Astronomical Data Analysis Software and Systems XI

By D. Bohlender, D. Durand, T. Handley. 2002

472 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/88412ae61b6769b2c610ac0b123a3b0b2ca1372e

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Citations in the corpus

The Optical Gravitational Lensing Experiment. Final Reductions of the OGLE-III Data (2008, methodology): “In the second step, a short list of identified stars and a preliminary transformation between theX,Y pixel coordinates from the OGLE database and the RA/DEC fromthe 2MASS Catalog list was found using the WCSTools software package (Mink 2002).”
MegaMorph - multiwavelength measurement of galaxy structure: complete Sersic profile information from modern surveys (2012, methodology): “Importantly, the images for all nine bands have been ‘micro-registered’ onto the same pixel grid, using SWarp (Bertin et al. 2002)5.”
THE DIFFERENCE IMAGING PIPELINE FOR THE TRANSIENT SEARCH IN THE DARK ENERGY SURVEY (2015, methodology): “Many of our DiffImg stages use publicly available Terapix/AstrOmatic codes40(Bertin et al. 2002) including SCAMP (Bertin 2006) for astrometry, SExtractor (Bertin & Arnouts 1996) to find objects, PSFEx (Bertin 2011) to determine the position-dependent PSF, and SWarp to sum individual exposures (to…”
Gaia Data Release 3. Catalogue validation (2022, methodology): “This work has made an extensive use of Aladin and the SIMBAD, VizieR databases operated at the Centre de Données Astronomiques (Strasbourg) in France and of the software TOPCAT (Taylor 2005).”
Galactic accretion and the outer structure of galaxies in the CDM model (2013, methodology): “We created 1 Mpc2 mosaics in the g, r and i bands centered on each galaxy in our sample using the ‘corrected’ sky-subtracted frames from the SDSS Data Release 9 image server and SWarp (Bertin et al. 2002).”
An absolutely calibrated survey of polarized emission from the northern sky at 1.4 GHz. Observations (2005, methodology): “Software for data acquisition, reduction, and calibration was written in glish, a programming language that is part of the AIPS++ environment (e.g.: Willis 2002; McMullin et al. 2004).”
CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products (2012, methodology): “…was found to be the most accurate) in addition to the robustness of the SCAMP astrometric software (Bertin 2006) and SWARP re-pixelisation software (Bertin et al. 2002), and the impact of the astrometric distortion correction, interpolation and re-pixelisation on the PSF and galaxy shapes using…”
The DES Science Verification weak lensing shear catalogues (2015, methodology): “MNRAS 000, 1–37 (2015) epoch images were registered and combined into a coadd image using the SCAMP and SWARP packages (Bertin et al. 2002; Bertin 2006).”
GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey - I. A low-frequency extragalactic catalogue (2016, methodology): “Throughout, we use the mosaicking software swarp (Bertin et al. 2002).”