Skip to main content
JSON Notices via Email, Kafka Cron Jobs, Submitter Profile, GCN is Hiring. See news and announcements

GCN Circular 495

Subject
GRB991216 Optical and IR observations
Date
1999-12-19T00:15:32Z (27 years ago)
From
Peter Garnavich at Center for Astrophysics <peterg@mars.harvard.edu>
P. Garnavich, S. Jha, K. Stanek, M. Pahre, M. Garcia, A. Szentgyorgyi
(CfA) and J. Tonry (U. Hawaii) report:

The object reported by Uglesich et al. (GCN 472) as a possible
afterglow of GRB991216 is detected on 5 sets of 120 sec. exposures
taken with the FLWO 1.2m+IRCam on Dec. 17 (UT) and on two sets of 540
sec. images taken Dec 18. A preliminary calibration provides the
following brightness estimates:

  UT Date     J     err
Dec. 17.35  16.99  0.05
Dec. 18.30  18.25  0.06

The power-law index derived from these data is -1.33. Our Dec. 18.
point is significantly fainter than the J-band observation reported by
Vreeswijk et al. (GCN 492) (UT 18.13).

The afterglow was again observed with the Hawaii 2.2-m in the R band
and calibrated using star "B" (Jha et al. GCN 476) with R=19.45 (Dolan
et al. GCN 486). These new brightness estimates are:

  UT Date     R    err
Dec 18.32  20.32  0.05
Dec 18.56  20.57  0.05

and when combined with previous R-band observations reported by Dolan
et. al (GCN 486), Henden et al. (GCN 473) and Jha et al. (GCN 476),
give a power-law index of -1.23+/-0.05. The Dec. UT 18.191 R-band
magnitude of 21.1 reported by Mattox (GCN 487) is significantly fainter
than our measurements.

This message can be cited.
Looking for U.S. government information and services? Visit USA.gov