We report a JOUST discovery of a new infrared transient candidate (AT 2023axi) in JWST observations of Arp 220. The target was detected in ERO program 2739 (PI:Klaus Pontoppidan) on MJD 59958.54 in 6 JWST NIRCam filters. The transient nature of the source is confirmed via image subtraction with an HST template image from MJD 58730, 1035 days prior. Preliminary AB magnitudes of the target are measured via simple aperture photometry using current JWST photometric calibration estimates:
Instrument: NIRCam
F090W 22.77 0.02
F150W 22.22 0.06
F200W 22.16 0.05
F277W 21.97 0.04
F356W 21.84 0.04
F444W 21.41 0.03
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Host Galaxy: Arp 220 (IC 4553)
Host Redshift: 0.0184
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Given the above, we suggest that the target is possibly a red nova, or an old, dust-obscured core-collapse supernova. Given the time since these data were taken, opportunity for follow-up is limited.
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The Transient Science@Space Telescope (TSST) collaboration studies stellar transients of varying types, including supernovae, kilonovae, super-luminous supernovae, TDE’s, and more. TSST develops and operates the transient monitor, JOUST, for the purpose of locating detections of known and new transients serendipitously in JWST data.
Catalog | Name | Reported RA | Reported DEC | Reported Obj-Type | Reported Redshift | Host Name | Host Redshift | Remarks | TNS RA | TNS DEC | TNS Obj-Type | TNS Redshift |
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TNS | 2023axi [joust2023y] | 15:34:57.494 | +23:30:14.30 | Arp 220 | 0.0184 | 15:34:57.494 | +23:30:14.30 |
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