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Pan-STARRS Pixel Processing: Detrending, Warping, Stacking
C. Z. Waters, E. A. Magnier, P. A. Price +17
The Pan-STARRS1 Science Consortium have carried out a set of imaging surveys using the 1.4 giga-pixel GPC1 camera on the PS1 telescope. As this camera is composed of many individua…
The Pan-STARRS1 Database and Data Products
H. A. Flewelling, E. A. Magnier, K. C. Chambers +37
This paper describes the organization of the database and the catalog data products from the Pan-STARRS1 Steradian Survey. The catalog data products are available in the form…
Hiding in Plain Sight - Recovering Clusters of Galaxies with the Strongest AGN in Their Cores
T. S. Green, A. C. Edge, H. Ebeling +8
A key challenge in understanding the feedback mechanism of AGN in Brightest Cluster Galaxies (BCGs) is the inherent rarity of catching an AGN during its strong outburst phase. This…
The size-frequency distribution of H>13 NEOs and ARM targets detected by Pan-STARRS1
Eva Schunová Lilly, Robert Jedicke, Peter Vereš +2
We determine the absolute magnitude (H) distribution (or size-frequency distribution, SFD; where is the slope of the distribution) for near-Earth objects…
Measuring the Properties of Dark Energy with Photometrically Classified Pan-STARRS Supernovae. I. Systematic Uncertainty from Core-Collapse Supernova Contamination
D. O. Jones, D. M. Scolnic, A. G. Riess +18
The Pan-STARRS (PS1) Medium Deep Survey discovered over 5,000 likely supernovae (SNe) but obtained spectral classifications for just 10% of its SN candidates. We measured spectrosc…
Dust in three dimensions in the Galactic Plane
R. J. Hanson, C. A. L. Bailer-Jones, W. S. Burgett +6
We present three dimensional maps in monochromatic extinction and the extinction parameter within a few degrees of the Galactic plane. These are inferred using ph…