Astronomical data analysis software and systems XII : proceedings of a meeting held at Baltimore, Maryland, USA, 13-16 October 2002

By H. Payne, R. Jędrzejewski, R. Hook. 2003

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Star formation in Perseus - Clusters, filaments and the conditions for star formation (2005, methodology): “This cannot be answered by looking at older populations of premain-sequence stars detectable in the infrared and optical because the typical velocities of the stars lead them to wander by 1 pc/Myr, and the environment in which they formed may Appendix is only available in electronic form at…”
THE CORES OF THE Fe Kα LINES IN ACTIVE GALACTIC NUCLEI: AN EXTENDED CHANDRA HIGH ENERGY GRATING SAMPLE (2010, methodology): “The spectra were analyzed using the spectral-fitting package XSPEC (Arnaud 1996).”
Infrared Spectral Energy Distributions of Nearby Galaxies (2005, methodology): “The data were processed with the SCUBA User Reduction Facility (Jenness & Lightfoot 1998).”
BUDDA: A New Two-dimensional Bulge/Disk Decomposition Code for Detailed Structural Analysis of Galaxies (2004, methodology): “Most of the available algorithms were developed to tackle specific problems, like, e.g., face-on late-type spirals (de Jong 1996a), distant galaxies (Simard 1998), or nearby galaxies observed with very high spatial resolution (Peng et al. 2002).”
Scuba-2: Iterative map-making with the sub-millimetre user reduction facility (2013, methodology): “Such was the basic recipe for the reduction of chopped data from SCUBA2’s predecessor SCUBA (Jenness & Lightfoot 1998; Jenness et al. 2000), and MAMBO (e.g., Omont et al. 2001), another camera from the same generation.”