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19962025
most citedPHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies

948 citations · 18.1k across the 214 of their papers we have counts for

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astro-ph2002★ 115 cited

A 1.2mm MAMBO/IRAM-30m Study of Dust Emission from optically luminous z~2 Quasars

A. Omont, A. Beelen, F. Bertoldi +5

We report 250GHz (1.2mm) observations of redshift 1.8 < z < 2.8 optically luminous (M_B < -27.0), radio quiet quasars using the Max-Planck Millimeter Bolometer (MAMBO) array at the…

astro-ph2002★ 210 cited

Spatially Resolved Millimeter Interferometry of SMMJ02399-0136: a Very Massive Galaxy at z=2.8

Reinhard Genzel, Andrew J. Baker, Linda J. Tacconi +4

We report high-resolution millimeter mapping with the IRAM Plateau de Bure interferometer of rest-frame 335 micron continuum and CO(3-2) line emission from the z=2.8 submillimeter…

astro-ph2002★ 137 cited

Infrared stellar populations in the central parts of the Milky Way galaxy

Jacco Th. van Loon, G. F. Gilmore, A. Omont +7

Near- and mid-IR survey data from DENIS and ISOGAL are used to investigate the structure and formation history of the inner 10 degree (1.4 kpc) of the Milky Way galaxy. Synthetic b…

astro-ph2002★ 59 cited

86 GHz SiO maser survey of late-type stars in the Inner Galaxy. I. Observational data

M. Messineo, H. J. Habing, L. O. Sjouwerman +2

We present 86 GHz (v = 1, J = 2 -1) SiO maser line observations with the IRAM 30-m telescope of a sample of 441 late-type stars in the Inner Galaxy (-4 degr < l < +30 degr). These…

astro-ph2002★ 43 cited

Young massive stars in the ISOGAL survey II. The catalogue of bright YSO candidates

M. Felli, L. Testi, F. Schuller +1

The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YS…

astro-ph2002★ 59 cited

Imaging low order CO emission from the z=4.12 QSO PSS 2322+1944

C. Carilli, P. Cox, F. Bertoldi +2

We present observations of CO 1-0 and CO 2-1 emission from the z = 4.12 QSO PSS 2322+1944 using the Very Large Array. The CO emission is extended on a spatial scale of 2''. This ex…