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3D Dust Mapping Reveals that Orion Forms Part of a Large Ring of Dust
E. F. Schlafly, G. Green, D. P. Finkbeiner +12
The Orion Molecular Complex is the nearest site of ongoing high-mass star formation, making it one of the most extensively studied molecular complexes in the Galaxy. We have develo…
The Main-Belt Comets: The Pan-STARRS1 Perspective
Henry H. Hsieh, Larry Denneau, Richard J. Wainscoat +17
We analyze 760475 observations of 333026 main-belt objects obtained by the Pan-STARRS1 (PS1) survey telescope between 2012 May 20 and 2013 November 9, a period during which PS1 dis…
Observational Constraints on the Catastrophic Disruption Rate of Small Main Belt Asteroids
Larry Denneau, Robert Jedicke, Alan Fitzsimmons +15
We have calculated 90% confidence limits on the steady-state rate of catastrophic disruptions of main belt asteroids in terms of the absolute magnitude at which one catastrophic di…
Wide, Cool and Ultracool Companions to Nearby Stars from Pan-STARRS1
Niall R. Deacon, Michael C. Liu, Eugene A. Magnier +18
We present the discovery of 61 wide (>5 arcsecond) separation, low-mass (stellar and substellar) companions to stars in the solar neighborhood identified from Pan-STARRS\,1 (PS1) d…
Supervoid Origin of the Cold Spot in the Cosmic Microwave Background
András Kovács, István Szapudi, Benjamin R. Granett +13
We use a WISE-2MASS-Pan-STARRS1 galaxy catalog to search for a supervoid in the direction of the Cosmic Microwave Background Cold Spot. We obtain photometric redshifts using our mu…
Measuring Quasar Variability with Pan-STARRS1 and SDSS
E. Morganson, W. S. Burgett, K. C. Chambers +10
We measure quasar variability using the Panoramic Survey Telescope and Rapid Response System 1 Survey (Pan-STARRS1 or PS1) and the Sloan Digital Sky Survey (SDSS) and establish a m…