The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample
Abstract
Analyses of Type Ia supernovae (SNe Ia) have found puzzling correlations between their standardized luminosities and host galaxy properties: SNe Ia in high-mass, passive hosts appear brighter than those in lower mass, star-forming hosts. We examine the host galaxies of SNe Ia in the Dark Energy Survey 3-yr spectroscopically confirmed cosmological sample, obtaining photometry in a series of ‘local’ apertures centred on the SN, and for the global host galaxy. Here, we study the differences in these host galaxy properties, such as stellar mass and rest-frame U – R colours, and their correlations with SN Ia parameters including Hubble residuals. We find all Hubble residual steps to be >3σ in significance, both for splitting at the traditional environmental property sample median and for the step of maximum significance. For stellar mass, we find a maximal local step of 0.098 ± 0.018 mag; ~0.03 mag greater than the largest global stellar mass step in our sample (0.070 ± 0.017 mag). When splitting at the sample median, differences between local and global U – R steps are small, both ~0.08 mag, but are more significant than the global stellar mass step (0.057 ± 0.017 mag). We split the data into sub-samples basedmore »
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- School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK;DISCnet Centre for Doctoral Training, University of Southampton, Southampton SO17 1BJ, UK
- School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
- School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK;Université de Lyon, Université de Lyon 1, Villeurbanne; CNRS/IN2P3, Institut de Physique des Deux Infinis, F-69622 Lyon, France
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA;Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
- Departamento de Física Teórica y del Cosmos, Universidad de Granada, E-18071 Granada, Spain
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA;Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
- Centre for Gravitational Astrophysics, College of Science, The Australian National University, Canberra, ACT 2601, Australia;The Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2601, Australia
- Université Clermont Auvergne, CNRS/IN2P3, LPC, F-63000 Clermont-Ferrand, France
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA
- Department of Physics, Duke University Durham, Durham, NC 27708, USA
- McDonald Observatory, The University of Texas at Austin, Fort Davis, TX 79734, USA
- Cerro Tololo Inter-American Observatory, NSF’s National Optical-Infrared Astronomy Research Laboratory, Casilla 603 La Serena, Chile
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil;Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro RJ-20921-400, Brazil
- Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
- CNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014 Paris, France;Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris, F-75014 Paris, France
- Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK
- Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA;SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
- Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain;Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA;National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
- Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Barcelona, Spain
- Institut d’Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain;Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
- INAF – Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy;Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy
- Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro RJ-20921-400, Brazil;Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro RJ - 20921-400, Brazil
- Department of Physics, IIT Hyderabad, Kandi 502285, India
- Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
- Institute of Theoretical Astrophysics, University of Oslo. P.O. Box 1029 Blindern, NO-0315 Oslo, Norway
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA
- Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA;Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA;Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA;SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA;Department of Physics, The Ohio State University, Columbus, OH 43210, USA
- Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
- Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA
- Australian Astronomical Optics, Macquarie University, North Ryde, NSW 2113, Australia;Lowell Observatory, 1400 Mars Hill Rd, Flagstaff, AZ 86001, USA
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA;Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA;Radcliffe Institute for Advanced Study, Harvard University, Cambridge, MA 02138, USA
- Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain;Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Barcelona, Spain
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, WI 53706-1390, USA
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain;Centre for Gravitational Astrophysics, College of Science, The Australian National University, Canberra, ACT 2601, Australia
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK;National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, UK
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Av. Complutense 40, E-28040, Madrid, Spain
- Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
- Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
- SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA;Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain;Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, D-85748 Garching, Germany;Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, D-81679 München, Germany
- Publication Date:
- Research Org.:
- Univ. of Michigan, Ann Arbor, MI (United States). Applied Physics Program; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Univ. of Chicago, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Basic Energy Sciences (BES)
- Contributing Org.:
- DES Collaboration
- OSTI Identifier:
- 1872384
- Alternate Identifier(s):
- OSTI ID: 1674993; OSTI ID: 1734756; OSTI ID: 1781656; OSTI ID: 1817471
- Report Number(s):
- FERMILAB-PUB-20-429-AE; DES-2019-0490; arXiv:2008.12101
Journal ID: ISSN 0035-8711; ST/P006760/1; ST/R000506/1; TRN: US2306876
- Grant/Contract Number:
- SC0019193; AC02-07CH11359; SC0009924; AC05-00OR22725; AC02-76SF00515; ST/R000506/1; ST/P006760/1
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 501; Journal Issue: 4; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; distance scale; supernovae: general; surveys
Citation Formats
Kelsey, L., Sullivan, M., Smith, M., Wiseman, P., Brout, D., Davis, T. M., Frohmaier, C., Galbany, L., Grayling, M., Gutiérrez, C. P., Hinton, S. R., Kessler, R., Lidman, C., Möller, A., Sako, M., Scolnic, D., Uddin, S. A., Vincenzi, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., Desai, S., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., Ferté, A., Flaugher, B., Fosalba, P., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Kim, A. G., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Marshall, J. L., Martini, P., Menanteau, F., Miquel, R., Morgan, R., Ogando, R. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sánchez, C., Sanchez, E., Serrano, S., Sevilla-Noarbe, I., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Walker, A. R., and Wilkinson, R. D. The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample. United States: N. p., 2020.
Web. doi:10.1093/mnras/staa3924.
Kelsey, L., Sullivan, M., Smith, M., Wiseman, P., Brout, D., Davis, T. M., Frohmaier, C., Galbany, L., Grayling, M., Gutiérrez, C. P., Hinton, S. R., Kessler, R., Lidman, C., Möller, A., Sako, M., Scolnic, D., Uddin, S. A., Vincenzi, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., Desai, S., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., Ferté, A., Flaugher, B., Fosalba, P., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Kim, A. G., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Marshall, J. L., Martini, P., Menanteau, F., Miquel, R., Morgan, R., Ogando, R. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sánchez, C., Sanchez, E., Serrano, S., Sevilla-Noarbe, I., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Walker, A. R., & Wilkinson, R. D. The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample. United States. https://doi.org/10.1093/mnras/staa3924
Kelsey, L., Sullivan, M., Smith, M., Wiseman, P., Brout, D., Davis, T. M., Frohmaier, C., Galbany, L., Grayling, M., Gutiérrez, C. P., Hinton, S. R., Kessler, R., Lidman, C., Möller, A., Sako, M., Scolnic, D., Uddin, S. A., Vincenzi, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., Desai, S., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., Ferté, A., Flaugher, B., Fosalba, P., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Kim, A. G., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Marshall, J. L., Martini, P., Menanteau, F., Miquel, R., Morgan, R., Ogando, R. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sánchez, C., Sanchez, E., Serrano, S., Sevilla-Noarbe, I., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Walker, A. R., and Wilkinson, R. D. Mon .
"The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample". United States. https://doi.org/10.1093/mnras/staa3924. https://www.osti.gov/servlets/purl/1872384.
@article{osti_1872384,
title = {The effect of environment on Type Ia supernovae in the Dark Energy Survey three-year cosmological sample},
author = {Kelsey, L. and Sullivan, M. and Smith, M. and Wiseman, P. and Brout, D. and Davis, T. M. and Frohmaier, C. and Galbany, L. and Grayling, M. and Gutiérrez, C. P. and Hinton, S. R. and Kessler, R. and Lidman, C. and Möller, A. and Sako, M. and Scolnic, D. and Uddin, S. A. and Vincenzi, M. and Abbott, T. C. and Aguena, M. and Allam, S. and Annis, J. and Avila, S. and Bacon, D. and Bertin, E. and Brooks, D. and Burke, D. L. and Carnero Rosell, A. and Carrasco Kind, M. and Carretero, J. and Castander, F. J. and Costanzi, M. and da Costa, L. N. and Desai, S. and Diehl, H. T. and Doel, P. and Everett, S. and Ferrero, I. and Ferté, A. and Flaugher, B. and Fosalba, P. and García-Bellido, J. and Gerdes, D. W. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Hollowood, D. L. and Honscheid, K. and James, D. J. and Kim, A. G. and Kuehn, K. and Kuropatkin, N. and Lahav, O. and Lima, M. and Marshall, J. L. and Martini, P. and Menanteau, F. and Miquel, R. and Morgan, R. and Ogando, R. C. and Palmese, A. and Paz-Chinchón, F. and Plazas, A. A. and Romer, A. K. and Sánchez, C. and Sanchez, E. and Serrano, S. and Sevilla-Noarbe, I. and Suchyta, E. and Tarle, G. and Thomas, D. and To, C. and Varga, T. N. and Walker, A. R. and Wilkinson, R. D.},
abstractNote = {Analyses of Type Ia supernovae (SNe Ia) have found puzzling correlations between their standardized luminosities and host galaxy properties: SNe Ia in high-mass, passive hosts appear brighter than those in lower mass, star-forming hosts. We examine the host galaxies of SNe Ia in the Dark Energy Survey 3-yr spectroscopically confirmed cosmological sample, obtaining photometry in a series of ‘local’ apertures centred on the SN, and for the global host galaxy. Here, we study the differences in these host galaxy properties, such as stellar mass and rest-frame U – R colours, and their correlations with SN Ia parameters including Hubble residuals. We find all Hubble residual steps to be >3σ in significance, both for splitting at the traditional environmental property sample median and for the step of maximum significance. For stellar mass, we find a maximal local step of 0.098 ± 0.018 mag; ~0.03 mag greater than the largest global stellar mass step in our sample (0.070 ± 0.017 mag). When splitting at the sample median, differences between local and global U – R steps are small, both ~0.08 mag, but are more significant than the global stellar mass step (0.057 ± 0.017 mag). We split the data into sub-samples based on SN Ia light-curve parameters: stretch (x1) and colour (c), finding that redder objects (c > 0) have larger Hubble residual steps, for both stellar mass and U – R, for both local and global measurements, of ~0.14 mag. Additionally, the bluer (star-forming) local environments host a more homogeneous SN Ia sample, with local U – R rms scatter as low as 0.084 ± 0.017 mag for blue (c < 0) SNe Ia in locally blue U – R environments.},
doi = {10.1093/mnras/staa3924},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 501,
place = {United States},
year = {Mon Dec 21 00:00:00 EST 2020},
month = {Mon Dec 21 00:00:00 EST 2020}
}
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