Results 11 to 20 of about 511 (183)
The MUSE Hubble Ultra Deep Field Survey [PDF]
We provide, for the first time, robust observational constraints on the galaxy major merger fraction up toz≈ 6 using spectroscopic close pair counts. Deep Multi Unit Spectroscopic Explorer (MUSE) observations in theHubbleUltra Deep Field (HUDF) andHubbleDeep Field South (HDF-S) are used to identify 113 secure close pairs of galaxies among a parent ...
Adrien Guérou +13 more
+30 more sources
The MUSE Hubble Ultra Deep Field Survey [PDF]
The C III] λλ1907, 1909 emission doublet has been proposed as an alternative to Lyman-α in redshift confirmations of galaxies at z ≳ 6 since it is not attenuated by the largely neutral intergalactic medium at these redshifts and is believed to be strong in the young, vigorously star-forming galaxies present at these early cosmic times.
T. Hashimoto +19 more
+28 more sources
The MUSEHubbleUltra Deep Field surveys: Data release II [PDF]
We present the second data release of the MUSEHubbleUltra-Deep Field surveys, which includes the deepest spectroscopic survey ever performed. The MUSE data, with their 3D content, amazing depth, wide spectral range, and excellent spatial and medium spectral resolution, are rich in information.
Roland Bacon +32 more
openalex +6 more sources
ULTRA-DEEP KS-BAND IMAGING OF THE HUBBLE FRONTIER FIELDS [PDF]
ABSTRACT We present an overview of the “KIFF” project, which provides ultra-deep K s -band imaging of all six of the Hubble Frontier Fields clusters, Abell 2744, MACS-0416, Abell S1063, Abell 370, MACS-0717, and MACS-1149. All of these fields have recently been observed with large
Gabriel B. Brammer +18 more
openalex +11 more sources
Distant Red Galaxies in the Hubble Ultra Deep Field [PDF]
Accepted for publication in ...
Sune Toft +6 more
openalex +3 more sources
The Hubble Ultra Deep Field [PDF]
44 pages, 18 figures, to appear in the Astronomical Journal October ...
Beckwith, Steven V. W. +14 more
openaire +4 more sources
The MUSE Hubble Ultra Deep Field Survey [PDF]
Star-forming galaxies have been found to follow a relatively tight relation between stellar mass ( M * ) and star formation rate (SFR), dubbed the “star formation sequence”. A turnover in the sequence has been observed, where galaxies with M * < 10 10 M ⊙ follow a steeper relation than their higher mass counterparts, suggesting that the low-mass
Boogaard, Leindert A +18 more
+9 more sources
Stars in the Hubble Ultra Deep Field [PDF]
We identified 46 unresolved source candidates in the Hubble Ultra Deep Field, down to i775 = 29.5. Unresolved objects were identified using a parameter S, which measures the deviation from the curve-of-growth of a point source. Extensive testing of this parameter was carried out, including the effects of decreasing signal-to-noise and of the apparent ...
N. Pirzkal +13 more
openalex +4 more sources
TADPOLE GALAXIES IN THE HUBBLE ULTRA DEEP FIELD [PDF]
19 pages, 16 figures, ApJ in press, vol 722, October 10 ...
Elmegreen, Bruce G. +1 more
openaire +2 more sources
Redshifts of Emission-Line Objects in the Hubble Ultra Deep Field [PDF]
30 pages, 5 figures.
Chun Xu +18 more
openalex +5 more sources

