activity
20142023
most citedAn ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies

278 citations · 1.4k across the 28 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2023★ 18 cited

Radio spectral properties of star-forming galaxies between 150-5000MHz in the ELAIS-N1 field

Fangxia An, M. Vaccari, P. N. Best +9

By combining high-sensitivity LOFAR 150MHz, uGMRT 400MHz and 1,250MHz, GMRT 610MHz, and VLA 5GHz data in the ELAIS-N1 field, we study the radio spectral properties of radio-detecte…

astro-ph.GA2023★ 5 cited

KAOSS: turbulent, but disc-like kinematics in dust-obscured star-forming galaxies at 1.3-2.6

Jack E. Birkin, A. Puglisi, A. M. Swinbank +13

We present spatially resolved kinematics of 27 ALMA-identified dust-obscured star-forming galaxies (DSFGs) at 1.3-2.6, as traced by H emission using VLT/KMOS near-infrare…

astro-ph.GA2022★ 34 cited

MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei

C. L. Hale, I. H. Whittam, M. J. Jarvis +22

We present deep 1.4 GHz source counts from 5 deg of the continuum Early Science data release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration (MIGH…

astro-ph.GA2022★ 52 cited

MIGHTEE: the nature of the radio-loud AGN population

I. H. Whittam, M. J. Jarvis, C. L. Hale +24

We study the nature of the faint radio source population detected in the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the COSMOS field…

astro-ph.GA2022★ 1 cited

The Physical Properties of Star-Forming Galaxies with Strong [O III] Lines at z=3.25

Run Wen, FangXia An, Xian Zhong Zheng +13

We present an analysis of physical properties of 34 [O III] emission-line galaxies (ELGs) at z=3.2540.029 in the Extended Chandra Deep Field South (ECDFS). These ELGs are sele…

astro-ph.GA2021★ 44 cited

Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation

Fangxia An, M. Vaccari, Ian Smail +17

We study the radio spectral properties of 2,094 star-forming galaxies (SFGs) by combining our early science data from the MeerKAT International GHz Tiered Extragalactic Exploration…

astro-ph.GA2020★ 45 cited

MIGHTEE: Are giant radio galaxies more common than we thought?

J. Delhaize, I. Heywood, M. Prescott +31

We report the discovery of two new giant radio galaxies (GRGs) using the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) survey. Both GRGs were found within a…

astro-ph.GA2020★ 25 cited

MAMMOTH: Confirmation of Two Massive Galaxy Overdensities at with H Emitters

XianZhong Zheng, Zheng Cai, FangXia An +2

Massive galaxy overdensities at the peak epoch of cosmic star formation provide ideal testbeds for the formation theories of galaxies and large-scale structure. We report the confi…

astro-ph.GA2020★ 104 cited

An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies

Jack E. Birkin, Axel Weiss, J. L. Wardlow +18

We present a survey of the molecular gas in 61 submillimetre galaxies (SMGs) selected from 870m continuum surveys of the COSMOS, UDS and ECDFS fields, using the Atacama Large Mi…

astro-ph.GA2020★ 92 cited

An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2 COSMOS field

J. M. Simpson, Ian Smail, U. Dudzeviciute +19

We present an ALMA study of the ~180 brightest sources in the SCUBA-2 map of the COSMOS field from the S2COSMOS survey, as a pilot study for AS2COSMOS - a full survey of the ~1,000…

astro-ph.GA2020★ 15 cited

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies

M. P. Koprowski, K. E. K. Coppin, J. E. Geach +26

We analyse 870um Atacama Large Millimetre Array (ALMA) dust continuum detections of 41 canonically-selected z~3 Lyman-break galaxies (LBGs), as well as 209 ALMA-undetected LBGs, in…

astro-ph.GA2019★ 28 cited

Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS

FangXia An, J. M. Simpson, Ian Smail +36

We identify multi-wavelength counterparts to 1,147 submillimeter sources from the S2COSMOS SCUBA-2 survey of the COSMOS field by employing a recently developed radiomachine-lear…

astro-ph.GA2019★ 278 cited

An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies

U. Dudzevičiūtė, Ian Smail, A. M. Swinbank +27

We analyse the physical properties of a large, homogeneously selected sample of ALMA-located sub-mm galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across the ~1 sq.deg.…

astro-ph.GA2019★ 67 cited

Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2

P. Lang, E. Schinnerer, Ian Smail +35

We combine high-resolution ALMA and HST/CANDELS observations of 20 submillimeter galaxies (SMGs) predominantly from the AS2UDS survey at z~2 with bright rest-frame optical counterp…

astro-ph.GA2019★ 29 cited

Radio spectra and sizes of ALMA-identified submillimetre galaxies: evidence of age-related spectral curvature and cosmic ray diffusion?

A. P. Thomson, Ian Smail, A. M. Swinbank +21

We analyse the multi-frequency radio spectral properties of 6GHz-detected ALMA-identified, submillimetre galaxies (SMGs), observed at 610MHz, 1.4GHz, 6GHz with GMRT and the VL…

astro-ph.GA2019★ 129 cited

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties

S. M. Stach, U. Dudzevičiūtė, I. Smail +26

We present the catalogue and properties of sources in AS2UDS, an 870-m continuum survey with the Atacama Large Millimetre/sub-millimetre Array (ALMA) of 716 single-dish sub-mill…

astro-ph.GA2019★ 7 cited

A machine learning approach for identifying the counterparts of submillimetre galaxies and applications to the GOODS-North field

Ruihan Henry Liu, Ryley Hill, Douglas Scott +7

Identifying the counterparts of submillimetre (submm) galaxies (SMGs) in multiwavelength images is a critical step towards building accurate models of the evolution of strongly sta…

astro-ph.GA2018★ 12 cited

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies

Yu-Yen Chang, Nicholas Ferraro, Wei-Hao Wang +25

We present structural parameters and morphological properties of faint 450-um selected submillimeter galaxies (SMGs) from the JCMT Large Program, STUDIES, in the COSMOS-CANDELS reg…

astro-ph.GA2018★ 36 cited

A machine-learning method for identifying multi-wavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS

FangXia An, S. M. Stach, Ian Smail +23

We describe the application of the supervised machine-learning algorithms to identify the likely multi-wavelength counterparts to submillimeter sources detected in panoramic, singl…

astro-ph.GA2018★ 97 cited

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: number counts of submillimeter galaxies

S. M. Stach, I. Smail, A. M. Swinbank +23

We report the first results of AS2UDS: an 870 m continuum survey with the Atacama Large Millimeter/Submillimeter Array (ALMA) of a total area of 50 arcmin comprising…

astro-ph.GA2018★ 38 cited

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Identifying candidate z~4.5 [CII] emitters

E. A. Cooke, Ian Smail, A. M. Swinbank +18

We report the results of a search for serendipitous [CII] 157.74m emitters at - using the Atacama Large Millimeter/submillimeter Array (ALMA). The search exploits…

astro-ph.GA2017★ 50 cited

Deep Imaging of the HCG 95 Field.I.Ultra-diffuse Galaxies

Dongdong Shi, Xianzhong Zheng, Haibin Zhao +7

We present a detection of 89 candidates of ultra-diffuse galaxies (UDGs) in a 4.9 degree field centered on the Hickson Compact Group 95 (HCG 95) using deep - and -band im…

astro-ph.GA2014★ 5 cited

The nature of [S III]λλ9096, 9532 emitters at z = 1.34 and 1.23

F. X. An, X. Z. Zheng, Y. Z. Meng +3

A study of [S III] emitters at = 1.34 and 1.23 is presented using our deep narrow-band (centered at 2.13 m) imaging survey of the Extended Chandra…