In the context of the VLA-COSMOS Deep project, additional VLA A array observations at 1.4 GHz were obtained for the central degree of the COSMOS field and combined with the existing data from the VLA-COSMOS Large project. A newly constructed Deep mosaic with a resolution of 2farcs5 was used to search for sources down to 4ÃÆ with 1ÃÆ Ã¢â°Ë 12 üJy beamââ¬â1 in the central 50' Ãâ 50'. This new catalog is combined with the catalog from the Large project (obtained at 1farcs5 Ãâ 1farcs4 resolution) to construct a new Joint catalog. All sources listed in the new Joint catalog have peak flux densities of >=5ÃÆ at 1farcs5 and/or 2farcs5 resolution to account for the fact that a significant fraction of sources at these low flux l...
We have used the Karl G. Jansky Very Large Array (VLA) to carry out the first molecular deep field o...
13 pages, Accepted for publication in Astronomy & AstrophysicsWe have conducted a deep survey (r.m.s...
We have conducted a deep survey (rms noise ${\simeq} 17~\mu$Jy) with the Very Large Array (VLA) at 1...
37 pages, 13 figures, accepted by AJ (sched. for November issue), for information and data see: http...
49 pages, 18 figures; accepted for publication in the ApJS, COSMOS special issue. The data will be a...
We present the VLA-COSMOS 3 GHz Large Project based on 384 h of observations with the Karl G. Jansky...
We present the VLA-COSMOS 3 GHz Large Project based on 384 h of observations with the Karl G. Jansky...
The VLA-COSMOS Large Project is described and its scientific objective is discussed. We present a ca...
International audienceWe present the VLA‐COSMOS 3 GHz Large Project based on 384 h of observations w...
We present 90 cm Very Large Array imaging of the COSMOS field, comprising a circular area of 3.14 sq...
We have observed the Extended Chandra Deep Field-South (E-CDF-S) using a mosaic of six deep Very Lar...
International audienceWe present 90 cm Very Large Array imaging of the COSMOS field, comprising a ci...
We have used the Karl G. Jansky Very Large Array (VLA) to carry out the first molecular deep field o...
13 pages, Accepted for publication in Astronomy & AstrophysicsWe have conducted a deep survey (r.m.s...
We have conducted a deep survey (rms noise ${\simeq} 17~\mu$Jy) with the Very Large Array (VLA) at 1...
37 pages, 13 figures, accepted by AJ (sched. for November issue), for information and data see: http...
49 pages, 18 figures; accepted for publication in the ApJS, COSMOS special issue. The data will be a...
We present the VLA-COSMOS 3 GHz Large Project based on 384 h of observations with the Karl G. Jansky...
We present the VLA-COSMOS 3 GHz Large Project based on 384 h of observations with the Karl G. Jansky...
The VLA-COSMOS Large Project is described and its scientific objective is discussed. We present a ca...
International audienceWe present the VLA‐COSMOS 3 GHz Large Project based on 384 h of observations w...
We present 90 cm Very Large Array imaging of the COSMOS field, comprising a circular area of 3.14 sq...
We have observed the Extended Chandra Deep Field-South (E-CDF-S) using a mosaic of six deep Very Lar...
International audienceWe present 90 cm Very Large Array imaging of the COSMOS field, comprising a ci...
We have used the Karl G. Jansky Very Large Array (VLA) to carry out the first molecular deep field o...
13 pages, Accepted for publication in Astronomy & AstrophysicsWe have conducted a deep survey (r.m.s...
We have conducted a deep survey (rms noise ${\simeq} 17~\mu$Jy) with the Very Large Array (VLA) at 1...