Stephanie Snedden

Stephanie A. Snedden is an American astronomer at the Apache Point Observatory of the New Mexico State University in New Mexico, United States.[1][2] The minor planet 133008 Snedden is named after her; it was discovered by the Sloan Digital Sky Survey at Apache Point Observatory on 5 October 2002.[2] She has published papers including The Case for Optically Thick High-Velocity Broad-Line Region Gas in Active Galactic Nuclei.[3]

Education

Snedden gained her BS from Sonoma State University in 1983,[1] her MS in physics and astronomy from the University of Nebraska in 1995,[4] and her PhD from University of Nebraska in 2001.[1]

Research interests

Snedden studies the physics of active galactic nuclei, particularly the structure and kinematics of gas in the broad-line region.[1]

Media

Snedden appeared on Nova, in the 13 April 2010 documentary Hunting the Edge of Space: The Ever-Expanding Universe.[5]

Bibliography
  • Ahn, Christopher P.; Alexandroff, Rachael; Snedden, Stephanie A.; et al. (April 2014). "The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment". The Astrophysical Journal Supplement Series. 211 (2). arXiv:1307.7735. Bibcode:2014ApJS..211...17A. doi:10.1088/0067-0049/211/2/17.
  • Snedden, Stephanie A.; Gaskell, C. Martin (November 2007). "The Case for Optically Thick High-Velocity Broad-Line Region Gas in Active Galactic Nuclei". The Astrophysical Journal. 669 (1): 126–134. arXiv:astro-ph/0402508. Bibcode:2007ApJ...669..126S. doi:10.1086/521290.
  • Naohisa, Inada; Masamune, Oguri; Snedden, Stephanie A.; et al. (April 2006). "SDSS J0806+2006 and SDSS J1353+1138: Two New Gravitationally Lensed Quasars from the Sloan Digital Sky Survey". The Astronomical Journal. 131 (4): 1934–1941. arXiv:astro-ph/0512239. Bibcode:2006AJ....131.1934I. doi:10.1086/500591.
  • Schmidt, Edward G.; Lee, Kevin M.; Snedden, Stephanie A.; et al. (August 2003). "The Spectra of Type II Cepheids. I. The Hα Line in Short-Period Stars". The Astronomical Journal. 126 (2): 906–917. Bibcode:2003AJ....126..906S. doi:10.1086/376845.
gollark: And CPU. And everything else.
gollark: Also, because more numberer → more betterer, naturally.
gollark: To not end up with weird floating point errors around the edges of the world?
gollark: I downloaded all the ones I watched, which is about 187.
gollark: Plus the Distant Lands miniseries coming SOON™.

References
  1. "Stephanie Snedden". New Mexico State University. 2016. Archived from the original on 6 October 2015. Retrieved 19 February 2016.
  2. "133008 Snedden (2002 TU325)". Minor Planet Center. Retrieved 5 August 2019.
  3. Snedden, Stephanie A.; Gaskell, C. Martin (November 2007). "The Case for Optically Thick High-Velocity Broad-Line Region Gas in Active Galactic Nuclei". The Astrophysical Journal. 669 (1): 126–134. arXiv:astro-ph/0402508. Bibcode:2007ApJ...669..126S. doi:10.1086/521290.
  4. "CSWA Women in Astronomy". Committee on the Status of Women in Astronomy. American Astronomical Society. 2000. Retrieved 19 February 2016.
  5. Stephanie Snedden on IMDb
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