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arxiv: 2606.25223 · v1 · pith:CMXWW55Jnew · submitted 2026-06-23 · 🌌 astro-ph.HE

Supernovae with the Square Kilometre Array

Poonam Chandra , Yuhei Iwata , A. J. Nayana , Miguel P\'erez-Torres , Kovi Rose This is my paper

Pith reviewed 2026-06-25 22:06 UTC · model grok-4.3

classification 🌌 astro-ph.HE
keywords supernovaecore-collapse supernovaeSquare Kilometre Arrayradio surveyscircumstellar interactionprogenitor mass lossvolumetric ratetime-domain astronomy
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The pith

The Square Kilometre Array will discover hundreds of core-collapse supernovae each year through wide-field radio surveys.

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

The paper argues that SKA1 and its pathfinders will shift radio studies of supernovae from rare detections to routine population statistics. Sensitive commensal wide-field surveys will catch hundreds of core-collapse events annually and supply a complete count of massive-star deaths without dust hiding any. The same observations will track how supernova material collides with surrounding gas and what the original stars lost before exploding. Targeted follow-up of thermonuclear supernovae can detect or rule out radio signals expected from certain progenitor channels. These capabilities will let radio data join optical and other wavelengths as a standard tool for mapping supernova diversity and rates.

Core claim

SKA1 and its pathfinders will transform the radio study of core-collapse supernovae through sensitive, commensal wide-field surveys capable of discovering hundreds of events per year, providing a dust-unbiased census of massive-star deaths and direct measurements of the volumetric CCSN rate. The same data will probe ejecta-circumstellar medium interaction, shock microphysics, and progenitor mass-loss histories. Deep, triggered observations of thermonuclear supernovae will allow tests of competing progenitor scenarios by detecting or definitively excluding prompt radio emission expected from single-degenerate systems.

What carries the argument

Commensal wide-field surveys with SKA1 and pathfinders for discovering and monitoring radio supernovae at scale.

If this is right

  • Hundreds of core-collapse supernovae discovered per year via commensal wide-field surveys
  • Dust-unbiased census of massive-star deaths across the observable volume
  • Direct measurements of the volumetric core-collapse supernova rate
  • Constraints on ejecta-CSM interaction, shock microphysics, and progenitor mass-loss histories from the survey sample
  • Tests of single-degenerate progenitor models for Type Ia supernovae through searches for prompt radio emission

Where Pith is reading between the lines

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

  • Statistical samples could reveal how supernova properties vary with host-galaxy type or metallicity
  • Radio detections might help identify which supernovae contribute to cosmic-ray or neutrino backgrounds when cross-matched with other facilities
  • Rapid alerts from the surveys could enable coordinated multi-wavelength campaigns on the earliest phases of shock evolution
  • Long-term monitoring of the same fields might uncover rare delayed-interaction events missed by shorter optical campaigns

Load-bearing premise

The SKA will be built and will deliver the planned sensitivity, survey speed, and commensal observing modes.

What would settle it

Early SKA1 wide-field data yielding far fewer than hundreds of new radio supernovae per year or failing to support volumetric rate calculations due to insufficient coverage or sensitivity.

Figures

Figures reproduced from arXiv: 2606.25223 by A. J. Nayana, Kovi Rose, Miguel P\'erez-Torres, Poonam Chandra, Yuhei Iwata.

Figure 1
Figure 1. Figure 1: Circumstellar interaction picture in a typical SN. The image shows ejecta-CSM interaction and the formation of various shocked and unshocked regions. The radio emission typically originates from the forward shock. unshocked ejecta or emission from the vicinity of the contact discontinuity can generate additional optical features such as H𝛼 emission (Chugai et al., 2007). Among these diagnostics, however, r… view at source ↗
Figure 2
Figure 2. Figure 2: Plot of 8 GHz radio light curve for various types of CCSNe. The diversity in the radio luminosity, time to peak and extent of the radio emission is apparent in different classes and indicate towards diversity in progenitors. The data are taken from Nayana et al. (2018); Weiler et al. (2007, 2011); Kulkarni et al. (1998); Gangopadhyay et al. (2023); Chandra et al. (2019); Nayana and Chandra (2020). Since su… view at source ↗
Figure 3
Figure 3. Figure 3: The contribution of the primary (blue dash–dotted lines) and secondary (red dashed lines) electrons to the total synchrotron emission (green solid line) for a wind density CSM for parameters mentioned in Petropoulou et al. (2016), the paper from which this figure is adapted and a distance of 40 Mpc is assumed. We also show 3-𝜎 SKA-Mid sensitivities at 1.7 GHz and15 GHz at 40 Mpc. There are growing pieces o… view at source ↗
Figure 4
Figure 4. Figure 4: (Left) Estimated number of detectable CCSNe per year and the maximum observable distance. Three cases of the peak spectral luminosity are shown: 𝐿𝜈 = 1025 , 1026, and 1027 erg s−1 Hz−1 . Vertical lines indicate the assumed 1-hour (5𝜎) sensitivities of SKA1-Low and SKA1-Mid for the AA4 configuration. (Right) Same as the left panel, but divided by SN type. The assumed SN fraction of each type is taken from M… view at source ↗
read the original abstract

This chapter presents the science potential of the Square Kilometre Array (SKA) for studying all classes of supernovae and their environments. It substantially updates and extends the earlier work of Perez-Torres et al. (2015), originally published in the 2015 Advancing Astrophysics with the SKA (AASKA14) volume, reflecting the dramatic progress in time-domain astronomy and radio instrumentation over the past decade. We outline how SKA1 and its pathfinders will transform the radio study of core-collapse supernovae (CCSNe) through sensitive, commensal wide-field surveys capable of discovering hundreds of events per year, providing a dust-unbiased census of massive-star deaths and direct measurements of the volumetric CCSN rate. The same data will probe ejecta-circumstellar medium (CSM) interaction, shock microphysics, and progenitor mass-loss histories. Deep, triggered observations of thermonuclear supernovae (SNe Ia) will allow the SKA to test competing progenitor scenarios by detecting -- or definitively excluding -- the prompt radio emission expected from single-degenerate systems. The chapter further explores superluminous supernovae (SLSNe), delayed interaction supernovae and synergies with facilities such as ALMA, ngVLA, CTA, IceCube-Gen2, and ULTRASAT. Collectively, these studies will turn radio supernova astrophysics from a discovery-limited field into one governed by population statistics.

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

0 major / 0 minor

Summary. This manuscript updates and extends the 2015 AASKA14 science case (Perez-Torres et al.) for radio observations of supernovae with the Square Kilometre Array. It argues that SKA1 and its pathfinders, through sensitive commensal wide-field surveys, will discover hundreds of core-collapse supernovae per year, enabling a dust-unbiased census of massive-star deaths, direct volumetric CCSN rate measurements, and studies of ejecta-CSM interaction and progenitor mass loss. It further outlines triggered observations to test SN Ia progenitor channels via prompt radio emission, plus science cases for superluminous and delayed-interaction supernovae and synergies with ALMA, ngVLA, CTA, IceCube-Gen2, and ULTRASAT.

Significance. If the stated instrumental performance is achieved, the outlined program would shift radio supernova astrophysics from a discovery-limited to a statistics-driven field, delivering population-level constraints on massive-star death rates and explosion physics that are inaccessible at other wavelengths. The manuscript is a standard, well-scoped forward-looking review that appropriately conditions all quantitative projections on SKA1 meeting its design sensitivity, survey speed, and commensal capabilities; no new derivations or data are presented.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for their positive review and recommendation to accept the manuscript. The summary accurately reflects the scope and intent of the chapter as an update to the 2015 AASKA14 science case.

Circularity Check

0 steps flagged

No significant circularity detected

full rationale

This is a forward-looking science case document outlining projected capabilities of the SKA for supernova studies. It contains no equations, fitted parameters, derivations, or load-bearing self-citations that reduce any claim to its own inputs by construction. All statements are conditional projections based on external telescope design specifications and prior literature, with no internal mathematical chain that could be circular. The update to Perez-Torres et al. (2015) is a normal extension of scope rather than a self-referential justification of results.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 0 invented entities

This is a review chapter on future observational capabilities. No free parameters, axioms, or invented entities are introduced in the provided abstract.

pith-pipeline@v0.9.1-grok · 5807 in / 1083 out tokens · 18238 ms · 2026-06-25T22:06:57.887173+00:00 · methodology

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Reference graph

Works this paper leans on

74 extracted references · 29 linked inside Pith

  1. [1]

    2014─2017 core-collapse supernovae and their subtypes

    Supernova rates and luminosity functions from ASAS-SN: II. 2014─2017 core-collapse supernovae and their subtypes. , keywords =. doi:10.1051/0004-6361/202556799 , archivePrefix =. 2508.10985 , primaryClass =

    doi:10.1051/0004-6361/202556799 2014

  2. [2]

    2026 ,publisher =

    Tao An and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  3. [3]

    2026 ,publisher =

    Maria Rioja and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  4. [4]

    2026 ,publisher =

    Alberto Colombo and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  5. [5]

    2026 ,publisher =

    Matthias Kadler and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  6. [6]

    , keywords =

    Constraints on the Progenitor System and the Environs of SN 2014J from Deep Radio Observations. , keywords =. doi:10.1088/0004-637X/792/1/38 , archivePrefix =. 1405.4702 , primaryClass =

    Pith/arXiv arXiv doi:10.1088/0004-637x/792/1/38

  7. [7]

    Pérez-Torres, M. A. and Alberdi, A. and Beswick, R. J. and Lundqvist, P. and others , title =. Advancing Astrophysics with the Square Kilometre Array (AASKA14) , year =

  8. [8]

    2019 , eprint=

    Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1) , author=. 2019 , eprint=

    2019

  9. [9]

    2015 , publisher=

    Advancing Astrophysics with the Square Kilometre Array (AASKA14) , author=. 2015 , publisher=

    2015

  10. [10]

    , year = 1966, month = mar, volume =

    The Hydrodynamic Behavior of Supernovae Explosions. , year = 1966, month = mar, volume =. doi:10.1086/148549 , adsurl =

    doi:10.1086/148549 1966

  11. [11]

    , keywords =

    Revival of a stalled supernova shock by neutrino heating. , keywords =. doi:10.1086/163343 , adsurl =

    doi:10.1086/163343

  12. [12]

    , keywords =

    Self-similar solutions for the interaction of stellar ejecta with an external medium. , keywords =. doi:10.1086/160126 , adsurl =

    doi:10.1086/160126

  13. [13]

    Science , keywords =

    Luminous Supernovae. Science , keywords =. doi:10.1126/science.1203601 , archivePrefix =. 1208.3217 , primaryClass =

    Pith/arXiv arXiv doi:10.1126/science.1203601

  14. [14]

    , keywords =

    The Most Luminous Supernovae. , keywords =. doi:10.1146/annurev-astro-081817-051819 , archivePrefix =. 1812.01428 , primaryClass =

    doi:10.1146/annurev-astro-081817-051819

  15. [15]

    , keywords =

    Late-time Radio and Millimeter Observations of Superluminous Supernovae and Long Gamma-Ray Bursts: Implications for Central Engines, Fast Radio Bursts, and Obscured Star Formation. , keywords =. doi:10.3847/1538-4357/abe9b8 , archivePrefix =. 2010.06612 , primaryClass =

    doi:10.3847/1538-4357/abe9b8 2010

  16. [16]

    , keywords =

    A Radio Source Coincident with the Superluminous Supernova PTF10hgi: Evidence for a Central Engine and an Analog of the Repeating FRB 121102?. , keywords =. doi:10.3847/2041-8213/ab18a5 , archivePrefix =. 1901.10479 , primaryClass =

    doi:10.3847/2041-8213/ab18a5 2041

  17. [17]

    , keywords =

    SN 2017ens: The Metamorphosis of a Luminous Broadlined Type Ic Supernova into an SN IIn. , keywords =. doi:10.3847/2041-8213/aaeb2e , archivePrefix =. 1808.04382 , primaryClass =

    Pith/arXiv arXiv doi:10.3847/2041-8213/aaeb2e 2041

  18. [18]

    , keywords =

    Long-Term Radio Monitoring of SN 1993J. , keywords =. doi:10.1086/523258 , archivePrefix =. 0709.1136 , primaryClass =

    Pith/arXiv arXiv doi:10.1086/523258

  19. [19]

    , keywords =

    Bridging between Type IIb and Ib Supernovae: SN IIb 2022crv with a Very Thin Hydrogen Envelope. , keywords =. doi:10.3847/1538-4357/acfa94 , archivePrefix =. 2309.07463 , primaryClass =

    doi:10.3847/1538-4357/acfa94

  20. [20]

    , keywords =

    Type Ib Supernova Master OT J120451.50+265946.6: Radio-emitting Shock with Inhomogeneities Crossing through a Dense Shell. , keywords =. doi:10.3847/1538-4357/ab1900 , archivePrefix =. 1904.06392 , primaryClass =

    Pith/arXiv arXiv doi:10.3847/1538-4357/ab1900 1904

  21. [21]

    , keywords =

    Observational Clues to the Progenitors of Type Ia Supernovae. , keywords =. doi:10.1146/annurev-astro-082812-141031 , archivePrefix =. 1312.0628 , primaryClass =

    Pith/arXiv arXiv doi:10.1146/annurev-astro-082812-141031

  22. [22]

    , keywords =

    Against the Wind: Radio Light Curves of Type Ia Supernovae Interacting with Low-density Circumstellar Shells. , keywords =. doi:10.3847/0004-637X/823/2/100 , archivePrefix =. 1604.00019 , primaryClass =

    Pith/arXiv arXiv doi:10.3847/0004-637x/823/2/100

  23. [23]

    , keywords =

    A Late-time Radio Survey of Type Ia-CSM Supernovae with the Very Large Array. , keywords =. doi:10.3847/1538-4357/ae17b0 , archivePrefix =. 2506.19071 , primaryClass =

    doi:10.3847/1538-4357/ae17b0

  24. [24]

    , keywords =

    Early Radio and X-Ray Observations of the Youngest nearby Type Ia Supernova PTF 11kly (SN 2011fe). , keywords =. doi:10.1088/0004-637X/746/1/21 , archivePrefix =. 1109.2912 , primaryClass =

    Pith/arXiv arXiv doi:10.1088/0004-637x/746/1/21

  25. [25]

    , year = 1997, month = jan, volume =

    Optical Spectra of Supernovae. , year = 1997, month = jan, volume =. doi:10.1146/annurev.astro.35.1.309 , adsurl =

    doi:10.1146/annurev.astro.35.1.309 1997

  26. [26]

    , keywords =

    An asymptotic-giant-branch star in the progenitor system of a type Ia supernova. , keywords =. doi:10.1038/nature01854 , archivePrefix =. astro-ph/0306270 , primaryClass =

    Pith/arXiv arXiv doi:10.1038/nature01854

  27. [27]

    , keywords =

    Radio view of a broad-line Type Ic supernova ASASSN-16fp. , keywords =. doi:10.1093/mnras/staa700 , archivePrefix =. 2003.02709 , primaryClass =

    doi:10.1093/mnras/staa700 2003

  28. [28]

    , year = 1998, month = oct, volume =

    Radio emission from the unusual supernova 1998bw and its association with the -ray burst of 25 April 1998. , year = 1998, month = oct, volume =. doi:10.1038/27139 , adsurl =

    doi:10.1038/27139 1998

  29. [29]

    , keywords =

    Long-term Behavior of a Type IIP Supernova SN 2004dj in the Radio Bands. , keywords =. doi:10.3847/1538-4357/aad17a , adsurl =

    doi:10.3847/1538-4357/aad17a

  30. [30]

    , keywords =

    Radio Emission from SN 1994I in NGC 5194 (M 51): The Best-studied Type Ib/c Radio Supernova. , keywords =. doi:10.1088/0004-637X/740/2/79 , archivePrefix =. 1108.2692 , primaryClass =

    Pith/arXiv arXiv doi:10.1088/0004-637x/740/2/79

  31. [31]

    Chevalier and Claes Fransson , title =

    Roger A. Chevalier and Claes Fransson , title =. Supernovae and Gamma-Ray Bursters , editor =. 2003 , publisher =

    2003

  32. [32]

    arXiv e-prints , keywords =

    Multiwavelength view of circumstellar interaction in supernovae. arXiv e-prints , keywords =. doi:10.48550/arXiv.2510.20913 , archivePrefix =. 2510.20913 , primaryClass =

    doi:10.48550/arxiv.2510.20913

  33. [33]

    , keywords =

    Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars. , keywords =. doi:10.1146/annurev-astro-081913-040025 , archivePrefix =. 1402.1237 , primaryClass =

    Pith/arXiv arXiv doi:10.1146/annurev-astro-081913-040025

  34. [34]

    , keywords =

    Luminous Radio Emission from the Superluminous Supernova 2017ens at 3.3 yr after Explosion. , keywords =. doi:10.3847/2041-8213/acf1fd , archivePrefix =. 2306.13730 , primaryClass =

    doi:10.3847/2041-8213/acf1fd 2041

  35. [35]

    , keywords =

    Radio emission from a decade old Type I superluminous supernova, PTF10hgi: comparison with FRB121102. , keywords =. doi:10.1093/mnras/staa2637 , archivePrefix =. 2008.11375 , primaryClass =

    doi:10.1093/mnras/staa2637 2008

  36. [36]

    arXiv e-prints , keywords =

    Superluminous supernovae. arXiv e-prints , keywords =. doi:10.48550/arXiv.2407.12302 , archivePrefix =. 2407.12302 , primaryClass =

    doi:10.48550/arxiv.2407.12302

  37. [37]

    , keywords =

    Synchrotron Self-Absorption in Radio Supernovae. , keywords =. doi:10.1086/305676 , adsurl =

    doi:10.1086/305676

  38. [38]

    , keywords =

    A radio-detected type Ia supernova with helium-rich circumstellar material. , keywords =. doi:10.1038/s41586-023-05916-w , archivePrefix =. 2210.07725 , primaryClass =

    doi:10.1038/s41586-023-05916-w

  39. [39]

    , keywords =

    The Radio Luminosity-risetime Function of Core-collapse Supernovae. , keywords =. doi:10.3847/1538-4357/abccd9 , archivePrefix =. 2011.11737 , primaryClass =

    doi:10.3847/1538-4357/abccd9 2011

  40. [40]

    , keywords =

    Radio synchrotron emission from secondary electrons in interaction-powered supernovae. , keywords =. doi:10.1093/mnras/stw920 , archivePrefix =. 1603.00891 , primaryClass =

    Pith/arXiv arXiv doi:10.1093/mnras/stw920

  41. [41]

    Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray , year = 2022, editor =

    The scientific payload of the Ultraviolet Transient Astronomy Satellite (ULTRASAT). Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray , year = 2022, editor =. doi:10.1117/12.2629850 , archivePrefix =. 2208.00159 , primaryClass =

    doi:10.1117/12.2629850 2022

  42. [42]

    , keywords =

    The radio and X-ray emission from type II supernovae. , keywords =. doi:10.1086/160167 , adsurl =

    doi:10.1086/160167

  43. [43]

    , keywords =

    Optical Signatures of Circumstellar Interaction in Type IIP Supernovae. , keywords =. doi:10.1086/518160 , archivePrefix =. astro-ph/0703468 , primaryClass =

    Pith/arXiv arXiv doi:10.1086/518160

  44. [44]

    , keywords =

    Mass loss from hot massive stars. , keywords =. doi:10.1007/s00159-008-0015-8 , archivePrefix =. 0811.0487 , primaryClass =

    Pith/arXiv arXiv doi:10.1007/s00159-008-0015-8

  45. [45]

    Reviews of Modern Physics , keywords =

    The evolution and explosion of massive stars. Reviews of Modern Physics , keywords =. doi:10.1103/RevModPhys.74.1015 , adsurl =

    doi:10.1103/revmodphys.74.1015

  46. [46]

    I - Presupernova evolution and triggering mechanisms

    Accreting white dwarf models for type I supernovae. I - Presupernova evolution and triggering mechanisms. , keywords =. doi:10.1086/159682 , adsurl =

    doi:10.1086/159682

  47. [47]

    , year = 1973, month = dec, volume =

    Binaries and Supernovae of Type I. , year = 1973, month = dec, volume =. doi:10.1086/152565 , adsurl =

    doi:10.1086/152565 1973

  48. [48]

    Supernovae and Nucleosynthesis: An Investigation of the History of Matter from the Big Bang to the Present

  49. [49]

    Jansky Very Large Array Sky Survey (VLASS)

    Luminous Late-time Radio Emission from Supernovae Detected by the Karl G. Jansky Very Large Array Sky Survey (VLASS). , keywords =. doi:10.3847/2041-8213/ac375e , archivePrefix =. 2106.09737 , primaryClass =

    doi:10.3847/2041-8213/ac375e 2041

  50. [50]

    , keywords =

    Circumstellar Emission from Type Ib and Ic Supernovae. , keywords =. doi:10.1086/507606 , archivePrefix =. astro-ph/0607196 , primaryClass =

    Pith/arXiv arXiv doi:10.1086/507606

  51. [51]

    , keywords =

    Off-Axis Afterglow Emission from Jetted Gamma-Ray Bursts. , keywords =. doi:10.1086/340991 , archivePrefix =. astro-ph/0201322 , primaryClass =

    Pith/arXiv arXiv doi:10.1086/340991

  52. [52]

    Handbook of Supernovae , year = 2017, editor =

    Pulsar Wind Nebulae. Handbook of Supernovae , year = 2017, editor =. doi:10.1007/978-3-319-21846-5_95 , adsurl =

    doi:10.1007/978-3-319-21846-5_95 2017

  53. [53]

    , keywords =

    Dinosaur in a Haystack: X-Ray View of the Entrails of SN 2023ixf and the Radio Afterglow of Its Interaction with the Medium Spawned by the Progenitor Star (Paper I). , keywords =. doi:10.3847/1538-4357/adc2fb , archivePrefix =. 2411.02647 , primaryClass =

    doi:10.3847/1538-4357/adc2fb

  54. [54]

    , keywords =

    Probing cosmic ray ion acceleration with radio-submm and gamma-ray emission from interaction-powered supernovae. , keywords =. doi:10.1093/mnras/stu384 , archivePrefix =. 1311.6778 , primaryClass =

    Pith/arXiv arXiv doi:10.1093/mnras/stu384

  55. [55]

    , keywords =

    New class of high-energy transients from crashes of supernova ejecta with massive circumstellar material shells. , keywords =. doi:10.1103/PhysRevD.84.043003 , archivePrefix =. 1012.2834 , primaryClass =

    Pith/arXiv arXiv doi:10.1103/physrevd.84.043003

  56. [56]

    Death of Massive Stars: Supernovae and Gamma-Ray Bursts , year = 2012, editor =

    X-rays, -rays and neutrinos from collisionless shocks in supernova wind breakouts. Death of Massive Stars: Supernovae and Gamma-Ray Bursts , year = 2012, editor =. doi:10.1017/S174392131201304X , archivePrefix =. 1106.1898 , primaryClass =

    Pith/arXiv arXiv doi:10.1017/s174392131201304x 2012

  57. [57]

    , keywords =

    High-energy Neutrino and Gamma-Ray Transients from Trans-relativistic Supernova Shock Breakouts. , keywords =. doi:10.1088/2041-8205/769/1/L6 , archivePrefix =. 1210.8147 , primaryClass =

    Pith/arXiv arXiv doi:10.1088/2041-8205/769/1/l6 2041

  58. [58]

    , year = 1973, month = mar, volume =

    A Theoretical Model for Type II Supernovae. , year = 1973, month = mar, volume =. doi:10.1086/181154 , adsurl =

    doi:10.1086/181154 1973

  59. [59]

    , keywords =

    SN 2006gy: An Extremely Luminous Supernova in the Galaxy NGC 1260. , keywords =. doi:10.1086/516749 , archivePrefix =. astro-ph/0612408 , primaryClass =

    Pith/arXiv arXiv doi:10.1086/516749

  60. [60]

    , keywords =

    Shell-shocked Diffusion Model for the Light Curve of SN 2006gy. , keywords =. doi:10.1086/524681 , archivePrefix =. 0710.3428 , primaryClass =

    Pith/arXiv arXiv doi:10.1086/524681

  61. [61]

    , keywords =

    Hydrogen-poor superluminous stellar explosions. , keywords =. doi:10.1038/nature10095 , archivePrefix =. 0910.0059 , primaryClass =

    Pith/arXiv arXiv doi:10.1038/nature10095

  62. [62]

    Nature Physics , keywords =

    Confined dense circumstellar material surrounding a regular type II supernova. Nature Physics , keywords =. doi:10.1038/nphys4025 , archivePrefix =. 1701.02596 , primaryClass =

    Pith/arXiv arXiv doi:10.1038/nphys4025

  63. [63]

    , keywords =

    The wind speeds, dust content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity. , keywords =. doi:10.1093/mnras/stw2708 , archivePrefix =. 1610.05761 , primaryClass =

    Pith/arXiv arXiv doi:10.1093/mnras/stw2708

  64. [64]

    Nature Astronomy , keywords =

    The delay of shock breakout due to circumstellar material evident in most type II supernovae. Nature Astronomy , keywords =. doi:10.1038/s41550-018-0563-4 , archivePrefix =. 1809.06379 , primaryClass =

    Pith/arXiv arXiv doi:10.1038/s41550-018-0563-4

  65. [65]

    , keywords =

    Late-time supernovae radio re-brightening in the VAST pilot survey. , keywords =. doi:10.1093/mnras/stae2289 , archivePrefix =. 2410.01375 , primaryClass =

    doi:10.1093/mnras/stae2289

  66. [66]

    , keywords =

    VAST: An ASKAP Survey for Variables and Slow Transients. , keywords =. doi:10.1017/pasa.2012.006 , archivePrefix =. 1207.1528 , primaryClass =

    Pith/arXiv arXiv doi:10.1017/pasa.2012.006 2012

  67. [67]

    , keywords =

    The ASKAP Variables and Slow Transients (VAST) Pilot Survey. , keywords =. doi:10.1017/pasa.2021.44 , archivePrefix =. 2108.06039 , primaryClass =

    doi:10.1017/pasa.2021.44 2021

  68. [68]

    , keywords =

    Discovery of a bright radio transient in M 82: a new radio supernova?. , keywords =. doi:10.1051/0004-6361/200912327 , archivePrefix =. 0904.2388 , primaryClass =

    Pith/arXiv arXiv doi:10.1051/0004-6361/200912327

  69. [69]

    , keywords =

    Radio Follow-up Observations of SN 2023ixf by Japanese and Korean Very Long Baseline Interferometers. , keywords =. doi:10.3847/1538-4357/ad9a62 , archivePrefix =. 2411.07542 , primaryClass =

    doi:10.3847/1538-4357/ad9a62

  70. [70]

    system description

    Australian square kilometre array pathfinder: I. system description. , keywords =. doi:10.1017/pasa.2021.1 , archivePrefix =. 2102.01870 , primaryClass =

    doi:10.1017/pasa.2021.1 2021

  71. [71]

    Catalogues and fractions of supernovae in a complete sample

    Supernovae at distances <40 Mpc: I. Catalogues and fractions of supernovae in a complete sample. , keywords =. doi:10.1051/0004-6361/202452684 , archivePrefix =. 2504.04393 , primaryClass =

    doi:10.1051/0004-6361/202452684

  72. [72]

    , keywords =

    The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations. , keywords =. doi:10.1093/mnras/stw3310 , archivePrefix =. 1612.06059 , primaryClass =

    Pith/arXiv arXiv doi:10.1093/mnras/stw3310

  73. [73]

    , keywords =

    Radio emission from supernovae. , keywords =

  74. [74]

    Lacy and S

    M. Lacy and S. A. Baum and C. J. Chandler and S. Chatterjee and T. E. Clarke and S. Deustua and J. English and J. Farnes and B. M. Gaensler and N. Gugliucci and G. Hallinan and B. R. Kent and A. Kimball and C. J. Law and T. J. W. Lazio and J. Marvil and S. A. Mao and D. Medlin and K. Mooley and E. J. Murphy and S. Myers and R. Osten and G. T. Richards and...

    doi:10.1088/1538-3873/ab63eb