Skip to main content
Testing. You are viewing the public testing version of GCN. For the production version, go to https://gcn.nasa.gov.
New Announcement Feature, Code of Conduct, Circular Revisions. See news and announcements

GCN Circular 32638

Subject
Swift J1913.1+1946: Liverpool Telescope imaging and spectroscopy
Date
2022-10-09T21:53:41Z (2 years ago)
From
Daniel Perley at Liverpool JMU <d.a.perley@ljmu.ac.uk>
D. A. Perley (LJMU) reports:

Imaging and spectroscopy were acquired of the optical counterpart of Swift J1913.1+1946 (Dichiara et al., GCN 32632; Lipunov et al., GCN 32634), potentially the optical afterglow of GRB 221009A (Kennea & Williams, GCN 32635; Veres et al., GCN 32636).

The spectrum, taken with SPRAT between 20:49 and 21:06 UT on 2022-10-09, covers a wavelength range of 4000-8000 Angstroms and reveals a red continuum with no strong features.  Due to the low resolution of the spectrograph, we cannot rule out potential narrow absorption lines.  The shape is consistent with a heavily dust-reddened afterglow.  Galactic extinction towards this direction is about 3.52 mag in r-band (from the NED extinction calculator).

Imaging was acquired using IO:O in the SDSS g, r, i, and z filters between 21:18 and 21:23 UT on the same night.  We measure the following magnitudes, calibrating relative to local PS1 secondary standards:

MJD          filter mag    emag
59861.88806  g      18.53  0.06
59861.88896  r      17.00  0.03
59861.88982  i      15.98  0.03
59861.89069  z      15.32  0.03

Analysis is ongoing, and additional observations are planned.



DisclaimerNone
Looking for U.S. government information and services? Visit USA.gov