Abstract / Description of output
We describe the astrometric calibration of the Gemini NICI Planet-Finding Campaign. The Campaign requires a relative astromefric accuracy of approximate to 20 mas across multiyear timescales in order to distinguish true companions from background stars by verifying common proper motion and parallax with their parent stars. The calibration consists of a correction for instrumental optical image distortion, plus on-sky imaging of astrometric fields to determine the pixel scale and image orientation. We achieve an accuracy of less than or similar to 7 mas between the center and edge of the 18" NICI field, meeting the 20 mas requirement. Most of the Campaign data in the Gemini Science Archive are accurate to this level but we identify a number of anomalies and present methods to correct the errors.
Original language | English |
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Pages (from-to) | 1112-1125 |
Number of pages | 14 |
Journal | Publications of the Astronomical Society of the Pacific |
Volume | 126 |
Issue number | 946 |
DOIs | |
Publication status | Published - Dec 2014 |
Keywords / Materials (for Non-textual outputs)
- GIANT PLANETS
- YOUNG
- DISCOVERY
- FREQUENCY
- COMPANION
- STARS
- DISK
- FITS