{
  "bibcode": "2022GCN.31729....1C",
  "body": "S. B. Cenko (NASA/GSFC), I. Andreoni (JSI/UMD/GSFC), and M. Coughlin (UMN) report on behalf of a larger collaboration:\n\nThe location of the transient source AT2022cmc (Andreoni et al., GCN 31590) was observed with the Hubble Space Telescope beginning at 2022 Mar 8 20:12:21 UT (~ 25.4 d after discovery). The field was imaged with the Wide-Field Camera 3 (WFC3) in the F606W (UVIS) and F160W (IR) filters for 1044 s and 1059 s, respectively.\n\nAT2022cmc is well detected in both bands. Using preliminary calibrations, we estimate AB magnitudes of F606W = 21.88 +/- 0.05 mag and F160W = 22.24 +/- 0.06 mag at this time. The source appears unresolved, without obvious evidence for extended emission directly underneath.\n\nA second HST epoch to constrain the presence of an underlying host galaxy is planned for July/August 2022.\n\nWe thank the HST operations team for the approval and rapid execution of these observations.",
  "circularId": 31729,
  "createdOn": 1646883246000,
  "email": "brad.cenko@nasa.gov",
  "subject": "ZTF22aaajecp/AT2022cmc: Hubble Space Telescope Observations",
  "submitter": "Brad Cenko at NASA/GSFC  <brad.cenko@nasa.gov>",
  "eventId": "ZTF22aaajecp"
}