Gratings Calibration Observation of AN Emission Line Source: Procyon

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

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cxo..prop..228c&link_type=abstract

Chandra Proposal ID #01200103

Physics

Chandra Proposal Id #01200103

Scientific paper

The F5 star Procyon is a strong source of soft x-ray emission lines. This observation will be used to determine the LSF for the HRC-I/LETG at many energies and orders. This observation will be conducted simultaneously with an EUVE observation to cross calibrate in the 100-160A region. EUVE can observe Procyon anytime between Oct. 18 and April 10. The integration time reflects an additional 50 ksec required by the Emission-Line Project.

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