HST Wide-Field Planetary Camera II Status Update

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We review the status of the Wide-Field Planetary Camera II (WFPC2) onboard the Hubble Space Telescope as well as recent enhancements to calibration and analysis methods. The instrument continues to perform extremely well after 70000 images. Low level effects such as CTE and dark current continue to increase with long-term radiation exposure, but still affect only a minority of observations; work continues to characterize and monitor these effects. The long-term photometric stability appears to be excellent, with most filters showing changes of a few percent or less. Recent work shows that aperture photometry for small apertures (1-2 pixel radius) will be affected at the 5% to 10% level by target position in the field-of-view due to small focus variations. A new "on-the-fly calibration" feature of the HST archive allows instant re-calibration of WFPC2 data with the latest reference files; this should be a great benefit to both new observers and archival WFPC2 users. Recent results on polarization calibration, CTE, and other topics are discussed.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

HST Wide-Field Planetary Camera II Status Update does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with HST Wide-Field Planetary Camera II Status Update, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HST Wide-Field Planetary Camera II Status Update will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1745185

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.