Thomas Matheson
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Thomas Matheson has a total of 21 co-authors. Here are the top co-authors by number of shared publications:
- A. E. Bragg
Department of Physics and Astronomy Bowling Green State University 43403 Bowling Green OH
1 shared publication - A. Mahdavi
Department of Physics and Astronomy University of Victoria V8W 3P6 Victoria BC Canada
1 shared publication B. J. Wilkes
Harvard-Smithsonian Center for Astrophysics 60 Garden Street 02138 Cambridge MA
1 shared publication- Emilio E. Falco
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
1 shared publication - Genevieve J. Graves
UCO/Lick Observatory University of California 95064 Santa Cruz CA
1 shared publication - Inseok Song
Spitzer Science Center IPAC/Caltech 91125 Pasadena CA
1 shared publication
Latest Publications
- Open Access
Optical Spectroscopy of Type Ia Supernovae
We present 432 low-dispersion optical spectra of 32 Type Ia supernovae (SNe Ia) that also have well-calibrated light curves. The coverage ranges from 6 epochs to 36 epochs of spectroscopy. Most of the data were obtained with the 1.5m Tillinghast telescope at the F. L. Whipple Observatory with typical wavelength coverage of 3700-7400A and a resolution of ~7A. The earliest spectra are thirteen days before B-band maximum; two-thirds of the SNe were observed before maximum brightness. Coverage for some SNe continues almost to the nebular phase. The consistency of the method of observation and the technique of reduction makes this an ideal data set for studying the spectroscopic diversity of SNe Ia.
Open AccessOptical Spectroscopy of Type Ia Supernovae
We present 432 low-dispersion optical spectra of 32 Type Ia supernovae (SNe Ia) that also have well-calibrated light curves. The coverage ranges from 6 epochs to 36 epochs of spectroscopy. Most of the data were obtained with the 1.5m Tillinghast telescope at the F. L. Whipple Observatory with typical wavelength coverage of 3700-7400A and a resolution of ~7A. The earliest spectra are thirteen days before B-band maximum; two-thirds of the SNe were observed before maximum brightness. Coverage for some SNe continues almost to the nebular phase. The consistency of the method of observation and the technique of reduction makes this an ideal data set for studying the spectroscopic diversity of SNe Ia.