Information Handling in Astronomy - Historical Vistas

By A. Heck. 2002

377 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/ffacfb04a37882584776430d458ea29b63b7c7a5

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In Astronomy and Astrophysics

In Computational Mechanics

Citations in the corpus

The GMRT 150 MHz all-sky radio survey - First alternative data release TGSS ADR1 (2016, background): “A small number of publications have been published using data from this initial release including Bagchi et al. (2011), Gopal-Krishna et al. (2012), Sirothia et al. (2014), and Krishna et al. (2014).”
The VLA-COSMOS Survey. II. Source Catalog of the Large Project (2006, methodology): “The data reduction was done using the Astronomical Imaging Processing System (AIPS; Greisen 2003) following the standard routines as described in the VLA handbook on Data Reduction.”
VLBA Determination of the Distance to Nearby Star-forming Regions. II. Hubble 4 and HDE 283572 in Taurus (2007, methodology): “In this article, we have reported multiepoch VLBA observations of two naked T Tauri stars in the Taurus complex and used these data to measure their trigonometric parallax and proper motions.”
VLBA DETERMINATION OF THE DISTANCE TO NEARBY STAR-FORMING REGIONS. III. HP TAU/G2 AND THE THREE-DIMENSIONAL STRUCTURE OF TAURUS (2009, methodology): “The data were edited and calibrated using the Astronomical Im ge Processing System (AIPS –Greisen 2003).”
THE FIRST ACCURATE PARALLAX DISTANCE TO A BLACK HOLE (2009, methodology): “Data were reduced according to standard procedures within AIPS (Greisen 2003), and the source position at each epoch was determined by fitting an elliptical Gaussian to the source.”
A Preliminary VLBA Distance to the Core of Ophiuchus, with an Accuracy of 4% (2008, methodology): “The data were edited and calibrated using the Astronomical Image Processing System (AIPS –Greisen 2003).”
LOFAR FACET CALIBRATION (2016, methodology): “Another technique that was developed to correct for the ionospheric phase errors is “field-based calibration” (Cotton et al. 2004; Cotton 2005).”