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Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas
T. H. Jarrett, F. Masci, C. W. Tsai +15
The Wide-field Infrared Survey Explorer (WISE) mapped the entire sky at mid-infrared wavelengths 3.4, 4.6, 12 and 22 microns. The mission was primarily designed to extract point so…
AT Cnc: A Second Dwarf Nova with a Classical Nova Shell
Michael M. Shara, Trisha Mizusawa, Peter Wehinger +5
We are systematically surveying all known and suspected Z Cam-type dwarf novae for classical nova shells. This survey is motivated by the discovery of the largest known classical n…
Halo Occupation Distribution Modeling of Green Valley Galaxies
Elisabeth Krause, Christopher M. Hirata, Christopher Martin +2
We present a clustering analysis of near ultraviolet (NUV) - optical color selected luminosity bin samples of green valley galaxies. These galaxy samples are constructed by matchin…
Constructing a WISE High Resolution Galaxy Atlas
T. H. Jarrett, F. Masci, C. W. Tsai +16
After eight months of continuous observations, the Wide-field Infrared Survey Explorer (WISE) mapped the entire sky at 3.4 μm, 4.6 μm, 12 μm and 22 μm. We have begun a dedicated WI…
The Inter-Eruption Timescale of Classical Novae from Expansion of the Z Camelopardalis Shell
Michael M. Shara, Trisha Mizusawa, David Zurek +3
The dwarf nova Z Camelopardalis is surrounded by the largest known classical nova shell. This shell demonstrates that at least some dwarf novae must have undergone classical nova e…
An ultraviolet-optical flare from the tidal disruption of a helium-rich stellar core
S. Gezari, R. Chornock, A. Rest +31
The flare of radiation from the tidal disruption and accretion of a star can be used as a marker for supermassive black holes that otherwise lie dormant and undetected in the centr…