Biography:Sangeeta Malhotra

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Short description: Astrophysicist
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

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

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

Infrared Properties of Galaxies

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

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

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

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.

Students

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

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

References

  1. ↑ 1.0 1.1 1.2 1.3 "Bio - Sangeeta Malhotra" (in en). https://science.gsfc.nasa.gov/sed/bio/sangeeta.malhotra. 
  2. ↑ Binney, James, 1950- (1998). Galactic astronomy. Merrifield, Michael, 1964-. Princeton, NJ: Princeton University Press. ISBN 0-691-00402-1. OCLC 39108765. https://www.worldcat.org/oclc/39108765. 
  3. ↑ Malhotra, S.; Helou, G.; Stacey, G.; Hollenbach, D.; Lord, S.; Beichman, C. A.; Dinerstein, H.; Hunter, D. A. et al. (1997-12-10). "[ITAL]Infrared Space Observatory[/ITAL] Measurements of [C [CSC]ii[/CSC]] Line Variations in Galaxies". The Astrophysical Journal 491 (1): L27–L30. doi:10.1086/311044. https://iopscience.iop.org/article/10.1086/311044. 
  4. ↑ Malhotra, S.; Kaufman, M. J.; Hollenbach, D.; Helou, G.; Rubin, R. H.; Brauher, J.; Dale, D.; Lu, N. Y. et al. (2001-11-10). "Far‐Infrared Spectroscopy of Normal Galaxies: Physical Conditions in the Interstellar Medium" (in en). The Astrophysical Journal 561 (2): 766–786. doi:10.1086/323046. ISSN 0004-637X. https://iopscience.iop.org/article/10.1086/323046. 
  5. ↑ Rhoads, James E.; Malhotra, Sangeeta; Dey, Arjun; Stern, Daniel; Spinrad, Hyron; Jannuzi, Buell T. (2000-12-20). "First Results from the Large-Area Lyman Alpha Survey". The Astrophysical Journal 545 (2): L85–L88. doi:10.1086/317874. https://iopscience.iop.org/article/10.1086/317874. 
  6. ↑ Partridge, R. B.; Peebles, P. J. E. (1967). "Are Young Galaxies Visible?" (in en). The Astrophysical Journal 147: 868. doi:10.1086/149079. ISSN 0004-637X. http://adsabs.harvard.edu/doi/10.1086/149079. 
  7. ↑ Malhotra, Sangeeta; Rhoads, James E. (2002-02-01). "Large Equivalent Width L[CLCy[/CLC]α line Emission at [FORMULA][F]z=4.5[/F][/FORMULA]: Young Galaxies in a Young Universe?"]. The Astrophysical Journal 565 (2): L71–L74. doi:10.1086/338980. https://iopscience.iop.org/article/10.1086/338980. 
  8. ↑ Malhotra, Sangeeta; Rhoads, James E.; Finkelstein, Steven L.; Hathi, Nimish; Nilsson, Kim; McLinden, Emily; Pirzkal, Norbert (2012-05-10). "SIZING UP Lyα AND LYMAN BREAK GALAXIES". The Astrophysical Journal 750 (2): L36. doi:10.1088/2041-8205/750/2/L36. ISSN 2041-8205. https://iopscience.iop.org/article/10.1088/2041-8205/750/2/L36. 
  9. ↑ Malhotra, Sangeeta; Rhoads, James E. (2004-12-10). "Luminosity Functions of Lyα Emitters at Redshifts z = 6.5 and z = 5.7: Evidence against Reionization at z ≤ 6.5" (in en). The Astrophysical Journal 617 (1): L5–L8. doi:10.1086/427182. ISSN 0004-637X. https://iopscience.iop.org/article/10.1086/427182. 
  10. ↑ Jenner, Lynn (2019-12-31). "Astronomers Spot Distant Galaxy Group Driving Ancient Cosmic Makeover". http://www.nasa.gov/feature/goddard/2020/astronomers-spot-distant-galaxy-group-driving-ancient-cosmic-makeover. 
  11. ↑ Tilvi, V.; Malhotra, S.; Rhoads, J. E.; Coughlin, A.; Zheng, Z.; Finkelstein, S. L.; Veilleux, S.; Mobasher, B. et al. (2020-02-27). "Onset of Cosmic Reionization: Evidence of an Ionized Bubble Merely 680 Myr after the Big Bang". The Astrophysical Journal 891 (1): L10. doi:10.3847/2041-8213/ab75ec. ISSN 2041-8213. https://iopscience.iop.org/article/10.3847/2041-8213/ab75ec. 
  12. ↑ "HST Treasury Proposals". http://archive.stsci.edu/hst/treasury.html. 
  13. ↑ Pirzkal, Norbert; Malhotra, Sangeeta; Ryan, Russell E.; Rothberg, Barry; Grogin, Norman; Finkelstein, Steven L.; Koekemoer, Anton M.; Rhoads, James et al. (2017-09-01). "FIGS—Faint Infrared Grism Survey: Description and Data Reduction" (in en). The Astrophysical Journal 846 (1): 84. doi:10.3847/1538-4357/aa81cc. ISSN 1538-4357. https://iopscience.iop.org/article/10.3847/1538-4357/aa81cc. 
  14. ↑ Malhotra, S.; Rhoads, J. E.; Pirzkal, N.; Haiman, Z.; Xu, C.; Daddi, E.; Yan, H.; Bergeron, L. E. et al. (2005-06-20). "An Overdensity of Galaxies at z = 5.9 + 0.2 in the Hubble Ultra Deep Field Confirmed Using the ACS Grism" (in en). The Astrophysical Journal 626 (2): 666–679. doi:10.1086/430047. ISSN 0004-637X. https://iopscience.iop.org/article/10.1086/430047. 
  15. ↑ Rhoads, James E.; Malhotra, Sangeeta; Stern, Daniel; Dickinson, Mark; Pirzkal, Norbert; Spinrad, Hyron; Reddy, Naveen; Hathi, Nimish et al. (2013-07-22). "A Lyman Break Galaxy in the Epoch of Reionization Fromhubble Space Telescopegrism Spectroscopy". The Astrophysical Journal 773 (1): 32. doi:10.1088/0004-637X/773/1/32. ISSN 0004-637X. https://iopscience.iop.org/article/10.1088/0004-637X/773/1/32. 
  16. ↑ Tilvi, V.; Pirzkal, N.; Malhotra, S.; Finkelstein, S. L.; Rhoads, J. E.; Windhorst, R.; Grogin, N. A.; Koekemoer, A. et al. (2016-08-05). "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. doi:10.3847/2041-8205/827/1/L14. ISSN 2041-8213. https://iopscience.iop.org/article/10.3847/2041-8205/827/1/L14. 
  17. ↑ Pirzkal, N.; Xu, C.; Ferreras, I.; Malhotra, S.; Mobasher, B.; Rhoads, J. E.; Pasquali, A.; Panagia, N. et al. (2006-01-10). "Morphology and Evolution of Emission‐Line Galaxies in the Hubble Ultra Deep Field" (in en). The Astrophysical Journal 636 (2): 582–591. doi:10.1086/498129. ISSN 0004-637X. https://iopscience.iop.org/article/10.1086/498129. 
  18. ↑ Xia, Lifang; Malhotra, Sangeeta; Rhoads, James; Pirzkal, Nor; Straughn, Amber; Finkelstein, Steven; Cohen, Seth; Kuntschner, Harald et al. (2012-07-01). "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. doi:10.1088/0004-6256/144/1/28. ISSN 0004-6256. https://iopscience.iop.org/article/10.1088/0004-6256/144/1/28. 
  19. ↑ Pharo, John; Malhotra, Sangeeta; Rhoads, James; Christensen, Lise; Finkelstein, Steven L.; Grogin, Norman; Harish, Santosh; Jiang, Tianxing et al. (2019-03-29). "Emission-line Metallicities from the Faint Infrared Grism Survey and VLT/MUSE". The Astrophysical Journal 874 (2): 125. doi:10.3847/1538-4357/ab08ec. ISSN 1538-4357. https://iopscience.iop.org/article/10.3847/1538-4357/ab08ec. 
  20. ↑ Pirzkal, N.; Sahu, K. C.; Burgasser, A.; Moustakas, L. A.; Xu, C.; Malhotra, S.; Rhoads, J. E.; Koekemoer, A. M. et al. (2005-03-20). "Stars in the Hubble Ultra Deep Field" (in en). The Astrophysical Journal 622 (1): 319–332. doi:10.1086/427896. ISSN 0004-637X. https://iopscience.iop.org/article/10.1086/427896. 
  21. ↑ Yang, Huan; Malhotra, Sangeeta; Gronke, Max; Rhoads, James E.; Dijkstra, Mark; Jaskot, Anne; Zheng, Zhenya; Wang, Junxian (2016-03-30). "GREEN PEA GALAXIES REVEAL SECRETS OF Ly α ESCAPE". The Astrophysical Journal 820 (2): 130. doi:10.3847/0004-637X/820/2/130. ISSN 1538-4357. https://iopscience.iop.org/article/10.3847/0004-637X/820/2/130. 
  22. ↑ Yang, Huan; Malhotra, Sangeeta; Gronke, Max; Rhoads, James E.; Leitherer, Claus; Wofford, Aida; Jiang, Tianxing; Dijkstra, Mark et al. (2017-08-03). "Ly α Profile, Dust, and Prediction of Ly α Escape Fraction in Green Pea Galaxies". The Astrophysical Journal 844 (2): 171. doi:10.3847/1538-4357/aa7d4d. ISSN 1538-4357. https://iopscience.iop.org/article/10.3847/1538-4357/aa7d4d. 
  23. ↑ "Sangeeta Malhotra - The Mathematics Genealogy Project". https://genealogy.math.ndsu.nodak.edu/id.php?id=138515&fChrono=1. 
  24. ↑ "2017 and Prior Fellows" (in en). http://www.stsci.edu/home/stsci-research/fellowships/nasa-hubble-fellowship-program/2017-and-prior-fellows. 
  25. ↑ "AAS Fellows Program | American Astronomical Society". https://aas.org/grants-and-prizes/aas-fellows. 





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