ULTRAVIOLET SPECTROSCOPY OF SUPERNOVAE: THE FIRST TWO YEARS OF SWIFT OBSERVATIONS

Journal Article · Sat Aug 01 00:00:00 EDT 2009 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/700/2/1456; COUNTRY OF INPUT: INTERNATIONAL ATOMIC ENERGY AGENCY (IAEA)· OSTI ID:21313780

Bufano, F ^[1]; Immler, S ^[2]; Turatto, M; Panagia, N ^[3]; Landsman, W; Gehrels, N ^[4]; Brown, P; Roming, P ^[5]; Benetti, S; Cappellaro, E; Mazzali, P; Zampieri, L ^[6]; Holland, S T ^[7]; Milne, P ^[8]; Pian, E ^[9]; Breeveld, A A ^[10]

---

1. Dipartimento di Astronomia, Universita' degli Studi di Padova, Padova IT 35122 (Italy)
2. NASA/Goddard Space Flight Center, Astrophysics Science Division, Code 662, Greenbelt, MD 20771 (United States)
3. INAF-Osservatorio Astronomico di Catania, Catania IT 95123 (Italy)
4. NASA/Goddard Space Flight Center, Astrophysics Science Division, Code 661, Greenbelt, MD 20771 (United States)
5. Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802 (United States)
6. INAF-Osservatorio Astronomico di Padova, Padova IT 35122 (Italy)
7. NASA/Goddard Space Flight Center, Astrophysics Science Division, Code 660.1, Greenbelt, MD 20771 (United States)
8. Department of Astronomy and Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States)
9. INAF-Osservatorio Astrofisico di Trieste, Trieste IT 34131 (Italy)
10. Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey RH5 6NT (United Kingdom)

We present the entire sample of ultraviolet (UV) spectra of supernovae (SNe) obtained with the Ultraviolet/Optical Telescope (UVOT) on board the Swift satellite during the first two years of observations (2005/2006). A total of 29 UV-grism and 22 V-grism spectra of nine SNe have been collected, of which six are thermonuclear (Type Ia) and three core-collapse (Type Ibc/II) SNe. All the spectra have been obtained during the photospheric phase. After a comparison of the spectra of our sample with those in the literature (SNe 1992A, 1990N, and 1999em), we confirm some degree of diversity in the UV emission of Type Ia SNe and a greater homogeneity in the Type II Plateau SN sample. Signatures of interaction between the ejecta and the circumstellar environment have been found in the UV spectrum of SN 2006jc, the only SN Type Ib/c for which UVOT grism data are available. Currently, Swift UVOT is the best suited instrument for early SN studies in the UV due to its fast response and flexible scheduling capabilities. However, in order to increase the quality of the data and significantly improve our understanding of the UV properties of SNe and to fully maximize the scientific potential of UVOT grism observations, a larger investment in observing time and longer exposures are needed.

• OSTI ID: 21313780
• Journal Information: Astrophysical Journal, Vol. 700, Issue 2; Other Information: DOI: 10.1088/0004-637X/700/2/1456; Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

99 GENERAL AND MISCELLANEOUS//MATHEMATICS, COMPUTING, AND INFORMATION SCIENCE
EMISSION
SATELLITES
SPECTROSCOPY
SUPERNOVAE
TELESCOPES
ULTRAVIOLET RADIATION
ULTRAVIOLET SPECTRA