Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program
Abstract
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near infrared (NIR) is a promising way to significantly reduce the systematic errors, as the strategy minimizes our reliance on the empirical width-luminosity relation and uncertain dust laws. Observations in the NIR are also crucial for our understanding of the origins and evolution of these events, further improving their cosmological utility. Any future experiments in the rest-frame NIR will require knowledge of the SN Ia NIR spectroscopic diversity, which is currently based on a small sample of observed spectra. Along with the accompanying paper, Phillips et al., we introduce the Carnegie Supernova Project-II (CSP-II), to follow-up nearby SNe Ia in both the optical and the NIR. In particular, this paper focuses on the CSP-II NIR spectroscopy program, describing the survey strategy, instrumental setups, data reduction, sample characteristics, and future analyses on the data set. Here, in collaboration with the Harvard-Smithsonian Center for Astrophysics (CfA) Supernova Group, we obtained 661 NIR spectra of 157 SNe Ia. Furthermore this sample, 451 NIR spectra of 90 SNe Ia have corresponding CSP-II follow-up light curves. Such a sample will allow detailed studies of the NIR spectroscopic properties of SNe Ia, providing amore »
- Authors:
-
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- Florida State Univ., Tallahassee, FL (United States)
- Carnegie Observatories, Casilla (Chile)
- Univ. of Texas, Austin, TX (United States)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Gordon and Betty Moore Foundation, Palo Alto, CA (United States)
- Univ. of Arizona, Tucson, AZ (United States)
- Observatories of the Carnegie Institution for Science, Pasadena, CA (United States)
- Aarhus Univ., Aarhus C (Denmark)
- Univ. of California, Davis, CA (United States)
- European Southern Observatory, Santiago (Chile)
- Yale Univ., New Haven, CT (United States)
- Homer L. Dodge Dept. of Physics and Astronomy, Santiago (Chile)
- Physical Research Lab., Gujarat (India)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Univ. Nacional de La Plata, La Plata (Argentina)
- Univ. of Chicago, Chicago, IL (United States)
- Millennium Institute of Astrophysics, Santiago (Chile); Univ. de Chile, Santiago (Chile)
- Univ. of Pittsburgh, Pittsburgh, PA (United States)
- Univ. of Copenhagen, Copenhagen (Denmark)
- CENTRA—Centro de Astrofísica e Gravitaçao, Lisbon (Portugal)
- Stockholm Univ., Stockholm (Sweden)
- Univ. de Chile, Santiago (Chile)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Texas A & M Univ., College Station, TX (United States)
- Australian National Univ. (Australia)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Carnegie Observatories, Casilla (China)
- Macquarie Univ., NSW (Australia)
- The Australian National Univ., Weston, ACT (Australia)
- Chinese Academy of Sciences (CAS), Beijing (China); Chinese Academy of Sciences South America Center for Astronomy, Santiago (Chile)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1494109
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Publications of the Astronomical Society of the Pacific
- Additional Journal Information:
- Journal Volume: 131; Journal Issue: 995; Journal ID: ISSN 0004-6280
- Publisher:
- Astronomical Society of the Pacific
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; (stars:) supernovae: general; (cosmology:) dark energy
Citation Formats
Hsiao, E. Y., Phillips, M. M., Marion, G. H., Kirshner, R. P., Morrell, N., Sand, D. J., Burns, C. R., Contreras, C., Hoeflich, P., Stritzinger, M. D., Valenti, S., Anderson, J. P., Ashall, C., Baltay, C., Baron, E., Banerjee, D. P. K., Davis, S., Diamond, T. R., Folatelli, G., Freedman, Wendy L., Förster, F., Galbany, L., Gall, C., González-Gaitán, S., Goobar, A., Hamuy, M., Holmbo, S., Kasliwal, M. M., Krisciunas, K., Kumar, S., Lidman, C., Lu, J., Nugent, P. E., Perlmutter, S., Persson, S. E., Piro, A. L., Rabinowitz, D., Roth, M., Ryder, S. D., Schmidt, B. P., Shahbandeh, M., Suntzeff, N. B., Taddia, F., Uddin, S., and Wang, L. Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program. United States: N. p., 2018.
Web. doi:10.1088/1538-3873/aae961.
Hsiao, E. Y., Phillips, M. M., Marion, G. H., Kirshner, R. P., Morrell, N., Sand, D. J., Burns, C. R., Contreras, C., Hoeflich, P., Stritzinger, M. D., Valenti, S., Anderson, J. P., Ashall, C., Baltay, C., Baron, E., Banerjee, D. P. K., Davis, S., Diamond, T. R., Folatelli, G., Freedman, Wendy L., Förster, F., Galbany, L., Gall, C., González-Gaitán, S., Goobar, A., Hamuy, M., Holmbo, S., Kasliwal, M. M., Krisciunas, K., Kumar, S., Lidman, C., Lu, J., Nugent, P. E., Perlmutter, S., Persson, S. E., Piro, A. L., Rabinowitz, D., Roth, M., Ryder, S. D., Schmidt, B. P., Shahbandeh, M., Suntzeff, N. B., Taddia, F., Uddin, S., & Wang, L. Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program. United States. https://doi.org/10.1088/1538-3873/aae961
Hsiao, E. Y., Phillips, M. M., Marion, G. H., Kirshner, R. P., Morrell, N., Sand, D. J., Burns, C. R., Contreras, C., Hoeflich, P., Stritzinger, M. D., Valenti, S., Anderson, J. P., Ashall, C., Baltay, C., Baron, E., Banerjee, D. P. K., Davis, S., Diamond, T. R., Folatelli, G., Freedman, Wendy L., Förster, F., Galbany, L., Gall, C., González-Gaitán, S., Goobar, A., Hamuy, M., Holmbo, S., Kasliwal, M. M., Krisciunas, K., Kumar, S., Lidman, C., Lu, J., Nugent, P. E., Perlmutter, S., Persson, S. E., Piro, A. L., Rabinowitz, D., Roth, M., Ryder, S. D., Schmidt, B. P., Shahbandeh, M., Suntzeff, N. B., Taddia, F., Uddin, S., and Wang, L. Tue .
"Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program". United States. https://doi.org/10.1088/1538-3873/aae961. https://www.osti.gov/servlets/purl/1494109.
@article{osti_1494109,
title = {Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program},
author = {Hsiao, E. Y. and Phillips, M. M. and Marion, G. H. and Kirshner, R. P. and Morrell, N. and Sand, D. J. and Burns, C. R. and Contreras, C. and Hoeflich, P. and Stritzinger, M. D. and Valenti, S. and Anderson, J. P. and Ashall, C. and Baltay, C. and Baron, E. and Banerjee, D. P. K. and Davis, S. and Diamond, T. R. and Folatelli, G. and Freedman, Wendy L. and Förster, F. and Galbany, L. and Gall, C. and González-Gaitán, S. and Goobar, A. and Hamuy, M. and Holmbo, S. and Kasliwal, M. M. and Krisciunas, K. and Kumar, S. and Lidman, C. and Lu, J. and Nugent, P. E. and Perlmutter, S. and Persson, S. E. and Piro, A. L. and Rabinowitz, D. and Roth, M. and Ryder, S. D. and Schmidt, B. P. and Shahbandeh, M. and Suntzeff, N. B. and Taddia, F. and Uddin, S. and Wang, L.},
abstractNote = {Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near infrared (NIR) is a promising way to significantly reduce the systematic errors, as the strategy minimizes our reliance on the empirical width-luminosity relation and uncertain dust laws. Observations in the NIR are also crucial for our understanding of the origins and evolution of these events, further improving their cosmological utility. Any future experiments in the rest-frame NIR will require knowledge of the SN Ia NIR spectroscopic diversity, which is currently based on a small sample of observed spectra. Along with the accompanying paper, Phillips et al., we introduce the Carnegie Supernova Project-II (CSP-II), to follow-up nearby SNe Ia in both the optical and the NIR. In particular, this paper focuses on the CSP-II NIR spectroscopy program, describing the survey strategy, instrumental setups, data reduction, sample characteristics, and future analyses on the data set. Here, in collaboration with the Harvard-Smithsonian Center for Astrophysics (CfA) Supernova Group, we obtained 661 NIR spectra of 157 SNe Ia. Furthermore this sample, 451 NIR spectra of 90 SNe Ia have corresponding CSP-II follow-up light curves. Such a sample will allow detailed studies of the NIR spectroscopic properties of SNe Ia, providing a different perspective on the properties of the unburned material; the radioactive and stable nickel produced; progenitor magnetic fields; and searches for possible signatures of companion stars.},
doi = {10.1088/1538-3873/aae961},
journal = {Publications of the Astronomical Society of the Pacific},
number = 995,
volume = 131,
place = {United States},
year = {Tue Nov 27 00:00:00 EST 2018},
month = {Tue Nov 27 00:00:00 EST 2018}
}
Web of Science
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