Dr. Shardha Jogee Department of Astronomy The University of Texas at Austin 1 University Station C1400, RLM 16.224 Austin, TX 78712-0259 Email: sj@astro.as.utexas.edu Phone: (512) 471 1395 Fax : (512) 471 6016 Office : RLM 16.224 URL : http://www.as.utexas.edu/~sj

B.S Physics (1992), M.A. Physics (1995), Cambridge University, England M. S. (1994), M. Phil. (1994), Ph.D. (1999), Astronomy, Yale University, U.S.A Postdoctoral Scholar, Astronomy, CalTech, U.S.A (1999-2002) Assistant Astronomer, Space Telescope Science Institute (which oversees the science operation of NASA's space facilities, including the Hubble Space Telesope and the James Webb Space Telescope) U.S.A (2002--2004) Assistant Professor, Department of Astronomy, University of Texas at Austin, USA (2004-2008) Associate Professor (Tenured), Department of Astronomy, University of Texas at Austin, USA (2009-2013) Professor, Department of Astronomy, University of Texas at Austin, USA (2014-Present) Department Associate Chair, Department of Astronomy, University of Texas at Austin, USA (2014) Department Chair, Department of Astronomy, University of Texas at Austin, USA (Sep. 2015-Present)

• GEMS (Galaxy Evolution From Morphology And SEDs): One of the first large (900 arcmin^2) contiguous field imaged with HST ACS in 2 filters (F606W) and F850LP). GEMS provides HST-based morphologies and accurate redshfits from COMBO-17 for 9,000 galaxies down to R<24 in the range z~0.2-1.2. Panchromatic coverage is provided by Spitzer, Chandra, and GALEX.

• GOODS (Great Observatories Origins Deep Survey): GOODS unites extremely deep observations from Spitzer Hubble, and Chandra, ESA's XMM-Newton.

• STAGES (Space Telescope Abell 901/902 Galaxy Evolution Survey): A multiwavelength survey to probe the physical drivers of galaxy evolution in dense environments, using HST (80 orbits; ACS F606W), Spitzer (MIPS +IRAC), GALEX (FUV,NUV), Chandra XMM-Newton, COMBO-17 spectro-photometric redshifts, and gravitational lensing mass maps.

• The HST ACS Treasury Survey of the Coma Cluster: This Treasury survey was allocated 164 HST orbits in Cycle 15 to map Coma, the richest galaxy cluster in the local Universe. Complementary Spitzer, GALEX,Chandra, and ground-based data are also available.

• The GOODS-NICMOS Survey of Massive Galaxies at z=1.7 to 3

• The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX)

• The VIRUS-P Exploration of Nearby Galaxies (VENGA): VENGA is the largest integral field spectroscopic survey of nearby spiral galaxies conducted to date. It uses 150 nights of observing time with the superb VIRUS-P Integral Field Unit (IFU) on the 2.7m telescope at McDonald Observatory.

The Hubble Ultra Deep Field (HUDF), the deepest visible-light image ever made of the Universe, (Credit: NASA, ESA, S Beckwith and HUDF home team ) shows the first galaxies to emerge from the so-called "dark ages," (the time shortly after the big bang when the first stars reheated the cold, dark universe), and chronicles a period when the universe was younger and more chaotic, with violent interactions between galaxies.

Please see CV for a detailed list. Below are a few selected activities:

• Voice America one hour radio interview highlighting UT Astronomy, academic leadership, and my journey as a female astronomer (2016)

• The Galaxies and Cosmos Explorer Tool (GCET)
  (funded by NASA grant NAG5-13063, NSF grant AST-0607748, and a FASTex award from the UT Division of Instructional Innovation and Assessment.)

• Building a Bridge to Texas High School Science Teachers and Students
  (funded by NSF grant AST-0607748 and NASA LTSA grant NAG5-13063)

• UT College of Natural Sciences Interview, April 2008

• Le Mauricien (in French)