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Christy A. Tremonti is an observational astronomer on the faculty at the University of Wisconsin–Madison. She was a 2005 Hubble Fellow while at the University of Arizona. She received her PhD from Johns Hopkins University in 2003 and her BS from Colgate University in 1994. She completed her dissertation, "The physical properties of low redshift star forming galaxies: Insights from the space-UV and 20,000 SDSS spectra", under the supervision of Timothy M. Heckman. Tremonti is a member of the International Astronomical Union.

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  • Christy A. Tremonti is an observational astronomer on the faculty at the University of Wisconsin–Madison. She was a 2005 Hubble Fellow while at the University of Arizona. She received her PhD from Johns Hopkins University in 2003 and her BS from Colgate University in 1994. She completed her dissertation, "The physical properties of low redshift star forming galaxies: Insights from the space-UV and 20,000 SDSS spectra", under the supervision of Timothy M. Heckman. Tremonti's primary interests involve galaxy formation and evolution, including star-forming galaxies, active galactic nucleus (AGN) feedback, galactic winds, and galaxy mergers. She is also interested in spectroscopy and data mining, and is a member of the Sloan Digital Sky Survey. She has over sixty journal articles in publications including the Astronomical Journal, Astrophysical Journal, and the Monthly Notices of the Royal Astronomical Society. Most of her articles can be found in full text on the arXiv. Tremonti has over 150 co-authors across her publications. Some of her most frequent collaborators are Timothy M. Heckman, Jon V. Brinkmann, and Donald P. Schneider. According to Scopus, her h-index as of March, 2015 is 44. As of March 15, 2015, Tremonti's top three most highly cited articles present research about the Sloan Digital Sky Survey, including the most highly cited article on which Tremonti was lead author, "The origin of the mass-metallicity relation: Insights from 53,000 star-forming galaxies in the Sloan Digital Sky Survey". She was one of the first to use the Sloan Digital Sky Survey's statistical power for galaxy evolution studies. Tremonti is a member of the International Astronomical Union. (en)
  • Christy A. Tremonti (AEB, XX.mendea) behaketa-astronomoa da Wisconsin-Madisongo Unibertsitatean. (eu)
  • Christy A. Tremonti es una astrónoma observacional en la Universidad de Wisconsin-Madison. Fue elegida para la Beca Hubble en 2005 mientras estaba en la Universidad de Arizona.​ Consiguió su Doctorado en la Universidad Johns Hopkins en 2003 y su Grado en la Universidad Colgate en 1994. Completó su disertación , "The physical properties of low redshift star forming galaxies: Insights from the space-UV and 20,000 SDSS spectra",​ bajo la supervisión del Dr. Timothy M. Heckman.​ Sus principales intereses implican la formación y evolución de las galaxias, incluyendo las galaxias formadas por estrellas, los núcleos galácticos activos (AGN), los vientos galácticos, y las fusiones de galaxias. También está interesada en la espectroscopia y la minería de datos, y es miembro de la Sloan Digital Sky Survey.​ Ha escrito más de sesenta artículos en publicaciones como Astronomical Journal, The Astrophysical Journal y Monthly Notices of the Royal Astronomical Society. La mayoría de sus artículos se encuentran completos en arXiv.org.​ Como muchos científicos, la Dra. Tremonti es altamente colaborativa, habiendo escrito con 150 co-autores a lo largo de muchas de sus publicaciones.​ Algunos de sus colaboradores frecuentes son Timothy M. Heckman,​ Jon V. Brinkmann, y Donald P. Schneider.​ De acuerdo con Scopus, su índice h a partir de marzo de 2015 es de 44.​ A partir del 15 de marzo de 2015, los tres artículos más citados de la Dra. Tremonti presentan una investigación sobre la Sloan Digital Sky Survey,.​ incluyendo el artículo más citado en el cual la Dra. Tremonti fue la autora jefa, "The origin of the mass-metallicity relation: Insights from 53,000 star-forming galaxies in the Sloan Digital Sky Survey".​ Fue una de las primeras en usar la potencia estadística para estudios de evolución de galaxias de Sloan Digital Sky Survey.​ La Dra. Tremonti es miembro de la Unión Astronómica Internacional. (es)
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  • Christy A. Tremonti (en)
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  • Associate Professor at University of Wisconsin–Madison (en)
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  • Christy A. Tremonti (AEB, XX.mendea) behaketa-astronomoa da Wisconsin-Madisongo Unibertsitatean. (eu)
  • Christy A. Tremonti is an observational astronomer on the faculty at the University of Wisconsin–Madison. She was a 2005 Hubble Fellow while at the University of Arizona. She received her PhD from Johns Hopkins University in 2003 and her BS from Colgate University in 1994. She completed her dissertation, "The physical properties of low redshift star forming galaxies: Insights from the space-UV and 20,000 SDSS spectra", under the supervision of Timothy M. Heckman. Tremonti is a member of the International Astronomical Union. (en)
  • Christy A. Tremonti es una astrónoma observacional en la Universidad de Wisconsin-Madison. Fue elegida para la Beca Hubble en 2005 mientras estaba en la Universidad de Arizona.​ Consiguió su Doctorado en la Universidad Johns Hopkins en 2003 y su Grado en la Universidad Colgate en 1994. Completó su disertación , "The physical properties of low redshift star forming galaxies: Insights from the space-UV and 20,000 SDSS spectra",​ bajo la supervisión del Dr. Timothy M. Heckman.​ La Dra. Tremonti es miembro de la Unión Astronómica Internacional. (es)
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  • Christy A. Tremonti (en)
  • Christy A. Tremonti (eu)
  • Christy A. Tremonti (es)
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  • Christy A. Tremonti (en)
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