Dawn M. Gelino, Ph.D.

Affiliations: 
2001 New Mexico State University, Las Cruces, NM, United States 
Area:
Astronomy and Astrophysics
Google:
"Dawn Gelino"
Mean distance: 4517.33
 

Parents

Sign in to add mentor
Thomas Edward Harrison grad student 2001 New Mexico State (Astronomy Tree)
 (Modeling infrared ellipsoidal variations: Determining the masses of black holes in soft x -ray transients.)
Bernard J. McNamara grad student 2001 New Mexico State
 (Modeling infrared ellipsoidal variations: Determining the masses of black holes in soft x -ray transients.)
BETA: Related publications

Publications

You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.

Smith KL, Mushotzky RF, Boyd PT, et al. (2018) TheKeplerLight Curves of AGN: A Detailed Analysis The Astrophysical Journal. 857: 141
Howell SB, Mason E, Boyd P, et al. (2016) RAPIDLY ROTATING, X-RAY BRIGHT STARS IN THEKEPLERFIELD The Astrophysical Journal. 831: 27
Smith KL, Boyd PT, Mushotzky RF, et al. (2015) KSwAGS: A SWIFT X-RAY and UV SURVEY of the KEPLER FIELD. I. Astronomical Journal. 150
Kane SR, Gelino DM. (2014) On the inclination and habitability of the HD 10180 system Astrophysical Journal. 792
Harrison TE, Gelino DM, Buxton M, et al. (2014) Herschel observations of circinus X-1 during outburst and quiescence Astronomical Journal. 148
Kane SR, Barclay T, Gelino DM. (2013) A potential super-venus in the kepler-69 system Astrophysical Journal Letters. 770
Kane SR, Gelino DM. (2013) Decoupling phase variations in multi-planet systems Astrophysical Journal. 762
Khargharia J, Froning CS, Robinson EL, et al. (2013) The mass of the black hole in xtej1118+480 Astronomical Journal. 145
Kane SR, Gelino DM. (2012) The habitable zone and extreme planetary orbits. Astrobiology. 12: 940-5
Kane SR, Ciardi DR, Gelino DM, et al. (2012) The exoplanet eccentricity distribution from Kepler planet candidates Monthly Notices of the Royal Astronomical Society. 425: 757-762
See more...