Core-collapse supernovae in the Dark Energy Survey: luminosity functions and host galaxy demographics

M. Grayling; C. P. Gutiérrez; M. Sullivan; P. Wiseman; M. Vincenzi; L. Galbany; A. Möller; D. Brout; T. M. Davis; C. Frohmaier; O. Graur; L. Kelsey; C. Lidman; B. Popovic; M. Smith; M. Toy; B. E. Tucker; Z. Zontos; T. M.C. Abbott; M. Aguena; S. Allam; F. Andrade-Oliveira; J. Annis; J. Asorey; D. Bacon; E. Bertin; S. Bocquet; D. Brooks; A. Carnero Rosell; D. Carollo; M. Carrasco Kind; J. Carretero; M. Costanzi; L. N. da Costa; M. E.S. Pereira; J. De Vicente; S. Desai; H. T. Diehl; P. Doel; S. Everett; I. Ferrero; D. Friedel; J. Frieman; J. García-Bellido; M. Gatti; D. Gruen; J. Gschwend; G. Gutierrez; S. R. Hinton; D. L. Hollowood; K. Honscheid; D. J. James; K. Kuehn; N. Kuropatkin; G. F. Lewis; U. Malik; M. March; F. Menanteau; R. Miquel; R. Morgan; R. L.C. Ogando; A. Palmese; F. Paz-Chinchón; A. Pieres; A. A.Plazas Malagón; M. Rodriguez-Monroy; A. K. Romer; A. Roodman; E. Sanchez; V. Scarpine; I. Sevilla-Noarbe; E. Suchyta; G. Tarle; C. To; D. L. Tucker; T. N. Varga

doi:10.1093/mnras/stad056

Core-collapse supernovae in the Dark Energy Survey: luminosity functions and host galaxy demographics

M. Grayling, C. P. Gutiérrez, M. Sullivan, P. Wiseman, M. Vincenzi, L. Galbany, A. Möller, D. Brout, T. M. Davis, C. Frohmaier, O. Graur, L. Kelsey, C. Lidman, B. Popovic, M. Smith, M. Toy, B. E. Tucker, Z. Zontos, T. M.C. Abbott, M. AguenaS. Allam, F. Andrade-Oliveira, J. Annis, J. Asorey, D. Bacon, E. Bertin, S. Bocquet, D. Brooks, A. Carnero Rosell, D. Carollo, M. Carrasco Kind, J. Carretero, M. Costanzi, L. N. da Costa, M. E.S. Pereira, J. De Vicente, S. Desai, H. T. Diehl, P. Doel, S. Everett, I. Ferrero, D. Friedel, J. Frieman, J. García-Bellido, M. Gatti, D. Gruen, J. Gschwend, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, K. Kuehn, N. Kuropatkin, G. F. Lewis, U. Malik, M. March, F. Menanteau, R. Miquel, R. Morgan, R. L.C. Ogando, A. Palmese, F. Paz-Chinchón, A. Pieres, A. A.Plazas Malagón, M. Rodriguez-Monroy, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, I. Sevilla-Noarbe, E. Suchyta, G. Tarle, C. To, D. L. Tucker, T. N. Varga

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Abstract

We present the luminosity functions and host galaxy properties of the Dark Energy Survey (DES) core-collapse supernova (CCSN) sample, consisting of 69 Type II and 50 Type Ibc spectroscopically and photometrically confirmed supernovae over a redshift range 0.045 < z < 0.25. We fit the observed DES griz CCSN light curves and K-correct to produce rest-frame R-band light curves. We compare the sample with lower redshift CCSN samples from Zwicky Transient Facility (ZTF) and Lick Observatory Supernova Search (LOSS). Comparing luminosity functions, the DES and ZTF samples of SNe II are brighter than that of LOSS with significances of 3.0σ and 2.5σ, respectively. While this difference could be caused by redshift evolution in the luminosity function, simpler explanations such as differing levels of host extinction remain a possibility. We find that the host galaxies of SNe II in DES are on average bluer than in ZTF, despite having consistent stellar mass distributions. We consider a number of possibilities to explain this – including galaxy evolution with redshift, selection biases in either the DES or ZTF samples, and systematic differences due to the different photometric bands available – but find that none can easily reconcile the differences in host colour between the two samples and thus its cause remains uncertain.

Original language	English
Pages (from-to)	684-701
Number of pages	18
Journal	Monthly Notices of the Royal Astronomical Society
Volume	520
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stad056
State	Published - Mar 1 2023

Funding

The DES data management system is supported by the National Science Foundation under Grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2015-71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA programme of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. The United States Government retains and the publisher, by accepting the article for publication, acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. Funding for the SDSS-IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. This work was supported by the Science and Technology Facilities Council (grant number ST/P006760/1) through the DISCnet Centre for Doctoral Training. MS acknowledges support from EU/FP7-ERC grant 615929. PW acknowledges support from the Science and Technology Facilities Council (STFC) grant ST/R000506/1. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.

Funders	Funder number
Brazilian Instituto Nacional de Ciência e Tecnologia
Collaborating Institutions in the Dark Energy Survey
DISCnet Centre for Doctoral Training	ST/R000506/1
Fermi Research Alliance, LLC	DE-AC02-07CH11359
Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University
Science and Technology Facilities Council of the United Kingdom
National Science Foundation	AST-1138766, AST-1536171
U.S. Department of Energy
Alfred P. Sloan Foundation
Office of Science
High Energy Physics
Ohio State University
University of Chicago
National Centre for Supercomputing Applications
Seventh Framework Programme
Higher Education Funding Council for England
Science and Technology Facilities Council	ST/P006760/1
European Commission
European Research Council	240672, 306478, 291329
Deutsche Forschungsgemeinschaft
Generalitat de Catalunya
Ministerio de Economía y Competitividad	SEV-2016-0588, SEV-2016-0597, ESP2015-66861, MDM-2015-0509, FPA2015-68048, AYA2015-71825
Ministério da Ciência, Tecnologia e Inovação
Conselho Nacional de Desenvolvimento Científico e Tecnológico	465376/2014-2
Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
Financiadora de Estudos e Projetos
Instituto Nacional de Ciência e Tecnologia para Excitotoxicidade e Neuroproteção
Ministry of Education and Science of Ukraine
European Regional Development Fund

Keywords

supernovae: general
surveys

Access to Document

10.1093/mnras/stad056

Cite this

Grayling, M., Gutiérrez, C. P., Sullivan, M., Wiseman, P., Vincenzi, M., Galbany, L., Möller, A., Brout, D., Davis, T. M., Frohmaier, C., Graur, O., Kelsey, L., Lidman, C., Popovic, B., Smith, M., Toy, M., Tucker, B. E., Zontos, Z., Abbott, T. M. C., ... Varga, T. N. (2023). Core-collapse supernovae in the Dark Energy Survey: luminosity functions and host galaxy demographics. Monthly Notices of the Royal Astronomical Society, 520(1), 684-701. https://doi.org/10.1093/mnras/stad056

@article{4980ffb465cf45eebde8121cbdc24730,

title = "Core-collapse supernovae in the Dark Energy Survey: luminosity functions and host galaxy demographics",

abstract = "We present the luminosity functions and host galaxy properties of the Dark Energy Survey (DES) core-collapse supernova (CCSN) sample, consisting of 69 Type II and 50 Type Ibc spectroscopically and photometrically confirmed supernovae over a redshift range 0.045 < z < 0.25. We fit the observed DES griz CCSN light curves and K-correct to produce rest-frame R-band light curves. We compare the sample with lower redshift CCSN samples from Zwicky Transient Facility (ZTF) and Lick Observatory Supernova Search (LOSS). Comparing luminosity functions, the DES and ZTF samples of SNe II are brighter than that of LOSS with significances of 3.0σ and 2.5σ, respectively. While this difference could be caused by redshift evolution in the luminosity function, simpler explanations such as differing levels of host extinction remain a possibility. We find that the host galaxies of SNe II in DES are on average bluer than in ZTF, despite having consistent stellar mass distributions. We consider a number of possibilities to explain this – including galaxy evolution with redshift, selection biases in either the DES or ZTF samples, and systematic differences due to the different photometric bands available – but find that none can easily reconcile the differences in host colour between the two samples and thus its cause remains uncertain.",

keywords = "supernovae: general, surveys",

author = "M. Grayling and Guti{\'e}rrez, {C. P.} and M. Sullivan and P. Wiseman and M. Vincenzi and L. Galbany and A. M{\"o}ller and D. Brout and Davis, {T. M.} and C. Frohmaier and O. Graur and L. Kelsey and C. Lidman and B. Popovic and M. Smith and M. Toy and Tucker, {B. E.} and Z. Zontos and Abbott, {T. M.C.} and M. Aguena and S. Allam and F. Andrade-Oliveira and J. Annis and J. Asorey and D. Bacon and E. Bertin and S. Bocquet and D. Brooks and Rosell, {A. Carnero} and D. Carollo and Kind, {M. Carrasco} and J. Carretero and M. Costanzi and {da Costa}, {L. N.} and Pereira, {M. E.S.} and {De Vicente}, J. and S. Desai and Diehl, {H. T.} and P. Doel and S. Everett and I. Ferrero and D. Friedel and J. Frieman and J. Garc{\'i}a-Bellido and M. Gatti and D. Gruen and J. Gschwend and G. Gutierrez and Hinton, {S. R.} and Hollowood, {D. L.} and K. Honscheid and James, {D. J.} and K. Kuehn and N. Kuropatkin and Lewis, {G. F.} and U. Malik and M. March and F. Menanteau and R. Miquel and R. Morgan and Ogando, {R. L.C.} and A. Palmese and F. Paz-Chinch{\'o}n and A. Pieres and Malag{\'o}n, {A. A.Plazas} and M. Rodriguez-Monroy and Romer, {A. K.} and A. Roodman and E. Sanchez and V. Scarpine and I. Sevilla-Noarbe and E. Suchyta and G. Tarle and C. To and Tucker, {D. L.} and Varga, {T. N.}",

note = "Publisher Copyright: {\textcopyright} 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.",

year = "2023",

month = mar,

day = "1",

doi = "10.1093/mnras/stad056",

language = "English",

volume = "520",

pages = "684--701",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

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Grayling, M, Gutiérrez, CP, Sullivan, M, Wiseman, P, Vincenzi, M, Galbany, L, Möller, A, Brout, D, Davis, TM, Frohmaier, C, Graur, O, Kelsey, L, Lidman, C, Popovic, B, Smith, M, Toy, M, Tucker, BE, Zontos, Z, Abbott, TMC, Aguena, M, Allam, S, Andrade-Oliveira, F, Annis, J, Asorey, J, Bacon, D, Bertin, E, Bocquet, S, Brooks, D, Rosell, AC, Carollo, D, Kind, MC, Carretero, J, Costanzi, M, da Costa, LN, Pereira, MES, De Vicente, J, Desai, S, Diehl, HT, Doel, P, Everett, S, Ferrero, I, Friedel, D, Frieman, J, García-Bellido, J, Gatti, M, Gruen, D, Gschwend, J, Gutierrez, G, Hinton, SR, Hollowood, DL, Honscheid, K, James, DJ, Kuehn, K, Kuropatkin, N, Lewis, GF, Malik, U, March, M, Menanteau, F, Miquel, R, Morgan, R, Ogando, RLC, Palmese, A, Paz-Chinchón, F, Pieres, A, Malagón, AAP, Rodriguez-Monroy, M, Romer, AK, Roodman, A, Sanchez, E, Scarpine, V, Sevilla-Noarbe, I, Suchyta, E, Tarle, G, To, C, Tucker, DL & Varga, TN 2023, 'Core-collapse supernovae in the Dark Energy Survey: luminosity functions and host galaxy demographics', Monthly Notices of the Royal Astronomical Society, vol. 520, no. 1, pp. 684-701. https://doi.org/10.1093/mnras/stad056

TY - JOUR

T1 - Core-collapse supernovae in the Dark Energy Survey

T2 - luminosity functions and host galaxy demographics

AU - Grayling, M.

AU - Gutiérrez, C. P.

AU - Sullivan, M.

AU - Wiseman, P.

AU - Vincenzi, M.

AU - Galbany, L.

AU - Möller, A.

AU - Brout, D.

AU - Davis, T. M.

AU - Frohmaier, C.

AU - Graur, O.

AU - Kelsey, L.

AU - Lidman, C.

AU - Popovic, B.

AU - Smith, M.

AU - Toy, M.

AU - Tucker, B. E.

AU - Zontos, Z.

AU - Abbott, T. M.C.

AU - Aguena, M.

AU - Allam, S.

AU - Andrade-Oliveira, F.

AU - Annis, J.

AU - Asorey, J.

AU - Bacon, D.

AU - Bertin, E.

AU - Bocquet, S.

AU - Brooks, D.

AU - Rosell, A. Carnero

AU - Carollo, D.

AU - Kind, M. Carrasco

AU - Carretero, J.

AU - Costanzi, M.

AU - da Costa, L. N.

AU - Pereira, M. E.S.

AU - De Vicente, J.

AU - Desai, S.

AU - Diehl, H. T.

AU - Doel, P.

AU - Everett, S.

AU - Ferrero, I.

AU - Friedel, D.

AU - Frieman, J.

AU - García-Bellido, J.

AU - Gatti, M.

AU - Gruen, D.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Hinton, S. R.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - James, D. J.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lewis, G. F.

AU - Malik, U.

AU - March, M.

AU - Menanteau, F.

AU - Miquel, R.

AU - Morgan, R.

AU - Ogando, R. L.C.

AU - Palmese, A.

AU - Paz-Chinchón, F.

AU - Pieres, A.

AU - Malagón, A. A.Plazas

AU - Rodriguez-Monroy, M.

AU - Romer, A. K.

AU - Roodman, A.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Sevilla-Noarbe, I.

AU - Suchyta, E.

AU - Tarle, G.

AU - To, C.

AU - Tucker, D. L.

AU - Varga, T. N.

PY - 2023/3/1

Y1 - 2023/3/1

N2 - We present the luminosity functions and host galaxy properties of the Dark Energy Survey (DES) core-collapse supernova (CCSN) sample, consisting of 69 Type II and 50 Type Ibc spectroscopically and photometrically confirmed supernovae over a redshift range 0.045 < z < 0.25. We fit the observed DES griz CCSN light curves and K-correct to produce rest-frame R-band light curves. We compare the sample with lower redshift CCSN samples from Zwicky Transient Facility (ZTF) and Lick Observatory Supernova Search (LOSS). Comparing luminosity functions, the DES and ZTF samples of SNe II are brighter than that of LOSS with significances of 3.0σ and 2.5σ, respectively. While this difference could be caused by redshift evolution in the luminosity function, simpler explanations such as differing levels of host extinction remain a possibility. We find that the host galaxies of SNe II in DES are on average bluer than in ZTF, despite having consistent stellar mass distributions. We consider a number of possibilities to explain this – including galaxy evolution with redshift, selection biases in either the DES or ZTF samples, and systematic differences due to the different photometric bands available – but find that none can easily reconcile the differences in host colour between the two samples and thus its cause remains uncertain.

AB - We present the luminosity functions and host galaxy properties of the Dark Energy Survey (DES) core-collapse supernova (CCSN) sample, consisting of 69 Type II and 50 Type Ibc spectroscopically and photometrically confirmed supernovae over a redshift range 0.045 < z < 0.25. We fit the observed DES griz CCSN light curves and K-correct to produce rest-frame R-band light curves. We compare the sample with lower redshift CCSN samples from Zwicky Transient Facility (ZTF) and Lick Observatory Supernova Search (LOSS). Comparing luminosity functions, the DES and ZTF samples of SNe II are brighter than that of LOSS with significances of 3.0σ and 2.5σ, respectively. While this difference could be caused by redshift evolution in the luminosity function, simpler explanations such as differing levels of host extinction remain a possibility. We find that the host galaxies of SNe II in DES are on average bluer than in ZTF, despite having consistent stellar mass distributions. We consider a number of possibilities to explain this – including galaxy evolution with redshift, selection biases in either the DES or ZTF samples, and systematic differences due to the different photometric bands available – but find that none can easily reconcile the differences in host colour between the two samples and thus its cause remains uncertain.

KW - supernovae: general

KW - surveys

UR - http://www.scopus.com/inward/record.url?scp=85161538843&partnerID=8YFLogxK

U2 - 10.1093/mnras/stad056

DO - 10.1093/mnras/stad056

M3 - Article

AN - SCOPUS:85161538843

SN - 0035-8711

VL - 520

SP - 684

EP - 701

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

Core-collapse supernovae in the Dark Energy Survey: luminosity functions and host galaxy demographics

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