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

Research output: Contribution to journal › Article › peer-review

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 (US)
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

Keywords

supernovae: general
surveys

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1093/mnras/stad056

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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

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

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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 (US)",

volume = "520",

pages = "684--701",

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

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

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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

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U2 - 10.1093/mnras/stad056

DO - 10.1093/mnras/stad056

M3 - Article

AN - SCOPUS:85161538843

SN - 0035-8711

VL - 520

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EP - 701

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

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ER -

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

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