The DEHVILS survey overview and initial data release: high-quality near-infrared Type Ia supernova light curves at low redshift

Peterson, Erik R.; Jones, David O.; Scolnic, Daniel; Sánchez, Bruno O.; Do, Aaron; Riess, Adam G.; Ward, Sam M.; Dwomoh, Arianna; de Jaeger, Thomas; Jha, Saurabh W.; Mandel, Kaisey S.; Pierel, Justin D. R.; Popovic, Brodie; Rose, Benjamin M.; Rubin, David; Shappee, Benjamin J.; Thorp, Stephen; Tonry, John L.; Tully, R. Brent; Vincenzi, Maria

doi:10.1093/mnras/stad1077

Title: The DEHVILS survey overview and initial data release: high-quality near-infrared Type Ia supernova light curves at low redshift

Journal Article · 12 April 2023 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stad1077 · OSTI ID:1971674

;

; Ward, Sam M.;

;

; Thorp, Stephen;

;

ABSTRACT While the sample of optical Type Ia supernova (SN Ia) light curves (LCs) usable for cosmological parameter measurements surpasses 2000, the sample of published, cosmologically viable near-infrared (NIR) SN Ia LCs, which have been shown to be good ‘standard candles,’ is still ≲ 200. Here, we present high-quality NIR LCs for 83 SNe Ia ranging from 0.002 < z < 0.09 as a part of the Dark Energy, H0, and peculiar Velocities using Infrared Light from Supernovae (DEHVILS) survey. Observations are taken using UKIRT’s WFCAM, where the median depth of the images is 20.7, 20.1, and 19.3 mag (Vega) for Y, J, and H-bands, respectively. The median number of epochs per SN Ia is 18 for all three bands (Y,J, and H) combined and 6 for each band individually. We fit 47 SN Ia LCs that pass strict quality cuts using three LC models, SALT3, snoopy, and B ayeSN and find scatter on the Hubble diagram to be comparable to or better than scatter from optical-only fits in the literature. Fitting NIR-only LCs, we obtain standard deviations ranging from 0.128 to 0.135 mag. Additionally, we present a refined calibration method for transforming 2MASS magnitudes to WFCAM magnitudes using HST CALSPEC stars that results in a 0.03 mag shift in the WFCAM Y-band magnitudes.

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Research Organization:: Duke Univ., Durham, NC (United States)

Sponsoring Organization:: USDOE; USDOE Office of Science (SC)

Grant/Contract Number:: SC0010007

OSTI ID:: 1971674

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 522; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United Kingdom

Language:: English

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A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s⁻¹ Mpc⁻¹ Uncertainty from the Hubble Space Telescope and the SH0ES Team Riess, Adam G.; Yuan, Wenlong; Macri, Lucas M. The Astrophysical Journal Letters, Vol. 934, Issue 1 https://doi.org/10.3847/2041-8213/ac5c5b	journal	July 2022
Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report Spergel, D.; Gehrels, N.; Baltay, C. arXiv https://doi.org/10.48550/arXiv.1503.03757	preprint	January 2015
The Pan-STARRS1 Surveys Chambers, K. C.; Magnier, E. A.; Metcalfe, N. arXiv https://doi.org/10.48550/arXiv.1612.05560	preprint	January 2016
A Reference Survey for Supernova Cosmology with the Nancy Grace Roman Space Telescope Rose, B. M.; Baltay, C.; Hounsell, R. arXiv https://doi.org/10.48550/arXiv.2111.03081	preprint	January 2021
An updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae Galbany, Lluís; de Jaeger, Thomas; Riess, Adam arXiv https://doi.org/10.48550/arXiv.2209.02546	preprint	January 2022
SN 2021hpr and its two siblings in the Cepheid calibrator galaxy NGC 3147: A hierarchical BayeSN analysis of a Type Ia supernova trio, and a Hubble constant constraint Ward, Sam M.; Thorp, Stephen; Mandel, Kaisey S. arXiv https://doi.org/10.48550/arXiv.2209.10558	preprint	January 2022
A BayeSN Distance Ladder: $H_0$ from a consistent modelling of Type Ia supernovae from the optical to the near infrared Dhawan, Suhail; Thorp, Stephen; Mandel, Kaisey S. arXiv https://doi.org/10.48550/arXiv.2211.07657	preprint	January 2022

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