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13 papers · 2 filters
The European Large Area ISO Survey (ELAIS): The Final Band-merged Catalogue
ELAIS Consortium, :, M. Rowan-Robinson +16
We present the final band-merged ELAIS catalogue at 6.7, 15, 90, and 175 m, and the associated data at u,g,r,i,z,J,H,K, and 20cm. The origin of the survey, infrared and radio ob…
Molecular Gas in the Host Galaxy of a Quasar at Redshift z=6.42
Fabian Walter, Frank Bertoldi, Chris Carilli +7
Observations of the molecular gas phase in quasar host galaxies provide fundamental constraints on galaxy evolution at the highest redshifts. Molecular gas is the material out of w…
High-excitation CO in a quasar host galaxy at z=6.42
F. Bertoldi, P. Cox, R. Neri +8
We report the detection of high excitation CO emission from the most distant quasar currently known, SDSS J114816.64+525150.3 (hereafter J1148+5251), at a redshift z=6.419. The CO…
Dust emission from the most distant quasars
F. Bertoldi, C. L. Carilli, P. Cox +5
We report observations of three SDSS z>6 QSOs at 250 GHz (1.2mm) using the 117-channel Max-Planck Millimeter Bolometer (MAMBO-2) array at the IRAM 30-meter telescope. J1148+5251 (z…
ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared
A. Omont, G. Gilmore, C. Alard +38
The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss…
The promise of interferometry in the mm range: ALMA
Alain Omont
The Atacama Large Millimeter Array (ALMA), a world-wide project (64x12m-dishes operating from 84 to 720 GHz, to be completed by 2011) will represent a jump of almost two orders of…
Explanatory Supplement of the ISOGAL-DENIS Point Source Catalogue
F. Schuller, S. Ganesh, M. Messineo +10
We present version 1.0 of the ISOGAL-DENIS Point Source Catalogue (PSC), containing more than 100,000 point sources detected at 7 and/or 15 micron in the ISOGAL survey of the inner…
Long Period Variables detected by ISO in the SMC
M. -R. L. Cioni, J. A. D. L. Blommaert, M. A. T. Groenewegen +8
This article presents the study of the light-curves extracted from the MACHO database of a sample of stars observed by the ISO in the SMC. These stars belong to the ISO-Mini-Survey…
A Molecular Einstein Ring: Imaging a Starburst Disk Surrounding a Quasi-Stellar Object
C. L. Carilli, G. F. Lewis, S. G. Djorgovski +4
Images of the CO 2-1 line emission, and the radio continuum emission, from the redshift 4.12 gravitationally lensed quasi-stellar object (QSO) PSS J2322+1944 reveal an Einstein rin…
Sensitive observations at 1.4 and 250 GHz of z > 5 QSOs
A. O. Petric, C. L. Carilli, F. Bertoldi +5
We present 1.4 and 5 GHz observations taken with the Very Large Array (VLA), and observations at 250 GHz obtained with the Max-Planck millimeter bolometer (MAMBO) at the IRAM 30~m…
Near-IR spectra of ISOGAL sources in the Inner Galactic Bulge
M. Schultheis, A. Lançon, A. Omont +2
In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15 m detected during the ISOGAL survey. Making use of the DENIS in…
Stellar sources in the ISOGAL intermediate bulge fields
D. K. Ojha, A. Omont, F. Schuller +3
We present a study of ISOGAL sources in the "intermediate" galactic bulge ( 2, 1--4), observed by ISOCAM at 7 and 15 . In…
CO emission and associated HI absorption from a massive gas reservoir surrounding the z=3 radio galaxy B3 J2330+3927
Carlos De Breuck, Roberto Neri, Raffaella Morganti +10
We present results of a comprehensive multi-frequency study of the radio galaxy B3 J2330+3927. The 1.9" wide radio source, consisting of 3 components, is bracketed by 2 objects in…