My current research program addreses addreses observational and theoretical aspects of the evolution, structure, and activities of disk galaxies across diverse environments,ranging from fields to rich clusters, and over a wide range of redshifts (z = 0 to 3) covering the last 12 billion years. This research program involves the analysis of space-based ( HST, Chandra, SIRTF ) and ground-based optical,NIR, and radio data, as well as a concurrent collaborative development of the theoretical framework addressing disk evolution. Below are some of the large projects and science I am involved in:

• GEMS (Galaxy Evolution from Morphology and SEDs): GEMS is the largest contiguous field ever imaged with HST (900 arcmin2) in 2 filters (F606W) and F850LP). GEMS provides HST-based morphologies and accurate redshfits from COMBO-17 for 10,000 galaxies down to R<24 in the range: 0.2
  • GOODS (Great Observatories Origins Deep Survey): GOODS unites extremely deep observations from the Spitzer Space Telescope, Hubble, and Chandra, ESA's XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the broadest range of wavelengths.
  • STAGES (Space Telescope A901/902 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: The survey will use 164 HST ACS orbits, along with Spitzer, GALEX, Chandra, and ground-based data of of Coma, the richest galaxy cluster in the local Universe, in order to study the impact of environment on galaxy evolution and provide a long-needed legacy database for comparison with environments at different densities and redshifts.
  • HUDF (Hubble Ultra Deep Field): HUDF is the deepest visible-light map ever made of the Universe, reaching more than 1.5 mag deeper than the original Hubble Deep Field (HDF). Memeber the HUDF home team that planned and implemented the HUDF: (1) "Planning of the ACS Ultra Deep Field" by Jogee, S., Ferguson, H., Stiavelli, M., Panagia, N., and Riess, A.; (2) "Radio and Sub-mm Considerations for the ACS Ultra Deep Field" by Koekomoer, A., Jogee, S., Beckwith, S. V. W., and Stiavelli, M.
  Research Interests
  
  • Galaxy Formation and Evolution
  • Structure and Dynamics of Galaxies from z=0 to 3, in particular : (1) Bar-Driven Evolution of Disk Galaxies ; (2) Strength and impact of tidal interactions/mergers on star formation, mass assembly history, and galaxy evolution.
  • Evolution and Fueling of Central Starbursts and Black Holes (AGN)
  • Interstellar Medium and Molecular Gas in Galaxies.
  
  Research Group/Advisees
  
  • Postdoctoral Fellows: Dr. Fabio Barazza (Mar 2004-Present; UT Austin); Dr. Ingo Berentzen (University of Kentucky/co-sponsored with Prof. Shlosman)

• Masters Level DA/Research Scientists: James Davies (Nov 2002--04/ STScI), Inge Heyer (Nov 2002-03/ STScI)

• Graduate Students: Irina Marinova (UT Austin); Naveen Reddy (Caltech)

• Undergraduate Students: Kyle Penner (Dean's Honors Program; UT Austin); Sarah Miller (Dean's Honors Program; UT Austin); Kyle Lake (UT Austin); Steven Roloff (UT Austin); Gabriel Lubell (Vassar College (2003--2004).

Excerpts of Research Projects

• Evolution of bars over the last 8 Gyr from the GEMS Survey: One third of present-day spirals host optically visible strong bars that drive their dynamical evolution. However, the fundamental question of how bars evolve over cosmological times has yet to be resolved. Drawing on a sample of 1590 galaxies from the GEMS survey, which provides morphologies from \it Hubble Space Telescope \rm Advanced Camera for Surveys (ACS) two-band images and accurate redshifts from the COMBO-17 survey, Jogee et al (2004) report that bars are abundant at intermediate redshifts of z ~0.2--1.0, and they certainly show no sign of a drastic decline at z >~0.7 as claimed by earlier studies (Abraham etal 1999). In fact, the large and similar bar fraction from the present-day out to different look-back times strongly suggests that on average bars have a long lifetime, well in excess of 2 Gyr. Thus, a comprehensive study of the impact and evolution of bars out to z~1 is a pre-requisite for developing any comprehensive picture of galaxy evolution over the last 8 Gyr. It is relevant for addressing the structural evolution of the Hubble sequence, and the dramatic decline in the cosmic UV luminosity density and SF rate (SFR) density from z~1 to the present-day.

Left: Examples of bars and spiral arms in galaxies at redshifts z~0.3 and 0.4. (top panel:left to right), and at z~0.5 and 0.9 (bottom panel:left to right),from the (GEMS) survey. Right: This figure illustrates how we characterizate bars via ellipse fits out to z~1 when the Universe was less than half of its present age. The GEMS image of a z ~0.5 galaxy with a bar, prominent spiral arms, and a disk is shown without (a) and with (b) an overlay of the fitted ellipses. (c) In the resulting radial plots of the surface brightness, ellipticity e, and P.A., the bar causes a characteristic rise in e out to a global maximum, while the P.A. has a plateau. Beyond the bar end (a~0.36"), the spiral arms lead to a twist in P.A. and varying ellipticity before the the disk of lower $e$ dominates. (From Jogee et al (2004) )

• Tidal Interactions and Mergers at Early Cosmic Times : We study the frequency and impact of tidal interactions and mergers out to z~1, when the Universe was half of its present age, in order to build a coherent picture of the decline in cosmic SFR density from z~1 to 0 and the mass assembly of galaxies (Jogee et al. 2003)

This figure shows a particularly spectacular double galaxy interaction in the GEMS field. In the foreground are two interacting spiral galaxies; while in the distant background there is another pair of interacting spiral galaxies (SOURCE: the GEMS collaboration)

• The HST/ACS Ultra Deep Field (HUDF): The HUDF provides the deepest optical view of the Universe and reaches more than 1.5 mag deeper than the original Hubble Deep Field (HDF). Scientific drivers of the UDF include probing the tail of the reionization epoch, constraining the star formation history of the Universe, probing the faint end of the galaxy luminosity function, and tracking the origin, structure, and merger history of galaxies as they evolve onto and off the Hubble sequence.

In 2004, HUDF team members planned and carried out observations lasting one million-seconds of the Hubble Ultra Deep Field (HUDF), the deepest visible-light image ever made of the Universe. These panels (Credit: NASA, ESA, S Beckwith and the HUDF team) from the HUDF reveal 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 Almost every panel shows oddball-shaped galaxies engaged in violent interactions with their neighbors and chronicles a period when the universe was younger and more chaotic. Order and structure were just beginning to emerge. The HUDF offers new insights into the origin, structure, and merger history of galaxies as they evolve onto and off the Hubble sequence, and sets constraints on what types of objects reionized the universe long ago.

• The Central regions of Barred Galaxies: Molecular Environment, Starbursts, and Secular Evolution

• Molecular gas in Active and Inactive Nuclei (MAIN) survey

• Fueling Central Starbursts and AGN: Nuclear bar in NGC 2782

• Fueling Central Starbursts : Bar-Driven Spiral density waves in NGC 5248