Near-infrared Supernova Ia Distances: Host Galaxy Extinction and Mass-step Corrections Revisited
Abstract
We present optical and near-infrared (NIR, Y-, J-, H-band) observations of 42 Type Ia supernovae (SNe Ia) discovered by the untargeted intermediate Palomar Transient Factory survey. This new data set covers a broad range of redshifts and host galaxy stellar masses, compared to previous SN Ia efforts in the NIR. We construct a sample, using also literature data at optical and NIR wavelengths, to examine claimed correlations between the host stellar masses and the Hubble diagram residuals. The SN magnitudes are corrected for host galaxy extinction using either a global total-to-selective extinction ratio, RV = 2.0, for all SNe, or a best-fit RV for each SN individually. Unlike previous studies that were based on a narrower range in host stellar mass, we do not find evidence for a "mass step," between the color- and stretch-corrected peak J and H magnitudes for galaxies below and above $$\mathrm{log}({M}_{* }/{M}_{\odot })=10$$. However, the mass step remains significant (3σ) at optical wavelengths (g, r, i) when using a global RV, but vanishes when each SN is corrected using their individual best-fit RV. Our study confirms the benefits of the NIR SN Ia distance estimates, as these are largely exempted from the empirical corrections dominating the systematic uncertainties in the optical.
- Authors:
-
[1];
[2];
[3];
[1];
[1];
[4];
[5];
[7];
[7];
[8];
[9];
[1];
[10];
[11];
[12];
[13];
[13];
[14]
- Stockholm Univ. (Sweden). Oskar Klein Centre
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland, College Park, MD (United States). Joint Space-Science Inst.
- Space Telescope Science Inst., Baltimore, MD (United States)
- Linköping Univ. (Sweden)
- Arizona State Univ., Tempe, AZ (United States)
- Univ. Nacional Autonoma de Mexico (UNAM), Mexico City (Mexico). Inst. de Astronomia
- California Institute of Technology (CalTech), Pasadena, CA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Univ. of Nova Gorica, Ajdovšc̆ina (Slovenia). Centre for Astrophysics and Cosmology
- California Institute of Technology (CalTech), Pasadena, CA (United States). Caltech Optical Observatories
- Univ. of California, Santa Barbara, CA (United States); Las Cumbres Observatory, Goleta, CA (United States)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Univ. of California, Santa Barbara, CA (United States); Las Cumbres Observatories, Goleta, CA (United States)
- Univ. of California, Davis, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); Swedish Research Council (SRC); Slovenian Research Agency; National Science Foundation (NSF)
- OSTI Identifier:
- 1863794
- Grant/Contract Number:
- AC02-05CH11231; 2016-03274; 2020-0344; I0-0033; P1-0031; J1-8136; Z1-1853; AST-1313484; AST-1911225; AST-1813176; AST-2008108
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 923; Journal Issue: 2; Journal ID: ISSN 0004-637X
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; supernovae; dust; extinction
Citation Formats
Johansson, J., Cenko, S. B., Fox, O. D., Dhawan, S., Goobar, A., Stanishev, V., Butler, N., Lee, W. H., Watson, A. M., Fremling, U. C., Kasliwal, M. M., Nugent, P. E., Petrushevska, T., Sollerman, J., Yan, L., Burke, J., Hosseinzadeh, G., Howell, D. A., McCully, C., and Valenti, S. Near-infrared Supernova Ia Distances: Host Galaxy Extinction and Mass-step Corrections Revisited. United States: N. p., 2021.
Web. doi:10.3847/1538-4357/ac2f9e.
Johansson, J., Cenko, S. B., Fox, O. D., Dhawan, S., Goobar, A., Stanishev, V., Butler, N., Lee, W. H., Watson, A. M., Fremling, U. C., Kasliwal, M. M., Nugent, P. E., Petrushevska, T., Sollerman, J., Yan, L., Burke, J., Hosseinzadeh, G., Howell, D. A., McCully, C., & Valenti, S. Near-infrared Supernova Ia Distances: Host Galaxy Extinction and Mass-step Corrections Revisited. United States. https://doi.org/10.3847/1538-4357/ac2f9e
Johansson, J., Cenko, S. B., Fox, O. D., Dhawan, S., Goobar, A., Stanishev, V., Butler, N., Lee, W. H., Watson, A. M., Fremling, U. C., Kasliwal, M. M., Nugent, P. E., Petrushevska, T., Sollerman, J., Yan, L., Burke, J., Hosseinzadeh, G., Howell, D. A., McCully, C., and Valenti, S. Fri .
"Near-infrared Supernova Ia Distances: Host Galaxy Extinction and Mass-step Corrections Revisited". United States. https://doi.org/10.3847/1538-4357/ac2f9e. https://www.osti.gov/servlets/purl/1863794.
@article{osti_1863794,
title = {Near-infrared Supernova Ia Distances: Host Galaxy Extinction and Mass-step Corrections Revisited},
author = {Johansson, J. and Cenko, S. B. and Fox, O. D. and Dhawan, S. and Goobar, A. and Stanishev, V. and Butler, N. and Lee, W. H. and Watson, A. M. and Fremling, U. C. and Kasliwal, M. M. and Nugent, P. E. and Petrushevska, T. and Sollerman, J. and Yan, L. and Burke, J. and Hosseinzadeh, G. and Howell, D. A. and McCully, C. and Valenti, S.},
abstractNote = {We present optical and near-infrared (NIR, Y-, J-, H-band) observations of 42 Type Ia supernovae (SNe Ia) discovered by the untargeted intermediate Palomar Transient Factory survey. This new data set covers a broad range of redshifts and host galaxy stellar masses, compared to previous SN Ia efforts in the NIR. We construct a sample, using also literature data at optical and NIR wavelengths, to examine claimed correlations between the host stellar masses and the Hubble diagram residuals. The SN magnitudes are corrected for host galaxy extinction using either a global total-to-selective extinction ratio, RV = 2.0, for all SNe, or a best-fit RV for each SN individually. Unlike previous studies that were based on a narrower range in host stellar mass, we do not find evidence for a "mass step," between the color- and stretch-corrected peak J and H magnitudes for galaxies below and above $\mathrm{log}({M}_{* }/{M}_{\odot })=10$. However, the mass step remains significant (3σ) at optical wavelengths (g, r, i) when using a global RV, but vanishes when each SN is corrected using their individual best-fit RV. Our study confirms the benefits of the NIR SN Ia distance estimates, as these are largely exempted from the empirical corrections dominating the systematic uncertainties in the optical.},
doi = {10.3847/1538-4357/ac2f9e},
journal = {The Astrophysical Journal},
number = 2,
volume = 923,
place = {United States},
year = {Fri Dec 24 00:00:00 EST 2021},
month = {Fri Dec 24 00:00:00 EST 2021}
}
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The Carnegie Supernova Project-I: Correlation between Type Ia Supernovae and Their Host Galaxies from Optical to Near-infrared Bands
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Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
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The First Data Release from SweetSpot: 74 Supernovae in 36 Nights on WIYN+WHIRC
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