LETGS Observations of Procyon: More Line Identifications using Improved Calibration and Laboratory data

Details LETGS Observations of Procyon: More Line Identifications using Improved Calibration and Laboratory data LETGS Observations of Procyon: More Line Identifications using Improved Calibration and Laboratory data

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aas...212.1102d&link_type=abstract

American Astronomical Society, AAS Meeting #212, #11.02; Bulletin of the American Astronomical Society, Vol. 40, p.203

Astronomy and Astrophysics

Astrophysics

Scientific paper

Recent EBIT measurements and line identifications of astrophysically abundant elements (Fe VII - Fe X, Lepson et al. 2002, Ar IX- Ar XVI, Lepson et al 2003, S VII- S XIV, Lepson et al 2004) provide an opportunity to identify many of the previously unassigned lines in Procyon (Raassen et al, 2002). We use the combined HRC-S/LETG spectra of Procyon, reprocessed using the newest Chandra calibration files, and recent EBIT laboratory data to make line assignments and compare the Procyon data with the Solar EUV reference data (Hinteregger et al, 1981).

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