Published March 10, 2017
| Version v1
Journal article
Photometric Observations of Supernova 2013cq Associated with GRB 130427A
Creators
- Becerra, R. L.1
- Watson, A. M.1
- Lee, W. H.1
- Fraija, N.1
- Diego, J. A. de1
- Georgiev, L. N.1
- González, J. J.1
- Butler, N. R.2
- Littlejohns, O. M.2
- Bloom, J. S.3
- Capone, J. I.4
- Toy, V. L.4
- Cucchiara, A.5
- Fox, O. D.6
- Gehrels, N.7
- Kutyrev, A. S.7
- Prochaska, J. X.8
- Ramirez-Ruiz, E.8
- Richer, M. G.9
- Román-Zúñiga, C. G.9
- and others
- 1. Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 70-264, 04510 México, D. F., México (Mexico)
- 2. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287 (United States)
- 3. Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States)
- 4. Department of Astronomy, University of Maryland, College Park, MD 20742 (United States)
- 5. NASA Postdoctoral Program Fellow, Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
- 6. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)
- 7. NASA, Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
- 8. Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States)
- 9. Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 106, 22800 Ensenada, Baja California, México (Mexico)
Description
We observed the afterglow of GRB 130427A with the Reionization and Transients Infrared Camera (RATIR) instrument on the 1.5 m Harold L. Johnson telescope of the Observatorio Astronómico Nacional in Sierra San Pedro Mártir. Our homogenous griZY JH photometry extends from the night of the burst to three years later. We fit a model for the afterglow. There is a significant positive residual that matches the behavior of SN 1998bw in the griZ filters; we suggest that this is a photometric signature of the supernova SN 2013cq associated with the Gamma-ray burst. The peak absolute magnitude of the supernova is .
Availability note (English)
Available from http://dx.doi.org/10.3847/1538-4357/aa610fAdditional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 837
- Journal Issue
- 2
- Journal Page Range
- [23 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51030985
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AFTERGLOW; COSMIC GAMMA BURSTS; FILTERS; PHOTOMETRY; SUPERNOVAE; TELESCOPES
- Descriptors DEC
- BINARY STARS; COSMIC RADIATION; ERUPTIVE VARIABLE STARS; IONIZING RADIATIONS; PRIMARY COSMIC RADIATION; RADIATIONS; STARS; VARIABLE STARS