REVIEW 2 major objections 5 minor 210 references
First fast radio burst search campaign at the Argentine Institute of Radio Astronomy
T0 review · 2 major / 5 minor · reviewed 2026-08-15 · deepseek-v4-flash
Pith's one-line read The paper claims that a 212-hour campaign with the Argentine Institute of Radio Astronomy's 30-meter dishes detected a credible fast radio burst candidate, FRB 20251018, which would be the first FRB from South America and demonstrates the…
desk verdict A careful first-search report from a new southern single-dish facility whose 'first FRB from South America' rests on a single, unconfirmed S/N=8.2 candidate. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing mechanism is the single-pulse search chain built around the ROACH backend: a 400 MHz band at 1400 MHz digitized at 41–82 μs, dedispersed over a trial-DM grid from 100 to 500 pc cm$^{-3}$, searched for $8\sigma$ single pulses up to about 29 ms width, and filtered by a deep-learning classifier that assigns each candidate a probability of being an astrophysical burst. The chain was validated by recovering seven known FRBs in archival Parkes data and six synthetic bursts injected into IAR observations, including a blind test. The DM uncertainty is derived from the width of the signal-to-noise versus trial-DM response, and a hierarchical channel-zapping test shows the candidate survives masking down to the cleanest 170 MHz of band.
What would settle it
Repoint both IAR antennas at A2870 for a sustained campaign and search for a burst appearing simultaneously in both receivers; also re-run the search on the 18 October 2025 data with the frequency mask varied and on an off-source control dataset. If no second burst ever appears, no dual-antenna coincidence is recorded, and the candidate disappears under slightly different RFI flagging, then the event is best explained as noise or interference rather than an astrophysical FRB.
Extended reading notes
Core claim
The paper's central claim is that the IAR 30 m antennas, equipped with ROACH digital backends, can detect fast radio bursts. The evidence is one candidate, FRB 20251018, observed on 18 October 2025 in the direction of the Phoenix-supercluster galaxy cluster A2870, with DM = $243\pm15\,\mathrm{pc\,cm^{-3}}$, a width of about 6 ms, signal-to-noise ratio 8.20, and a machine-learning classification probability $p=0.99$. The burst's DM exceeds the expected Milky Way contribution of roughly 20–31 pc cm$^{-3}$ by about 170–220 pc cm$^{-3}$, implying an extragalactic origin at redshift $z\lesssim0.2$, consistent with A2870 itself or a background source. The paper also lists five more marginal candidates and notes that no repeat burst from the candidate position has been seen in continued monitoring. The authors state that, to their knowledge, this would be the first FRB detected from South America.
Load-bearing premise
The load-bearing premise is that FRB 20251018 is a genuine astrophysical burst rather than a statistical fluctuation or radio-frequency interference; with a signal-to-noise ratio of 8.2 just above the $8\sigma$ threshold, no independent confirmation from a second antenna or another facility, and no repeat burst, the single event is the most fragile premise on which the 'first FRB from South America' and the capability claim rest.
Editorial extensions
If this is right
- If FRB 20251018 is real, the IAR 30 m dishes can join FRB science, adding a flexible southern-hemisphere single-dish station.
- Continued monitoring of A2870 and A4013 can test whether the candidate repeats, which would confirm an astrophysical origin and enable repeat-burst studies.
- Dual-antenna (A1+A2) coincident observations will provide a decisive test against local interference for near-threshold candidates.
- The implied all-sky rate, about $2\times10^{4}$ sky$^{-1}$ day$^{-1}$ above the survey sensitivity, is consistent with published rates and suggests additional detections with longer campaigns.
- Cross-matching IAR candidates with gravitational-wave events and other transients can constrain FRB progenitor channels in the southern sky.
Reading between the lines
- If the candidate is ultimately confirmed by a second receiver or a repeat burst, its large host-frame DM excess would suggest that some FRBs arise in dense cluster environments, a property targeted cluster surveys could quantify.
- The capability claim currently rests on a single near-threshold event; the paper's own statement that no repeat or coincident detection exists means the 'first South American FRB' status remains provisional rather than established.
- The demonstrated recovery of injected bursts with signal-to-noise ratios as low as 10 implies the IAR system could serve as a template for low-cost single-dish FRB searches at other southern observatories.
- A natural extension the paper does not carry out is a systematic cross-match of IAR candidates with published FRB catalogs to look for repeaters or multi-telescope coincident events.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper reports the first blind fast radio burst (FRB) search campaign at the Argentine Institute of Radio Astronomy (IAR), using the A2 30 m antenna with a ROACH backend over 212 hours of observations toward the Ophiuchus, Shapley, Sculptor, and Phoenix supercluster fields. The search uses PRESTO for dedispersion and single-pulse detection in the DM range 100–500 pc cm−3, followed by FETCH classification and visual inspection. The pipeline is validated on seven Parkes archival FRBs and six synthetic injections, including a blind test. The campaign yields one candidate, FRB 20251018 (S/N=8.2, DM=243 pc cm−3, FETCH p=0.99), in the direction of A2870, which the authors argue would be the first FRB detected from South America. Five marginal candidates are also listed. The paper concludes that the IAR antennas are capable of detecting FRBs and derives an all-sky rate estimate consistent with literature values.
Significance. The paper's principal strength is its validation strategy: recovering all seven Parkes archival FRBs and all six injected bursts, including a blind injection analyzed by three independent team members, is a meaningful demonstration that the PRESTO+FETCH pipeline can find dispersed transients in IAR data. The authors are also refreshingly transparent about the marginality of their candidate, the absence of a repeat burst, and the need for future dual-antenna confirmation. If FRB 20251018 is genuine, the result would show that a 30 m single dish with a modest 400 MHz backend can contribute to FRB science and would open a new southern-hemisphere monitoring capability. However, the central claim of a 'first FRB from South America' and the implied capability demonstration rest on a single candidate whose signal-to-noise ratio is only 0.2 above the search threshold and for which no false-positive rate is measured. The significance of the paper is therefore conditional on the reality of FRB 20251018; the validation tests alone establish pipeline sensitivity, but not the astrophysical nature of the one reported event.
major comments (2)
- [§5 and Table A.1] The capability claim and the 'first FRB from South America' headline rest on FRB 20251018 (S/N=8.2, DM=243 pc cm−3, FETCH p=0.99; Section 5), but the paper does not provide a measured false-positive rate for the full PRESTO+FETCH+visual-inspection pipeline on real IAR noise/RFI data. This issue is load-bearing because Table A.1 lists five other candidates with S/N 8.40–12.47 and FETCH p up to 0.997 that are rejected as marginal on the basis of diagnostic plots; hence high S/N and high FETCH p do not by themselves establish astrophysical origin in this dataset. Since FRB 20251018 sits only 0.2σ above the search threshold and has no second-antenna coincidence, repeat burst, or external confirmation, the paper should quantify how often the pipeline produces a candidate at least as convincing as this one from noise/RFI alone (for example, by running the identical pipeline on time-reversed or scrambled noise-only observations from the same fields). Without such a number, the single detection is not statistically distinguished from the false-positive tail that produced the Table A.1 candidates.
- [§5, Appendix A, and ATel Prajapati et al. (2026)] The astrophysical nature of FRB 20251018 is currently supported only by visual inspection and by a hierarchical channel-zapping test described solely in an Astronomer's Telegram (Prajapati et al. 2026), not in this manuscript. The paper itself states that no repeat burst has been identified and that dual-antenna observations are needed as a 'decisive discriminator' against local interference. I ask the authors either to include the full channel-zapping results and diagnostic plots for FRB 20251018 in the paper, or to explicitly relabel the event as a candidate and to rest the capability demonstration on the injection/archival validation in Appendix B, which is strong and independent of this event. As written, the conclusion that 'the IAR antennas are capable of detecting FRBs' conflates pipeline recovery of injected signals with the detection of a real astrophysical burst.
minor comments (5)
- [Table A.1] The column header 'Datet start' appears to be a typo; it should read 'Date of t_start' or a similarly clear label indicating that the date belongs to the start of the observation.
- [§5] The flux-density estimate quotes 3.0±0.5 Jy and a fluence of 27±5 Jy ms using W_eq≈9 ms, whereas the ATel reports 3.9±0.9 Jy using the FWHM of the profile; the paper should state explicitly which width definition is used in each place and clarify that the difference reflects that choice rather than an inconsistency.
- [Appendix B] The sentence about the Parkes validation is ambiguous: after saying the archival set comprises seven FRBs, the text says 'In particular, we focused on the detection of FRB 110703, and we also injected a synthetic signal with FRB-faker that was successfully recovered' — it is unclear whether the injection was into the Parkes data or into a separate observation; please clarify.
- [§4] The rough rate estimate that 'a detection is likely after ~1000 h' is presented without an explicit derivation of the beam solid-angle factor; giving the assumed all-sky rate and showing ΔΩ = πθ_FWHM^2/4 with the adopted 30′ beam would make the estimate more reproducible.
- [Data availability] The statement that data are available 'upon reasonable request' is weaker than current FAIR expectations for a survey paper; making candidate cutouts, the static RFI mask, and pipeline configuration files publicly available would strengthen reproducibility.
Circularity Check
No circularity found: the pipeline validation is external, the system parameters are prior independent measurements, and the single-candidate claim rests on unconfirmed data rather than on a self-referential derivation.
full rationale
Walked the derivation chain. Instrument characterization is imported from Gancio et al. (2020) and Araujo Furlan et al. (2026), which are prior published measurements of the same IAR front ends; these are externally falsifiable system parameters (T_sys = 50 +/- 8 K, G ~ 0.077 K/Jy) and are not fitted to the candidate. The detection pipeline is validated twice: on Parkes archival filterbanks containing seven known FRBs (Keane & Petroff 2015 data, not from IAR) and on FRB-faker synthetic bursts injected into IAR data, including a blind test analyzed by three team members. These tests establish that PRESTO+FETCH can recover dispersed transients with correct time and DM; they do not assume the target candidate. The candidate FRB 20251018 is found at S/N 8.2, DM 243, p = 0.99; its flux and fluence use the radiometer equation with previously published system parameters and the measured profile, so no fitted parameter is renamed as a prediction. The all-sky rate ~2e4 sky^-1 day^-1 is the Poisson inverse of one event over 212 h and a 30' beam, compared with external Petroff et al. (2019) rates; it is not derived from those rates. Self-citations to Prajapati et al. (2026) are the group's own ATel reporting the same candidate, not an independent authority invoked to prove the claim. The main weakness - an unconfirmed single candidate and no measured false-positive rate - is a statistical and robustness concern, not a circularity. No step reduces to its own input.
Assumptions & free parameters
assumptions (3)
- domain assumption The dispersed pulse search assumes DM range 100-500 pc cm^-3 captures extragalactic FRBs while excluding Galactic sources.
- domain assumption The Macquart relation is used to convert extragalactic DM excess to a redshift upper limit.
- domain assumption FETCH model A correctly distinguishes FRBs from RFI in the IAR data.
Cite this review
Pith. "Pith review of First fast radio burst search campaign at the Argentine Institute of Radio Astronomy." pith.science (2026). https://pith.science/paper/5OJ6DCOG
@misc{pith2026260803914,
author = {Pith},
title = {Pith review of: First fast radio burst search campaign at the Argentine Institute of Radio Astronomy},
year = {2026},
howpublished = {\url{https://pith.science/paper/5OJ6DCOG}},
note = {Machine review of arXiv:2608.03914}
}
abstract
Fast radio bursts (FRBs) are intense millisecond-duration radio transients of extragalactic origin whose physical nature remains under active investigation, and which also serve as probes of the intergalactic medium. We report on the first FRB search campaign carried out at the Argentine Institute of Radio Astronomy (IAR) between December 2024 and March 2026, targeting nearby galaxy superclusters in the southern sky. We observed fields in the Ophiuchus, Shapley, and Sculptor/Phoenix supercluster regions with one of the two 30~m antennas of the IAR, using a ROACH-based backend with 400~MHz of bandwidth centred at 1400~MHz and a time resolution of 41--82~$\mu$s, for a total net observing time of 212~h. The data were searched for dispersed single pulses with \texttt{PRESTO} in the dispersion measure range $100 \leq \mathrm{DM} \leq 500$, and candidates were classified with the FETCH machine learning classifier. The pipeline was validated on archival Parkes data containing known FRBs and on synthetic bursts injected into IAR observations. One FRB candidate, FRB~20251018, was identified on 18 October 2025 in an observation pointed towards the galaxy cluster A2870, in the Phoenix supercluster, with a dispersion measure of $243$, a signal-to-noise ratio of 8.2, and a FETCH probability of $p=0.99$. To the best of our knowledge, this would be the first FRB detected from South America. A set of more marginal candidates is also presented. These results demonstrate the capability of the IAR antennas to detect FRBs and support the continuation and extension of the monitoring campaign, including coincident dual-antenna observations and cross-matches with gravitational-wave events and electromagnetic transients.
Figures
Reference graph
Works this paper leans on
-
[1]
Hickish, J and Dennett, F and Foster, G and Kruizinga, O and Price, D. C. and van Straten, W and Werthimer, D and others , journal=. A decade of developing radio-astronomy instrumentation using. 2016 , publisher=
2016
-
[2]
Study of the 2024 major Vela glitch at the Argentine Institute of Radioastronomy. , keywords =. doi:10.1051/0004-6361/202554098 , archivePrefix =. 2502.06704 , primaryClass =
arXiv 2024
-
[3]
Giant radio pulses in the magnetar XTE J1810 - 197 detected with the IAR's telescopes. , keywords =. doi:10.1051/0004-6361/202556571 , archivePrefix =. 2603.00295 , primaryClass =
-
[5]
Glitch-induced pulse profile change of PSR J0742 - 2822 observed from the IAR. , keywords =. doi:10.1051/0004-6361/202452693 , archivePrefix =. 2412.17766 , primaryClass =
-
[6]
Timing irregularities and glitches from the pulsar monitoring campaign at IAR. , keywords =. doi:10.1051/0004-6361/202450441 , archivePrefix =. 2406.17099 , primaryClass =
-
[7]
The Astronomer's Telegram , keywords =
Detection of FRB 20251018 by the PuMA Collaboration at the Argentine Institute of Radio Astronomy. The Astronomer's Telegram , keywords =
-
[8]
Keane, E. F. and Petroff, E. Fast radio bursts: search sensitivities and completeness. 2015. doi:10.1093/mnras/stu2650. arXiv:1409.6125
arXiv 2015
-
[9]
Blinkverse: A Database of Fast Radio Bursts , url =
Xu, Jiaying and Feng, Yi and Li, Di and Wang, Pei and Zhang, Yongkun and Xie, Jintao and Chen, Huaxi and Wang, Han and Kang, Zhixuan and Hu, Jingjing and Zheng, Yun and Tsai, Chao-Wei and Chen, Xianglei and Zhou, Dengke , doi =. Blinkverse: A Database of Fast Radio Bursts , url =. Universe , number =. 2023 , bdsk-url-1 =
2023
Show all 210 references
-
[10]
and others
Abbott, R. and others. Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO Virgo Observing Run O3a. 2023. doi:10.3847/1538-4357/acd770. arXiv:2203.12038
2023 arXiv
-
[11]
and Hessels, J
Michilli, D. and Hessels, J. W. T. and Lyon, R. J. and Tan, C. M. and Bassa, C. and Cooper, S. and Kondratiev, V. I. and Sanidas, S. and Stappers, B. W. and van Leeuwen, J. Single-pulse classifier for the LOFAR Tied-Array All-sky Survey. 2018. doi:10.1093/mnras/sty2072. arXiv:...
2018 arXiv
-
[12]
Science , volume=
A bright millisecond radio burst of extragalactic origin , author=. Science , volume=. 2007 , publisher=
2007
-
[13]
2019 , publisher=
A second source of repeating fast radio bursts , journal=. 2019 , publisher=
2019
-
[14]
Nature Astronomy , volume=
The prevalence of repeating fast radio bursts , author=. Nature Astronomy , volume=. 2019 , publisher=
2019
-
[15]
, volume=
An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102 , author=. , volume=. 2018 , publisher=
2018
-
[16]
2020 , publisher=
Periodic activity from a fast radio burst source , journal=. 2020 , publisher=
2020
-
[17]
, volume=
Fast radio burst source properties and curvature radiation model , author=. , volume=. 2017 , publisher=
2017
-
[18]
, volume=
Fast radio bursts as synchrotron maser emission from decelerating relativistic blast waves , author=. , volume=. 2019 , publisher=
2019
-
[19]
, volume=
A model for fast extragalactic radio bursts , author=. , volume=. 2014 , publisher=
2014
-
[20]
, volume=
A fast radio burst associated with a Galactic magnetar , author=. , volume=. 2020 , publisher=
2020
-
[21]
Astronomy & Astrophysics , volume=
Fast radio bursts: the last sign of supramassive neutron stars , author=. Astronomy & Astrophysics , volume=. 2014 , publisher=
2014
-
[22]
, volume=
The physical mechanisms of fast radio bursts , author=. , volume=. 2020 , publisher=
2020
-
[23]
, volume=
A census of baryons in the Universe from localized fast radio bursts , author=. , volume=. 2020 , publisher=
2020
-
[24]
, volume=
The host galaxies and progenitors of fast radio bursts localized with the Australian Square Kilometre Array Pathfinder , author=. , volume=. 2020 , publisher=
2020
-
[25]
Nature Astronomy , volume=
Detection of ultra-fast radio bursts from FRB 20121102A , author=. Nature Astronomy , volume=. 2023 , publisher=
2023
-
[26]
Science , volume=
A population of fast radio bursts at cosmological distances , author=. Science , volume=. 2013 , publisher=
2013
-
[27]
, volume=
A repeating fast radio burst , author=. , volume=. 2016 , publisher=
2016
-
[28]
Modern Physics Letters A , volume=
Fast radio bursts—A brief review: Some questions, fewer answers , author=. Modern Physics Letters A , volume=. 2016 , publisher=
2016
-
[29]
Publications of the Astronomical Society of Japan , volume=
Cosmological fast radio bursts from binary neutron star mergers , author=. Publications of the Astronomical Society of Japan , volume=. 2013 , publisher=
2013
-
[30]
, volume=
Locating the “missing” baryons with extragalactic dispersion measure estimates , author=. , volume=. 2013 , publisher=
2013
-
[31]
, volume=
Identifying the source of perytons at the Parkes radio telescope , author=. , volume=. 2015 , publisher=
2015
-
[32]
, volume=
The first CHIME/FRB fast radio burst catalog , author=. , volume=. 2021 , publisher=
2021
-
[33]
Burst morphology , author=
FAST observations of an extremely active episode of FRB 20201124A: I. Burst morphology , author=. Research in Astronomy and Astrophysics , volume=. 2022 , publisher=
2022
-
[34]
, volume=
Five new fast radio bursts from the HTRU high-latitude survey at Parkes: first evidence for two-component bursts , author=. , volume=. 2016 , publisher=
2016
-
[35]
, volume=
Fast radio burst morphology in the first CHIME/FRB catalog , author=. , volume=. 2021 , publisher=
2021
-
[36]
, volume=
FRB 121102 bursts show complex time--frequency structure , author=. , volume=. 2019 , publisher=
2019
-
[37]
, volume=
A fast radio burst source at a complex magnetized site in a barred galaxy , author=. , volume=. 2022 , publisher=
2022
-
[38]
, volume=
Diverse polarization angle swings from a repeating fast radio burst source , author=. , volume=. 2020 , publisher=
2020
-
[39]
, volume=
High time resolution and polarization properties of ASKAP-localized fast radio bursts , author=. , volume=. 2020 , publisher=
2020
-
[40]
, volume=
LOFAR detection of 110--188 MHz emission and frequency-dependent activity from FRB 20180916B , author=. , volume=. 2021 , publisher=
2021
-
[41]
, volume=
Highest frequency detection of FRB 121102 at 4--8 GHz using the breakthrough listen digital backend at the green bank telescope , author=. , volume=. 2018 , publisher=
2018
-
[42]
, volume=
FRB microstructure revealed by the real-time detection of FRB170827 , author=. , volume=. 2018 , publisher=
2018
-
[43]
, volume=
The detection of an extremely bright fast radio burst in a phased array feed survey , author=. , volume=. 2017 , publisher=
2017
-
[44]
, volume=
CRAFTS for fast radio bursts: extending the dispersion--fluence relation with new FRBs detected by FAST , author=. , volume=. 2021 , publisher=
2021
-
[45]
New FRB discoveries and their follow-up , author=
The SUrvey for Pulsars and Extragalactic Radio Bursts--II. New FRB discoveries and their follow-up , author=. , volume=. 2018 , publisher=
2018
-
[46]
, volume=
A direct localization of a fast radio burst and its host , author=. , volume=. 2017 , publisher=
2017
-
[47]
, volume=
INTEGRAL discovery of a burst with associated radio emission from the magnetar SGR 1935+ 2154 , author=. , volume=. 2020 , publisher=
1935
-
[48]
, volume=
Electromagnetic fireworks: fast radio bursts from rapid reconnection in the compressed magnetar wind , author=. , volume=. 2022 , publisher=
2022
-
[49]
FRB coherent emission from decay of Alfv
Kumar, Pawan and Bo. FRB coherent emission from decay of Alfv. , volume=. 2020 , publisher=
2020
-
[50]
, volume=
Fast radio bursts as precursor radio emission from monster shocks , author=. , volume=. 2025 , publisher=
2025
-
[51]
, volume=
Fast radio bursts from reconnection in a magnetar magnetosphere , author=. , volume=. 2020 , publisher=
2020
-
[52]
, volume=
Fast radio bursts as probes of magnetic fields in the intergalactic medium , author=. , volume=. 2016 , publisher=
2016
-
[53]
, volume=
A unified picture of Galactic and cosmological fast radio bursts , author=. , volume=. 2020 , publisher=
2020
-
[54]
, volume=
Future cosmological constraints from fast radio bursts , author=. , volume=. 2018 , publisher=
2018
-
[55]
Nature Communications , volume=
Strongly lensed repeating fast radio bursts as precision probes of the universe , author=. Nature Communications , volume=. 2018 , publisher=
2018
-
[56]
, volume=
Exploring the epoch of hydrogen reionization using FRBs , author=. , volume=. 2021 , publisher=
2021
-
[57]
, volume=
Probing cosmology and gastrophysics with fast radio bursts: cross-correlations of dark matter haloes and cosmic dispersion measures , author=. , volume=. 2022 , publisher=
2022
-
[58]
, volume=
CHIME/FRB catalog 1 results: statistical cross-correlations with large-scale structure , author=. , volume=. 2021 , publisher=
2021
-
[59]
, volume=
Use of fast radio burst dispersion measures as distance measures , author=. , volume=. 2019 , publisher=
2019
-
[60]
Reviews of Modern Physics , volume=
The physics of fast radio bursts , author=. Reviews of Modern Physics , volume=. 2023 , publisher=
2023
-
[61]
Annual Review of Nuclear and Particle Science , volume=
Multiwavelength and Multimessenger Counterparts of Fast Radio Bursts , author=. Annual Review of Nuclear and Particle Science , volume=. 2024 , publisher=
2024
-
[62]
and Fiore, William and Thomas, Reshma Anna and Ransom, Scott M
Aggarwal, Kshitij and Agarwal, Devansh and Kania, Joseph W. and Fiore, William and Thomas, Reshma Anna and Ransom, Scott M. and Demorest, Paul B. and Wharton, Robert S. and Burke-Spolaor, Sarah and Lorimer, Duncan R. and McLaughlin, Maura A. and Garver-Daniels, Nathaniel , tit...
2020
-
[63]
Your: Your Unified Reader
Aggarwal, Kshitij and others. Your: Your Unified Reader. J. Open Source Softw. 2020. doi:10.21105/joss.02750. arXiv:2011.07627
2020 arXiv
-
[64]
Cordes, J. M. and Lazio, T. J. W. , title =. arXiv e-prints , eprint =
-
[65]
Yao, J. M. and Manchester, R. N. and Wang, N. , title =. , volume =. 2017 , doi =
2017
-
[66]
and Totani, T
Yamasaki, S. and Totani, T. , title =. , volume =. 2020 , doi =
2020
-
[67]
, volume =
Faint galaxy population in clusters: X-ray emission, cD halos, and projection effects , author =. , volume =
-
[68]
, year = 2016, month = aug, volume =
Deep Chandra study of the truncated cool core of the Ophiuchus cluster. , year = 2016, month = aug, volume =
2016
-
[69]
, year = 2020, month = mar, volume =
Discovery of a Giant Radio Fossil in the Ophiuchus Galaxy Cluster. , year = 2020, month = mar, volume =
2020
-
[70]
, year = 1989, month = apr, volume =
A marked concentration of galaxy clusters: is this the origin of Great Attractor motion?. , year = 1989, month = apr, volume =
1989
-
[71]
, year = 1989, month = nov, volume =
The distribution of galaxies in the direction of the 'Great Attractor'. , year = 1989, month = nov, volume =
1989
-
[72]
, year = 1989, month = may, volume =
A catalog of rich clusters of galaxies. , year = 1989, month = may, volume =
1989
-
[73]
, year = 1999, month = nov, volume =
A Compilation of Redshifts and Velocity Dispersions for ACO Clusters. , year = 1999, month = nov, volume =
1999
-
[74]
Testori, J. C. and Reich, P. and Bava, J. A. and Colomb, F. R. and Hurrel, E. E. and Larrarte, J. J. and Reich, W. and Sanz, A. J. A radio continuum survey of the southern sky at 1420 mhz. observations and data reduction. Astron. Astrophys. 2001. doi:10.1051/0004-6361:20010088...
2001 arXiv
-
[75]
Kalberla, Peter M. W. and Burton, W. B. and Hartmann, Dap and Arnal, E. M. and Bajaja, E. and Morras, R. and Poppel, W. G. L. The Leiden/Argentine/Bonn (LAB) survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections...
2005 arXiv
-
[76]
and Arnal, E
Bajaja, E. and Arnal, E. M. and Larrarte, J. J. and Morras, R. and Poppel, W. G. L. and Kalberla, Peter M. W. A High sensitivity HI survey of the sky at delta < = -25 deg. Final data release. Astron. Astrophys. 2005. doi:10.1051/0004-6361:20041863. arXiv:astro-ph/0504136
2005 arXiv
-
[77]
, keywords =
First results of the glitching pulsars monitoring program at the Argentine Institute of Radioastronomy. , keywords =. doi:10.1093/mnras/stad723 , archivePrefix =. 2210.03770 , primaryClass =
-
[78]
, keywords =
Vela pulsar: single pulses analysis with machine learning techniques. , keywords =. doi:10.1093/mnras/stab3287 , archivePrefix =. 2108.13462 , primaryClass =
-
[79]
Boletin de la Asociacion Argentina de Astronomia La Plata Argentina , keywords =
Estudio de alta precisi \'o n del p \'u lsar J0437-4715 desdeel Instituto Argentino de Radioastronom \' a. Boletin de la Asociacion Argentina de Astronomia La Plata Argentina , keywords =
-
[80]
, keywords =
Upgraded antennas for pulsar observations in the Argentine Institute of Radio astronomy. , keywords =. doi:10.1051/0004-6361/201936525 , archivePrefix =. 1908.07049 , primaryClass =
1908 arXiv
-
[81]
Hasasia: A Python package for Pulsar Timing Array Sensitivity Curves , url =
Hazboun, Jeffrey and Romano, Joseph and Smith, Tristan , pages =. Hasasia: A Python package for Pulsar Timing Array Sensitivity Curves , url =. Journal of Open Source Software , doi =. 2019 , month =
2019
-
[82]
, archivePrefix = "arXiv", eprint =
Modeling the Black Hole Merger of QSO 3C 186. , archivePrefix = "arXiv", eprint =. doi:10.3847/2041-8213/aa733c , adsurl =
-
[83]
Neutron Star Population Dynamics. I. Millisecond Pulsars. , keywords =. doi:10.1086/304179 , archivePrefix =. astro-ph/9706162 , primaryClass =
-
[84]
Interstellar Seeing. II. The Case of the Vela Pulsar: Source Unresolved. arXiv e-prints , keywords =
-
[85]
Handbook of Pulsar Astronomy
-
[86]
2014 , eprint=
Auto-Encoding Variational Bayes , author=. 2014 , eprint=
2014
-
[87]
, keywords =
Intensity dependence of the pulse profile and polarization of the VELA pulsar. , keywords =. doi:10.1086/160682 , adsurl =
-
[88]
and Klekociuk, Andrew and Hamilton, P
Mcculloch, P. and Klekociuk, Andrew and Hamilton, P. and Royle, Greg , year =. Daily Observations of Three Period Jumps of the Vela Pulsar , volume =. Australian Journal of Physics , doi =
-
[89]
The Astronomer's Telegram , keywords =
Radio observations following the recent glitch of Vela Pulsar (PSR B0833-45). The Astronomer's Telegram , keywords =. 2019
2019
-
[90]
The Astronomer's Telegram , keywords =
Detection of a new glitch in the pulsar PSR J1740-3015. The Astronomer's Telegram , keywords =
-
[91]
The Astronomer's Telegram , keywords =
Confirmation of glitch event observed in PSR J0742-2822 at the Argentine Institute of Radioastronomy (IAR). The Astronomer's Telegram , keywords =
-
[92]
The Astronomer's Telegram , keywords =
A very large glitch in the radio pulsar PSR B0740-28. The Astronomer's Telegram , keywords =
-
[93]
Improving pulsar timing precision with single pulses
Kerr, Matthew. Improving pulsar timing precision with single pulses. 2015. doi:10.1093/mnras/stv1296. arXiv:1506.03527
2015 arXiv
-
[94]
, keywords =
Fast radio bursts. , keywords =. doi:10.1007/s00159-019-0116-6 , archivePrefix =. 1904.07947 , primaryClass =
1904 arXiv
-
[95]
Fast Radio Burst 121102 Pulse Detection and Periodicity: A Machine Learning Approach
Zhang, Yunfan Gerry and Gajjar, Vishal and Foster, Griffin and Siemion, Andrew and Cordes, James and Law, Casey and Wang, Yu. Fast Radio Burst 121102 Pulse Detection and Periodicity: A Machine Learning Approach. 2018. doi:10.3847/1538-4357/aadf31. arXiv:1809.03043
2018 arXiv
-
[96]
Applying Deep Learning to Fast Radio Burst Classification
Connor, Liam and van Leeuwen, Joeri. Applying Deep Learning to Fast Radio Burst Classification. 2018. doi:10.3847/1538-3881/aae649. arXiv:1803.03084
2018 arXiv
-
[97]
and Tang, Benyang and Thompson, David R
Wagstaff, Kiri L. and Tang, Benyang and Thompson, David R. and Khudikyan, Shakeh and Wyngaard, Jane and Deller, Adam T. and Palaniswamy, Divya and Tingay, Steven J. and Wayth, Randall B. A Machine Learning Classifier for Fast Radio Burst Detection at the VLBA. 2016. doi:10.108...
2016 arXiv
-
[98]
and On, Alvina Y
Chen, Bo Han and Hashimoto, Tetsuya and Goto, Tomotsugu and Kim, Seong Jin and Santos, Daryl Joe D. and On, Alvina Y. L. and Lu, Ting-Yi and Hsiao, Tiger Y. -Y. Uncloaking hidden repeating fast radio bursts with unsupervised machine learning. 2021. doi:10.1093/mnras/stab2994. ...
2021 arXiv
-
[99]
Machine learning classification of CHIME fast radio bursts II
Zhu-Ge, Jia-Ming and Luo, Jia-Wei and Zhang, Bing. Machine learning classification of CHIME fast radio bursts II. Unsupervised methods. 2022. doi:10.1093/mnras/stac3599. arXiv:2210.02471
2022 arXiv
-
[100]
Machine learning classification of CHIME fast radio bursts I
Luo, Jia-Wei and Zhu-Ge, Jia-Ming and Zhang, Bing. Machine learning classification of CHIME fast radio bursts I. Supervised methods. 2022. doi:10.1093/mnras/stac3206. arXiv:2210.02463
2022 arXiv
-
[101]
, keywords =
FETCH: A deep-learning based classifier for fast transient classification. , keywords =. doi:10.1093/mnras/staa1856 , archivePrefix =. 1902.06343 , primaryClass =
1902 arXiv
-
[102]
and Weltman, A
Platts, E. and Weltman, A. and Walters, A. and Tendulkar, S. P. and Gordin, J. E. B. and Kandhai, S. A Living Theory Catalogue for Fast Radio Bursts. 2019. doi:10.1016/j.physrep.2019.06.003. arXiv:1810.05836
2019 arXiv
-
[103]
ENTERPRISE: Enhanced Numerical Toolbox Enabling a Robust PulsaR Inference SuitE
-
[104]
Borges , title =
Jorge L. Borges , title =
-
[105]
Laser Interferometer Space Antenna
Amaro-Seoane, Pau and others. Laser Interferometer Space Antenna. 2017. arXiv:1702.00786
2017 arXiv
-
[106]
and others
Parthasarathy, A. and others. Measurements of pulse jitter and single-pulse variability in millisecond pulsars using MeerKAT. 2021. doi:10.1093/mnras/stab037. arXiv:2101.08531
2021 arXiv
-
[107]
Lam, M. T. and Hazboun, J. S. Precision Timing of PSR J0437 4715 with the IAR Observatory and Implications for Low-frequency Gravitational Wave Source Sensitivity. 2021. doi:10.3847/1538-4357/abeb64. arXiv:2007.00260
2021 arXiv
-
[108]
JPL pulsar timing observations. III. Pulsar rotation fluctuations. , keywords =. doi:10.1086/191076 , adsurl =
-
[109]
, keywords =
Timing, polarimetry and physics of the bright, nearby millisecond pulsar PSR J0437-4715 - a single-pulse perspective. , keywords =. 2014. doi:10.1093/mnras/stu804 , archivePrefix =. 1405.2638 , primaryClass =
2014 arXiv
-
[110]
, keywords =
Three Millisecond Pulsars in Fermi LAT Unassociated Bright Sources. , keywords =. 2011. doi:10.1088/2041-8205/727/1/L16 , archivePrefix =. 1012.2862 , primaryClass =
2011 arXiv
-
[111]
, archivePrefix = "arXiv", eprint =
Limitations in timing precision due to single-pulse shape variability in millisecond pulsars. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stu1213 , adsurl =
-
[112]
, archivePrefix = "arXiv", eprint =
The NANOGrav Nine-year Data Set: Noise Budget for Pulsar Arrival Times on Intraday Timescales. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/819/2/155 , adsurl =
-
[113]
, archivePrefix = "arXiv", eprint =
Optimizing Pulsar Timing Array Observational Cadences for Sensitivity to Low-frequency Gravitational-wave Sources. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/aae533 , adsurl =
-
[114]
Observations and data reduction
A radio continuum survey of the southern sky at 1420 MHz. Observations and data reduction. , eprint =. doi:10.1051/0004-6361:20010088 , adsurl =
-
[115]
, eprint =
PSRCHIVE and PSRFITS: An Open Approach to Radio Pulsar Data Storage and Analysis. , eprint =. doi:10.1071/AS04022 , adsurl =
-
[116]
Science , archivePrefix = "arXiv", eprint =
A single fast radio burst localized to a massive galaxy at cosmological distance. Science , archivePrefix = "arXiv", eprint =. doi:10.1126/science.aaw5903 , adsurl =
-
[117]
An overview
TEMPO2, a new pulsar-timing package - I. An overview. , eprint =. doi:10.1111/j.1365-2966.2006.10302.x , adsurl =
2006
-
[118]
, keywords =
Five Years of Pulsar Flux Density Monitoring: Refractive Scintillation and the Interstellar Medium. , keywords =. doi:10.1086/309201 , adsurl =
-
[119]
Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI. Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections. , eprint =. doi:10.1051/0004-6361:20041864 , adsurl =
-
[120]
Final data release
A high sensitivity HI survey of the sky at -25 . Final data release. , eprint =. doi:10.1051/0004-6361:20041863 , adsurl =
-
[121]
Journal of Astronomical Instrumentation , archivePrefix = "arXiv", eprint =
A Decade of Developing Radio-Astronomy Instrumentation using CASPER Open-Source Technology. Journal of Astronomical Instrumentation , archivePrefix = "arXiv", eprint =. doi:10.1142/S2251171716410014 , adsurl =
-
[122]
Science , archivePrefix = "arXiv", eprint =
A Bright Millisecond Radio Burst of Extragalactic Origin. Science , archivePrefix = "arXiv", eprint =. doi:10.1126/science.1147532 , adsurl =
-
[123]
, archivePrefix = "arXiv", eprint =
The Repeating Fast Radio Burst FRB 121102: Multi-wavelength Observations and Additional Bursts. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/833/2/177 , adsurl =
-
[124]
, archivePrefix = "arXiv", eprint =
A second source of repeating fast radio bursts. , archivePrefix = "arXiv", eprint =. doi:10.1038/s41586-018-0864-x , adsurl =
-
[125]
, archivePrefix = "arXiv", eprint =
A Radio Source Coincident with the Superluminous Supernova PTF10hgi: Evidence for a Central Engine and an Analog of the Repeating FRB 121102?. , archivePrefix = "arXiv", eprint =. doi:10.3847/2041-8213/ab18a5 , adsurl =
-
[126]
, archivePrefix = "arXiv", eprint =
Second Repeating FRB 180814.J0422+73: Ten-year Fermi-LAT Upper Limits and Implications. , archivePrefix = "arXiv", eprint =. doi:10.3847/2041-8213/ab13af , adsurl =
-
[127]
, archivePrefix = "arXiv", eprint =
A new fast radio burst in the data sets containing the Lorimer burst. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnrasl/slz023 , adsurl =
-
[128]
, archivePrefix = "arXiv", eprint =
A southern sky search for repeating fast radio bursts using the Australian SKA Pathfinder. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stz804 , adsurl =
-
[129]
, archivePrefix = "arXiv", eprint =
Optimizing Pulsar Timing Arrays to Maximize Gravitational Wave Single-source Detection: A First Cut. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/730/1/17 , adsurl =
-
[130]
Reports on Progress in Physics , year = 2015, month = dec, volume = 78, number = 12, eid =
Pulsar timing arrays: the promise of gravitational wave detection. Reports on Progress in Physics , year = 2015, month = dec, volume = 78, number = 12, eid =. doi:10.1088/0034-4885/78/12/124901 , adsurl =
2015 doi
-
[131]
, keywords =
Upper limits on the isotropic gravitational radiation background from pulsar timing analysis. , keywords =. doi:10.1086/183954 , adsurl =
-
[132]
, archivePrefix = "arXiv", eprint =
The International Pulsar Timing Array: First data release. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stw347 , adsurl =
-
[133]
, archivePrefix = "arXiv", eprint =
High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stw483 , adsurl =
-
[134]
, archivePrefix = "arXiv", eprint =
Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stv2395 , adsurl =
-
[135]
, archivePrefix = "arXiv", eprint =
The NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4365/aab5b0 , adsurl =
-
[136]
Gravitational wave research using pulsar timing arrays
Hobbs, George and Dai, Shi. Gravitational wave research using pulsar timing arrays. Natl. Sci. Rev. 2017. doi:10.1093/nsr/nwx126. arXiv:1707.01615
2017 arXiv
-
[137]
, archivePrefix = "arXiv", eprint =
Gravitational wave beacons. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.99.064023 , adsurl =
-
[138]
, archivePrefix = "arXiv", eprint =
Single sources in the low-frequency gravitational wave sky: properties and time to detection by pulsar timing arrays. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/sty689 , adsurl =
-
[139]
, archivePrefix = "arXiv", eprint =
Detection and localization of single-source gravitational waves with pulsar timing arrays. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stv381 , adsurl =
-
[140]
, archivePrefix = "arXiv", eprint =
Multi-messenger Observations of a Binary Neutron Star Merger. , archivePrefix = "arXiv", eprint =. doi:10.3847/2041-8213/aa91c9 , adsurl =
-
[141]
, archivePrefix = "arXiv", eprint =
Quasi-periodic Behavior of Mini-disks in Binary Black Holes Approaching Merger. , archivePrefix = "arXiv", eprint =. doi:10.3847/2041-8213/aaa756 , adsurl =
-
[142]
, archivePrefix = "arXiv", eprint =
Electromagnetic Emission from Supermassive Binary Black Holes Approaching Merger. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/aad8b4 , adsurl =
-
[143]
, archivePrefix = "arXiv", eprint =
Quasi-periodicity of Supermassive Binary Black Hole Accretion Approaching Merger. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/ab2453 , adsurl =
-
[144]
, eprint =
The Australia Telescope National Facility Pulsar Catalogue. , eprint =. doi:10.1086/428488 , adsurl =
-
[145]
, archivePrefix = "arXiv", eprint =
A New Electron-density Model for Estimation of Pulsar and FRB Distances. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/835/1/29 , adsurl =
-
[146]
arXiv e-prints , archivePrefix = "arXiv", eprint =
GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs. arXiv e-prints , archivePrefix = "arXiv", eprint =
-
[147]
, eprint =
Simulation of a population of isolated neutron stars evolving through the emission of gravitational waves. , eprint =. doi:10.1111/j.1365-2966.2005.08975.x , adsurl =
2005
-
[148]
, archivePrefix = "arXiv", eprint =
First Search for Gravitational Waves from Known Pulsars with Advanced LIGO. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/aa677f , adsurl =
-
[149]
, archivePrefix = "arXiv", eprint =
Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015 2017 LIGO Data. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/ab20cb , adsurl =
2015 doi
-
[150]
arXiv e-prints , archivePrefix = "arXiv", eprint =
Magnetars: a short review and some sparse considerations. arXiv e-prints , archivePrefix = "arXiv", eprint =
-
[151]
A review
Magnetars: the physics behind observations. A review. Reports on Progress in Physics , archivePrefix = "arXiv", eprint =. doi:10.1088/0034-4885/78/11/116901 , adsurl =
-
[152]
, archivePrefix = "arXiv", eprint =
Search for transient gravitational waves in coincidence with short-duration radio transients during 2007-2013. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.93.122008 , adsurl =
2007 doi
-
[153]
, archivePrefix = "arXiv", eprint =
An anti-glitch in a magnetar. , archivePrefix = "arXiv", eprint =. doi:10.1038/nature12159 , adsurl =
-
[154]
, archivePrefix = "arXiv", eprint =
Detection of the magnetar SGR J1745-2900 up to 291 GHz with evidence of polarized millimetre emission. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stw2757 , adsurl =
-
[155]
, eprint =
Polarized Radio Emission from the Magnetar XTE J1810-197. , eprint =. doi:10.1086/516630 , adsurl =
-
[156]
, eprint =
Transient pulsed radio emission from a magnetar. , eprint =. doi:10.1038/nature04986 , adsurl =
-
[157]
, archivePrefix = "arXiv", eprint =
Radio Disappearance of the Magnetar XTE J1810-197 and Continued X-ray Timing. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/820/2/110 , adsurl =
-
[158]
, eprint =
Discovery of a Transient Magnetar: XTE J1810-197. , eprint =. doi:10.1086/422636 , adsurl =
-
[159]
, archivePrefix = "arXiv", eprint =
Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO's Second Observing Run. , archivePrefix = "arXiv", eprint =. doi:10.3847/1538-4357/ab0e15 , adsurl =
-
[160]
Pulsar Astrophysics the Next Fifty Years , year = 2018, series =
Pulsar Glitches. Pulsar Astrophysics the Next Fifty Years , year = 2018, series =. doi:10.1017/S1743921317009607 , adsurl =
2018 doi
-
[161]
, archivePrefix = "arXiv", eprint =
Detection of 107 glitches in 36 southern pulsars. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/sts366 , adsurl =
-
[163]
International Journal of Modern Physics D , archivePrefix = "arXiv", eprint =
Models of pulsar glitches. International Journal of Modern Physics D , archivePrefix = "arXiv", eprint =. doi:10.1142/S0218271815300086 , adsurl =
-
[164]
, archivePrefix = "arXiv", eprint =
Pulsar Glitches: The Crust is not Enough. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.109.241103 , adsurl =
-
[165]
, archivePrefix = "arXiv", eprint =
Crustal Entrainment and Pulsar Glitches. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.110.011101 , adsurl =
-
[166]
, archivePrefix = "arXiv", eprint =
Pulsar glitches: The crust may be enough. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevC.90.015803 , adsurl =
-
[167]
, eprint =
The Astronomer's Telegram: A Web-based Short-Notice Publication System for the Professional Astronomical Community. , eprint =. doi:10.1086/316184 , adsurl =
-
[168]
, archivePrefix = "arXiv", eprint =
Modelling annual and orbital variations in the scintillation of the relativistic binary PSR J1141-6545. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stz643 , adsurl =
-
[169]
doi:10.5281/zenodo.1420585 , adsurl =
Precision Radio-Frequency Pulsar Timing Interstellar Scintillometry. doi:10.5281/zenodo.1420585 , adsurl =
-
[170]
, archivePrefix = "arXiv", eprint =
Scintillation Arcs in Low-frequency Observations of the Timing-array Millisecond Pulsar PSR J0437-4715. , archivePrefix = "arXiv", eprint =. doi:10.3847/0004-637X/818/1/86 , adsurl =
-
[171]
, archivePrefix = "arXiv", eprint =
Testing gravity with pulsar scintillation measurements. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.95.084049 , adsurl =
-
[172]
arXiv e-prints , archivePrefix = "arXiv", eprint =
Review on tests of General Relativity And Modified Gravity Using Pulsar Timing. arXiv e-prints , archivePrefix = "arXiv", eprint =
-
[173]
, archivePrefix = "arXiv", eprint =
Constraining Alternative Theories of Gravity Using Pulsar Timing Arrays. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.120.181101 , adsurl =
-
[174]
, keywords =
Fast Radio Bursts: An Extragalactic Enigma. , keywords =. 2019. doi:10.1146/annurev-astro-091918-104501 , archivePrefix =. 1906.05878 , primaryClass =
2019 arXiv
-
[175]
Journal of Instrumentation , keywords =
A Radio-Frequency-over-Fiber link for large-array radio astronomy applications. Journal of Instrumentation , keywords =. 2013. doi:10.1088/1748-0221/8/10/T10003 , archivePrefix =. 1308.5481 , primaryClass =
2013 arXiv
-
[176]
, eprint =
Fourier Techniques for Very Long Astrophysical Time-Series Analysis. , eprint =. doi:10.1086/342285 , adsurl =
-
[177]
, eprint =
A New Search Technique for Short Orbital Period Binary Pulsars. , eprint =. doi:10.1086/374806 , adsurl =
-
[178]
American Astronomical Society Meeting Abstracts , year = 2001, series =
New Search Techniques for Binary Pulsars. American Astronomical Society Meeting Abstracts , year = 2001, series =
2001
-
[179]
The Astronomer's Telegram , keywords =
Glitch detected in the Vela Pulsar (PSR J0835-4510). The Astronomer's Telegram , keywords =. 2019
2019
-
[180]
The Astronomer's Telegram , keywords =
Fermi LAT Detection of the Recent Glitch in the Vela Pulsar (PSR J0835-4510). The Astronomer's Telegram , keywords =. 2019
2019
-
[181]
astro-ph.HE
Spin frequency evolution and pulse profile variations of the recently re-activated radio magnetar XTE J1810-197. , volume =. doi:10.1093/mnras/stz2074 , adsurl =. arXiv:1903.02660 , primaryClass = "astro-ph.HE", keywords =
1903 arXiv
-
[182]
The Astronomer's Telegram , keywords =
Intense radio flare from the magnetar XTE J1810-197. The Astronomer's Telegram , keywords =
-
[183]
The Astronomer's Telegram , keywords =
Follow up of the radio flare from the magnetar XTE J1810-197 at 1.4 GHz. The Astronomer's Telegram , keywords =. 2018
2018
-
[184]
The prevalence of repeating fast radio bursts
Ravi, Vikram. The prevalence of repeating fast radio bursts. Nat. Astron. 2019. doi:10.1038/s41550-019-0831-y. arXiv:1907.06619
2019 arXiv
-
[185]
, keywords =
One Year of Monitoring the Vela Pulsar Using a Phased Array Feed. , keywords =. 2017. doi:10.1017/pasa.2017.19 , archivePrefix =. 1705.08355 , primaryClass =
2017 arXiv
-
[186]
The Journal of Open Source Software , archivePrefix = "arXiv", eprint =
psrqpy: a python interface for querying the ATNF pulsar catalogue. The Journal of Open Source Software , archivePrefix = "arXiv", eprint =. doi:10.21105/joss.00538 , adsurl =
-
[187]
, archivePrefix = "arXiv", eprint =
Super-luminous Type Ic Supernovae: Catching a Magnetar by the Tail. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/770/2/128 , adsurl =
-
[188]
and Palfreyman, Jim and Stappers, Benjamin and Weltevrede, Patrick
Keitel, David and Woan, Graham and Pitkin, Matthew and Schumacher, Courtney and Pearlstone, Brynley and Riles, Keith and Lyne, Andrew G. and Palfreyman, Jim and Stappers, Benjamin and Weltevrede, Patrick. First search for long-duration transient gravitational waves after glitc...
2019 arXiv
-
[189]
arXiv e-prints , keywords =
CHIME/FRB Detection of Eight New Repeating Fast Radio Burst Sources. arXiv e-prints , keywords =. 2019
2019
-
[191]
, archivePrefix = "arXiv", eprint =
Pulsar timing signal from ultralight scalar dark matter. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2014/02/019 , adsurl =
2014 doi
-
[192]
, archivePrefix = "arXiv", eprint =
Statistical characterization of pulsar glitches and their potential impact on searches for continuous gravitational waves. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.96.063004 , adsurl =
-
[193]
, keywords =
A semicoherent glitch-robust continuous-gravitational-wave search method. , keywords =. 2018. doi:10.1103/PhysRevD.98.063011 , archivePrefix =. 1805.03314 , primaryClass =
2018 arXiv
-
[194]
, keywords =
Search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar. , keywords =. 2011. doi:10.1103/PhysRevD.83.042001 , archivePrefix =. 1011.1357 , primaryClass =
2006 arXiv
-
[195]
, archivePrefix = "arXiv", eprint =
Search method for long-duration gravitational-wave transients from neutron stars. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.84.023007 , adsurl =
-
[196]
, archivePrefix = "arXiv", eprint =
Evidence for a Minimum Ellipticity in Millisecond Pulsars. , archivePrefix = "arXiv", eprint =. doi:10.3847/2041-8213/aad86a , adsurl =
-
[197]
, archivePrefix = "arXiv", eprint =
The glitch activity of neutron stars. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201731519 , adsurl =
-
[198]
, archivePrefix = "arXiv", eprint =
A study of multifrequency polarization pulse profiles of millisecond pulsars. , archivePrefix = "arXiv", eprint =. doi:10.1093/mnras/stv508 , adsurl =
-
[199]
Astrophysics and Space Science Library , year = "2018", editor =
Gravitational Waves from Single Neutron Stars: An Advanced Detector Era Survey. Astrophysics and Space Science Library , year = "2018", editor =. doi:10.1007/978-3-319-97616-7_12 , archivePrefix =. 1709.07049 , primaryClass =
2018 arXiv
-
[200]
, archivePrefix = "arXiv", eprint =
Fast radio bursts. , archivePrefix = "arXiv", eprint =. doi:10.1007/s00159-019-0116-6 , adsurl =
-
[201]
arXiv e-prints , archivePrefix = "arXiv", eprint =
Fundamental Physics with the Square Kilometre Array. arXiv e-prints , archivePrefix = "arXiv", eprint =
-
[202]
, keywords =
Pulsar Timing as a Probe of Non-Einsteinian Polarizations of Gravitational Waves. , keywords =. doi:10.1086/591080 , adsurl =
-
[203]
, archivePrefix = "arXiv", eprint =
Pulsar timing sensitivities to gravitational waves from relativistic metric theories of gravity. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.83.123529 , adsurl =
-
[204]
, archivePrefix = "arXiv", eprint =
Stochastic backgrounds in alternative theories of gravity: Overlap reduction functions for pulsar timing arrays. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.85.082001 , adsurl =
-
[205]
, keywords =
Pulsar timing measurements and the search for gravitational waves. , keywords =. doi:10.1086/157593 , adsurl =
-
[206]
2014", month =
Development of an Electromagnetic Interference Monitor from 1 GHz to 18 GHz. International VLBI Service for Geodesy and Astrometry 2014 General Meeting Proceedings: ''VGOS: The New VLBI Network , year = "2014", month = "Dec", pages =
2014
-
[207]
, keywords =
High signal-to-noise ratio observations and the ultimate limits of precision pulsar timing. , keywords =. 2011. doi:10.1111/j.1365-2966.2011.19578.x , archivePrefix =. 1108.0812 , primaryClass =
2011
-
[208]
Perera, B. B. P. and others. The International Pulsar Timing Array: Second data release. 2019. doi:10.1093/mnras/stz2857. arXiv:1909.04534
2019 arXiv
-
[209]
, keywords =
FRB 121102 Is Coincident with a Star-forming Region in Its Host Galaxy. , keywords =. 2017. doi:10.3847/2041-8213/aa7a0c , archivePrefix =. 1705.07698 , primaryClass =
2017 arXiv
-
[210]
, keywords =
A direct localization of a fast radio burst and its host. , keywords =. 2017. doi:10.1038/nature20797 , archivePrefix =. 1701.01098 , primaryClass =
2017 arXiv
-
[211]
, keywords =
A repeating fast radio burst. , keywords =. 2016. doi:10.1038/nature17168 , archivePrefix =. 1603.00581 , primaryClass =
2016 arXiv
-
[212]
Theory and Experiment in Gravitational Physics
Will, Clifford M. Theory and Experiment in Gravitational Physics. 2018
2018
-
[213]
and Will, Clifford M
Blanchet, Luc and Iyer, Bala R. and Will, Clifford M. and Wiseman, Alan G. Gravitational wave forms from inspiralling compact binaries to second postNewtonian order. Class. Quant. Grav. 1996. doi:10.1088/0264-9381/13/4/002. arXiv:gr-qc/9602024
1996 arXiv
Reviewed August 15, 2026 · model on record in the stance chip above.
Discussion (0). Continue with ORCID to comment.