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- California Institute of TechnologyUS19 papers
- Infrared Processing and Analysis CenterUS8 papers
- University of WashingtonUS7 papers
- University of ArizonaUS6 papers
- University of Maryland, College ParkUS6 papers
- Jet Propulsion LaboratoryUS5 papers
- Massachusetts Institute of TechnologyUS5 papers
- Princeton UniversityUS5 papers
- Space Telescope Science InstituteUS5 papers
- University of TorontoCA5 papers
- Columbia UniversityUS4 papers
- University of Notre DameUS4 papers
26 papers · 1 filter
The Variable Stars of the Draco Dwarf Spheroidal Galaxy - Revisited
K. Kinemuchi, H. C. Harris, Horace A. Smith +4
We present a CCD survey of variable stars in the Draco dwarf spheroidal galaxy. This survey, which has the largest areal coverage since the original variable star survey by Baade &…
Fueling QSOs: The Relevance of Mergers
Nicola Bennert, Gabriela Canalizo, Bruno Jungwiert +4
To study the relevance of mergers for the fueling of QSOs, we are currently conducting an HST imaging campaign of a sample of QSO host galaxies classified as ellipticals in the lit…
The HD 163296 Circumstellar Disk in Scattered Light: Evidence of Time-Variable Self-Shadowing
John P. Wisniewski, Mark Clampin, Carol A. Grady +6
We present the first multi-color view of the scattered light disk of the Herbig Ae star HD 163296, based on coronagraphic observations from the Hubble Space Telescope Advanced Came…
The NStED Stellar and Exoplanet Hosting Star Service
S. Ramirez, B. Ali, R. Baker +14
The NASA Star and Exoplanet Database (NStED) is a general purpose stellar archive with the aim of providing support for NASA's planet finding and characterization goals, stellar as…
The NStED Exoplanet Transit Survey Service
K. von Braun, M. Abajian, B. Ali +15
The NASA Star and Exoplanet Database (NStED) is a general purpose stellar archive with the aim of providing support for NASA's planet finding and characterization goals, stellar as…
The Contribution of Radio Selected Star Forming Galaxies to the IR Energy Density Budget
N. Seymour, T. Dwelly, D. Moss +6
We have used several different methods (radio morphology, radio spectral index, mid-IR to radio and near-IR to radio flux density ratios) to discriminate between AGN and SFGs in fa…