Lirgs PowerPoint PPT Presentations

LBGs at z1, LIRGs at z1

COBE - 240 mm. LIRGs dominate the CSFR above z=0.6. At z=1: 70 % CSFR. LIRGs ... Red line: Spitzer-MIPS 24 mm galaxies. No excess correlation for GOODS sources. ...

regulating processes unrelated to galaxy interactions (Granato 04) ... galaxies, either passive or very actively starforming (LIRGs) ...

LIRGs are witnessing the major morphological changes. Merger (minor & major), gas infall related to galaxy interaction, ... aligned with the disk major axis. ...

Delphine Marcillac. Moriond 2005 When UV meets IR ... 1. IR properties ... Faint Objects = long time exposure. it needs a good correction for the attenuation. ...

Title: 1m ANIR LIRG Pa Author: toshikawa Last modified by: toshikawa Created Date

16 micron Imaging in the GOODS fields with the Spitzer IRS. Harry Teplitz ... Pilot Study: GTO 16 mm in GOODS-N ... GOODS South. Data obtained in Feb 05. Some ...

Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon Molecular Gas Mass as traced by CO emission and the star ...

Luminous Infrared Galaxies with the Submillimeter Array: Probing the Extremes of Star Formation

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 ...

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 ...

Cosmic Microwave Background (CMB) is an 'echo' of the Big Bang. ... Has same spectral behavior as CMB anisotropy. Difficult to correct for, but relatively minor. ...

To accelerate a particle efficiently it must cross the shocks ... Observational panorama: composition. Arrival directions & clustering. H.E.S.S.. 17 h data ...

Black Hole Feeding & Feedback: what can we learn from nearby AGN? Richard Davies, Eckhard Sturm Max Planck Institute for Extraterrestrial Physics, Germany

... radio map of the nearby star LS 5039 obtained with VLBA and VLA in ... No WR or Of massive stars in the field, no X-ray binaries or black hole candidates ...

LoCuSS: The midinfrared ButcherOemler effect Chris Haines University of Birmingham LoCuSS: Graham Sm

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 ...

Chandra and XMM-Newton: detailed information for nearby galaxies ( 100Mpc) Antennae ... Chandra & XMM-Newton wide-angle shallow surveys find galaxies at z~0.1 ...

About half of the galaxy formation and evolution gets out ... Dole et al 2006. Compilation by Hopkins 2004. ULIRGs. L 1011 Lo. L 1011 Lo. total ...

I. Kinematics & Dynamics of nearby galaxies (in tight ... absorption lines (Kelson et al. 2000) Long-slit spectroscopy (Keck Telescope) Low spectral res. ...

Formation and evolution of early-type galaxies Pieter van Dokkum (Yale)

Relation to (sub)mm galaxies (Barger, Chapman, Blain, Dannerbauer, ... Temperature redshift degeneracy: measure (1 z)/T_D (Blain 1999) ...

with gas-rich major merger Mathieu PUECH GEPI Observatoire de Paris, R. Delgado, M. Rodrigues, S. Fouquet + J.L. Wang, L. Athanassoula, P. Hopkins

Location of the emission-line galaxies in the merging cluster Abell 3921 ... a field effect (general evolution of galaxies falling in the cluster) ...

All EGRET blazars with peak gamma-ray flux above 10-6 photons cm-2 s-1 were ... 66 out of 116 northern EGRET sources have at least one plausible blazar like ...

CIB vs COB vs CMB. Extragalactic Background Light SED now well constrained ... COB ~ CIB ~ 24/23 nW m-2 sr-1. EBL: for 1 visible photon = 115 IR photons. EBL ...

Luminosity Function from 2dF Quasar Survey. Luminosity Function from 2dF Quasar Survey. Luminosity Function from 2dF Quasar Survey ...

... of the planets and their satellites; ... Generally, planets are large with respect to an ALMA beam ... To that of satellites and smaller bodies. Comets ...

... Herschel probes the rest-frame bolometric emission from galaxies as they formed most of their stars Wedding Cake Survey GOODS-S 0.04 deg^2 GOODS-N 0.04 ...

Title: Diapositiva 1 Author: caretta Last modified by: Caretta Created Date: 2/10/2006 2:26:37 AM Document presentation format: On-screen Show (4:3)

Star formation histories and environment Bianca M. Poggianti INAF Osservatorio Astronomico di Padova WE ARE ALL AFTER THE BIG PICTURE: To what extent, environment

The other side of galaxy formation: radio line and continuum ... Extreme gas rich galaxies without extreme starbursts. Gas depletion timescales 5 x108 yrs ...

... galaxies. A simple two color selection for culling galaxies ... Classify galaxies as star-forming or passive systems. The selection is independent of reddening ...

Thermal (free-free) emission (radio) Thermal dust emission (FIR) ... probing thermal (free-free) radio emission for z 3.5. VLA-COSMOS Large Project limits ...

There are only ~200 SMGs in ALMA-accessible fields... Mix of detailed investigation of well-studied SMGs, detection of fainter pops ...

Open questions: relative contribution SB and AGN. Need of observation above 10 keV ... To calibrate a SFR IR-X ray indicator is fundamental a direct measure of the ...

The Blessing and Curse of Cold Flows

m me si les r sultats actuels marquants viennent plut t de la cosmologie (SNLS, ... les r percutions sur le fonctionnement actuel d'un CFH aujourd'hui tr s ...

The other side of galaxy formation: radio deep fields

... pipeline-processed data enter the public domain immediately, thereby enabling ... SCosmos (IRAC, MIPS Imaging of COSMOS Field) D. Sanders ...

Demographics of Local StarForming Galaxies and Starbursts

Galaxy formation: radio through submm view

3C Radio Galaxies at 60mm with IRAS. Only ~30% of 3CR radio galaxies at z 0.5. were detected by IRAS at 60mm. Spitzer/MIPS observations of complete samples of ...

Total extinction map (6') with contours of the extinction overlaid. ... Extinction map with contours overlaid of the HI intensity (Stil & Israel 2002) at 13.5' ...

... type galaxy with SF activity in the Virgo cluster ... along the CM relation in Virgo Cluster (PID 3419 cycle 1 - PI ... with MIR signs of SF activity: ...

The Coevolution of SMBHs

Eelco van Kampen, Institute for Astrophysics, Innsbruck ... Miller Crawford (Edinburgh), Gian Luigi Granato ... Duncan Farrah estimated that we need to reach ...

deep Ha, UV imaging of volume-complete 11 Mpc samples - Spitzer followup proposed ... Ha imaging followup of Arecibo ALFALFA HI survey. Fourth Generation: blind ...

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The SWIRE Spitzer survey has detected by far the largest set of Sub-Millimeter ... Chapman, Blain, Smail, Ivison 2005. SCUBA(-MAMBO) census of high-z ULIRGs ...

more from existing resources, so more pressure for performance (and its measurement) ... indicators of library collections, personnel, and services by using a variety ...

high amount of special grants - awards, honours. Evidence needed: The library supports ... Learning outcomes - Higher education outcomes research review ...

EQUINOX. JUBILEE. JUSTEIS. Evalued project & toolkit. E-measures project. Outcomes project ... EQUINOX. JUBILEE. JUSTEIS. Outcomes project. SCONUL QAA ...