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Abstract With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report observations in the only field that has received four epochs (spanning 126 days) of JWST NIRCam observations in Cycle 1. This field is toward MACS J0416.1−2403, which is a rich galaxy cluster at redshiftz= 0.4 and is one of the Hubble Frontier Fields. We have discovered 14 transients from these data. Twelve of these transients happened in three galaxies (withz= 0.94, 1.01, and 2.091) crossing a lensing caustic of the cluster, and these transients are highly magnified by gravitational lensing. These 12 transients are likely of a similar nature to those previously reported based on the Hubble Space Telescope (HST) data in this field, i.e., individual stars in the highly magnified arcs. However, these 12 could not have been found by HST because they were too red and too faint. The other two transients are associated with background galaxies (z= 2.205 and 0.7093) that are only moderately magnified, and they are likely supernovae. They indicate a demagnified supernova surface density, when monitored at a time cadence of a few months to a ∼3–4μm survey limit of AB ∼28.5 mag, of ∼0.5 arcmin−2integrated toz≈ 2. This survey depth is beyond the capability of HST but can be easily reached by JWST.
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This content will become publicly available on February 5, 2027
PEARLS: 21 Transients Found in the Three-epoch NIRCam Observations in the Continuous Viewing Zone of the James Webb Space Telescope
Abstract We present 21 transients from our three-epoch, four-band NIRCam observations covering 14.16 arcmin2in the Spitzer IRAC Dark Field (IDF), taken by the JWST Prime Extragalactic Areas for Reionization and Lensing Science program with a time cadence of ∼6 months. A separate Hubble Space Telescope program provided Advanced Camera for Surveys optical imaging contemporaneous with the second and third epochs of the NIRCam observations. The NIRSpec spectroscopy on three transients confirmed a Type Ia supernova atz= 1.63 and the host galaxies of the other two atz= 2.64 and 1.90, respectively. Combining these with the photometric redshifts (zph) of the host galaxies in the rest of the sample, we find that the transients are in either a “mid-z” group atz > 1.6 withMV ≲ − 16.0 mag or a “low-z” group atz < 0.4 withMH ≳ − 14.0 mag. The mid-ztransients are consistent with supernovae. In contrast, the low-ztransients’ luminosities fall in the range of the so-called “gap transients” between supernovae and novae. However, this latter conclusion is only tentative due to possible catastrophic failures inzphthat could bias them to low-z. Conversely, if they are indeed atz < 0.4, it would be worth studying similar transients in the future. Our work further demonstrates the power of NIRCam in transient science and also shows that it would be more fruitful to carry out a long-term monitoring program with more passbands, a higher cadence, and prompt follow-up spectroscopy. Being in the continuous viewing zone of the JWST, the IDF is an ideal field for this purpose.
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- Award ID(s):
- 2307447
- PAR ID:
- 10704037
- Author(s) / Creator(s):
- ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »
- Publisher / Repository:
- IOP Science
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 998
- Issue:
- 1
- ISSN:
- 0004-637X
- Page Range / eLocation ID:
- 115
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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