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20032026
most citedA survey of molecular gas in luminous sub-millimetre galaxies

486 citations · 1.3k across the 30 of their papers we have counts for

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astro-ph2008★ 23 cited

New CO detections of lensed submillimeter galaxies in A2218: Probing molecular gas in the LIRG regime at high redshift

K. K. Knudsen, R. Neri, J. -P. Kneib +1

Context: Submillimeter galaxies (SMGs) are distant, dusty galaxies undergoing star formation at prodigious rates. Recently there has been major progress in understanding the nature…

astro-ph2008★ 31 cited

Interferometric CO Observations of submillimeter-faint, radio-selected starburst galaxies at z~2

S. C. Chapman, R. Neri, F. Bertoldi +9

High-redshift, dust-obscured galaxies -- selected to be luminous in the radio but relatively faint at 850um -- appear to represent a different population from the ultra-luminous su…

astro-ph2007★ 59 cited

The dark nature of GRB 051022 and its host galaxy

A. J. Castro-Tirado, M. Bremer, S. McBreen +17

We present multiwavelength (X-ray/optical/near-infrared/millimetre) observations of GRB 051022 between 2.5 hours and ~1.15 yr after the event. It is the most intense gamma-ray burs…

astro-ph2006★ 39 cited

Atomic Carbon in APM 08279+5255 at z=3.91

J. Wagg, D. J. Wilner, R. Neri +2

We present a detection of [CI] line emission in the lensed quasar APM 08279+5255 at z=3.91 using the IRAM Plateau de Bure interferometer. The [CI] line velocity and width are simil…

astro-ph2004★ 86 cited

Detection of Two Massive CO Systems in 4C 41.17 at z = 3.8

Carlos De Breuck, Dennis Downes, Roberto Neri +4

We have detected CO(4-3) in the z=3.8 radio galaxy 4C 41.17 with the IRAM Interferometer. The CO is in two massive (M_dyn ~ 6 x 10^10 M_Sun) systems separated by 1.8" (13 kpc), and…

astro-ph2003★ 197 cited

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…