349 citations
- The Ohio State UniversityUS42 papers
- Kyoto UniversityJP40 papers
- University of WarsawPL33 papers
- University of AucklandNZ31 papers
- University of Notre DameUS31 papers
- European Southern ObservatoryCL29 papers
- Nagoya UniversityJP29 papers
- Centre National de la Recherche ScientifiqueFR28 papers
- Chungbuk National UniversityKR28 papers
- Korea Astronomy and Space Science InstituteKR28 papers
- University of CambridgeGB28 papers
- Las Cumbres Observatory Global Telescope NetworkUS27 papers
5 papers · 1 filter
SN 2005at - A neglected type Ic supernova at 10 Mpc
E. Kankare, M. Fraser, S. Ryder +7
We present a photometric and spectroscopic study of a reddened type Ic supernova (SN) 2005at. We report our results based on the available data of SN 2005at, including late-time ob…
Evidence from stellar rotation of enhanced disc dispersal: (I) The case of the triple visual system BD-21 1074 in the Pictoris association
S. Messina, B. Monard, K. Biazzo +2
The early stage of stellar evolution is characterized by a star-disc locking mechanism. The disc-locking prevents the star to spin its rotation up, and its timescale depends on the…
Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VI: The Sixth Year (2013-2014)
Taichi Kato, Pavol A. Dubovsky, Igor Kudzej +83
Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv:0905.1757), we collected times of superhump maxima for 56 SU UMa-type dwarf novae mainly observed durin…
OGLE-2012-BLG-0455/MOA-2012-BLG-206: Microlensing event with ambiguity in planetary interpretations caused by incomplete coverage of planetary signal
H. Park, C. Han, A. Gould +55
Characterizing a microlensing planet is done from modeling an observed lensing light curve. In this process, it is often confronted that solutions of different lensing parameters r…
MOA-2013-BLG-220Lb: Massive Planetary Companion to Galactic-Disk Host
J. C. Yee, C. Han, A. Gould +70
We report the discovery of MOA-2013-BLG-220Lb, which has a super-Jupiter mass ratio relative to its host. The proper motion, $μ=12.5\pm 1\, {\rm mas}…