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Sangeeta Malhotra

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Sangeeta Malhotra
EducationDelhi University (BA, Physics, 1988)
Indian Institute of Technology, Kanpur (M.A., Physics, 1990)
Princeton University(Ph.D., 1995)
OccupationAstrophysicist

Sangeeta Malhotra is an astrophysicist who studies galaxies, their contents, and their effects on the universe around them. The objects she studies range from our own Milky Way galaxy to some of the earliest and most distant known galaxies in the epoch of cosmic dawn.

Malhotra works at the NASA Goddard Space Flight Center, where she is part of the Nancy Grace Roman Space Telescope project.[1] She was previously a tenured full professor at Arizona State University.

Education

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Malhotra received her bachelor's degree in Physics from Delhi University in 1988, and her Master's degree in Physics from the Indian Institute of Technology - Kanpur in 1990. In 1995, she became the first woman of color to receive a PhD in Astrophysics from Princeton University.[1] Her Ph.D. supervisor at Princeton was Professor Gillian Knapp. Malhotra's Ph.D. thesis examined the distribution of atomic and molecular gas in the Milky Way galaxy. Results from her thesis work are reproduced in the textbook "Galactic Structure", by Binney and Merrifield.[2]

Career

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After completing her Ph.D., Malhotra first held a postdoctoral fellowship at the California Institute of Technology.[1] She next won a NASA Hubble Fellowship, which she held at the National Optical Astronomy Observatory in Tucson and subsequently at the Johns Hopkins University in Baltimore, Maryland. She then joined the science staff at the Space Telescope Science Institute in Baltimore, where she worked from 2001-2005. She moved to a faculty position at Arizona State University in Tempe, Arizona in 2006, where she helped build up the new School of Earth and Space Exploration.[1] She moved to NASA's Goddard Space Flight Center in early 2017 to take up a position working on development of the Nancy Grace Roman Space Telescope.

Research

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Infrared Properties of Galaxies

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Malhotra and collaborators used Infrared Space Observatory data to study the far-infrared line emission from galaxies. In particular, she demonstrated that the 158 micron emission line of ionized carbon becomes a relatively less prominent spectral feature in galaxies with higher infrared luminosity and/or warmer interstellar dust.[3][4]

Lyman Alpha Galaxies and Cosmological Reionization

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Malhotra initiated the Large Area Lyman Alpha survey[5] in the late 1990s. This was one of the first research projects to successfully identify galaxies in the early universe using their Lyman alpha emission lines, a method that had been first proposed in 1967 by Bruce Partridge and Jim Peebles.[6] She has gone on to study galaxies with strong Lyman alpha lines in detail. In particular, she demonstrated that they tend to be young, with extreme star formation properties[7] and (for galaxies) small sizes.[8]

She also pioneered the technique of using Lyman alpha galaxies to study cosmological reionization, leading a 2004 paper that demonstrated that the gas between galaxies was already mostly ionized at redshift 6.5, when the universe was less than a billion years old.[9] Recently, she, her former Ph.D. student V. S. Tilvi, and other collaborators identified the most distant galaxy group so far known (EGS77), and found evidence that these galaxies are ionizing their surroundings.[10][11] She is the US principal investigator of the ongoing multinational LAGER project (Lyman Alpha Galaxies in the Epoch of Reionization), which is identifying hundreds of Lyman alpha galaxies in the epoch of cosmic dawn.

Slitless Spectroscopy from Space

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Malhotra has led three Hubble Space Telescope treasury programs[12] (GRAPES, PEARS, and FIGS[13]) that have collectively advanced the application of slitless spectroscopic observations from space. While initially designed to identify galaxies in the distant universe,[14][15][16] these projects have also proven invaluable for identifying galaxies at intermediate distances,[17] studying the chemical compositions of those galaxies,[18][19] and even studying stars in our own Galaxy.[20] Further developments of these techniques form a core part of the planned observing programs for ESA's Euclid mission and NASA's Roman mission, and Malhotra is helping develop plans for the Roman application.

Pea galaxies

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Malhotra has directed multiple PhD students in studying Green Pea galaxies. She and her collaborators have demonstrated that these comparatively local objects bear striking similarities to Lyman alpha galaxies in the early universe,[21][22] which is valuable because the pea galaxies are easier to study in detail than their more distant counterparts.[citation needed]

Students

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Malhotra has advised over a half dozen Ph.D. thesis students, including Steven Finkelstein, Nimish Hathi, Vithal Tilvi, Lifang Xia, Huan Yang, Tianxing Jiang, and John Pharo.[23]

Awards and honors

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Malhotra was awarded a NASA Hubble Fellowship in 1998.[24]
She is a Legacy Fellow of the American Astronomical Society.[25]

References

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  1. ^ a b c d "Bio - Sangeeta Malhotra". science.gsfc.nasa.gov. Retrieved 9 May 2020.
  2. ^ Binney, James, 1950- (1998). Galactic astronomy. Merrifield, Michael, 1964-. Princeton, NJ: Princeton University Press. ISBN 0-691-00402-1. OCLC 39108765.{{cite book}}: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link)
  3. ^ Malhotra, S.; Helou, G.; Stacey, G.; Hollenbach, D.; Lord, S.; Beichman, C. A.; Dinerstein, H.; Hunter, D. A.; Lo, K. Y.; Lu, N. Y.; Rubin, R. H. (10 December 1997). "Infrared Space Observatory Measurements of [C ii] Line Variations in Galaxies". The Astrophysical Journal. 491 (1): L27–L30. doi:10.1086/311044.
  4. ^ Malhotra, S.; Kaufman, M. J.; Hollenbach, D.; Helou, G.; Rubin, R. H.; Brauher, J.; Dale, D.; Lu, N. Y.; Lord, S.; Stacey, G.; Contursi, A. (10 November 2001). "Far‐Infrared Spectroscopy of Normal Galaxies: Physical Conditions in the Interstellar Medium". The Astrophysical Journal. 561 (2): 766–786. arXiv:astro-ph/0106485. Bibcode:2001ApJ...561..766M. doi:10.1086/323046. ISSN 0004-637X.
  5. ^ Rhoads, James E.; Malhotra, Sangeeta; Dey, Arjun; Stern, Daniel; Spinrad, Hyron; Jannuzi, Buell T. (20 December 2000). "First Results from the Large-Area Lyman Alpha Survey". The Astrophysical Journal. 545 (2): L85–L88. arXiv:astro-ph/0003465. Bibcode:2000ApJ...545L..85R. doi:10.1086/317874. S2CID 16732902.
  6. ^ Partridge, R. B.; Peebles, P. J. E. (1967). "Are Young Galaxies Visible?". The Astrophysical Journal. 147: 868. Bibcode:1967ApJ...147..868P. doi:10.1086/149079. ISSN 0004-637X.
  7. ^ Malhotra, Sangeeta; Rhoads, James E. (1 February 2002). "Large Equivalent Width L[CLC]y[/CLC]α line Emission at z=4.5: Young Galaxies in a Young Universe?". The Astrophysical Journal. 565 (2): L71–L74. arXiv:astro-ph/0111126. doi:10.1086/338980.
  8. ^ Malhotra, Sangeeta; Rhoads, James E.; Finkelstein, Steven L.; Hathi, Nimish; Nilsson, Kim; McLinden, Emily; Pirzkal, Norbert (10 May 2012). "SIZING UP Lyα AND LYMAN BREAK GALAXIES". The Astrophysical Journal. 750 (2): L36. arXiv:1106.2816. Bibcode:2012ApJ...750L..36M. doi:10.1088/2041-8205/750/2/L36. ISSN 2041-8205. S2CID 119194628.
  9. ^ Malhotra, Sangeeta; Rhoads, James E. (10 December 2004). "Luminosity Functions of Lyα Emitters at Redshifts z = 6.5 and z = 5.7: Evidence against Reionization at z ≤ 6.5". The Astrophysical Journal. 617 (1): L5–L8. arXiv:astro-ph/0407408. Bibcode:2004ApJ...617L...5M. doi:10.1086/427182. ISSN 0004-637X. S2CID 118915884.
  10. ^ Jenner, Lynn (31 December 2019). "Astronomers Spot Distant Galaxy Group Driving Ancient Cosmic Makeover". NASA. Retrieved 9 May 2020.
  11. ^ Tilvi, V.; Malhotra, S.; Rhoads, J. E.; Coughlin, A.; Zheng, Z.; Finkelstein, S. L.; Veilleux, S.; Mobasher, B.; Wang, J.; Probst, R.; Swaters, R. (27 February 2020). "Onset of Cosmic Reionization: Evidence of an Ionized Bubble Merely 680 Myr after the Big Bang". The Astrophysical Journal. 891 (1): L10. arXiv:2001.00873. Bibcode:2020ApJ...891L..10T. doi:10.3847/2041-8213/ab75ec. ISSN 2041-8213. S2CID 209832401.
  12. ^ "HST Treasury Proposals". archive.stsci.edu. Retrieved 8 May 2020.
  13. ^ Pirzkal, Norbert; Malhotra, Sangeeta; Ryan, Russell E.; Rothberg, Barry; Grogin, Norman; Finkelstein, Steven L.; Koekemoer, Anton M.; Rhoads, James; Larson, Rebecca L.; Christensen, Lise; Cimatti, Andrea (1 September 2017). "FIGS—Faint Infrared Grism Survey: Description and Data Reduction". The Astrophysical Journal. 846 (1): 84. arXiv:1706.02669. Bibcode:2017ApJ...846...84P. doi:10.3847/1538-4357/aa81cc. hdl:10150/625750. ISSN 1538-4357. S2CID 38863528.
  14. ^ Malhotra, S.; Rhoads, J. E.; Pirzkal, N.; Haiman, Z.; Xu, C.; Daddi, E.; Yan, H.; Bergeron, L. E.; Wang, J.; Ferguson, H. C.; Gronwall, C. (20 June 2005). "An Overdensity of Galaxies at z = 5.9 + 0.2 in the Hubble Ultra Deep Field Confirmed Using the ACS Grism". The Astrophysical Journal. 626 (2): 666–679. arXiv:astro-ph/0501478. Bibcode:2005ApJ...626..666M. doi:10.1086/430047. ISSN 0004-637X. S2CID 55026837.
  15. ^ Rhoads, James E.; Malhotra, Sangeeta; Stern, Daniel; Dickinson, Mark; Pirzkal, Norbert; Spinrad, Hyron; Reddy, Naveen; Hathi, Nimish; Grogin, Norman; Koekemoer, Anton; Peth, Michael A. (22 July 2013). "A Lyman Break Galaxy in the Epoch of Reionization Fromhubble Space Telescopegrism Spectroscopy". The Astrophysical Journal. 773 (1): 32. arXiv:1302.7005. Bibcode:2013ApJ...773...32R. doi:10.1088/0004-637X/773/1/32. ISSN 0004-637X.
  16. ^ Tilvi, V.; Pirzkal, N.; Malhotra, S.; Finkelstein, S. L.; Rhoads, J. E.; Windhorst, R.; Grogin, N. A.; Koekemoer, A.; Zakamska, N. L.; Ryan, R.; Christensen, L. (5 August 2016). "FIRST RESULTS FROM THE FAINT INFRARED GRISM SURVEY (FIGS): FIRST SIMULTANEOUS DETECTION OF Ly α EMISSION AND LYMAN BREAK FROM A GALAXY AT z = 7.51". The Astrophysical Journal. 827 (1): L14. arXiv:1605.06519. Bibcode:2016ApJ...827L..14T. doi:10.3847/2041-8205/827/1/L14. ISSN 2041-8213. S2CID 119295160.
  17. ^ Pirzkal, N.; Xu, C.; Ferreras, I.; Malhotra, S.; Mobasher, B.; Rhoads, J. E.; Pasquali, A.; Panagia, N.; Koekemoer, A. M.; Ferguson, H. C.; Gronwall, C. (10 January 2006). "Morphology and Evolution of Emission‐Line Galaxies in the Hubble Ultra Deep Field". The Astrophysical Journal. 636 (2): 582–591. arXiv:astro-ph/0509551. Bibcode:2006ApJ...636..582P. doi:10.1086/498129. ISSN 0004-637X. S2CID 6560960.
  18. ^ Xia, Lifang; Malhotra, Sangeeta; Rhoads, James; Pirzkal, Nor; Straughn, Amber; Finkelstein, Steven; Cohen, Seth; Kuntschner, Harald; Kümmel, Martin; Walsh, Jeremy; Windhorst, Rogier A. (1 July 2012). "METALLICITIES OF EMISSION-LINE GALAXIES FROM HST ACS PEARS AND HST WFC3 ERS GRISM SPECTROSCOPY AT 0.6 < z < 2.4". The Astronomical Journal. 144 (1): 28. arXiv:1205.3172. Bibcode:2012AJ....144...28X. doi:10.1088/0004-6256/144/1/28. ISSN 0004-6256. S2CID 118501972.
  19. ^ Pharo, John; Malhotra, Sangeeta; Rhoads, James; Christensen, Lise; Finkelstein, Steven L.; Grogin, Norman; Harish, Santosh; Jiang, Tianxing; Kim, Keunho; Koekemoer, Anton; Pirzkal, Norbert (29 March 2019). "Emission-line Metallicities from the Faint Infrared Grism Survey and VLT/MUSE". The Astrophysical Journal. 874 (2): 125. arXiv:1810.12342. Bibcode:2019ApJ...874..125P. doi:10.3847/1538-4357/ab08ec. hdl:11585/732007. ISSN 1538-4357. S2CID 56066945.
  20. ^ Pirzkal, N.; Sahu, K. C.; Burgasser, A.; Moustakas, L. A.; Xu, C.; Malhotra, S.; Rhoads, J. E.; Koekemoer, A. M.; Nelan, E. P.; Windhorst, R. A.; Panagia, N. (20 March 2005). "Stars in the Hubble Ultra Deep Field". The Astrophysical Journal. 622 (1): 319–332. arXiv:astro-ph/0412097. Bibcode:2005ApJ...622..319P. doi:10.1086/427896. ISSN 0004-637X. S2CID 7588745.
  21. ^ Yang, Huan; Malhotra, Sangeeta; Gronke, Max; Rhoads, James E.; Dijkstra, Mark; Jaskot, Anne; Zheng, Zhenya; Wang, Junxian (30 March 2016). "GREEN PEA GALAXIES REVEAL SECRETS OF Ly α ESCAPE". The Astrophysical Journal. 820 (2): 130. arXiv:1506.02885. Bibcode:2016ApJ...820..130Y. doi:10.3847/0004-637X/820/2/130. ISSN 1538-4357. S2CID 118400206.
  22. ^ Yang, Huan; Malhotra, Sangeeta; Gronke, Max; Rhoads, James E.; Leitherer, Claus; Wofford, Aida; Jiang, Tianxing; Dijkstra, Mark; Tilvi, V.; Wang, Junxian (3 August 2017). "Ly α Profile, Dust, and Prediction of Ly α Escape Fraction in Green Pea Galaxies". The Astrophysical Journal. 844 (2): 171. arXiv:1701.01857. Bibcode:2017ApJ...844..171Y. doi:10.3847/1538-4357/aa7d4d. hdl:10852/60241. ISSN 1538-4357. S2CID 56422449.
  23. ^ "Sangeeta Malhotra - The Mathematics Genealogy Project". genealogy.math.ndsu.nodak.edu. Retrieved 9 May 2020.
  24. ^ "2017 and Prior Fellows". STScI.edu. Retrieved 8 May 2020.
  25. ^ "AAS Fellows Program | American Astronomical Society". aas.org. Retrieved 8 May 2020.
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