Mark Seibert
0000-0002-1143-5515
Carnegie Institution for Science
200 papers found
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The GALEX Time Domain Survey. I. Selection and Classification of Over a Thousand Ultraviolet Variable Sources
Calibration of the Mid-infrared Tully-Fisher Relation
Non-parametric cell-based photometric proxies for galaxy morphology: methodology and application to the morphologically defined star formation--stellar mass relation of spiral galaxies in the local universe
The diffuse galactic far-ultraviolet sky
The Carnegie Hubble Program: The Infrared Leavitt Law in IC 1613
The Mid-Infrared RR Lyrae Period-Luminosity Relation
Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant
Galaxy Structure in the Ultraviolet: Case studies for Galaxy Evolution
Herschel-ATLAS/GAMA: A Census of Dust in Optically Selected Galaxies from Stacking at Sub-mm Wavelengths
ERRATUM:“THE CARNEGIE HUBBLE PROGRAM: THE LEAVITT LAW AT 3.6 $μ$m and 4.5 $μ$m IN THE LARGE MAGELLANIC CLOUD”(2011, ApJ, 743, 76)
GALEX AND OPTICAL DATA ON V455 ANDROMEDAE AT THREE YEARS POST-OUTBURSTBased on observations obtained with the Apache Point Observatory (APO) 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium (ARC), the McDonald Observatory 2.1 m telescope which is owned and operated by the University of Texas at Austin, the Manastash Ridge Observatory 0.76 m telescope which is operated by the University of Washington, and observations made with the NASA Galaxy Evolution Explorer. GALEX is operated for NASA by the California Institute of Technology under NASA contract NAS5-98034.
The Inter-Eruption Timescale of Classical Novae from Expansion of the Z Camelopardalis Shell
The Northern Middle Lobe of Centaurus A: Circumgalactic Gas in a Starburst Wind
The Carnegie Hubble Program: From parallaxes to the Tully--Fisher relation
The Galaxy Evolution Explorer (GALEX) Source Catalogs
AT Cnc: A Second Dwarf Nova with a Classical Nova Shell
The Carnegie Hubble Program: The Leavitt Law at 3.6 and 4.5 $μ$m in the Milky Way
The CARNEGIE HUBBLE PROGRAM: THE LEAVITT LAW AT 3.6 μm AND 4.5 μm IN THE LARGE MAGELLANIC CLOUD
The Carnegie Hubble Program
How Radiation Feedback Affects Fragmentation and the IMF
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