The Solar Blind Channel Bright Object Limits for Astronomical Objects

Details The Solar Blind Channel Bright Object Limits for Astronomical Objects The Solar Blind Channel Bright Object Limits for Astronomical Objects

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acs..rept....7b&link_type=abstract

ACS Instrument Science Report 99-07, 13 pages

Physics

Hubble Space Telescope, Hst, Space Telescope Science Institute, Advanced Camera For Surveys, Acs, Stsci

Scientific paper

Tables of limiting magnitudes for all observation modes of the ACS Solar Blind Channel are calculated for a range of stellar energy distributions, using Kurucz model fluxes and observed standard stars. For K and M stars, the observed Bruzual flux distributions extend down to only 2000 A. New prototypes for K and M stars are extracted from the IUE archive for determining the bright object limits for these late Morgan-Keenan spectral classes.

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