Lirg PowerPoint PPT Presentations

... extrapolated from current situation (as methodology would determine) Is there an Internet waiting to pounce? Emergent issues more interesting than the Assumptions ...

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

LBGs at z1, LIRGs at z1

Who is involved in the LIRG/SCONUL Impact Initiative? ... Staffordshire. University. Information skills for. research postgraduates. Brunel. University ...

Three Mirrors of LIS Practice. Reflective Practice (how we learn from our ... New fund-raising strategy beyond capitation? Target other bodies for collaboration ...

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. ...

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

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 ...

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 ...

Publicity (PR) Promotion. Library communications mix. Advertising. posters. print publications ... publicity most effective. personal selling least effective ...

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 ...

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 ...

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 ...

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

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. ...

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

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

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 ...

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 ...

No time or money to do it. Poor quality of LIS research ... Influence UK policy-makers, research funders and employers to support ...

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

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

Title: PowerPoint Presentation Author: Zaphod Document presentation format: Custom Other titles: Times New Roman Tahoma Monotype Corsiva Symbol Default Design Slide 1

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

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

Ten years of 'toolkit' development to assist in performance measurement and improvement ... New missing measurement instruments & frameworks ...

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 ...

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

Building a resource for practical assessment: adding value to value and impact Stephen Town University of York, UK Library Assessment Conference, Seattle

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

(from the Library Assessment Conference, Charlottesville, Va, September 2006) ... This also implies that 'competitive' data will be highly valued. The SCONUL Response ...

Hubble Space Telescope Images of Post-Starburst Quasars Michael S. Brotherton, S. Cales, R. Ganguly, Z. Shang (University of Wyoming) G. Canalizo (University of ...

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

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

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

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 ...

Glasgow Caledonian University. SFEU 2005 Libnet Conference. Presentation overview. Background ... Glasgow and Strathclyde Universities ...

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 ...

Electronic Information Services (EIS) usage by staff and students at Glasgow ... Universities of Sheffield Webber and Strathclyde. Sheila Webber & Bill Johnston ...

Value publications/research datasets/ICT resources/ IL interventions... To secure the library as a main source of information in conducting research in the field ...

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

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

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

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 ...

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

6th Northumbria International Conference on Performance Measures in Libraries ... note-taker. 9 interviews. c.1 hour. Faculty Librarian note-taker. Number ...

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

mid-IR: C-C/C=C/H2. Luminosities involved: 3x1011 L/Lsun 1014. The spectrum of a ULIRG: a `field guide' From Blain (2003) October 27, 2006. SKA Workshop, Paris ...

... 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 ...

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