Frontiers of Astrophysics, Journal Club
Fall 2009
Fri @ 12-1 p.m., Room 7 Bryant
DATE |
SPEAKER |
TITLE |
References, Additional info. |
Aug 28 Frontiers |
Ata Sarajedini |
Overview of Research |
...
|
Aug 28 JC |
Dan Gettings |
TBD |
...
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Sept 4 Frontiers |
Fred Hamann |
Quasars and Active Galaxies |
...
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Sept 4 JC |
Sara Gonzalez |
UF Libraries |
...
|
Sept 11 Frontiers |
Oleg Kargaltsev |
Non-accreting Neutron Stars through the eyes of the flagship space observatories |
...
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Sept 11 JC |
Michael Butler |
Some recent results on Infrared Dark Clouds |
...
|
Sept 25 Research Talk |
Martin Durant |
Optical Emission in X-ray Binaries: death of the reprocessing scenario and birth of dynamic interaction |
...
|
Oct 2 Frontiers |
Jonathan Tan |
Star Formation Near and Far |
...
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Oct 9 Frontiers |
Vicki Sarajedini |
Overview of Research |
...
|
Oct 9 JC |
Amanda Townsend |
TBD |
...
|
Oct 16 |
No talk |
Homecoming Holiday |
...
|
Oct 23 JC |
Enrique Lopez Rodriguez (UF) |
The dusty heart of nearby active galaxies |
Hoenig, S. & Kishimoto, M., arXiv:0909.4539v1
|
Oct 23 JC |
Jesus Martinez |
Living in a void: Testing the Copernican Principle with Distant
Supernovae |
(Clifton et al. 2008, arXiv:0807.1443)
|
Oct 30 Guest Research Talk |
Aaron Grocholski (STScI) |
New Deep HST/ACS Photometry of NGC 1569: Constraining the Evolution of
the Strongest Starburst in the Nearby Universe |
Massive starbursts drive the evolution of galaxies at high redshift, but
they can only be studied in detail in the nearby Universe where they are
much rarer. The dwarf irregular galaxy NGC 1569 has always been considered
the closest example of a true starburst, with exceptionally high sustained
star formation (SF) over the last Gyr. This recent SF has been extensively
constrainted by HST studies that reached to near the presumed magnitude of
the tip of the red giant branch (TRGB). These studies could not address
the onset of the most ancient SF or the triggering mechanism of the
current starburst. Here we present new deep HST ACS/WFC photometry of the
resolved stars in NGC 1569 that goes some 4 mag deeper than any previous
HST observations. These data allowed us to unequivocally detect and
measure the TRGB for the first time and show that NGC 1569 is considerably
farther away than previously believed. At ~3 Mpc it is actually a member
of the IC 342 group of galaxies, instead of being a starburst in
isolation. In addition to the TRGB, our increased photometric depth also
gives access to the fainter red clump and horizontal branch features in
the I vs V-I color-magnitude diagram (CMD) of NGC 1569, allowing us to
constrain for the first time even the most ancient SFH of this extreme
starburst through the use of synthetic CMDs. The area sampled by our
ACS/WFC observations is some 25 times larger than in previous HST studies,
allowing us to characterize the spatial variations of the SFH, from the
central star forming regions of NGC 1569 out into the older and more
sparsely populated "halo". The results reveal the evolutionary status of
this extreme starburst over cosmic time.
|
Nov 6 Frontiers |
Steve Eikenberry |
Black Hole Astrophysics and the FLAMINGOS-2 Early Science Surveys |
...
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Nov 6 JC |
Benjamin Nelson |
Applying Gravitational Lensing to the Exoplanet Search |
...
|
Nov 13 Guest Research Talk |
Roger Griffith (JPL) |
The Advanced Camera for Surveys General Catalog (ACS-GC) |
We use publicly available data obtained with the Advanced Camera for Surveys
(ACS) instrument on the Hubble Space Telescope to construct the ACS General Cata-
log (ACS-GC). The ACS-GC includes over 490,000 astronomical sources (stars + galax-
ies) derived from the AEGIS, COSMOS, GEMS, and GOODS surveys. We include
publicly available redshifts from the DEEP2, COMBO-17, TKRS, PEARS and zCOS-
MOS surveys to supply redshifts for a considerable fraction (~62%) of the imaging
sample. GALAPAGOS was used to construct photometric (SExtractor) and morpho-
logical (GALFIT) catalogs. The morphological analysis assumes a single Sersic model
for each object to derive quantitative structural parameters. Galaxy Zoo will measure
visual morphologies for a large fraction of these galaxies. The ACS-GC includes color images,
GALFIT residual images, a galaxy atlas, and a photometry + morphology + redshift
catalog. The entire data set will be made publicly available through the NASA Extragalactic
Database (NED) and LEVEL5.
|
Nov 20 JC |
Robert Morehead |
TBD |
...
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Nov 20 JC |
Bo Ma |
TBD |
...
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Dec 4 Frontiers |
Charlie Telesco |
TBD |
...
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Dec 4 JC |
Knicole Colon |
TBD |
...
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