Aug. 25
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Steven Finkelstein
University of Texas at Austin
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Organizational Meeting
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Sep. 1
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11:00 a.m. this week only
Kelly Lockhart
Institute for Astronomy, University of Hawaii - Manoa
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Testing Theories of in situ Star Formation in the Nucleus of M31
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Sep. 8
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No talk scheduled
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Sep. 15
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Steve Finkelstein
The University of Texas at Austin
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A Semi-empirical Model of Reionization
abstract
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Sep. 22
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No talk scheduled
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Sep. 29
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No talk scheduled
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Oct. 6
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Anson D’Aloisio
University of Washington
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Probing Cosmological Reionization with the High-redshift Lyman-alpha Forest
abstract
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Oct. 13 (Talk #1)
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Jackie Champagne
The University of Texas at Austin
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Title: TBA
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Oct. 13 (Talk #2)
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Rebecca Larson
The University of Texas at Austin
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A Blind Search for Ly-a Emission from Galaxies at z = 6-8 with Deep HST Grism Spectra
abstract
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Oct. 20
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Marcelo Alvarez
Canadian Institute for Theoretical Astrophyics, University of Toronto
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Fundamental Physics with the Next Generation of Large Scale Structure Surveys
abstract
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Oct. 27
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No talk scheduled
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Nov. 3 (Talk #1)
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Kristy McQuinn
The University of Texas at Austin
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JWST Science Case: Resolved Stellar Populations
abstract
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Nov. 3 (Talk #2)
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Patrick Drew
The University of Texas at Austin
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Title: TBA
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Nov. 10
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Irene Shivaei
University of California, Riverside
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A Multi-Wavelength Census of Star Formation and Dust in Galaxies at z ~ 2
Redshift of z ~ 2 is an important era in the history of the universe, as it contains the peak of star formation rate density and quasar activity. I will talk about the properties of galaxies during this era from two different, yet complementary, aspects: star formation and mass assembly, and galactic dust enrichment. In this study, I use a wealth of spectroscopic data obtained by the MOSDEF survey. I will introduce the MOSDEF survey, which is a multi-institutional project that uses the near-IR MOSFIRE spectrograph on the Keck I telescope to characterize the gaseous and stellar contents of ~ 1500 rest-frame optically selected galaxies at 1.37 < z < 3.80. Furthermore, I incorporate the mid- and far-IR data from the Spitzer and Herschel telescopes to obtain a complete census of obscured and unobscured star formation in galaxies. Specifically, I explore the star-formation rate and stellar mass relation at z ~ 2, using multi-wavelength star-formation rate tracers (UV, Hα, 24 micron, and far-IR). Moreover, I investigate, for the first time, the variation of the PAH emission at 7.7 micron, traced by Spitzer/MIPS 24 micron, in galaxies spanning a wide range in metallicity at z ~ 2. Our results have important implications for high-redshift studies that adopt 24 micron flux to derive total IR luminosity and star-formation rate.
close
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Nov. 17
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Andreia Carrillo
The University of Texas at Austin
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Characterizing dw1335-29, a dwarf galaxy of M83
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Nov. 24
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Thanksgiving Holiday
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Dec. 1
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Allison Strom
California Institute of Technology
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Star-formation history and chemical enrichment in the early Universe: clues from the rest-UV and rest-optical spectra of high-redshift galaxies
abstract
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