Sara M. Petty, Ph.D.

Affiliations: 
2009 Physics The Catholic University of America, Washington, DC 
Area:
Astrophysics Physics
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"Sara Petty"
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Parents

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Duilia F. de Mello grad student 2009 Catholic University
 (Quantifying the physical properties of high-redshift galaxies: A multi-wavelength survey on the progenitors of local galaxies.)
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Publications

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Farrah D, Petty S, Connolly B, et al. (2017) The Role of the Most Luminous Obscured AGNs in Galaxy Assembly atz∼ 2 The Astrophysical Journal. 844: 106
Harris K, Farrah D, Schulz B, et al. (2016) Star formation rates in luminous quasars at 2 < z < 3 Monthly Notices of the Royal Astronomical Society. 457: 4179-4194
Psychogyios A, Charmandaris V, Diaz-Santos T, et al. (2016) Morphological classification of local luminous infrared galaxies Astronomy and Astrophysics. 591
Tsai CW, Eisenhardt PRM, Wu J, et al. (2015) The most luminous galaxies discovered by wise Astrophysical Journal. 805
Petty SM, Armus L, Charmandaris V, et al. (2014) The FUV to near-IR morphologies of luminous infrared galaxies in the goals sample Astronomical Journal. 148
Farrah D, Lebouteiller V, Spoon HWW, et al. (2013) Far-infrared fine-structure line diagnostics of ultraluminous infrared galaxies Astrophysical Journal. 776
Petty SM, Neill JD, Jarrett TH, et al. (2013) Uv-bright nearby early-type galaxies observed in the mid-infrared: Evidence for a multi-stage formation history by way of wise and Galex Imaging Astronomical Journal. 146
Stern D, Assef RJ, Benford DJ, et al. (2012) Mid-infrared selection of active galactic nuclei with the Wide-field Infrared Survey Explorer. I. Characterizing WISE-selected active galactic nuclei in cosmos Astrophysical Journal. 753
Davy Kirkpatrick J, Cushing MC, Gelino CR, et al. (2011) The first hundred brown dwarfs discovered by the Wide-field Infrared Survey Explorer (WISE) Astrophysical Journal, Supplement Series. 197
Petty SM, De Mello DF, Gallagher JS, et al. (2009) Structures of local galaxies compared to high-redshift star-forming galaxies Astronomical Journal. 138: 362-375
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