| Issue |
A&A
Volume 393, Number 2, October II 2002
|
|
|---|---|---|
| Page(s) | 445 - 451 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361:20021010 | |
| Published online | 23 September 2002 | |
The bright optical afterglow of the long GRB 001007 *
1
Real Instituto y Observatorio de la Armada, Sección de Astronomía, 11.110 San Fernando-Naval (Cádiz), Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
2
Instituto de Astrofísica de Andalucía (CSIC), Apartado de Correos, 3.004, 18.080 Granada, Spain, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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3
Danish Space Research Institute, Juliane Maries Vej 30, 2 100 Copenhagen Ø, Denmark, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
4
Laboratorio de Astrofísica Espacial y Física Fundamental (INTA), Apartado de Correos, 50.727, 28.080 Madrid, Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
5
Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, 2 100 Copenhagen Ø, Denmark e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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European Southern Observatory, Karl Schwarzschild Straße 2, 85 748 Garching, Germany, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
7
Division of Astronomy, PO Box 3 000, 90 014 University of Oulu, Finland, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
8
Instituto de Astrofísica de Canarias, 38.200 La Laguna (Tenerife), Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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Departamento de Ciencias de la Navegación y de la Tierra, Universidad de la Coruña, 15.011 La Coruña, Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
10
Department of Physics, Michigan Technological University, 1 400 Townsend Drive, Houghton MI 49 931-1 295, USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
11
School of Physics and Astronomy, University of Nottingham, University Park NG7 2RD Nottingham, UK, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
12
Department of Astronomy, University of Toronto, 60 St. George Street, Toronto ON, M5S 3H8 Canada e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
13
Space Telescope Science Institute, 3 700 San Martín Drive, Baltimore MD 21 218, USA, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
14
Astrophysikalisches Institut, An der Sternwarte 16, 14 482 Potsdam, Germany, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
15
Osservatorio Astronomico di Trieste, Via Tiepolo 11, 34 131 Trieste, Italy, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
16
University of Amsterdam, Kruislaan 403, 1 098 SJ Amsterdam, The Netherlands e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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Goddard Space Flight Centre (NASA), Greenbelt MD 20 771 USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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18
Istituto di Astrofisica Spaziale e Fisica Cosmica, Sezione di Bologna (CNR), Via Gobetti 101, 40 129 Bologna, Italy e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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19
Thüringer Landessternwarte Tautenburg, 07 778 Tautenburg, Germany, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
20
Marshall Space Flight Centre (NASA), SD-50, Huntsville AL 35 812, USA, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
21
Clemson University, Clemson SC 29 634, USA, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
22
University of California, Berkeley, Space Sciences Laboratory, Berkeley CA 94 720-7 450, USA, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
23
Ioffe Physico-Technical Institute, 26 Polytekhnicheskaya, St. Petersburg 194 021, Russia, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
24
Lawrence Livermore National Laboratory, Livermore CA 94 550, USA, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
25
Department of Physical Sciences, University of Hertfordshire, College Lane, Hatfield, Herts AL10 9AB, UK e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
26
Department of Physics and Astronomy, State University of New York, Stony Brook NY 11 794-3800, USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
27
Steward Observatory, Tucson AZ 85 721, USA, e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
Corresponding author: J. M. Castro Cerón, This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
25
March
2002
Accepted:
8
July
2002
Abstract
We present optical follow up observations of the long GRB 001007 between 6.14 hours and ~468 days after the event. An unusually bright optical afterglow (OA) was seen to decline following a steep power law decay with index α = -2.03 ± 0.11, possibly indicating a break in the light curve at
3.5 days, as found in other bursts. Upper limits imposed by the LOTIS alerting system 6.14 hours after the gamma ray event provide tentative (1.2σ) evidence for a break in the optical light curve. The spectral index β of the OA yields -1.24 ± 0.57. These values may be explained both by several fireball jet models and by the cannonball model. Fireball spherical expansion models are not favoured. Late epoch deep imaging revealed the presence of a complex host galaxy system, composed of at least two objects located
1.2´´ (1.7σ) and 1.9´´ (2.7σ) from the afterglow position.
Key words: gamma rays: bursts / techniques: photometric / cosmology: observations
Based on observations collected: at the European Southern Observatory, in La Silla and Paranal (Chile), ESO Large Programmes 165.H-0464(G), 165.H-0464(I) and 265.D-5742(A), granted to the GRACE Team; with the Livermore Optical Transient Imaging System's 0.11 m telephoto lenses, at the Lawrence Livermore National Laboratory, in California (USA); with the Instituto de Astrofísica de Canarias's 0.82 m telescope, at the Observatorio del Teide, in the island of Tenerife (Spain); with the Danish 1.54 m telescope, at the European Southern Observatory, in La Silla (Chile); and with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos, of the Instituto de Astrofísica de Canarias.
© ESO, 2002
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