Spectral PSF subtraction I: the SPSF look-up-table method

Details Spectral PSF subtraction I: the SPSF look-up-table method Spectral PSF subtraction I: the SPSF look-up-table method

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000msngr..99...31m&link_type=abstract

Messenger, vol. 99, p.31-33 (2000)

Computer Science

11

Scientific paper

Introduction: Why Spectral PSF Subtraction? The first FORS follow-up run of the STIS/NICMOS survey for Damped Lya (DLA) galaxies was completed in August 1999. The purpose of the FORS spectroscopy is to search for Lya emission lines from candidate DLA galaxies with projected distances from the underlying quasars as small as 0.30 arcsec. The candidate DLA galaxies are typically some 8-10 magnitudes fainter than the underlying quasars.

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