Faint Supernovae and Supernova Impostors: Case studies of SN2002kg/NGC2403-V37 and SN 2003gm
(2006)
Blue Luminous Stars in Nearby Galaxies: Quantitative Spectral Analysis of M33 B-Type Supergiant Stars**The WHT is operated on the island of La Palma by the ING in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. ****Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
The Astrophysical Journal American Astronomical Society 635:1 (2005) 311-335
POINT-AGAPE pixel lensing survey of M 31
Astronomy & Astrophysics EDP Sciences 443:3 (2005) 911-928
The progenitor of SN 2005cs in the Whirlpool Galaxy
Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 364:1 (2005) l33-l37
Classical novae from the POINT-AGAPE microlensing survey of M31 -- II. Rate and statistical characteristics of the nova population
(2005)