activity
20012011
collaborators

9 papers

astro-ph.CO2011

The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample

N. Suzuki, D. Rubin, C. Lidman +62

We present ACS, NICMOS, and Keck AO-assisted photometry of 20 Type Ia supernovae SNe Ia from the HST Cluster Supernova Survey. The SNe Ia were discovered over the redshift interval…

astro-ph.CO2010

The Hubble Space Telescope Cluster Supernova Survey: II. The Type Ia Supernova Rate in High-Redshift Galaxy Clusters

K. Barbary, G. Aldering, R. Amanullah +40

We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.45 from the Hubble Space Telescope (HST) Cluster Supernova Survey. This is the first…

astro-ph2006

The Rest-frame Optical Colors of 99,000 SDSS Galaxies

V. Smolcic, Z. Ivezic, M. Gacesa +17

We synthesize the rest-frame Stroemgren colors using SDSS spectra for 99,088 galaxies selected from Data Release 1. This narrow-band ~200 AA photometric system (uz, vz, bz, yz), fi…

astro-ph2005

The Milky Way Tomography with SDSS: I. Stellar Number Density Distribution

Mario Juric, Zeljko Ivezic, Alyson Brooks +23

Abridged: We estimate the distances to ~48 million stars detected by the Sloan Digital Sky Survey and map their 3D number density distribution in 100 < D < 20 kpc range over 6,500…

astro-ph2002

Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample

Michael A. Strauss, David H. Weinberg, Robert H. Lupton +1

We describe the algorithm that selects the main sample of galaxies for spectroscopy in the Sloan Digital Sky Survey from the photometric data obtained by the imaging survey. Galaxy…

astro-ph2001

Higher Order Moments of the Angular Distribution of Galaxies from Early SDSS Data

István Szapudi, Joshua A. Frieman, Roman Scoccimarro +13

We present initial results for counts in cells statistics of the angular distribution of galaxies in early data from the Sloan Digital Sky Survey (SDSS). We analyze a rectangular s…