activity
20132026
most citedA lack of evolution in the very bright-end of the galaxy luminosity function from z = 8-10

218 citations · 694 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

Constraining reionization-era Ly escape with JELS-MUSE: a highly complete H-selected sample at

A. L. Patrick, K. J. Duncan, Z. Li +16

The Ly escape fraction, , probes both the interstellar medium (ISM) conditions governing ionizing photon escape and the rising neutral fraction of the I…

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.IM2026

HARMONI@ELT: instrument design, performance, and science capabilities

B. Neichel, J. Dunlop, S. Chittick +17

HARMONI is the integral field spectrograph for the Extremely Large Telescope (ELT). Designed as the primary workhorse near-infrared spectrograph of the ELT, it will deliver spatial…

astro-ph.GA2024★ 8 cited

The JWST Emission Line Survey (JELS): Extending rest-optical narrow-band emission line selection into the Epoch of Reionization

K. J. Duncan, D. J. McLeod, P. N. Best +20

We present the JWST Emission Line Survey (JELS), a JWST imaging programme exploiting the wavelength coverage and sensitivity of NIRCam to extend narrow-band rest-optical emission l…

astro-ph.GA2024★ 5 cited

The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z=4.41 from Ultraviolet to Near-Infrared Wavelengths

Ryan L. Sanders, Alice E. Shapley, Michael W. Topping +28

We use JWST/NIRSpec observations from the Assembly of Ultradeep Rest-optical Observations Revealing Astrophysics (AURORA) survey to constrain the shape of the nebular attenuation c…

astro-ph.GA2024★ 2 cited

The AURORA Survey: A New Era of Emission-line Diagrams with JWST/NIRSpec

Alice E. Shapley, Ryan L. Sanders, Michael W. Topping +28

We present results on the emission-line properties of z=1.4-7.5 star-forming galaxies in the Assembly of Ultradeep Rest-optical Observations Revealing Astrophysics (AURORA) Cycle 1…

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.GA2024★ 23 cited

Charting the main sequence of star-forming galaxies out to redshifts z<5.7

M. P. Koprowski, J. V. Wijesekera, J. S. Dunlop +4

We present a new determination of the star-forming main sequence (MS), obtained through stacking 100k K-band-selected galaxies in the far-infrared (FIR) Herschel and James Clerk Ma…

astro-ph.GA2023★ 1 cited

The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10

F. Cullen, D. J. McLeod, R. J. McLure +11

We present an analysis of the ultraviolet (UV) continuum slopes () for a sample of galaxy candidates at selected from a combination of JWST NI…

astro-ph.GA2023★ 2 cited

The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z = 4-8 revealed by the IRX- and relations

R. A. A. Bowler, H. Inami, L. Sommovigo +23

We investigate the degree of dust obscured star formation in 49 massive () Lyman-break galaxies (LBGs) at - observed as par…

astro-ph.CO2023★ 1 cited

An optimal ALMA image of the Hubble Ultra Deep Field in the era of JWST: obscured star formation and the cosmic far-infrared background

Ryley Hill, Douglas Scott, Derek J. McLeod +3

We combine archival ALMA data targeting the Hubble Ultra Deep Field (HUDF) to produce the deepest currently attainable 1-mm maps of this key region. Our deepest map covers 4.2arcmi…

astro-ph.GA2023★ 1 cited

Connecting the escape fraction of Lyman-alpha and Lyman-continuum photons in star-forming galaxies at

R. Begley, F. Cullen, R. J. McLure +7

We present a study of the connection between the escape fraction of Lyman-alpha (Ly) and Lyman-continuum (LyC) photons within a sample of N=152 star-forming galaxies selected fr…

astro-ph.GA2019★ 218 cited

A lack of evolution in the very bright-end of the galaxy luminosity function from z = 8-10

R. A. A. Bowler, M. J. Jarvis, J. S. Dunlop +5

We utilize deep near-infrared survey data from the UltraVISTA fourth data release (DR4) and the VIDEO survey, in combination with overlapping optical and Spitzer data, to search fo…

astro-ph.GA2019★ 12 cited

Maximising the power of deep extragalactic imaging surveys with the James Webb Space Telescope

T. W. Kemp, J. S. Dunlop, R. J. McLure +3

We present a new analysis of the potential power of deep, near-infrared, imaging surveys with the James Webb Space Telescope (JWST) to improve our knowledge of galaxy evolution. In…

astro-ph.GA2016★ 163 cited

Unveiling the nature of bright z ~ 7 galaxies with the Hubble Space Telescope

R. A. A. Bowler, J. S. Dunlop, R. J. McLure +1

We present new Hubble Space Telescope/Wide Field Camera 3 imaging of 25 extremely luminous (-23.2 < M_ UV < -21.2) Lyman-break galaxies (LBGs) at z ~ 7. The sample was initially se…

astro-ph.GA2014★ 195 cited

The galaxy luminosity function at z ~ 6 and evidence for rapid evolution in the bright end from z ~ 7 to 5

R. A . A. Bowler, J. S. Dunlop, R. J. McLure +8

We present the results of a search for bright (-22.7 < M_UV < -20.5) Lyman-break galaxies at z ~ 6 within a total of 1.65 square degrees of imaging in the UltraVISTA/COSMOS and UKI…

astro-ph.IM2014★ 7 cited

Science Case and Requirements for the MOSAIC Concept for a Multi-Object Spectrograph for the European Extremely Large Telescope

C. J. Evans, M. Puech, B. Barbuy +55

Over the past 18 months we have revisited the science requirements for a multi-object spectrograph (MOS) for the European Extremely Large Telescope (E-ELT). These efforts span the…

astro-ph.CO2013★ 49 cited

A reassessment of the redshift distribution and physical properties of luminous (sub-)millimetre galaxies

M. P. Koprowski, J. S. Dunlop, M. J. Michalowski +2

Motivated by the current controversy over the redshift distribution and physical properties of luminous (sub-)mm sources, we have undertaken a new study of the brightest sample of…