Gratings Calibration Observation of AN Emission Line Source: Capella

Details Gratings Calibration Observation of AN Emission Line Source: Capella Gratings Calibration Observation of AN Emission Line Source: Capella

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cxo..prop..343c&link_type=abstract

Chandra Proposal ID #01200100

Physics

Chandra Proposal Id #01200100

Scientific paper

The RS CVn star Capella is the brightest coronal emission line source in the sky. The X-ray spectrum of Capella exhibits strong emission lines over most of the LETG and HETG energy bands. These observations will be used to determine the LSF for the HRC-I/LETG and ACIS-S/HETG at many energies and orders. These observations will be conducted simultaneously with EUVE observations which can observe Capella anytime between 9/14 and 3/7. The integration times reflect an additional 100 ksec required for the emission-line project.

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