Jul 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hstc.worke..68b&link_type=abstract
"2010 Space Telescope Science Institute Calibration Workshop - Hubble after SM4. Preparing JWST, held 21-23 July 2010 at Space T
Physics
Scientific paper
In order to verify if any of the WFC3/IR imaging filters presents variations in its thickness (filter wedge) we observed the young and bright star cluster NGC 1850 through all the WFC3/IR filters consecutively within 1 orbit. We found that, with the exception of the F098M and F126N filters, the positions of stars observed though different filters differ on average by less than 0.14 ± 0.06 pixels.
Borders Tiffany
MacKenty John
Sabbi Elena
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