The JADES Transient Survey: Discovery and Classification of Supernovae in the JADES Deep Field

Abstract The JWST Advanced Deep Extragalactic Survey (JADES) is a multicycle JWST program that has taken among the deepest near- and mid-infrared images to date (down to ∼30 AB mag) over ∼25 arcmin 2 in the GOODS-S field in two sets of observations with 1 yr of separation. This presented the first opportunity to systematically search for transients, mostly supernovae (SNe), out to z > 2. We found 79 SNe: 38 at z < 2, 23 at 2 < z < 3, 8 at 3 < z < 4, 7 at 4 < z < 5, and 3 with undetermined redshifts, where the redshifts are predominantly based on spectroscopic or highly reliable JADES photometric redshifts of the host galaxies. At this depth, the detection rate is ∼1–2 arcmin –2 yr –1 , demonstrating the power of JWST as an SN discovery machine. We also conducted multiband follow-up NIRCam observations of a subset of the SNe to better constrain their light curves and classify their types. Here, we present the survey, sample, search parameters, spectral energy distributions, light curves, and classifications. Even at z ≥ 2, the NIRCam data quality is high enough to allow SN classification via multiepoch light-curve fitting with confidence. The multiepoch SN sample includes a Type Ia SN at z spec = 2.90, a Type IIP SN at z spec = 3.61, and a Type Ic-BL SN at z spec = 2.83. We also found that two z ∼ 16 galaxy candidates from the first imaging epoch were actually transients that faded in the second epoch, illustrating the possibility that moderate/high-redshift SNe could mimic high-redshift dropout galaxies.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-01-29
DOI
https://doi.org/10.3847/1538-4357/ad8fab
Citations
21
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
24.25

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article

The JADES Transient Survey: Discovery and Classification of Supernovae in the JADES Deep Field

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21 citations
The Astrophysical Journal
Gamma-ray bursts and supernovae
24.25
article

The JADES Transient Survey: Discovery and Classification of Supernovae in the JADES Deep Field

Qinan Wang, Eiichi Egami, Bhavin Joshi, George H. Rieke, Fengwu Sun, R. Maiolino, Benjamin D. Johnson, Takashi J. Moriya, A. Rest, Kevin Hainline, J. Jencson, Matthew R. Siebert, Michael Engesser, Sandro Tacchella, S. M. Khairnar, Chris J. Willott, Louis-Gregory Strolger, S. Charlot, Mirko Curti, Yossef Zenati, Jianwei Lyu, Christina C. Williams, Ori D. Fox, Christa DeCoursey, Daniel J. Eisenstein, D. A. Coulter, Christopher N. A. Willmer, Andrew J. Bunker, Phillip A. Cargile, Melissa Shahbandeh, Brant E. Robertson, Sebastián Gómez, Marcia Rieke, Suvi Gezari, Justin Pierel, Wenlei Chen, Shea Defour-Remy, R. Quimby
article en
21 citations

Abstract

Abstract The JWST Advanced Deep Extragalactic Survey (JADES) is a multicycle JWST program that has taken among the deepest near- and mid-infrared images to date (down to ∼30 AB mag) over ∼25 arcmin 2 in the GOODS-S field in two sets of observations with 1 yr of separation. This presented the first opportunity to systematically search for transients, mostly supernovae (SNe), out to z > 2. We found 79 SNe: 38 at z < 2, 23 at 2 < z < 3, 8 at 3 < z < 4, 7 at 4 < z < 5, and 3 with undetermined redshifts, where the redshifts are predominantly based on spectroscopic or highly reliable JADES photometric redshifts of the host galaxies. At this depth, the detection rate is ∼1–2 arcmin –2 yr –1 , demonstrating the power of JWST as an SN discovery machine. We also conducted multiband follow-up NIRCam observations of a subset of the SNe to better constrain their light curves and classify their types. Here, we present the survey, sample, search parameters, spectral energy distributions, light curves, and classifications. Even at z ≥ 2, the NIRCam data quality is high enough to allow SN classification via multiepoch light-curve fitting with confidence. The multiepoch SN sample includes a Type Ia SN at z spec = 2.90, a Type IIP SN at z spec = 3.61, and a Type Ic-BL SN at z spec = 2.83. We also found that two z ∼ 16 galaxy candidates from the first imaging epoch were actually transients that faded in the second epoch, illustrating the possibility that moderate/high-redshift SNe could mimic high-redshift dropout galaxies.

The Astrophysical JournalVol. 979(2)
Institut d'Astrophysique de Paris (FR)
National Science Foundation, National Aeronautics and Space Administration, University of California, Santa Cruz, Space Telescope Science Institute, UK Research and Innovation, European Commission, Science and Technology Facilities Council
Affordable and clean energy
Openalex Percentile: Top 0%
Gamma-ray bursts and supernovae
24.25
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