Results 31 to 40 of about 100,039 (213)

THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: MOLECULAR GAS RESERVOIRS IN HIGH-REDSHIFT GALAXIES [PDF]

open access: yes, 2016
We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (ASPECS) that targets an ∼1 arcmin2 region in the Hubble Ultra Deep Field (UDF), a blind survey of CO emission (tracing molecular gas) in the 3 and 1 mm ...
R. Decarli   +31 more
semanticscholar   +1 more source

KILOPARSEC-SCALE DUST DISKS IN HIGH-REDSHIFT LUMINOUS SUBMILLIMETER GALAXIES [PDF]

open access: yesAstrophysical Journal, 2016
We present high-resolution (0.″16) 870 μm Atacama Large Millimeter/submillimeter Array (ALMA) imaging of 16 luminous ( ) submillimeter galaxies (SMGs) from the ALESS survey of the Extended Chandra Deep Field South.
J. Hodge   +23 more
semanticscholar   +1 more source

Formation of globular cluster candidates in merging proto-galaxies at high redshift: a view from the FIRE cosmological simulations [PDF]

open access: yes, 2017
Using a state-of-the-art cosmological simulation of merging proto-galaxies at high redshift from the FIRE project, with explicit treatments of star formation and stellar feedback in the interstellar medium, we investigate the formation of star clusters ...
Ji-hoon Kim   +28 more
semanticscholar   +1 more source

High-redshift lensed galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2006
AbstractWe present the results obtained from our deep survey of lensing clusters aimed at constraining the abundance of star-forming galaxies at z∼6–11.
Pelló, Roser   +10 more
openaire   +3 more sources

The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies [PDF]

open access: yes, 2017
We have conducted a two-layered spectroscopic survey (1′ × 1′ ultra deep and 3′ × 3′ deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE).
H. Inami   +30 more
semanticscholar   +1 more source

RECONCILING THE STELLAR AND NEBULAR SPECTRA OF HIGH-REDSHIFT GALAXIES [PDF]

open access: yes, 2016
We present a combined analysis of rest-frame far-UV (FUV; 1000–2000 Å) and rest-frame optical (3600–7000 Å) composite spectra formed from very deep Keck/LRIS and Keck/MOSFIRE observations of a sample of 30 star-forming galaxies with , selected to be ...
C. Steidel   +5 more
semanticscholar   +1 more source

Disk Galaxies at High Redshift? [PDF]

open access: yesProceedings of the International Astronomical Union, 2007
AbstractThe successful implementation of integral field near-infrared spectrographs fed by adaptive optics is providing unprecedented views of gas motions within galaxies at redshifts z = 2 − 3, when the universe was forming stars at its peak rate. A complex picture of galaxy kinematics is emerging, with inflows, rotation within sometimes extended and ...
openaire   +2 more sources

The Size Evolution of High-Redshift Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2004
5 pages, including 3 figures; uses emulateapj style; accepted by ApJL for publication in a special issue of early GOODS ...
Daniel Stern   +18 more
openaire   +5 more sources

The fate of high-redshift massive compact galaxies [PDF]

open access: yes, 2016
Massive high-redshift quiescent compact galaxies (nicknamed red nuggets) have been traditionally connected to present-day elliptical galaxies, often overlooking the relationships that they may have with other galaxy types.
I. G. D. L. Rosa   +6 more
semanticscholar   +1 more source

Galaxies at High Redshift [PDF]

open access: yes, 2000
Within just the last few years, we have advanced from knowing only a few galaxies at z>2 to having redshifts for nearly 1000 z~2-5 objects. The majority of this sample has been detected through the photometric ``drop-out'' technique used so successfully by Steidel and his collaborators. In addition, a handful of objects have already been detected at
openaire   +3 more sources

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