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The On-Orbit Performance of WFPC2

Abstract

The second Wide Field and Planetary Camera (WFPC2) was successfully installed in the Hubble Space Telescope during the STS-61 servicing mission in 1993 December. The primary objective of this new camera is to provide diffraction-limited photometric imaging over a wide field and a spectral range from 0.12 to 1.0 micrometer. Here we provide an overview of the characteristics of the new instrument and offer our perspectives based on the first 6 months of operations on-orbit.


Publication:
The Astrophysical Journal
Pub Date:
November 1994
DOI:

10.1086/187580

Bibcode:
1994ApJ...435L...3T
Keywords:
  • Astronomical Photometry;
  • Diffraction Limited Cameras;
  • Hubble Space Telescope;
  • Optical Waveguides;
  • Performance Tests;
  • Calibrating;
  • Mirrors;
  • Mission Planning;
  • Satellite-Borne Instruments;
  • Spaceborne Photography;
  • Astronomy;
  • INSTRUMENTATION: MISCELLANEOUS;
  • METHODS: OBSERVATIONAL;
  • SPACE VEHICLES
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