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published · living versions
W_j8xvwu42·v1 · currentpublished
A Census of the High-Density Molecular Gas in M82
with B. J. Naylor, C. M. Bradford, J. E. Aguirre, J. J. Bock +7
1 version

Preprints & journals

212 papers in the corpus · 2008–2026
The ALMA REBELS Survey: The [C II] Luminosity Function of UV-Selected Galaxies at z∼7z\sim72610.27052v2 · Thomas Herard-Demanche, Pascal A. Oesch, Rychard Bouwens et al.2026 · 0 citationsarXiv
PAHSPECS: JWST/MIRI Spectroscopy of PAHs at Cosmic Noon2609.29955v1 · Irene Shivaei, Tanio D'iaz Santos, Leindert A. Boogaard et al.2026 · 0 citationsarXiv
JWST/NIRSpec Reveals Diverse Nuclear Environments in Dwarf Galaxies Hosting AGN2609.04315v1 · Thomas Bohn, Archana Aravindan, Gabriela Canalizo et al.2026 · 0 citationsarXiv
REBELS-25: multi-phase morphology and kinematics at z = 7.312608.25982v1 · Lucie E. Rowland, Hiddo S. B. Algera, Jacqueline Hodge et al.2026 · 0 citationsarXiv
Tracing Lyman alpha escape in the CRISTAL-02 galaxy at z~5.32608.19439v2 · Arshi Ali, Lucia Guaita, Manuel Aravena et al.2026 · 0 citationsarXiv
Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.152608.08015v1 · Gitanjali Rajulal, Hiddo S. B. Algera, Yuma Sugahara et al.2026 · 0 citationsarXiv
KCWI Discovery of a Spatially Resolved Kpc-Scale Ionized Outflow in NGC 12752608.08331v1 · Kylie Yui Dan, Hanae Inami, Thomas Bohn et al.2026 · 0 citationsarXiv
PAHSPECS: Polycyclic aromatic hydrocarbon properties at cosmic noon with JWST/MIRI MRS2606.18230v1 · Cristina Maria Lofaro, Tanio D'iaz Santos, Irene Shivaei et al.2026 · 0 citationsarXiv
PAHSPECS: Spatially Resolved PAH Spectroscopy at cosmic noon with JWST MIRI MRS2606.18244v2 · Fergus R. Donnan, Karin Sandstrom, Irene Shivaei et al.2026 · 1 citationarXiv
Direct detection of cool molecular gas in a star-forming galaxy at z=7.31z=7.312606.13393v1 · Karin Cescon, Jacqueline A. Hodge, Leindert A. Boogaard et al.2026 · 1 citationMNRAS, Volume 549, Issue 3, July 2026, stag924
Multiphase images of a powerful supernova-driven wind in the early Universe2606.10271v1 · Rebecca L. Davies, D. B. Fisher, R. Herrera-Camus et al.2026 · 1 citationarXiv
GOALS-JWST: Resolved multi-phase molecular gas in IRAS 20551-4250 using JWST and ALMA2604.18671v1 · D. Kakkad, Y. Song, T. S.-Y. Lai et al.2026 · 0 citationsarXiv
3D-Herschel: Constraining Dust Emission with Panchromatic Modeling of 3D-HST Galaxies2602.22384v2 · Seamus McNulty, Mimi Song, Katherine E. Whitaker et al.2026 · 0 citationsarXiv
A precessing jet from an active galactic nucleus drives gas outflow from a disk galaxy.41505246 · Kader, Justin A, U, Vivian, Barcos-Muñoz, Loreto et al.2026 · 4 citationsScience (New York, N.Y.). 2026;391(6788):911-916
Probing Infrared eXcess to Investigate Early-Universe Dust (PIXIEDust)2512.07964v1 · Tom J. L. C. Bakx, Hiddo S. B. Algera, Jean-Baptiste Jolly et al.2025 · 5 citationsarXiv
Probing AGN Feedback in Dwarf Galaxies with Spatially Resolved NIR Coronal Lines from JWST2512.05041v2 · Archana Aravindan, Thomas Bohn, Gabriela Canalizo et al.2025 · 0 citationsarXiv
PRIMA General Observer Science Book Volume 22511.10927v2 · A. Moullet (NRAO), D. Burgarella, T. Kataria et al.2025 · 0 citationsarXiv
A warm ultra-luminous infrared galaxy just 600 million years after the Big Bang2511.08327v1 · T. J. L. C. Bakx, Laura Sommovigo, Yoichi Tamura et al.2025 · 5 citationsarXiv
The ALPINE-CRISTAL-JWST Survey: Stellar and nebular dust attenuation of main-sequence galaxies at z~4-62510.18248v2 · Akiyoshi Tsujita, Seiji Fujimoto, Andreas Faisst et al.2025 · 4 citationsarXiv
The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~52510.16106v2 · Andreas L. Faisst, Lun-Jun Liu, Yohan Dubois et al.2025 · 4 citationsarXiv
REBELS-IFU: Linking damped Lyman-α\alpha absorption to [CII] emission and dust content in the EoR2510.11351v1 · Lucie E. Rowland, Kasper E. Heintz, Hiddo Algera et al.2025 · 1 citationarXiv
REBELS-IFU: on the origin of the elevated [OIII]/[CII] ratios in the early Universe2509.16071v1 · Hiddo Algera, Lucie Rowland, Renske Smit et al.2025 · 2 citationsarXiv
The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at z∼5z\sim52508.13136v1 · C. Accard, M. B'ethermin, M. Boquien et al.2025 · 3 citationsA&A 702, A206 (2025)
Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint2506.24128v2 · R.J. Bouwens, E. Banados, R. Decarli et al.2025 · 1 citationarXiv
REBELS-MOSFIRE: Weak CIII] Emission is Typical Among Extremely UV-bright, Massive Galaxies at z∼7z\sim72506.21674v2 · Ryan Endsley, Alice E. Shapley, Michael W. Topping et al.2025 · 0 citationsarXiv
Shockingly Effective: Cluster Winds as Engines of Feedback in Starburst Galaxy VV 1142506.16624v1 · Justin A. Kader, Vivian U, Jeffrey A. Rich et al.2025 · 2 citationsarXiv
ALMA Observations of [OI]145um and [NII]205um Emission lines from Star-Forming Galaxies at z∼7z\sim72504.03831v1 · Yoshinobu Fudamoto, Akio K. Inoue, Rychard Bouwens et al.2025 · 1 citationarXiv
A Spectroscopically Calibrated Prescription for Extracting PAH Flux from JWST MIRI Imaging2501.19397v1 · Grant P. Donnelly, Thomas S.-Y. Lai, Lee Armus et al.2025 · 0 citationsarXiv
REBELS-IFU: Dust Build-up in Massive Galaxies at Redshift 72501.10508v2 · Hiddo Algera, Lucie Rowland, Mauro Stefanon et al.2025 · 19 citationsMon Not R Astron Soc (2025)
REBELS-IFU: Dust attenuation curves of 12 massive galaxies at z≃7z\simeq72501.10541v1 · Rebecca Fisher, Rebecca A. A. Bowler, Mauro Stefanon et al.2025 · 0 citationsarXiv
REBELS-IFU: Evidence for metal-rich massive galaxies at z~6-82501.10559v1 · Lucie E. Rowland, Mauro Stefanon, Rychard Bouwens et al.2025 · 17 citationsarXiv
The Arp 240 Galaxy Merger: A Detailed Look at the Molecular Kennicutt-Schmidt Star Formation Law on Sub-kpc Scales2412.07985v1 · Alejandro Saravia, Eduardo Rodas-Quito, Loreto Barcos-Munoz et al.2024 · 2 citationsarXiv
GOALS-JWST: Constraining the Emergence Timescale for Massive Star Clusters in NGC 32562409.16503v1 · Sean T. Linden, Thomas Lai, Aaron S. Evans et al.2024 · 18 citationsarXiv
Career total: at least 499 works. 212 are in this corpus.Showing the 50 most recent.

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