ACS Post-SMOV UV Contamination Monitor

Details ACS Post-SMOV UV Contamination Monitor ACS Post-SMOV UV Contamination Monitor

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002hst..prop.9655d&link_type=abstract

HST Proposal ID #9655

Physics

Hst Proposal Id #9655

Scientific paper

A standard star field {NGC6681} is observed about once a month through all the ACS broad band UV filters. NGC6681 hosts several UV spectro - photometric standard stars for which accurate spectra have been {and will continue to be} measured with STIS. The target cannot be observed for three months from mid november through to mid february, so the standard star GRW+70 will be observed twice in its stead. This programme continues the UV sensitivity monitoring campaign {ACS SMOV proposal 9010} of the HRC and SBC after the end of the SMOV period. An SBC dark current measurement is taken as the last exposure of each SBC sequence.

Affiliated with

Also associated with

No associations

Rating

ACS Post-SMOV UV Contamination Monitor 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 ACS Post-SMOV UV Contamination Monitor, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ACS Post-SMOV UV Contamination Monitor will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-733762