AIPS, the VLA, and the VLBA

By E. Greisen. 2003

491 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/7e67512f34d94fa0c7b02eb58fe054d2bda5e943

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. E. Berger
2. S. Smartt
3. J. Silverman
4. Ryan Chornock
5. Bing Zhang
6. A. Riess
7. C. Carilli
8. D. M. Alexander

In Nuclear and High Energy Physics

1. Y. Kovalev
2. A. Pushkarev
3. T. Savolainen
4. M. Lister
5. A. Lobanov
6. Torsten A. Ensslin
7. C. Carilli
8. J. Zensus

Citations in the corpus

• LOFAR FACET CALIBRATION (2016, methodology): “In addition, AIPS does not allow one to solve for more general calibration problems.”
• First M87 Event Horizon Telescope Results. III. Data Processing and Calibration (2019, unknown): “The NRAO Astronomical Image Processing System ( AIPS ; Greisen 2003 ) is the most commonly used reduction package for centimeter VLBI data.”
• THE GOULD’S BELT DISTANCES SURVEY (GOBELINS). II. DISTANCES AND STRUCTURE TOWARD THE ORION MOLECULAR CLOUDS (2016, methodology): “The data were reduced in the AIPS (Greisen 2003) following the standard prescription for the VLBA data.”
• THE ULTRAVIOLET-BRIGHT, SLOWLY DECLINING TRANSIENT PS1-11af AS A PARTIAL TIDAL DISRUPTION EVENT (2013, methodology): “In all epochs, we use standard data reduction procedures in AIPS (Greisen 2003).”
• The Very Large Array Low-frequency Sky Survey Redux (VLSSr) (2014, methodology): “These preliminary data reduction steps were performed in an older version of the Astronomical Image Processing System (31DEC03 AIPS: Greisen 2003), using the run-files and specialized reduction tasks developed for the VLSS.”
• 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).”
• MOJAVE: Monitoring of Jets in Active galactic nuclei with VLBA Experiments (2012, methodology): “The initial calibration was performed with the NRAO Astronomical Image Processing System (AIPS) (Greisen 2003) following the standard techniques.”
• VLBA Determination of the Distance to Nearby Star-forming Regions. II. Hubble 4 and HDE 283572 in Taurus (2007, methodology): “The data were edited and calibrated using the Astronomical Image Processing System (AIPS; Greisen 2003).”
• VLBA Determination of the Distance to Nearby Star-forming Regions. I. The Distance to T Tauri with 0.4% Accuracy (2007, methodology): “The data were edited and calibrated using the Astronomical Image Processing System (AIPS; Greisen 2003).”
• THE VLA-COSMOS SURVEY. IV. DEEP DATA AND JOINT CATALOG (2010, methodology): “…the data reduction procedure adopted for the Large project (Schinnerer et al. 2007) which uses the Astronomical Imaging Processing System (AIPS; Greisen 2003). uv data points affected by RFI (radio frequency interference) were again flagged by hand using the task TVFLAG and by excluding…”
• 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 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.”
• THE EXPANDED VERY LARGE ARRAY: A NEW TELESCOPE FOR NEW SCIENCE (2011, methodology): “There are problems with AIPS, however, that prevent its continued long-term use for EVLA data post-processing.”
• 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 PANCHROMATIC VIEW OF THE RESTLESS SN 2009ip REVEALS THE EXPLOSIVE EJECTION OF A MASSIVE STAR ENVELOPE (2013, methodology): “We reduced all data using standard procedures in the Astronomical Image Processing System (AIPS; Greisen 2003).”