Optical and Near-infrared Observations of the Afterglow of GRB 980329 from 15 Hours to 10 Days

Space Telescope Science Institute, Baltimore, Maryland, United States
The Astrophysical Journal (Impact Factor: 5.99). 01/2009; 517(2):692. DOI: 10.1086/307210
Source: arXiv


We report I-band observations of the GRB 980329 field made on 1998 March 29 with the 1.34 m Tautenberg Schmidt telescope, R-, J- and K-band observations made on 1998 April 1 with the APO 3.5 m telescope, R- and I-band observations made on 1998 April 3 with the Mayall 4 m telescope at KPNO, and J- and K-band observations made 1998 April 6-8 with the Keck-I 10 m telescope. We show that these and other reported measurements are consistent with a power-law fading of the optical/near-infrared source that is coincident with the variable radio source VLA J0702+3850. This firmly establishes that this source is the afterglow of GRB 980329.


Available from: Francisco Javier Castander
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