Astrometric Reference Stars: From UCAC to URAT

Abstract

Currently available astrometric catalogs will be reviewed, and instrumentation and observational issues discussed, particularly systematic errors and their control. The U.S. Naval Observatory (USNO) CCD Astrograph Catalog (UCAC) is an all-sky astrometric survey to 16th magnitude. It was observed with a semi-automated telescope on a low budget. The second data release (July 2003) contains positions, proper motions, and photometry for over 48 million stars; the final release is expected in 2006. Design studies have been performed for a new 0.9-meter aperture USNO Robotic Astrometric Telescope (URAT) with a single chip (~ 100 Mpixel), 3 degree FOV and circular symmetric pupil. Its operation is envisioned to be fully automatic, generating stellar positions on the 5 to 10 mas level to at least 18th magnitude with a limiting magnitude of about 20 to 21. These reference stars, being on an inertial system (linked to quasars), will be very beneficial for LSST, PanSTARRS and other projects. With a few years of observing, absolute trigonometric paraUaxes (5-20 mas, depending on magnitude) could be obtained for all stars accessible by URAT from an initially southern hemisphere location.

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Document Details

Document Type
Technical Report
Publication Date
Oct 31, 2004
Accession Number
ADA594154

Entities

People

  • Norbert Zacharias

Organizations

  • United States Naval Observatory

Tags

Communities of Interest

  • Air Platforms
  • Autonomy
  • Materials and Manufacturing Processes
  • Space

DTIC Thesaurus Topics

  • Accuracy
  • Cameras
  • Catalogs
  • Coordinate Systems
  • Detectors
  • Distortion
  • Errors
  • Focal Planes
  • Instrumentation
  • Observation
  • Observatories
  • Observers
  • Operating Systems
  • Precision
  • Quality Control
  • Quantum Efficiency
  • Southern Hemisphere

Fields of Study

  • Physics

Readers

  • Astronomy/Astrophysics

Technology Areas

  • AI & ML
  • AI & ML - Bayesian Inference
  • Autonomy
  • Space