01734 , primaryClass =

    work page doi:10.1093/mnras/staa2355 2005

  78. [90]

    The Origin and Optical Depth of Ionizing Radiation in the "Green Pea" Galaxies

    The Origin and Optical Depth of Ionizing Radiation in the ``Green Pea'' Galaxies. , keywords =. doi:10.1088/0004-637X/766/2/91 , archivePrefix =. 1301.0530 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/766/2/91

  79. [91]

    Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range

    Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range. , keywords =. doi:10.1051/0004-6361/201322803 , archivePrefix =. 1312.3442 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201322803

  80. [92]

    The dust content of the most metal-poor star-forming galaxies

    The dust content of the most metal-poor star-forming galaxies. , keywords =. doi:10.1093/mnras/stw114 , archivePrefix =. 1601.01686 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stw114

Showing first 80 references.