Gratings Calibration Observation of AN Emission Line Source: HR 1099

Details Gratings Calibration Observation of AN Emission Line Source: HR 1099 Gratings Calibration Observation of AN Emission Line Source: HR 1099

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cxo..prop..229c&link_type=abstract

Chandra Proposal ID #01200104

Physics

Chandra Proposal Id #01200104

Scientific paper

The RS CVn star HR1099 is a strong source of hard x-ray emission lines.
This observation will be used to determine the LSF for the ACIS-S/HETG
at many energies and orders. This observation will be conducted
simultaneously with an EUVE observation. The observing window for EUVE
is 8/14 through 2/1.

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