Rachel A. Osten, Ph.D.

Affiliations: 
2002 University of Colorado, Boulder, Boulder, CO, United States 
Area:
Astronomy and Astrophysics
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"Rachel Osten"
Mean distance: 30.26
 
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Parents

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Thomas R. Ayres grad student 2002 CU Boulder
 (Multiwavelength observations of flares and variability in the coronae of active binary systems.)
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Publications

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Brasseur CE, Osten RA, Fleming SW. (2019) Short-duration Stellar Flares in GALEX Data The Astrophysical Journal. 883: 88
Airapetian VS, Barnes R, Cohen O, et al. (2019) Impact of space weather on climate and habitability of terrestrial-type exoplanets International Journal of Astrobiology. 19: 136-194
Osten RA, Melis C, Stelzer B, et al. (2015) The deepest constraints on radio and X-ray magnetic activity in ultracool dwarfs from wise J104915.57-531906.1 Astrophysical Journal Letters. 805
Osten RA, Wolk SJ. (2015) Connecting flares and transient mass-loss events in magnetically active stars Astrophysical Journal. 809
Kowalski AF, Hawley SL, Carlsson M, et al. (2015) New Insights into White-Light Flare Emission from Radiative-Hydrodynamic Modeling of a Chromospheric Condensation Solar Physics. 290: 3487-3523
Kowalski AF, Hawley SL, Wisniewski JP, et al. (2013) Time-resolved properties and global trends in dme flares from simultaneous photometry and spectra Astrophysical Journal, Supplement Series. 207
Osten RA, Kowalski A, Sahu K, et al. (2012) Drafts: A deep, rapid archival flare transient search in the galactic bulge Astrophysical Journal. 754
Schrijver CJ, Beer J, Baltensperger U, et al. (2012) Estimating the frequency of extremely energetic solar events, based on solar, stellar, lunar, and terrestrial records Journal of Geophysical Research: Space Physics. 117
Forbrich J, Osten RA, Wolk SJ. (2011) Simultaneous X-ray and radio observations of young stellar objects in NGC 1333 and IC 348 Astrophysical Journal. 736
Jaeger TR, Osten RA, Lazio TJ, et al. (2011) 325MHz very large array observations of ultracool dwarfs TVLM 513-46546 and 2MASS J0036+1821104 Astronomical Journal. 142
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