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Close-up view of a luminous star-forming galaxy at z=2.95
S. Berta, A. J. Young, P. Cox +35
(Abridged) Exploiting the sensitivity and broad band width of NOEMA, we have studied the molecular gas and dust in the galaxy HerBS-89a, at z=2.95. High angular resolution images r…
Exploiting NIKA2/XMM-Newton imaging synergy for intermediate mass, high- galaxy clusters within the NIKA2 SZ Large Program
F. Kéruzoré, F. Mayet, G. W. Pratt +40
High-resolution mapping of the intra-cluster medium (ICM) up to high redshift and down to low masses is crucial to derive accurate mass estimates of the galaxy cluster and to under…
Evidence for Infalling Gas in a Lyman- Blob
Yiping Ao, Zheng Zheng, Christian Henkel +11
Lyman- blobs (LABs) are spatially extended nebulae of emission in the Ly line of hydrogen, seen at high redshifts, and most commonly found in the dense environment of…
First detection of the 448 GHz ortho-H2O line at high redshift: probing the structure of a starburst nucleus at z = 3.63
C. Yang, E. González-Alfonso, A. Omont +4
Submillimeter rotational lines of H2O are a powerful probe in warm gas regions of the ISM, tracing scales and structures ranging from kpc disks to the most compact and dust-obscure…
A hyper luminous starburst at z=4.72 magnified by a lensing galaxy pair at z=1.48
L. Ciesla, M. Béthermin, E. Daddi +23
[Abridged] We discovered in the Herschel Reference Survey an extremely bright IR source with ~120mJy (Red Virgo 4 - RV4). Based on IRAM/EMIR and IRAM/NOEMA detections of t…