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Dr. Scott W. Fleming
@scottwfleming.bsky.social
Branch Manager at Space Telescope Science Institute working in the MAST archive. Astronomy PhD. Studies stars and exoplanets. Loves programming. Opinions are my own. He/Him/His
197 followers198 following78 posts
DSscottwfleming.bsky.social

MSTARPANSPEC adds data for LTT 1445A and GJ 486, the two closest M-dwarfs with transiting exoplanets. Panchromatic spectra are constructed from UV and X-ray observations, Ly-a reconstructions, DEM estimates, and BT-settl models. archive.stsci.edu/hlsp/mstarpa... 🔭

This figure shows the panchromatic spectrum of GJ 486, with wavelength on the x-axis and flux density on the y-axis. Different wavelength regions are shaded in color, from the X-ray observations from XMM-Newton (shaded in purple), the DEM estimate in the EUV (shaded in blue), the optical spectrum including a Ly-a reconstruction from HST observations (shaded in green), and a BT-settl model of the IR (shaded in yellow).
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DS
Dr. Scott W. Fleming
@scottwfleming.bsky.social
Branch Manager at Space Telescope Science Institute working in the MAST archive. Astronomy PhD. Studies stars and exoplanets. Loves programming. Opinions are my own. He/Him/His
197 followers198 following78 posts
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