Astronomical Data Analysis Software and Systems

By B. Argyle, P. Bunclark, J. Lewis. 2008

301 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/39b511e0e4f303c30cd7827264bb0e58da61a051

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Citations in the corpus

Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release (2010, methodology): “The data frames (over 12 000) are then stitched into single images using the SWARP software developed by the TERAPIX group (Bertin et al. 2002), resulting in 27 20-Gb images each of 12 × 4 deg2 at 0.4 × 0.4 arcsec2 pixel sampling.”
THE CLUSTERING OF MASSIVE GALAXIES AT z ∼ 0.5 FROM THE FIRST SEMESTER OF BOSS DATA (2010, methodology): “(7) was done by Riemann sum using 100 linearly spaced bins in and the correlation matrix,Ci j/(σiσ j) is quoted in the lower part of the table.”
THE FUNDAMENTAL PLANE OF ACCRETION ONTO BLACK HOLES WITH DYNAMICAL MASSES (2009, methodology): “X-ray Spectral Fitting We modeled the reduced spectra using XSPEC12 (Arnaud 1996).”
The Sloan Digital Sky Survey Quasar Catalog. IV. Fifth Data Release (2007, methodology): “The survey data-processing software measures the properties of each detected object in the imaging data in all five bands and determines and applies both astrometric and photometric calibrations (Pier et al. 2003; Lupton et al. 2001; Ivezić et al. 2004).”
Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey (2007, methodology): “For 55 sources with more than 50 net counts, the column density is estimated through spectral modeling with XSPEC (Arnaud 1996) (for more details see Paper II).”
The Sun in Time: Activity and Environment (2007, methodology): “The line fluxes given in Table 4 are normalized to a distance of 1AU and have also been normalized to the radius our Sun had at (2)The solar line fluxes of Oviii, O vii, Nvii, and Cvi were determined from a model spectrum synthesized in the XSPEC software (Arnaud, 1996) using the vapec model (Smith ”
The Coincidence of Nuclear Star Clusters and Active Galactic Nuclei (2008, methodology): “All the Chandra data come from XAssist (an automated extraction pipeline for X-ray data; Ptak & Griffiths 2003); these are the sources with an “X” prefix in Table 4.”
THE EXTREME SPIN OF THE BLACK HOLE IN CYGNUS X-1 (2011, methodology): “…16 http://cxc.harvard.edu/ciao/threads/spectrahetgacis/ The data analysis and model fitting throughout this paper were performed using XSPEC17 version 12.6.0 (Arnaud 1996) and, unless otherwise indicated, errors are everywhere reported at the1σ level of confidence.”