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20142026
most citedPHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

642 citations · 3.7k across the 70 of their papers we have counts for

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Showing 2023Show all

11 papers · 1 filter

astro-ph.GA2023★ 13 cited

Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic Star-Formation Rate Density 300 Myr after the Big Bang

Brant Robertson, Benjamin D. Johnson, Sandro Tacchella +33

We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest imaging field observed with JWST. We make use of the ancillary Hubble optical images (5…

astro-ph.GA2023

High dust content of a quiescent galaxy at z~2 revealed by deep ALMA observation

Minju M. Lee, Charles C. Steidel, Gabriel Brammer +9

We report the detection of cold dust in an apparently quiescent massive galaxy () at (G4). The source is identified as a serendipitou…

astro-ph.GA2023★ 25 cited

Metal enrichment and evolution in four z > 6.5 quasar sightlines observed with JWST/NIRSpec

L. Christensen, P. Jakobsen, C. Willott +7

We present JWST/NIRSpec R~2700 spectra of four high-redshift quasars: VDES J0020-3653 (z = 6.860), DELS J0411-0907 (z = 6.825), UHS J0439+1634 (z = 6.519) and ULAS J1342+0928 (z =…

astro-ph.GA2023★ 29 cited

The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release

Daniel J. Eisenstein, Benjamin D. Johnson, Brant Robertson +58

We summarize the properties and initial data release of the JADES Origins Field (JOF), the longest single pointing yet imaged with the James Webb Space Telescope (JWST). This field…

astro-ph.GA2023★ 1 cited

GA-NIFS: JWST/NIRSpec IFU observations of HFLS3 reveal a dense galaxy group at z~6.3

G. C. Jones, H. Ubler, M. Perna +19

Massive, starbursting galaxies in the early Universe represent some of the most extreme objects in the study of galaxy evolution. One such source is HFLS3 (z~6.34), which was origi…

astro-ph.GA2023

Minor merger growth in action: JWST detects faint blue companions around massive quiescent galaxies at 0.5 < z < 3

Katherine A. Suess, Christina C. Williams, Brant Robertson +17

Minor mergers are thought to drive the structural evolution of massive quiescent galaxies; however, existing HST imaging is primarily sensitive to stellar mass ratios >1:10. Here,…

astro-ph.GA2023★ 6 cited

A core in a star-forming disc as evidence of inside-out growth in the early Universe

William M. Baker, Sandro Tacchella, Benjamin D. Johnson +36

The physical processes that establish the morphological evolution and the structural diversity of galaxies are key unknowns in extragalactic astrophysics. Here we report the findin…

astro-ph.GA2023★ 16 cited

JADES Initial Data Release for the Hubble Ultra Deep Field: Revealing the Faint Infrared Sky with Deep JWST NIRCam Imaging

Marcia J. Rieke, Brant E. Robertson, Sandro Tacchella +56

JWST has revolutionized the field of extragalactic astronomy with its sensitive and high-resolution infrared view of the distant universe. Adding to the new legacy of JWST observat…

astro-ph.GA2023★ 3 cited

Evidence for Large-scale, Rapid Gas Inflows in z~2 Star-forming Disks

R. Genzel, J. -B. Jolly, D. Liu +23

We report high-quality H/CO, imaging spectroscopy of nine massive (log median stellar mass = 10.65 ), disk galaxies on the star-forming, main sequence (henceforth `SF…

astro-ph.GA2023★ 67 cited

The ionising photon production efficiency at z~6 for Lyman-alpha emitters using JEMS and MUSE

Charlotte Simmonds, Sandro Tacchella, Michael V. Maseda +21

We study the ionising photon production efficiency at the end of the Epoch of Reionisation () for a sample of 30 Lyman- emitters. This is a crucial quantity to…

astro-ph.GA2023★ 169 cited

JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr After the Big Bang

Sandro Tacchella, Daniel J. Eisenstein, Kevin Hainline +45

We present JWST NIRCam 9-band near-infrared imaging of the luminous galaxy GN-z11 from the JWST Advanced Deep Extragalactic Survey (JADES) of the GOODS-N field. We find a…