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Tod R. Lauer

From Wikipedia, the free encyclopedia
American astronomer (born 1957)
Tod R. Lauer
Born1957 (age 67–68)[citation needed]
Ohio, United States[citation needed]
Alma materCaltech
UC Santa Cruz
AwardsNASA Medal for Exceptional Scientific Achievement (1992)
Scientific career
FieldsAstronomy
InstitutionsNSFNOIRLab
Princeton University
ThesisHigh resolution surface photometry of elliptical galaxies (1983)
Doctoral advisorSandra M. Faber

Tod Richard Lauer (born 1957)[citation needed] is an American astronomer on the research staff of the NSFNOIRLab.

Early life and education

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Lauer studied Astronomy at theCalifornia Institute of Technology and graduated with a BS degree in 1979. He received his PhD degree in Astronomy from theUniversity of California, Santa Cruz in 1983 forHigh resolution surface photometry of elliptical galaxies.[1]

Career

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Lauer was a member of theHubble Space TelescopeWide Field and Planetary Camera team, and is a founding member of theNuker Team. His research interests includes observational searches for massiveblack holes[2] in the centers ofgalaxies, the structure ofelliptical galaxies,stellar populations,large-scale structure of the universe, and astronomicalimage processing.[3] He was the Principal Investigator of theDestinyJDEM concept study,[4] one of the precursors to theNancy Grace Roman Space Telescope mission. Asteroid3135 Lauer is named for him. He appears in an episode of the documentary seriesNaked Science.[5] He joined theNew Horizons Pluto team in order to apply his extensive experience with deep space imaging to theNew Horizons data, yielding significantly clearer and mathematically accurate images ofPluto andCharon.

Awards and honors

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An asteroid, (3135) Lauer, was named in his honor in 1981.[6] In 1992, Lauer was awarded theNASA Exceptional Scientific Achievement Medal for his work with the Wide-Field and Planetary Camera aboard the Hubble Space Telescope.[7] Lauer has been twice awarded the AURA Outstanding Achievement Award for Outstanding Science for 1993[8] and 2016[9] by theAssociation of Universities for Research in Astronomy. As a member of the New Horizons team, Lauer shared the 2017NASA Group Achievement Award.[10] As a member of theEvent Horizon Telescope collaboration, Lauer shared the 2020Breakthrough Prize in Fundamental Physics.

References

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  1. ^Lauer, Tod Richard (1983).High resolution surface photometry of elliptical galaxies (Ph.D. thesis). University of California, Santa Cruz.OCLC 964197423.ProQuest 303126469.
  2. ^Lauer, T. R.; et al. (2007). "The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes".Astrophysical Journal.662 (2):808–834.arXiv:astro-ph/0606739.Bibcode:2007ApJ...662..808L.doi:10.1086/518223.S2CID 26415900.
  3. ^Lauer, T. R. (1999). "Combining Undersampled Dithered Images".Publications of the Astronomical Society of the Pacific.111 (756):227–237.arXiv:astro-ph/9810394.Bibcode:1999PASP..111..227L.doi:10.1086/316319.S2CID 16376086.
  4. ^Benford, D. J.; Lauer, T. R. (2006). "Destiny: A candidate architecture for the Joint Dark Energy Mission". In Mather, John C; MacEwen, Howard A; De Graauw, Mattheus W. M (eds.).Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter.Proceedings of the SPIE. Vol. 6265. p. 626528.arXiv:astro-ph/0608413.Bibcode:2006SPIE.6265E..28B.doi:10.1117/12.672135.S2CID 7504996.
  5. ^"IMDB Entry for Naked Science episode #78, 'Hubble's Amazing Universe'".IMDb.
  6. ^"(3135) Lauer".Dictionary of Minor Planet Names. Berlin and Heidelberg: Springer-Verlag. 2007. p. 259.doi:10.1007/978-3-540-29925-7_3136.ISBN 978-3-540-00238-3.
  7. ^"NASA Funds Development of Destiny: The Dark Energy Space Telescope".National Optical Astronomy Observatory. August 3, 2006 – via SpaceRef Interactive.
  8. ^"AURA Award Winners 1990–2012".Association of Universities for Research in Astronomy.
  9. ^"2016 AURA Awards"(PDF).Association of Universities for Research in Astronomy. 2016.
  10. ^"New Horizons Team Earns NASA, International Awards".New Horizons. February 7, 2017 – via The Johns Hopkins University Applied Physics Laboratory.

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