Astronomical Data Analysis

By Jean-Luc Starck, Fionn Murtagh. 2007

2,252 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/d14472595a65929c0ae92cb67d0e53ab2eef28a0

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1. P. Hopkins
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• GASP. I. Gas Stripping Phenomena in Galaxies with MUSE (2017, background): “On a cosmic scale, this leads to a drop in the star formation rate density of the universe (Madau & Dickinson 2014).”
• First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass (2022, methodology): “2020a, 2020b), one CLEAN-based deconvolution algorithm (DIFMAP; Shepherd 1997), and two “regularized maximum likelihood” (RML) algorithms (eht-imaging,Chael et al.”
• ORBITAL PHASE VARIATIONS OF THE ECCENTRIC GIANT PLANET HAT-P-2b (2013, background): “07 AU from its host star, indicating that it must have migrated inward via a process such as gas disk migration (Lin et al. 1996), planet–planet scattering (Rasio & Ford 1996), secular interactions (Wu & Lithwick 2011), or Kozai migration (Weidenschilling & Marzari 1996; Naoz et al.”
• THE CLIMATE OF HD 189733b FROM FOURTEEN TRANSITS AND ECLIPSES MEASURED BY SPITZER (2010, background): “…well as Rayleigh scattering at blue wavelengths (Grillmair et al. 2007; Tinetti et al. 2007; Barnes et al. 2007; Redfield et al. 2008; Barman 2008; Swain et al. 2008, 2009; Charbonneau et al. 2008; Sing et al. 2009; Madhusudhan and Seager 2009; Pont et al. 2008; Lecavelier Des Etangs et al. 2008).”
• THE GOULD’S BELT DISTANCES SURVEY (GOBELINS). II. DISTANCES AND STRUCTURE TOWARD THE ORION MOLECULAR CLOUDS (2016, methodology): “Kraus et al. (2009) obtained a dynamical distance of 410±20 pc based on The Astrophysical Journal, 834:142 (17pp), 2017 January 10 doi:10.”
• An Exploratory Chandra Survey of a Well-defined Sample of 35 Large Bright Quasar Survey Broad Absorption Line Quasars (2006, unknown): “…spectroscopic observations of individual BAL quasars with Chandra and XMM-Newton have generally upheld these results (e.g., Chartas et al. 2002; Aldcroft & Green 2003; Chartas et al. 2003; Grupe et al. 2003; Page et al. 2005) with only a few exceptions where intrinsic X-ray faintness cannot be…”
• The Slitless Spectroscopy Data Extraction Software aXe (2008, unknown): “Malhotra et al. 2009, in preparation), and searches for high-z supernovae (Riess et al. 2004; Strolger et al. 2004). By generating instrument-specific configuration and calibration files, aXe can also be applied to slitless spectroscopic data from other HST instruments (e.g., NICMOS) and even from g”
• THE HERSCHEL REFERENCE SURVEY: DUST IN EARLY-TYPE GALAXIES AND ACROSS THE HUBBLE SEQUENCE (2011, background): “O’Sullivan & Ponman (2004) found that its X-ray luminosity was two order of magnitudes lower than expected for its optical luminosity and there are signs of a small dust disk in absorption (Tran et al. 2001).”
• THE 4 Ms CHANDRA DEEP FIELD-SOUTH NUMBER COUNTS APPORTIONED BY SOURCE CLASS: PERVASIVE ACTIVE GALACTIC NUCLEI AND THE ASCENT OF NORMAL GALAXIES (2012, methodology): “…have focused on measuring their cosmic evolution (see Brandt & Hasinger 2005 for a review), and in particular, the evolution of their X-ray luminosity function (XLF; e.g., Cowie et al. 2003; Ueda et al. 2003; Hasinger et al. 2005; Silverman et al. 2008; Ebrero et al. 2009; Aird et al. 2010).”
• ON THE ORIGIN OF THE EXTENDED Hα FILAMENTS IN COOLING FLOW CLUSTERS (2010, methodology): “The elements were assumed to be present in the solar ratios, as measured by Anders & Grevesse (1989).”
• Automated data reduction workflows for astronomy (2013, methodology): “While this approach is relatively new for the field of astronomy (e.g. Ballester et al., 2011; Schaa ff et al., 2012), it has been widely used in other fields of science including biology and chemistry (Abhishek and Sekharb,, 2007), meteorology (Barseghian et al., 2009) and economics (Lud¨ascher et…”
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• The Hubble Space Telescope PanCET Program: Exospheric Mg ii and Fe ii in the Near-ultraviolet Transmission Spectrum of WASP-121b Using Jitter Decorrelation (2019, methodology): “For the model, we used the 3D stellar model from the Stagger-grid (Magic et al. 2015) with the model (Teff=6500, log g=4, [Fe/H]= 0.0), which was closest to the measured values of WASP-121A in effective temperature, gravity, and metallicity (Teff= 6460±140 K, log10 g = 4.242±0.2 cgs, [Fe/H] = +0.13±”