Calendar

Sep 1 @ 3:15 pm – 4:15 pm BX102
A Faint Flux-Limited LAE Sample at z = 0.3 Isak Wold, UT Austin Observational surveys of Lya emitters (LAEs) have proven to be an efficient method to identify and study large numbers of galaxies over...
Continue Reading »
Oct 16 @ 12:30 pm – 1:30 pm AY 119
Dark Sky Images Ken Naiff Ken, an retired engineer, is a highly technically skilled and artistic astrophotographer.  He will be sharing some of his work and elaborating on the technical methods and processing techniques he...
Continue Reading »
Apr 6 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Sten Hasselquist, NMSU AbstractShare this:TweetPrint
Sep 21 @ 3:15 pm – 4:15 pm BX102
Fresh Perspectives on Star Formation from LEGUS, the Legacy ExtraGalactic Ultraviolet Survey David Thilker, Johns Hopkins University The Legacy ExtraGalactic Ultraviolet Survey (LEGUS) was a Cycle 21 Large Treasury HST program which obtained ~parsec resolution NUV- to I-band WFC3 imaging for 50 nearby, representative star-forming Local Volume galaxies, with a primary goal of...
Continue Reading »
Apr 22 @ 12:30 pm – 1:30 pm AY 119
ASTR 598Share this:TweetPrint
Apr 29 @ 12:30 pm – 1:30 pm AY 119
ASTR 598Share this:TweetPrint
Oct 4 @ 3:15 pm – 4:15 pm BX102
The SPLASH Survey of the Andromeda Galaxy Raja Guhathurkurta, University of California, Santa Cruz Our nearest large spiral galaxy neighbor, the Andromeda galaxy (M31), and its dwarf satellites, offer a panoramic yet detailed view of...
Continue Reading »
Dec 2 @ 12:30 pm – 1:30 pm AY 119
ASTR 598 Farhan Hasan and Oana VesaShare this:TweetPrint
Dec 4 @ 12:00 pm – 1:00 pm AY 119
ASTR 598 Ali Hyder and Matt VarakianShare this:TweetPrint
Dec 6 @ 3:15 pm – 4:15 pm BX102
Revealing reionization with the thermal history of the intergalactic medium Elisa Boera, SISSA Trieste During hydrogen reionization the UV radiation from the first luminous sources injected vast amount of energy into the intergalactic medium, photo-heating...
Continue Reading »
Dec 9 @ 12:30 pm – 1:15 pm AY 119
ASTR 598 Minje BoemShare this:TweetPrint