Nicholas B. Suntzeff

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Nicholas Suntzeff
Nbs2009 02.jpg
Houston, Texas 2009
Born (1952-11-22) November 22, 1952 (age 71)
Alma mater Stanford University
University of California at Santa Cruz
Lick Observatory
Known forObservational cosmology based on supernovae
Scientific career
Fields Astronomy
Cosmology
Institutions Texas A&M University,
United States Department of State
Doctoral advisor Robert Kraft

Nicholas B. Suntzeff (born November 22, 1952, San Francisco) is an American astronomer and cosmologist. He is a university distinguished professor and holds the Mitchell/Heep/Munnerlyn Chair of Observational Astronomy in the Department of Physics & Astronomy at Texas A&M University where he is director of the Astronomy Program. He is an observational astronomer specializing in cosmology, supernovae, stellar populations, and astronomical instrumentation. With Brian Schmidt he founded the High-z Supernova Search Team, which was honored with the Nobel Prize in Physics in 2011 to Schmidt and Adam Riess.

Contents

Education

Suntzeff graduated from Neil Cummins Elementary School in Corte Madera, California and Redwood High School in Larkspur, California. He received his B.S. with distinction in mathematics from Stanford University in 1974 and his Ph.D. in astronomy & astrophysics from the University of California, Santa Cruz and Lick Observatory in 1980. While undergraduates at Stanford University, Suntzeff and engineering student Michael Kast built the Stanford Student Observatory. [1] [2]

Work

After graduating in 1980, he worked as a postdoctoral research associate with Professor George Wallerstein in the Department of Astronomy at University of Washington. From 1982 to 1986 he was a Carnegie/Las Campanas Fellow at the Mount Wilson & Las Campanas Observatories, now called the Observatories of the Carnegie Institution for Science.

After moving to Chile in 1986, Suntzeff working with Mark M. Phillips and Mario Hamuy at CTIO used the newly developed cryogenic CCD cameras to produce the first modern light curve of a Type Ia supernova. [3] The fundamental calibration for distances to Type Ia supernovae was invented by the Calán/Tololo Supernova Survey, [4] [5] founded by Mario Hamuy, Jose Maza, Mark M. Phillips, and Suntzeff. The Survey, formed after discussions at the Santa Cruz meeting on supernovae [6] and the encouragement by Allan R. Sandage to use Type Ia supernovae to measure the Hubble constant H0 and the deceleration parameter q0, ran from 1990 to 1995, and provided the pioneering method to measure precision distances to external galaxies, [7] leading to a precise value of the Hubble constant. [8] [9]

Continuing the work of the Calán/Tololo Survey, Suntzeff with Brian P. Schmidt co-founded the High-Z Supernova Search Team in 1994 that used observations of extragalactic supernovae to discover the accelerating universe. [10] [11] This universal acceleration implies the existence of dark energy consistent with the cosmological constant of Albert Einstein's theory of General Relativity, and was voted the top science breakthrough of 1998 by Science magazine. [12]

Prior to 2006, he was the associate director of science at the US National Optical Astronomy Observatory, and astronomer at Cerro Tololo Inter-American Observatory. In 2007, he was elected councilor of the American Astronomical Society, and in 2010, he was elected vice president of the same society. He has been awarded a 2010 Jefferson Senior Science Fellowship [13] of the National Academy of Sciences to work at the US Department of State where he is a Humanitarian Affairs Officer in the Bureau of Human Rights of the Office of International Organization Affairs. He is also an adjunct professor in the Department of Astronomy at the University of Texas at Austin.

In announcing his award as a 2023 American Astronomical Society Fellow, he was cited "For his transformational leadership in the foundation of supernova cosmology, the discovery of the accelerated expansion of the universe, and precision measurements of the Hubble–Lemaître flow; for his service to the national and international astronomical communities; for considerable efforts on behalf of human rights, especially the LGBTQ community, both within astronomy and globally; and for establishing the astronomy program at Texas A&M University." [14]

Honors and awards


Ancestry and personal life

He is a native of San Francisco and grew up in Corte Madera, California. He is the paternal grandson of Matvei Andrianovich Evdokimov (1887–1920) (Russian: Матвей Андрианович Евдокимов), one of the principal private arms manufacturers in czarist Russia, located in Izhevsk. [31] The Evdokimov factory in Izhevsk began in the 1860s by Andrian Nikandrovich Evdokimov (1844–1917 (Russian: Андриан Никандрович Евдокимов), and by 1890, was manufacturing Mosin–Nagant and Berdan rifles. [31] [32] They continued production until the Russian Civil War in 1917. These rifles were used during the Revolution and World War I, [33] and were retooled for use during World War II, especially by the Finnish Army.

Although not supporters of the White cause, for their safety the family of Matvei fled east with Admiral Kolchak, the White Army, and the Czech Legion when the Whites captured Perm in 1918. [34] Matvei died at Manchurian Station (Manzhouli) near Chita. His only child, Nicholai Matveevich Evdiokimov (1918–1995) (Russian: Николай Матвеевич Евдокимов) continued with Matvei's wife Zoya Vasilevna Suntzeva (Russian: Зоя Васильевна Сунцевa) (1897–1976), with the Suntzeff family to Harbin China and then to the San Francisco in 1928. Nicholai assumed the last name of his mother and immigrated into the US as Nicholas Matveevich Suntzeff (Russian: Николай Матвеевич Сунцев). The Suntzeff family, prominent merchants from the Ural region, came from Motovilikha (now part of Perm, Russia) and have ancestry in the Udmurt people. A bridge "Сунцев мост" in Motovilikha was named after the family store nearby. [35]

Suntzeff is mentioned in the Alan Alda memoir, Never Have Your Dog Stuffed: and Other Things I've Learned. [36]

Related Research Articles

<span class="mw-page-title-main">Supernova</span> Explosion of a star at its end of life

A supernova is a powerful and luminous explosion of a star. A supernova occurs during the last evolutionary stages of a massive star, or when a white dwarf is triggered into runaway nuclear fusion. The original object, called the progenitor, either collapses to a neutron star or black hole, or is completely destroyed to form a diffuse nebula. The peak optical luminosity of a supernova can be comparable to that of an entire galaxy before fading over several weeks or months.

<span class="mw-page-title-main">SN 1987A</span> 1987 supernova event in the constellation Dorado

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<span class="mw-page-title-main">Type Ia supernova</span> Type of supernova in binary systems

A Type Ia supernova is a type of supernova that occurs in binary systems in which one of the stars is a white dwarf. The other star can be anything from a giant star to an even smaller white dwarf.

<span class="mw-page-title-main">Robert Kirshner</span> American astronomer

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The Supernova Cosmology Project is one of two research teams that determined the likelihood of an accelerating universe and therefore a positive cosmological constant, using data from the redshift of Type Ia supernovae. The project is headed by Saul Perlmutter at Lawrence Berkeley National Laboratory, with members from Australia, Chile, France, Portugal, Spain, Sweden, the United Kingdom, and the United States.

<span class="mw-page-title-main">Alex Filippenko</span> American astrophysicist

Alexei Vladimir "Alex" Filippenko is an American astrophysicist and professor of astronomy at the University of California, Berkeley. Filippenko graduated from Dos Pueblos High School in Goleta, California. He received a Bachelor of Arts in physics from the University of California, Santa Barbara in 1979 and a Ph.D. in astronomy from the California Institute of Technology in 1984, where he was a Hertz Foundation Fellow. He was a postdoctoral Miller Fellow at Berkeley from 1984 to 1986 and was appointed to Berkeley's faculty in 1986. In 1996 and 2005, he was a Miller Research Professor, and he is currently a Senior Miller Fellow. His research focuses on supernovae and active galaxies at optical, ultraviolet, and near-infrared wavelengths, as well as on black holes, gamma-ray bursts, and the expansion of the Universe.

<span class="mw-page-title-main">High-Z Supernova Search Team</span> International cosmology research group (1994–2002)

The High-Z Supernova Search Team was an international cosmology collaboration which used Type Ia supernovae to chart the expansion of the universe. The team was formed in 1994 by Brian P. Schmidt, then a post-doctoral research associate at Harvard University, and Nicholas B. Suntzeff, a staff astronomer at the Cerro Tololo Inter-American Observatory (CTIO) in Chile. The original team submitted a proposal on September 29, 1994 called A Pilot Project to Search for Distant Type Ia Supernova to the CTIO. The team on the first observing proposal comprised: Nicholas Suntzeff (PI); Brian Schmidt (Co-I); R. Chris Smith, Robert Schommer, Mark M. Phillips, Mario Hamuy, Roberto Aviles, Jose Maza, Adam Riess, Robert Kirshner, Jason Spiromilio, and Bruno Leibundgut. The project was awarded four nights of telescope time on the CTIO Víctor M. Blanco Telescope on the nights of February 25, 1995, and March 6, 24, and 29, 1995. The pilot project led to the discovery of supernova SN1995Y. In 1995, the HZT elected Brian P. Schmidt of the Mount Stromlo Observatory which is part of the Australian National University to manage the team.

<span class="mw-page-title-main">Adam Riess</span> American astrophysicist (born 1969)

Adam Guy Riess is an American astrophysicist and Bloomberg Distinguished Professor at Johns Hopkins University and the Space Telescope Science Institute. He is known for his research in using supernovae as cosmological probes. Riess shared both the 2006 Shaw Prize in Astronomy and the 2011 Nobel Prize in Physics with Saul Perlmutter and Brian P. Schmidt for providing evidence that the expansion of the universe is accelerating.

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Mark M. Phillips (born March 31, 1951) is an American astronomer who works on the observational studies of all classes of supernovae. He has worked on SN 1986G, SN 1987A, the Calán/Tololo Supernova Survey, the High-Z Supernova Search Team, and the Phillips relationship. This relationship has allowed the use of Type Ia supernovae as standard candles, leading to the precise measurements of the Hubble constant H0 and the deceleration parameter q0, the latter implying the existence of dark energy or a cosmological constant in the Universe.

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<span class="mw-page-title-main">Calán/Tololo Survey</span>

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<span class="mw-page-title-main">Phillips relationship</span> Relationship in astrophysics

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Maryam Modjaz is a German-American astrophysicist who is a professor and Director of Equity and Inclusion at the New York University. Her research considers the death of massive stars. She was awarded an Alexander von Humboldt Foundation Fellowship in 2018, which she spent at the Max Planck Institute for Astronomy.

References

  1. "Student Observatory". physics.stanford.edu.
  2. "Domains: Eye on the Sky". alumni.stanford.edu.
  3. Phillips, M. M.; et al. (July 1987). "The Type Ia Supernova 1986G in NGC 5128 - Optical Photometry and Spectra". Publications of the Astronomical Society of the Pacific . 99: 592–605. Bibcode:1987PASP...99..592P. doi:10.1086/132020.
  4. Phillips, M. M. (August 1993). "The absolute magnitudes of Type IA supernovae". Astrophysical Journal Letters. 413: L105–L108. Bibcode:1993ApJ...413L.105P. doi:10.1086/186970.
  5. Hamuy, M.; et al. (December 1993). "The 1990 Calan/Tololo Supernova Search" (PDF). The Astronomical Journal. 106 (6): 2392–2407. Bibcode:1993AJ....106.2392H. doi:10.1086/116811.
  6. Supernovae. The Tenth Santa Cruz Workshop in Astronomy and Astrophysics, held July 9–21, 1989, Lick Observatory. Editor, S.E. Woosley; Springer-Verlag, New York, 1991.
  7. Hamuy, M.; et al. (1996). "The Morphology of Type IA Supernovae Light Curves". The Astronomical Journal. 112: 2438–2447. arXiv: astro-ph/9609063 . Bibcode:1996AJ....112.2438H. doi:10.1086/118193. S2CID   18539194.
  8. Suntzeff, N.B.; et al. (March 1999). "Optical Light Curve of the Type IA Supernova 1998BU in M96 and the Supernova Calibration of the Hubble Constant". The Astronomical Journal. 117 (3): 1175–1184. arXiv: astro-ph/9811205 . Bibcode:1999AJ....117.1175S. doi:10.1086/300771. S2CID   119332674.
  9. Freedman, W. (2001). "Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant". The Astrophysical Journal. 553 (1): 47–72. arXiv: astro-ph/0012376 . Bibcode:2001ApJ...553...47F. doi:10.1086/320638. S2CID   119097691.
  10. Riess, A.; et al. (1998). "Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant". The Astronomical Journal. 116 (3): 1009–1038. arXiv: astro-ph/9805201 . Bibcode:1998AJ....116.1009R. doi:10.1086/300499. S2CID   15640044.
  11. Perlmutter, S.; et al. (1999). "Measurements of Omega and Lambda from 42 High-Redshift Supernovae". The Astrophysical Journal. 517 (2): 565–586. arXiv: astro-ph/9812133 . Bibcode:1999ApJ...517..565P. doi:10.1086/307221. S2CID   118910636.
  12. James Glanz (18 December 1998). "BREAKTHROUGH OF THE YEAR: ASTRONOMY: Cosmic Motion Revealed". Science. 282 (5397): 2156–2157. Bibcode:1998Sci...282.2156G. doi:10.1126/science.282.5397.2156a. S2CID   117807831.
  13. 1 2 "Jefferson Science Fellowship". nationalacademies.org. 19 February 2015.
  14. "AAS Names 22 New Fellows for 2023".
  15. "ASP: Past Winners of the Trumpler Award". astrosociety.org.
  16. "Recent Fellows at the Carnegie Observatories". The Carnegie Observatories.
  17. "AURA Awards". aura-astronomy.org. Archived from the original on 2003-03-29. Retrieved 2008-01-15.
  18. James Glanz (1998). "BREAKTHROUGH OF THE YEAR. ASTRONOMY: Cosmic Motion Revealed". Science . 282 (5397): 2156–2157. Bibcode:1998Sci...282.2156G. doi:10.1126/science.282.5397.2156a. S2CID   117807831.
  19. "Chairs and Professorships". science.tamu.edu. Archived from the original on 2016-07-21. Retrieved 2015-09-06.
  20. "| College of Science, Texas A&M University". Archived from the original on 2016-07-21. Retrieved 2015-09-06.
  21. "Brian Schmidt & the High-z Supernova Search Team". yale.edu.
  22. "Association of Former Students University-level Distinguished Achievement Awards". tamu.edu. Archived from the original on 2014-12-17.
  23. "List of Distinguished Professors". tamu.edu. Archived from the original on 2013-12-20.
  24. "PPO - Bush Excellence Awards for Faculty". tamu.edu. Archived from the original on 2018-10-19. Retrieved 2014-12-17.
  25. "Breakthrough Prize". breakthroughprize.org.
  26. "APS Fellow Archive".
  27. "Regents Recognize Exemplary Faculty and Professionals". 2017-11-03.
  28. "Suntzeff Elected As 2023 American Astronomical Society Fellow". Archived from the original on 2023-05-17. Retrieved 2023-02-17.
  29. "17 Faculty Elected 2023 Fellows of the American Association for the Advancement of Science". 18 April 2024.
  30. "2023 AAAS Fellows | American Association for the Advancement of Science (AAAS)".
  31. 1 2 Алексеева, Эрнестина Витальевна (2009). Родословная ижевских фабрикантов охотничьего оружия. XIX-XX вв. Ижевск: КнигоГрад. ISBN   978-5-9631-0053-0.
  32. "Arms factory of A.N. Evdokimov | Qirme.org". Archived from the original on 2016-03-06. Retrieved 2014-11-01.
  33. "Удмуртская правда / Сельский обыватель - оружейник, фабрикант - филантроп". udmpravda.ru. Archived from the original on 2014-12-15. Retrieved 2014-11-24.
  34. "Missouri Women in the Health Sciences - In Her Words - Valentina Suntzeff - Autobiography (Chapter 1)". wustl.edu.
  35. "Сунцев мост - Мотовилиха - Фотографии старинной Перми - Фотоальбом - Неизвестная Пермь".
  36. Alda, Alan (2006). Never Have Your Dog Stuffed: and Other Things I've Learned . New York: Random House. ISBN   978-1-4000-6409-0.