activity
19992026
most citedALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass

281 citations · 1.2k across the 37 of their papers we have counts for

collaborators

38 papers

astro-ph.GA2026

Resolved SED modelling with JWST and ALMA: the role of stellar mass surface density in regulating star formation in cosmic noon galaxies

Cheng-Lin Liao, Leindert A. Boogaard, Jacqueline A. Hodge +27

We present kpc-scale () physical property maps of 35 main-sequence galaxies at , with stellar masses of and star f…

astro-ph.GA2026

The JWST Emission Line Survey (JELS): A narrow-band determination of the H Luminosity Function and Cosmic Star Formation into the Epoch of Reionization

C. A. Pirie, K. J. Duncan, P. N. Best +19

The recent star-formation activity in galaxies can be optimally traced by the H emission line, with the resulting H luminosity function (LF) at a given epoch providing a reli…

astro-ph.GA2026★ 1 cited

Investigating the role of turbulence in the interstellar medium in dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps

B. A. Westoby, J. A. Hodge, P. Sharda +28

We present ALMA high-resolution (0.25/2 kpc) CO(5-4) and CO(4-3) observations of three submillimetre-selected dusty galaxies from the ALESS survey.…

astro-ph.GA2026★ 1 cited

Extending the ALMA survey of the SCUBA-2 CLS UDS field: Tracing the obscured formation of spheroids across z~1-4

Ian Smail, Steven Gillman, Ugne Dudzeviciute +1

We investigate the properties of 870-um selected galaxies at z~1-4 with FIR luminosities of LIR~1e11-1e13Lo, encompassing systems that dominate obscured activity at the peak of cos…

astro-ph.GA2026★ 1 cited

ALESS--JWST: Dust-driven Morphologies and Hidden Stellar Mass in Sub-millimeter Galaxies

J. Li, E. da Cunha, J. A. Hodge +17

We present JWST/NIRCam and MIRI observations of twelve sub-millimeter galaxies (SMGs) from the ALESS survey, combined with high-resolution () ALMA 870m i…

astro-ph.GA2026

JWST's PEARLS: A clumpy ring galaxy at

David Vizgan, Ming-Yang Zhuang, Ian Smail +22

Ring galaxies are an uncommon class of galaxies whose morphology is closely related to dynamical processes that govern galaxy evolution. Some ring galaxies, known as "collisional r…

astro-ph.GA2025

KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at

Zefeng Li, Ugnė Dudzevičiūtė, Annagrazia Puglisi +13

Gas-phase oxygen abundance (metallicity) properties can be constrained through emission line analyses, and are of great importance to investigate galaxy evolution histories. We pre…

astro-ph.GA2025

The VLA Frontier Fields Survey: A 6GHz High-resolution Radio Survey of Abell2744

Esteban A. Orozco, Eric F. Jiménez-Andrade, Eric J. Murphy +5

We present 6GHz radio continuum observations of the galaxy cluster Abell 2744 () obtained with the Karl G. Jansky Very Large Array (VLA) as part of the VLA Frontier Fiel…

astro-ph.GA2025★ 2 cited

ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09

Shuo Huang, Hideki Umehata, Ian Smail +6

Protoclusters represent the densest regions of cosmic large-scale structure in the early universe and are the environment where present-day massive elliptical galaxies are assemble…

astro-ph.GA2025★ 1 cited

ADF22-WEB: ALMA and JWST (sub)kpc-scale views of dusty star-forming galaxies in a 3 proto-cluster

Hideki Umehata, Mariko Kubo, Ian Smail +4

We present a morphological analysis of ALMA and JWST NIRCam images of nine dusty star-forming galaxies (DSFGs) at zspec=3.09, all embedded within the cosmic web filaments at the SS…

astro-ph.GA2025

ALMA/SCUBA-2 COSMOS Survey: Properties of X-ray- and SED-selected AGNs in Bright Submillimeter Galaxies

Ryosuke Uematsu, Yoshihiro Ueda, David M. Alexander +11

We investigate the properties of active galactic nuclei (AGNs) in the brightest submillimeter galaxies (SMGs) in the COSMOS field. We utilize the bright sample of ALMA/SCUBA-2 COSM…

astro-ph.GA2024

The properties of the interstellar medium in dusty, star-forming galaxies at : The shape of the CO spectral line energy distributions

Dominic J. Taylor, A. M. Swinbank, Ian Smail +15

The molecular gas in the interstellar medium (ISM) of star-forming galaxy populations exhibits diverse physical properties. We investigate the CO excitation of twelve dusty,…

astro-ph.GA2024★ 5 cited

CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around star-forming galaxies at high redshift

Matus Rybak, J. T. Jansen, M. Frias Castillo +15

Massive, intensely star-forming galaxies at high redshift require a supply of molecular gas from their gas reservoirs, replenished by infall from the surrounding circumgalactic med…

astro-ph.GA2024

The MUSE Ultra Deep Field (MUDF) VII. Probing high-redshift gas structures in the surroundings of ALMA-identified massive dusty galaxies

A. Pensabene, M. Galbiati, M. Fumagalli +12

We present new ALMA continuum and spectral observations of the MUSE Ultra Deep Field (MUDF), a arcmin region with ultradeep multiwavelength imaging and spectroscopy…

astro-ph.GA2024★ 1 cited

The JWST Emission Line Survey (JELS): An untargeted search for H emission line galaxies at and their physical properties

C. A. Pirie, P. N. Best, K. J. Duncan +19

We present the first results of the JWST Emission Line Survey (JELS). Utilising the first NIRCam narrow-band imaging at 4.7m, over 63 arcmin in the PRIMER/COSMOS field, we…

astro-ph.GA2024

ALESS-JWST: Joint (sub-)kiloparsec JWST and ALMA imaging of submillimeter galaxies reveals heavily obscured bulge formation events

Jacqueline A. Hodge, Elisabete da Cunha, Sarah Kendrew +25

We present JWST NIRCam imaging targeting 13 infrared-luminous () galaxies from the ALESS survey with uniquely deep, high-resolution…

astro-ph.GA2024

A 100 Mpc structure traced by hyperluminous galaxies around a massive = 2.85 protocluster

George C. P. Wang, Scott C. Chapman, Nikolaus Sulzenauer +9

We present wide-field mapping at 850 m and 450 m of the = 2.85 protocluster in the HS154919 field using the Submillimetre Common User Bolometer Array 2 (SCUBA-2). Spec…

astro-ph.GA2024

ALMA Lensing Cluster Survey: Physical characterization of near-infrared-dark intrinsically faint ALMA sources at z=2-4

Akiyoshi Tsujita, Kotaro Kohno, Shuo Huang +33

We present results from Atacama Large Millimeter/submillimeter Array (ALMA) spectral line-scan observations at 3-mm and 2-mm bands of three near-infrared-dark (NIR-dark) galaxies b…

astro-ph.GA2024★ 39 cited

The Structure of Massive Star-Forming Galaxies from JWST and ALMA: Dusty, High Redshift Disk Galaxies

Steven Gillman, Ian Smail, Bitten Gullberg +15

We present an analysis of the JWST NIRCam and MIRI morphological properties of 80 massive (=11.20.1) dusty star-forming galaxies at 2.7$^{+…

astro-ph.GA2024★ 7 cited

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 m and Data Release for the COSMOS Field

Zhen-Kai Gao, Chen-Fatt Lim, Wei-Hao Wang +19

We present confusion-limited SCUBA-2 450-m observations in the COSMOS-CANDELS region as part of the JCMT Large Program, SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). Our maps…

astro-ph.CO2024★ 1 cited

Beyond MACS: Physical properties of extremely X-ray luminous clusters at

H. Ebeling, J. Richard, B. Beauchesne +3

We present a sample of over 100 highly X-ray luminous galaxy clusters at 0.5-0.9, discovered by the extended Massive Cluster Survey (eMACS) in ROSAT All-Sky Survey (RASS) d…

astro-ph.GA2024

A Comparative Study of the Ground State Transitions of CO and [C I] as Molecular Gas Tracers at High Redshift

Marta Frias Castillo, Matus Rybak, Jacqueline A. Hodge +22

The CO(1--0) and [\ion{C}{1}](1--0) emission lines are well-established tracers of cold molecular gas mass in local galaxies. At high redshift, where the interstellar medium (ISM)…

astro-ph.GA2024★ 1 cited

The onset of bar formation in a massive galaxy at

Aristeidis Amvrosiadis, Samuel Lange, James Nightingale +13

We examine the morphological and kinematical properties of SPT-2147, a strongly lensed, massive, dusty, star-forming galaxy at . Combining data from JWST, HST, and ALMA,…

astro-ph.GA2024★ 20 cited

Primordial Rotating Disk Composed of 15 Dense Star-Forming Clumps at Cosmic Dawn

S. Fujimoto, M. Ouchi, K. Kohno +43

Early galaxy formation, initiated by the dark matter and gas assembly, evolves through frequent mergers and feedback processes into dynamically hot, chaotic structures. In contrast…