Shock cooling of a red-supergiant supernova at redshift 3 in lensed images.


Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
11 2022
Historique:
received: 07 02 2022
accepted: 18 08 2022
entrez: 9 11 2022
pubmed: 10 11 2022
medline: 10 11 2022
Statut: ppublish

Résumé

The core-collapse supernova of a massive star rapidly brightens when a shock, produced following the collapse of its core, reaches the stellar surface. As the shock-heated star subsequently expands and cools, its early-time light curve should have a simple dependence on the size of the progenitor

Identifiants

pubmed: 36352131
doi: 10.1038/s41586-022-05252-5
pii: 10.1038/s41586-022-05252-5
doi:

Types de publication

Journal Article Research Support, Non-U.S. Gov't

Langues

eng

Sous-ensembles de citation

IM

Pagination

256-259

Informations de copyright

© 2022. The Author(s), under exclusive licence to Springer Nature Limited.

Références

Waxman, E. & Katz, B. in Handbook of Supernovae (eds Alsabti, A. & Murdin, P.) 967–1015 (Springer, 2017).
Garnavich, P. M. et al. Shock breakout and early light curves of type II-P supernovae observed with Kepler. Astrophys. J. 820, 23 (2016).
doi: 10.3847/0004-637X/820/1/23
Arcavi, I. et al. SN 2011dh: discovery of a type IIb supernova from a compact progenitor in the nearby galaxy M51. Astrophys. J. Lett. 742, L18 (2011).
doi: 10.1088/2041-8205/742/2/L18
Morales-Garoffolo, A. et al. SN 2011fu: a type IIb supernova with a luminous double-peaked light curve. Mon. Not. R. Astron. Soc 454, 95–114 (2015).
doi: 10.1093/mnras/stv1972
Ben-Ami, S. et al. Discovery and early multi-wavelength measurements of the energetic type Ic supernova PTF12gzk: a massive-star explosion in a dwarf host galaxy. Astrophys. J. Lett. 760, L33 (2012).
doi: 10.1088/2041-8205/760/2/L33
Valenti, S. et al. The first month of evolution of the slow-rising type IIP SN 2013ej in M74. Mon. Not. R. Astron. Soc. Lett. 438, L101–L105 (2014).
doi: 10.1093/mnrasl/slt171
Bersten, M. C. et al. A surge of light at the birth of a supernova. Nature 554, 497–499 (2018).
pubmed: 29469097 doi: 10.1038/nature25151
Tartaglia, L. et al. The progenitor and early evolution of the type IIb SN 2016gkg. Astrophys. J. Lett. 836, L12 (2017).
doi: 10.3847/2041-8213/aa5c7f
Arcavi, I. et al. Constraints on the progenitor of SN 2016gkg from its shock-cooling light curve. Astrophys. J. Lett. 837, L2 (2017).
doi: 10.3847/2041-8213/aa5be1
Piro, A. L., Haynie, A. & Yao, Y. Shock cooling emission from extended material revisited. Astrophys. J. 909, 209 (2021).
doi: 10.3847/1538-4357/abe2b1
Szalai, T. et al. The type II-P supernova 2017eaw: from explosion to the nebular phase. Astrophys. J. 876, 19 (2019).
doi: 10.3847/1538-4357/ab12d0
Rui, L. et al. Probing the final-stage progenitor evolution for type IIP supernova 2017eaw in NGC 6946. Mon. Not. R. Astron. Soc 485, 1990–2000 (2019).
doi: 10.1093/mnras/stz503
Xiang, D. et al. Observations of SN 2017ein reveal shock breakout emission and a massive progenitor star for a type Ic supernova. Astrophys. J. 871, 176 (2019).
doi: 10.3847/1538-4357/aaf8b0
Soumagnac, M. T. et al. SN 2018fif: the explosion of a large red supergiant discovered in its infancy by the Zwicky Transient Facility. Astrophys. J. Letters 902, 6 (2020).
doi: 10.3847/1538-4357/abb247
Lotz, J. M. et al. The Frontier Fields: survey design and initial results. Astrophys. J. 837, 97 (2017).
doi: 10.3847/1538-4357/837/1/97
Struble, M. F. & Rood, H. J. A compilation of redshifts and velocity dispersions for Abell clusters (Epoch 1991.2). Astrophys. J. Suppl. Ser. 77, 363–377 (1991).
doi: 10.1086/191608
Benítez, N. Bayesian photometric redshift estimation. Astrophys. J. 536, 571–583 (2000).
doi: 10.1086/308947
Brammer, G. B., van Dokkum, P. G. & Coppi, P. EAZY: a fast, public photometric redshift code. Astrophys. J. 686, 1503–1513 (2008).
doi: 10.1086/591786
Kawamata, R. et al. Size–luminosity relations and UV luminosity functions at z = 6–9 simultaneously derived from the complete Hubble Frontier Fields data. Astrophys. J. 855, 4 (2018).
doi: 10.3847/1538-4357/aaa6cf
Kawamata, R., Oguri, M., Ishigaki, M., Shimasaku, K. & Ouchi, M. Precise strong lensing mass modeling of four Hubble Frontier Field clusters and a sample of magnified high-redshift galaxies. Astrophys. J. 819, 114 (2016).
doi: 10.3847/0004-637X/819/2/114
Oguri, M. The mass distribution of SDSS J1004.4112 revisited. Publ Astron. Soc. Jpn 62, 1017–1024 (2010).
doi: 10.1093/pasj/62.4.1017
Oguri, M. Fast calculation of gravitational lensing properties of elliptical Navarro–Frenk–White and Hernquist density profiles. Publ. Astron. Soc. Pacif. 133, 074504 (2021).
doi: 10.1088/1538-3873/ac12db
Nakar, E. & Sari, R. Early supernovae light curves following the shock breakout. Astrophys. J. 725, 904–921 (2010).
doi: 10.1088/0004-637X/725/1/904
Rabinak, I. & Waxman, E. The early UV/optical emission from core-collapse supernovae. Astrophys. J. 728, 63 (2011); erratum 770, 81 (2013).
doi: 10.1088/0004-637X/728/1/63
Nakar, E. & Piro, A. L. Supernovae with two peaks in the optical light curve and the signature of progenitors with low-mass extended envelopes. Astrophys. J. 788, 193 (2014).
doi: 10.1088/0004-637X/788/2/193
Piro, A. L. Using double-peaked supernova light curves to study extended material. Astrophys. J. Lett. 808, L51 (2015).
doi: 10.1088/2041-8205/808/2/L51
Sapir, N. & Waxman, E. UV/optical emission from the expanding envelopes of type II supernovae. Astrophys. J. 838, 130 (2017).
doi: 10.3847/1538-4357/aa64df
Morozova, V., Piro, A. L. & Valenti, S. Unifying type II supernova light curves with dense circumstellar material. Astrophys. J. 838, 28 (2017).
doi: 10.3847/1538-4357/aa6251
Morozova, V., Piro, A. L. & Valenti, S. Measuring the progenitor masses and dense circumstellar material of type II supernovae. Astrophys. J. 858, 15 (2018).
doi: 10.3847/1538-4357/aab9a6
Margalit, B. Analytic light curves of dense CSM shock breakout and cooling. Astrophys. J. 933, 238 (2022).
doi: 10.3847/1538-4357/ac771a
Kass, R. E. & Raftery, A. E. Bayes factors. J. Am. Stat. Assoc. 90, 773–795 (1995).
doi: 10.1080/01621459.1995.10476572
Li, W. et al. Nearby supernova rates from the Lick Observatory Supernova Search – II. The observed luminosity functions and fractions of supernovae in a complete sample. Mon. Not. R. Astron. Soc 412, 1441–1472 (2011).
doi: 10.1111/j.1365-2966.2011.18160.x
Kelly, P. L. et al. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens. Science 347, 1123–1126 (2015).
doi: 10.1126/science.aaa3350
Goobar, A. et al. iPTF16geu: a multiply imaged, gravitationally lensed type Ia supernova. Science 356, 291–295 (2017).
pubmed: 28428419 doi: 10.1126/science.aal2729
Rodney, S. A. et al. A gravitationally lensed supernova with an observable two-decade time delay. Nat. Astron. 5, 1118–1125 (2021).
Oguri, M. Strong gravitational lensing of explosive transients. Rep. Prog. Phys. 82, 126901 (2019).
pubmed: 31634885 doi: 10.1088/1361-6633/ab4fc5
Foxley-Marrable, M. et al. Observing the earliest moments of supernovae using strong gravitational lenses. Mon. Not. R. Astron. Soc 495, 4622–4637 (2020).
doi: 10.1093/mnras/staa1289
Grogin, N. A. et al. CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey. Astrophys. J. Suppl. Ser. 197, 35 (2011).
doi: 10.1088/0067-0049/197/2/35
Postman, M. et al. The cluster lensing and supernova survey with Hubble: an overview. Astrophys. J. Suppl. Ser. 199, 25 (2012).
doi: 10.1088/0067-0049/199/2/25
Strolger, L. G. et al. The rate of core collapse supernovae to redshift 2.5 from the CANDELS and CLASH supernova surveys. Astrophys. J. 813, 93 (2015).
doi: 10.1088/0004-637X/813/2/93
Schmidt, B. P. et al. The distance of five type II supernovae using the expanding photosphere method and the value of H
doi: 10.1086/174546
Hamuy, M. & Pinto, P. A. Type II supernovae as standardized candles. Astrophys. J. 566, L63–L66 (2002).
doi: 10.1086/339676
Kelly, P. L. & Kirshner, R. P. Core-collapse supernovae and host galaxy stellar populations. Astrophys. J. 759, 107 (2012).
doi: 10.1088/0004-637X/759/2/107
Drout, M. R. et al. The first systematic study of type Ibc supernova multi-band light curves. Astron. J. 741, 97 (2011); erratum 753, 180 (2012).
doi: 10.1088/0004-637X/741/2/97
Prentice, S. J. et al. The bolometric light curves and physical parameters of stripped-envelope supernovae. Mon. Not. R. Astron. Soc 458, 2973–3002 (2016).
doi: 10.1093/mnras/stw299
Madau, P. & Dickinson, M. Cosmic star-formation history. Annu. Rev. Astron. Astrophys. 52, 415–486 (2014).
doi: 10.1146/annurev-astro-081811-125615
Salpeter, E. D. The luminosity function and stellar evolution. Astrophys. J. 121, 161–167 (1955).
doi: 10.1086/145971
Fruchter, A. S., Hack, W., Dencheva, M., Droettboom, M., & Greenfield, P. BetaDrizzle: a redesign of the MultiDrizzle package. In 2010 Space Telescope Science Institute Calibration Workshop (eds Deustua, S. & Oliveira, C.) 382–387 (Space Telescope Science Institute, 2010).
Jones, D. O., Scolnic, D. M., & Rodney, S. A. PythonPhot: simple DAOPHOT-type photometry in Python. Astrophysics Source Code Library https://www.ascl.net/1501.010 (2015).
Stetson, P. B. DAOPHOT: a computer program for crowded-field stellar photometry. Publ. Astron. Soc. Pacif. 99, 191–222 (1987).
doi: 10.1086/131977
Peng, C. Y., Ho, L. C., Impey, C. D. & Rix, H.-W. Detailed structural decomposition of galaxy images. Astron. J. 124, 266–293 (2002).
doi: 10.1086/340952
Dong, S. et al. ASASSN-15lh: a highly super-luminous supernova. Science 351, 257–260 (2016).
pubmed: 26816375 doi: 10.1126/science.aac9613
Bradač, M. et al. Hubble Frontier Field photometric catalogues of Abell 370 and RXC J2248.7-4431: multiwavelength photometry, photometric redshifts, and stellar properties. Mon. Not. R. Astron. Soc. 489, 99–107 (2019).
Maraston, C. & Strömbäck, G. Stellar population models at high spectral resolution. Mon. Not. R. Astron. Soc 418, 2785–2811 (2011).
doi: 10.1111/j.1365-2966.2011.19738.x
Schulze, S. et al. The Palomar Transient Factory core-collapse supernova host-galaxy sample. I. Host-galaxy distribution functions and environment dependence of core-collapse supernovae. Astron. J. Suppl. Ser. 255, 29 (2021).
doi: 10.3847/1538-4365/abff5e
Schmidt, G. D., Weymann, R. J. & Foltz, C. B. A moderate-resolution, high-throughput CCD channel for the MMT spectrograph. Publ. Astron. Soc. Pacif. 101, 713–724 (1989).
doi: 10.1086/132495
Rothberg, B. et al. Current status of the facility instrumentation suite at the Large Binocular Telescope Observatory. In Proc. SPIE 10702: Ground-based and Airborne Instrumentation for Astronomy VII (eds Evans, C. J. et al.) 1070205 (SPIE, 2018).
McLean, I. S. et al. MOSFIRE, the multi-object spectrometer for infrared exploration at the Keck Observatory. In Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV (eds McLean, I. S. et al.) 84460J (SPIE, 2012).
Prochaska, J. X. et al. PypeIt: the Python spectroscopic data reduction pipeline. Preprint at https://arxiv.org/abs/2005.06505 (2020).
Prochaska, J. X. et al. pypeit/PypeIt: release 1.0.0. Zenodo https://doi.org/10.5281/zenodo.3743493 (2020).
Konidaris, N. & Steidel, C. MOSFIRE DRP https://keck-datareductionpipelines.github.io/MosfireDRP/#mosfire-drp (2018).
Wilkinson, D. M., Maraston, C., Goddard, D., Thomas, D. & Parikh, T. FIREFLY (Fitting IteRativEly For Likelihood analYsis): a full spectral fitting code. Mon. Not. R. Astron. Soc 472, 4297–4326 (2017).
doi: 10.1093/mnras/stx2215
Reddy, N. A. et al. The MOSDEF Survey: significant evolution in the rest-frame optical emission line equivalent widths of star-forming galaxies at z = 1.4–3.8. Astrophys. J. 869, 92 (2018).
doi: 10.3847/1538-4357/aaed1e
Keeton, C. R. On modeling galaxy-scale strong lens systems. Gen. Rel. Grav. 42, 2151–2176 (2010).
doi: 10.1007/s10714-010-1041-1
McCully, C., Keeton, C. R., Wong, K. C. & Zabludoff, A. I. A new hybrid framework to efficiently model lines of sight to gravitational lenses. Mon. Not. R. Astron. Soc 443, 3631–3642 (2014).
doi: 10.1093/mnras/stu1316
Ammons, S. M., Wong, K. C., Zabludoff, A. I. & Keeton, C. R. Mapping compound cosmic telescopes containing multiple projected cluster-scale halos. Astron. J. 781, 2 (2014).
doi: 10.1088/0004-637X/781/1/2
Johnson, T. L. et al. Lens models and magnification maps of the six Hubble Frontier Fields clusters. Astron. J. 797, 48 (2014).
doi: 10.1088/0004-637X/797/1/48
Jullo, E. et al. A Bayesian approach to strong lensing modelling of galaxy clusters. New J. Phys. 9, 447 (2007).
doi: 10.1088/1367-2630/9/12/447
Faber, S. M. & Jackson, R. E. Velocity dispersions and mass-to-light ratios for elliptical galaxies. Astrophys. J. 204, 668–683 (1976).
doi: 10.1086/154215
Witt, H. J. & Mao, S. On the magnification relations in quadruple lenses: a moment approach. Mon. Not. R. Astron. Soc 311, 689–697 (2000).
doi: 10.1046/j.1365-8711.2000.03122.x
Drout, M. R. et al. Rapidly evolving and luminous transients from Pan-STARRS1. Astrophys. J. 794, 23 (2014).
doi: 10.1088/0004-637X/794/1/23
Ho, A. Y. Q. et al. AT2018cow: a luminous millimeter transient. Astrophys. J. 871, 73 (2019); erratum 935, 62 (2022).
doi: 10.3847/1538-4357/aaf473
Margutti, R. et al. An embedded X-ray source shines through the aspherical AT2018cow: revealing the inner workings of the most luminous fast-evolving optical transients. Astrophys. J. 872, 18 (2019).
doi: 10.3847/1538-4357/aafa01
Foreman-Mackey, D., Hogg, D. W., Lang, D. & Goodman, J. emcee: the MCMC hammer. Publ. Astron. Soc. Pacif. 125, 306–312 (2013).
doi: 10.1086/670067
Chen, W. Additional data for ‘Shock cooling of a red-supergiant supernova at redshift 3 in lensed images’. Zenodo https://doi.org/10.5281/zenodo.6725770 (2022).
Kriek, M. et al. An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z = 2.2. Astrophys. J. 700, 221–231 (2009).
doi: 10.1088/0004-637X/700/1/221
Schreiber, C. & Dickinson, H. FAST++ v1.3.1. GitHub https://github.com/cschreib/fastpp (2021).
Morishita, T. et al. Characterizing intracluster light in the Hubble Frontier Fields. Astrophys. J. 846, 139 (2017).
doi: 10.3847/1538-4357/aa8403
Diego, J. M. et al. Dark matter under the microscope: constraining compact dark matter with caustic crossing events. Astrophys. J. 857, 25 (2018).
doi: 10.3847/1538-4357/aab617
Menzies, J. W. et al. Spectroscopic and photometric observations of SN 1987a: the first 50 days. Mon. Not. R. Astron. Soc 227, 39P–49P (1987).
doi: 10.1093/mnras/227.1.39P
Hosseinzaden, G. et al. Weak mass loss from the red supergiant progenitor of the type II SN 2021yja. Preprint at https://arxiv.org/abs/2203.08155 (2022).
Bullivant, C. et al. SN 2013fs and SN 2013fr: exploring the circumstellar-material diversity in type II supernovae. Mon. Not. R. Astron. Soc 476, 1497–1518 (2018).
doi: 10.1093/mnras/sty045
Valenti, S. et al. The diversity of type II supernova versus the similarity in their progenitors. Mon. Not. R. Astron. Soc 459, 3939–3962 (2016).
doi: 10.1093/mnras/stw870
Ho, A. Y. Q. et al. SN 2020bvc: a broad-line type Ic supernova with a double-peaked optical light curve and a luminous X-ray and radio counterpart. Astrophys. J. 902, 86 (2020).
doi: 10.3847/1538-4357/aba630
Yang, Y. et al. The young and nearby normal type Ia supernova 2018gv: UV–optical observations and the earliest spectropolarimetry. Astrophys. J. 902, 46 (2020).
doi: 10.3847/1538-4357/aba759
Ho, A. Y. Q. et al. The Koala: a fast blue optical transient with luminous radio emission from a starburst dwarf galaxy at z = 0.27. Astrophys. J. 895, 49 (2020).
doi: 10.3847/1538-4357/ab8bcf
Richardson, D., Jenkins, R. L. III, Wright, J. & Maddox, L. Absolute-magnitude distributions of supernovae. Astrophys. J. 147, 118 (2014).
Taylor, M. et al. The core collapse supernova rate from the SDSS-II supernova survey. Astrophys. J. 792, 135 (2014).
doi: 10.1088/0004-637X/792/2/135
Hatano, K., Branch, D. & Deaton, J. Extinction and radial distribution of supernova properties in their parent galaxies. Astrophys. J. 502, 177–181 (1998).
doi: 10.1086/305903
Calzetti, D. et al. The dust content and opacity of actively star-forming galaxies. Astrophys. J. 533, 682–695 (2000).
doi: 10.1086/308692
Jeffreys, H. An invariant form for the prior probability in estimation problems. Proc. R. Soc. Lond. A 186, 453–461 (1946).
doi: 10.1098/rspa.1946.0056
Kelly, P. L. & Refsdal, S. N. et al. Classification as a luminous and blue SN 1987A-like type II supernova. Astrophys. J. 831, 205 (2016).
doi: 10.3847/0004-637X/831/2/205
Pastorello, A. et al. SN 2009E: a faint clone of SN 1987A. Astron. Astrophys. 537, A141 (2012).
doi: 10.1051/0004-6361/201118112
Taddia, F. et al. Long-rising type II supernovae from Palomar Transient Factory and Caltech Core-Collapse Project. Astron. Astrophys. 588, A5 (2016).
doi: 10.1051/0004-6361/201527811
Coe, D., Benítez, N., Broadhurst, T. & Moustakas, L. A. A high-resolution mass map of galaxy cluster substructure: LensPerfect analysis of A1689. Astrophys. J. 723, 1678 (2010).
doi: 10.1088/0004-637X/723/2/1678

Auteurs

Wenlei Chen (W)

School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA. chen6339@umn.edu.

Patrick L Kelly (PL)

School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA.

Masamune Oguri (M)

Center for Frontier Science, Chiba University, Chiba, Japan.
Research Center for the Early Universe, University of Tokyo, Tokyo, Japan.
Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), University of Tokyo, Chiba, Japan.

Thomas J Broadhurst (TJ)

Department of Theoretical Physics, University of the Basque Country UPV/EHU, Bilbao, Spain.
DIPC, Basque Country UPV/EHU, San Sebastian, Spain.
Ikerbasque, Basque Foundation for Science, Bilbao, Spain.

Jose M Diego (JM)

IFCA, Instituto de Física de Cantabria (UC-CSIC), Santander, Spain.

Najmeh Emami (N)

School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA.

Alexei V Filippenko (AV)

Department of Astronomy, University of California, Berkeley, CA, USA.

Tommaso L Treu (TL)

Department of Physics and Astronomy, University of California, Los Angeles, CA, USA.

Adi Zitrin (A)

Physics Department, Ben-Gurion University of the Negev, Beer-Sheva, Israel.

Classifications MeSH