Abstract
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.
Original language | English (US) |
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Pages (from-to) | 692-699 |
Number of pages | 8 |
Journal | Astrophysical Journal |
Volume | 517 |
Issue number | 2 PART 1 |
DOIs | |
State | Published - Jun 1 1999 |
Externally published | Yes |
Keywords
- Gamma rays: bursts
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science