activity
20142026
most citedThe MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8

442 citations · 6.3k across the 166 of their papers we have counts for

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Showing 2024Show all

28 papers · 1 filter

astro-ph.GA2024★ 2 cited

A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution

Matteo Bonato, David Leisawitz, Gianfranco De Zotti +10

Far-infrared (FIR) surveys are critical to probing the co-evolution of black holes and galaxies, since of order half the light from accreting black holes and active star formation…

astro-ph.GA2024★ 8 cited

An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy

Ivo Labbe, Jenny E. Greene, Jorryt Matthee +37

We present a detailed exploration of the most optically-luminous Little Red Dot (erg/s, erg/s, F444W=22AB) found to date. Located in the Abell 2744 fie…

astro-ph.GA2024

Constraining the link between the 2175Å dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI

A. J. Battisti, I. Shivaei, H. -J. Park +5

The 2175Å bump is a prominent absorption feature at ultraviolet (UV) wavelengths in dust extinction and attenuation curves. Understanding the relative strength of this feature is i…

astro-ph.GA2024★ 1 cited

Not Just a Dot: the complex UV morphology and underlying properties of Little Red Dots

P. Rinaldi, N. Bonaventura, G. H. Rieke +31

We analyze 99 photometrically selected Little Red Dots (LRDs) at in the GOODS fields, leveraging ultra-deep JADES NIRCam short-wavelength (SW) data. We examine the…

astro-ph.GA2024

Dynamics of Star-forming Galaxies in a Massive Structure at \lowercase{} 2.2: Evidence for Galaxy Harassment in high- Environments

Behnam Darvish, Nima Chartab, Zahra Sattari +5

We spectroscopically confirm a new protocluster in the COSMOS field at =2.24430 with Keck/MOSFIRE, dubbed CC2.2B, which is in the immediate vicinity of CC2.2A protocluster, orig…

astro-ph.GA2024★ 1 cited

Application of Manifold Learning to Selection of Different Galaxy Populations and Scaling Relation Analysis

Sogol Sanjaripour, Shoubaneh Hemmati, Bahram Mobasher +8

The growing volume of data produced by large astronomical surveys necessitates the development of efficient analysis techniques capable of effectively managing high-dimensional dat…

astro-ph.GA2024★ 6 cited

All the Little Things in Abell 2744: 1000 Gravitationally Lensed Dwarf Galaxies at from JWST NIRCam Grism Spectroscopy

Rohan P. Naidu, Jorryt Matthee, Ivan Kramarenko +31

Dwarf galaxies hold the key to crucial frontiers of astrophysics, however, their faintness renders spectroscopy challenging. Here we present the JWST Cycle 2 survey, All the Little…

astro-ph.GA2024★ 1 cited

SMILES: Potentially Higher Ionizing Photon Production Efficiency in Overdense Regions

Yongda Zhu, Stacey Alberts, Jianwei Lyu +14

The topology of reionization and the environments where galaxies efficiently produce ionizing photons are key open questions. For the first time, we investigate the trend between i…

astro-ph.GA2024

Stacking and Analyzing MOSDEF Galaxies by Spectral Types: Implications for Dust Geometry and Galaxy Evolution

Brian Lorenz, Mariska Kriek, Alice E. Shapley +12

We examine star-formation and dust properties for a sample of 660 galaxies at in the MOSDEF survey by dividing them into groups with similarly-shaped spectral…

astro-ph.GA2024★ 1 cited

Extended hot dust emission around the earliest massive quiescent galaxy

Zhiyuan Ji, Christina C. Williams, George H. Rieke +14

A major unsolved problem in galaxy evolution is the early appearance of massive quiescent galaxies that no longer actively form stars only billion years after the Big Ban…

astro-ph.GA2024★ 11 cited

The tight correlation of PAH and CO emission from z~0-4

Irene Shivaei, Leindert Boogaard

Aim: The cold molecular gas mass is one of the crucial, yet challenging parameters in galaxy evolution studies. Here, we introduce a new calibration for estimating molecular gas ma…

astro-ph.GA2024★ 25 cited

No evidence for a significant evolution of - relation in massive galaxies up to z4

Yang Sun, Jianwei Lyu, George H. Rieke +19

Over the past two decades, tight correlations between black hole masses () and their host galaxy properties have been firmly established for massive galaxies ($\log(M_*/…

astro-ph.GA2024

The SMILES Mid-Infrared Survey

George Rieke, Stacey Alberts, Irene Shivaei +4

The Mid-Infrared Instrument (MIRI) for JWST is supplied with a suite of imaging bandpass filters optimized for full spectral coverage in eight intermediate-width bands from 5 to 26…

astro-ph.GA2024★ 1 cited

SMILES Initial Data Release: Unveiling the Obscured Universe with MIRI Multi-band Imaging

Stacey Alberts, Jianwei Lyu, Irene Shivaei +12

The James Webb Space Telescope (JWST) is revolutionizing our view of the Universe through unprecedented sensitivity and resolution in the infrared, with some of the largest gains r…

astro-ph.GA2024

5-25 m Galaxy Number Counts from Deep JWST Data

Meredith A. Stone, Stacey Alberts, George H. Rieke +5

Galaxy number counts probe the evolution of galaxies over cosmic time, and serve as a valuable comparison point to theoretical models of galaxy formation. We present new galaxy num…

astro-ph.GA2024★ 36 cited

Photometric detection at of a galaxy beyond redshift with JWST/MIRI

Jakob M. Helton, George H. Rieke, Stacey Alberts +31

The James Webb Space Telescope (JWST) has spectroscopically confirmed numerous galaxies at . While weak rest-ultraviolet emission lines have only been seen in a handful of…

astro-ph.GA2024★ 46 cited

JWST FRESCO: a comprehensive census of H+[OIII] emitters at 6.8<z<9.0 in the GOODS fields

R. A. Meyer, P. A. Oesch, E. Giovinazzo +27

We present the census of H+[OIII] 4960,5008 Åemitters at 6.8<z<9.0 from the JWST FRESCO survey over 124 arcmin in the GOODS-North and GOODS-South fields. Our unbiased spectr…

astro-ph.GA2024★ 19 cited

JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields

Francesco D'Eugenio, Alex J. Cameron, Jan Scholtz +51

We present the third data release of JADES, the JWST Advanced Deep Extragalactic Survey, providing both imaging and spectroscopy in the two GOODS fields. Spectroscopy consists of m…

astro-ph.GA2024★ 25 cited

A First Look at Spatially Resolved Star Formation at with JWST FRESCO NIRCam Slitless Spectroscopy

Jasleen Matharu, Erica J. Nelson, Gabriel Brammer +19

We present the first results on the spatial distribution of star formation in 454 star-forming galaxies at using H-Alpha emission-line maps and F444W imaging tracing th…

astro-ph.GA2024★ 1 cited

FRESCO: The Paschen- Star Forming Sequence at Cosmic Noon

Chloe Neufeld, Pieter van Dokkum, Yasmeen Asali +17

We present results from the JWST First Reionization Epoch Spectroscopically Complete Observations survey (FRESCO) on the star forming sequence of galaxies at , around th…

astro-ph.GA2024★ 39 cited

JADES: Primaeval Lyman- emitting galaxies reveal early sites of reionisation out to redshift

Joris Witstok, Roberto Maiolino, Renske Smit +30

$\require{mediawiki-texvc}$Given the sensitivity of the resonant Lyman- (Ly) transition to absorption by neutral hydrogen, observations of Ly emitting…

astro-ph.GA2024★ 8 cited

Resolving the nature and putative nebular emission of GS9422: an obscured AGN without exotic stars

Sandro Tacchella, William McClymont, Jan Scholtz +27

Understanding the sources that power nebular emission in high-redshift galaxies is fundamentally important not only for shedding light onto the drivers of reionisation, but to cons…

astro-ph.IM2024★ 34 cited

JWST MIRI Flight Performance: Imaging

Dan Dicken, Macarena García Marín, Irene Shivaei +37

The Mid-Infrared Instrument (MIRI) aboard the James Webb Space Telescope (JWST) provides the observatory with a huge advance in mid-infrared imaging and spectroscopy covering the w…

astro-ph.GA2024★ 13 cited

Evidence of extended [CII] and dust emission in local dwarf galaxies

M. Romano, D. Donevski, Junais +8

The evolution of dwarf galaxies is dramatically affected by gaseous and dusty outflows, which can easily deprive their interstellar medium of the material needed for the formation…