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How do SEDs of various AGNs types differ? Are dust SEDs consistent ... HST imaging of Galactic Nuclei. Martel et al. 2000, ApJS 130, 267. Dust Heating in AGNs ...
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How do SEDs of various AGNs types differ? Are dust SEDs consistent ... Model 1 (e.g. Farrah et al. 2003, MNRAS 345, 585 ; Rowand-Robinson 2000, MNRAS 316, 575) ...
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ISOCAM Survey of 3C Sources. Freudling et al. 2003, ApJ Letters 599, L13 ... ISO data suggest that dust throughout the host is heated by the central engine, ...
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Are there disks around BDs? How do they compare to cTTS disks? ... NIR not adequate cold BD photosphere! SED. ISOCAM 6.7&14.3 m excess detected for ~ 10 young BD ...
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Source/Loss Cone Energetic Particle Spectrometer (CEPPAD/SEPS) Hot ... A ring of organic molecules around HD 97300 (ESA/ISO/ISOCAM and R. Siebenmorgen et al. ...
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Delphine Marcillac. Moriond 2005 When UV meets IR ... 1. IR properties ... Faint Objects = long time exposure. it needs a good correction for the attenuation. ...
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present-day stars, it would be logical. to expect to detect a large ... 4 Populations: Spiral (M51), Starburst (M82), AGN1 (Elvis et al. 94) & AGN2 (Circinus) ...
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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 ...
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Radio-IR Astrometry ... Radio/submm observations of the ISM can complement PILOT's capabilities, ... Large FOV facilitates astrometry with radio maps. ...
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C.Doucet, P-O Lagage, E. Pantin (CEA Saclay SAp) E. Habart (IAS, Orsay) ... Doucet et al. 2006,submitted A&A. PAH stochastically heated by UV radiation from the star ...
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Raw materials delivered as a flexible sheet called 'Green Tape' LTCC Advantages. Process ... Ionization Tube Segment. Initial Conductor Ring. Drift Voltage ...
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SPIRE : Maps on the large scale (eg of galactic plane, see ... HIFI : Water and detailed kinematics of star forming regions. Dusty04, Paris, Oct. 27-29 2004 ...
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Star formation at intermediate scales: HII regions and Super-Star Clusters M. Sauvage, A. Contursi, L. Vanzi, S. Plante, T. X. Thuan, S. Madden
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... a mosaic with a final pixel scale of 1.2'. GOODS EN1 mosaic (13' ... GOODS EN1 mosaic processed with the CLEAN algorithm. Zoom of 2.2'x1.4' in the GOODS EN1 map. ...
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large telescopes (2 to 3.5 m) for Herschel-Planck can be cooled down below 50 K ... bolometer arrays will fly on Herschel-PACS ...
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dust emission with a scale of 100-400 AU. Outer radius ... Calvet et al. (1994) showed SEDs can be explained by dust emission from an infalling envelope ...
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Cristina Ramos Almeida, Ana M. P rez Garc a. and. Jose A. Acosta-Pulido ... Reuni n Estallidos - Madrid - 26 de Enero Cristina Ramos Almeida ...
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For simple VO protocols, it was decided long ago to offer only 1 of such images ... Once the data provider delivers the mapping recipes ...
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A handy modeling code & simulation tool generating source counts redshift ... Herschel, Planck, Akari ... Modeling the FIR & Sub-mm Era Long-wavelength ...
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High Redshift Galaxies
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Resolving contribution of unexpected EBL sources ... galactic. sources. CTA HE. COBE data (Hauser & Dwek, 2001) Goal 3: distance = Hubble parameter ...
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The Successor to Hubble The James Webb Space Telescope
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Location of the emission-line galaxies in the merging cluster Abell 3921 ... a field effect (general evolution of galaxies falling in the cluster) ...
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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. ...
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Attended lecture course on a large range of topics including many in astrophysics. ... blue YMCs, for whom the blue photosphere of the young stars is directly visible ...
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ALMA and distant galaxies
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Why is the study of ... Trumpler (1930) found that distant stars dimmed by something ... YMCs, for whom the blue photosphere of the young stars is directly ...
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1*gAMA *PLTE n n n efeefdfOdTdOFOTtTF Ftst S spsSGSp pGaG aa ... ...
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ALMA will see CO structure in detail. ALMA ... May not see most important region in the optical ... Heterodyne R 106 and 8-GHz bandwidth: ALMA can see details ...
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AGN IN THE SPITZER ERA: UNVEILING OBSCURED ACCRETION. Carlotta Gruppioni (INAF-OABO) ... annular ring (torus) around the central BH. ...
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will be included in Mengel et al. (2004, in preparation) Narrow band line ratios (Brg and Ha) ... estimates into expected bolometric luminosities according to ...
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