Astronomical data analysis software and systems X : proceedings of a meeting held at Boston, Massachusetts, U.S.A., 12-15 November 2000
By F. R. Harnden, F. Primini, H. Payne. 2001
333 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/7250656c1c2ec48f8716d53b04de4d0240f66a93
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- L. Hernquist
Citations in the corpus
- Dust Reddening in Sloan Digital Sky Survey Quasars (2004, methodology): “These papers used median colors as a function of redshift; however, a population of dust-reddened quasars will shift the median quasar colors redder but will leave the mode unaffected.”
- THE SLOAN DIGITAL SKY SURVEY-II SUPERNOVA SURVEY: SEARCH ALGORITHM AND FOLLOW-UP OBSERVATIONS (2007, methodology): “The SDSS 2.5m telescope nominally performs observations every night during the search seasons, so the data must be processed within 24 hours to avoid a backlog of unprocessed data and to rapidly identify SN candidates for spectroscopic follow-up observations.”
- Quasars Probing Quasars. I. Optically Thick Absorbers near Luminous Quasars (2006, methodology): “The imaging data are processed by the astrometric pipeline (Pier et al. 2003) and photometric pipeline (Lupton et al. 2001) and are photometrically calibrated to a standard-star network (Smith et al. 2002; Hogg et al. 2001).”
- Active Galactic Nuclei in the Sloan Digital Sky Survey. I. Sample Selection (2005, methodology): “Key words: galaxies: active — galaxies: Seyfert — galaxies: starburst — quasars: emission lines — surveys”
- The Second Data Release of the Sloan Digital Sky Survey (2004, methodology): “The imaging data are processed through a series of pipelines that locate and measure the properties of all detected objects (Lupton et al. 2001) and carry out photometric and astrometric calibration (Pier et al. 2003).”
- Red and Reddened Quasars in the Sloan Digital Sky Survey (2003, methodology): “The automated extraction of point-spread function magnitudes from the images is discussed by Lupton et al. (2001), and Pier et al. (2003) present the details of the SDSS astrometric solution.”
- Environmental Dependence of Properties of Galaxies in the Sloan Digital Sky Survey (2006, background): “…DR4+, of the SDSS (York et al. 2000; Blanton et al. 2003a; Fukugita et al. 1996; Gunn et al. 1998, 2006; Hogg et al. 2001; Ivezić et al. 2004; Lupton et al. 2001; Pier et al. 2003; Smith et al. 2002; Stoughton et al. 2002; Tucker et al. 2006) from the New York University Value-Added…”
- THE DEEP2 GALAXY REDSHIFT SURVEY: DESIGN, OBSERVATIONS, DATA REDUCTION, AND REDSHIFTS (2012, methodology): “The ATV image display tool created by Aaron Barth, SPLOT created by David Schlegel, the IDL Astronomy User’s Library supported by the Goddard Space Flight Center, and the idlutils package were all instrumental in this work.”