... dust continuum emission from cosmologically-distant galaxies (SMGs, LBGs, EROs) ... sources and determine FIR properties of LBGs and EROs as well as SMGs ...
New Views Conference, Dec 12, 2005 ... The Highest Redshift Quasars and Galaxies. SDSS i-dropout Survey: ... Stacking X-ray image of LBGs in UDF... too few faint AGNs ...
Clustering of LAE, LBG and AGN at z~3 in MUSYC (MUltiwavelength Survey by Yale-Chile) ... 1385 LBGs and 58 AGN selected using Optical UBVR NB5000 and X-ray data ...
There is a spectrum of density perturbations gravitational potential ... day L* galaxies; similar to big bulges and intermediate-luminosity Ellipticals ...
Lyman Break Galaxies in Large Quasar Groups at z~1 G Williger (Louisville/JHU), R Clowes (Central Lancashire), L Campusano (U de Chile), L Haberzettl & J Lauroesch ...
a: this work, narrow-band (OII 44) photometry; b: Steidel et al.(2001) ... Narrow-band photometry can put a stronger constraint on the escape fraction of ...
Chris Simpson. Liverpool John Moores University. and a cast of ... Ouchi et al. 2005, ApJ, 620, L1, Discovery of primeval LSS with forming clusters at z=6 ...
Title: PowerPoint Presentation Author: Joe Lal Last modified by: Joe Lal Created Date: 8/29/2006 3:49:24 PM Document presentation format: On-screen Show
Supervisor: Anja C. Andersen. Dust in Young Galaxies. 2. The code. Radiative transfer ... Dust Extinction in Starburst Galaxies at z = 3 6. Dust Creation in ...
Dust absorbs the radiation produced by starbursts or AGN ... sufficient to blow away. all of the gas in a galaxy ... If L LM, AGN can blow dusty gas out of. its ...
During the mid-90's, with improved instrumentation, the commissioning of the 8-m ... VLA, ultra deep HDF-N ( Merlin, WSRT) JCMT SCUBA sub-mm maps of HDF-N ...
Search for a statistical description of the dark matter / galaxy distribution ... Based on GIF/VIRGO N-body. simulations by Jenkins et al. (1998) At z=3: r0~1 ...
Collaborators : B. Cl ment (LAM), P. Hibon (KIAS) J.Willis (Univ. Victoria), C. ... as the change in the far-UV LF is much milder. Data for z=6.5 : ...
It is very important to understand how we select sample galaxies and what we see in them. ... Some galaxies are only detected in one of the two wavelengths, ...
Panoramic Survey of the Deep Universe Observing Galaxy Formation at High Redshift Toru Yamada National Astronomical Observatory of Japan Opt/IR Div., Subaru Telescope
derived stellar masses indicating. the relation of the stellar mass ... Convolve with filter. response function. Model SED. Observed SEDs. Minimization method: ...
Teach how to use design software. General PR. Media channel. Practical design: Adobe Photoshop & Illustrator. Writing and editing skills. beKNOWN 4 ...
z 6 = Low order molecular transitions redshift to the short ... coeval formation of giant elliptical galaxy SMBH within 870 Myr of Big Bang. 1' CII CO 3-2 ...
Double Imaging Spectrograph. Simultaneous red and blue spectra. 3600 to 8000 0.8 to 3 /pixel. GrIm II infrared imager and spectrograph. 1 m to 2.5 m ...
Methodology adopted in the Demo is shared by a broad range of ... Comparing SEDs with models: the case of Lyman Break Galaxies (drop-outs) (Dickinson 2000) ...
SNUQSO (Seoul National University Bright Quasar Survey in Optical) ... QSONG (AKARI Spectroscopy Study of Quasars) ... Quasars (high redshift/low redshift) Low ...
GALAXY EVOLUTION OPTICAL AND IR SURVEYS Lucia Pozzetti INAF Osservatorio Astronomico di Bologna PEOPLE INVOLVED IN BOLOGNA INAF-OAB: Bardelli, Cappi, Ciliegi ...
10's 100's galaxies per night. Slit positions pre-set based on optical/submm/radio/Xray imaging ... Selection with 1.4 GHz imaging gets 50% to 75% at 10's ...
'Damped Lyman Alpha Systems' by. Wolfe, Arthur M., Gawiser, E. and ... wavelengths, but any observations are plagued by the brightness of the background QSO. ...
Need multiobject spectrograph for unbiased search for CO, other molecules in ... Submm gals: Dz_phot ~ 0.2 = ~2 GHz/source. Potentially trade-off of slits' for ...
OBAR SYSTEMS PROVIDING VOC AND RADON SERVICES SINCE 1985 Over 20,000 systems installed since 1985 NJDEP and EPA approved contractor Testing, Design and Installation
Optical and UV photons are scattered and absorbed by dust, and re-emitted as FIR ... Since UV is a direct measure of current star formation, dust emission carries ...
Andrew Baker (Rutgers), Lee Armus (IPAC), Paul Ho, Satoki Matsushita (ASIAA) ... al. 2004, Beelin et al. 2004, Hainline et al. 2004, Solomon & van den Bout 2005 ...
Collaborators: Ranga Chary (SSC), Mark Dickinson (NOAO), David Frayer (SSC) ... GO2 program 90 hours PI: R. Chary. Pope et al. in prep. Composite spectrum ...
0. Introductory remarks about galaxy formation & evolution and why clusters ... for overdensities in galaxies (Miley, Rottgering, de Breuck, Kurk, Overzier) ...
Andrey Kravtsov. Kavli Institute for Cosmological Physics (KICP) The University of Chicago ... The sexiest simulation? http://www.this-wonderful-life.com. SDSS survey ...
The Luminosity Function of. High Redshift QSOs (astro-ph/0608664) Fabio Fontanot. Max Planck Institute for Astronomy - Heidelberg. Deep06 Sintra, 11/10/06 ...
HI Column Densities (DLAs and sub-DLAs) Kinematics. Element Abundances. Model Implications ... IRTF K-band imaging of DLA and sub-DLA fields at z 1. Strong MgII ...
Robust identification of distant Compton-thick AGNs. IR AGN ... First insight into AGN activity in a Distant Protocluster. Lehmer, Alexander, et al., in prep ...
WHIM Backlight Scaling relation fudge factor Point source contaminant Cooling problem get-out clause AGN/GALAXY COEVOLUTION Kirpal Nandra Imperial College London
Extragalactic Studies on Galaxy Evolution with a Wide ... Given the known characteristics of galaxies ... IRAS discovered Ultra Luminous IR Galaxies (ULIRG) ...
G.K. Miley (Leiden),H.J.A.Rottgering (Leiden), J Kurk (MPIA) B.Venemans (IoA ... is several times higher than in the rest of the field (Miley et al, 06 in press) ...
red and dead' Eg. Zheng, Noeske, Damen... Massive galaxies form most of their stars at high z ... Dawn of Downsizing: SFR/M* vs. M* 5x. tH-1 (z=1.8) z=0.3. 1. ...