Results 161 to 170 of about 405,217 (280)

JADES: Resolving the Stellar Component and Filamentary Overdense Environment of Hubble Space Telescope (HST)-dark Submillimeter Galaxy HDF850.1 at z = 5.18

open access: yesThe Astrophysical Journal
HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at z = 5.18.
Fengwu Sun   +30 more
doaj   +1 more source

Lyman Continuum Leakers at z > 3 in the GOODS-S Field: Starburst or Not?

open access: yesThe Astrophysical Journal Letters
We investigate the star-forming properties of 23 Lyman continuum (LyC) leakers at z > 3 in the Great Observatories Origins Deep Survey-South field based on a systematic review of LyC observations from the literature.
Shuairu Zhu   +4 more
doaj   +1 more source

ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CO LUMINOSITY FUNCTIONS AND THE EVOLUTION OF THE COSMIC DENSITY OF MOLECULAR GAS [PDF]

open access: bronze, 2016
Roberto Decarli   +39 more
openalex   +1 more source

Photometric Redshifts in Hubble Deep Field South

open access: yes, 1999
We apply both a traditional `dropout' approach and a photometric redshift estimation technique to the Hubble Deep Field South data. We give a list of dropout selected z$\sim$3 objects, and show their images. We then discuss our photometric redshift estimation technique, demonstrate both its effectiveness and the role played by near-IR data, and then ...
openaire   +2 more sources

The AstroSat UV Deep Field South. II. A Diverse Set of Lyman-continuum Leakers at z ∼ 1

open access: yesThe Astrophysical Journal
We report the detection of five newly identified Lyman-continuum (LyC) leaker candidates at redshifts 0.99–1.42 in the AstroSat UV Deep Field South F154W image.
Soumil Maulick   +2 more
doaj   +1 more source

MIDIS: The Relation between Strong (Hβ + [O iii]) Emission, Star Formation, and Burstiness around the Epoch of Reionization

open access: yesThe Astrophysical Journal
We investigate the properties of strong (H β + [O iii ]) emitters before and after the end of the “Epoch of Reionization” from z = 8 to z = 5.5. We make use of ultradeep JWST / NIRCam imaging in the parallel field (P2) of the MIRI Deep Imaging Survey ...
K. I. Caputi   +27 more
doaj   +1 more source

High‐Redshift Extremely Red Objects in theHubble Space TelescopeUltra Deep Field Revealed by the GOODS Infrared Array Camera Observations [PDF]

open access: bronze, 2004
Haojing Yan   +11 more
openalex   +1 more source

The MUSE Ultra Deep Field (MUDF). VI. The Relationship between Galaxy Properties and Metals in the Circumgalactic Medium

open access: yesThe Astrophysical Journal
We present initial results associating galaxies in the Multi-Unit Spectroscopic Explorer (MUSE) Ultra Deep Field (MUDF) with gas seen in absorption along the line of sight to two bright quasars in this field to explore the dependence of metals in the ...
Alexander Beckett   +12 more
doaj   +1 more source

MIDIS: Strong (Hb + [OIII]) and Ha emitters at redshift $z \simeq 7-8$ unveiled with JWST/NIRCam and MIRI imaging in the Hubble eXtreme Deep Field (XDF) [PDF]

open access: green, 2023
Pierluigi Rinaldi   +46 more
openalex   +1 more source

Home - About - Disclaimer - Privacy