Scattered light in the echelle modes

Details Scattered light in the echelle modes Scattered light in the echelle modes

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7931l&link_type=abstract

HST Proposal ID #7931

Other

Hst Proposal Id #7931

Scientific paper

Observations of the reddened O star CPD-59D2603 done as part of ERO suggest significant scattering in the echelle modes. The effect is strongest at the shortest wavelengths. The purpose of this program is to quantify the scattering by extending the ERO observations to all other modes and wavelengths of interest to observers. CPD-59D2603 will be observed with E140M/H, E230M/H, G140M. and G230M. The 0.2x0.2, 0.1x0.09, and 0.2x0.06 apertures are used. The observations will be complemented by data taken in a Cycle 7 GO program. All spectral ranges contain strong saturated interstellar lines. The count rates in the line cores allow us to quantify the amount of scattered light.

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