258 citations · 1.3k across the 18 of their papers we have counts for
18 papers
Hidden in Plain Sight: Searching for Globular Clusters Within JWST Observations of the PLCK G165.7+67.0 Galaxy Cluster
Tyler R. Hinrichs, Patrick S. Kamieneski, Rogier A. Windhorst +21
Although the James Webb Space Telescope (JWST) has received much attention for its ability to search deeper into the cosmos than ever before, it also enhances our capability to stu…
Nessie: A Rust-Powered, Fast, Flexible, and Generalized Friends-of-Friends Galaxy-Group Finder in R and Python
Trystan S. Lambert, A. S. G. Robotham, M. Bravo +4
We introduce Nessie, a galaxy group finder implemented in Rust and distributed as both a Python and R package. Nessie employs the friends-of-friends (FoF) algorithm and requires on…
Galaxy And Mass Assembly (GAMA): Environment-dependent galaxy stellar mass functions in the low-redshift Universe
A. Sbaffoni, J. Liske, S. P. Driver +2
From a carefully selected sample of galaxies and groups, we investigate the variation of the low-redshift galaxy stellar mass function (GSMF) in the equatorial…
ProSpect: Generating Spectral Energy Distributions with Complex Star Formation and Metallicity Histories
A. S. G. Robotham, S. Bellstedt, C. del P. Lagos +4
We introduce ProSpect, a generative galaxy spectral energy distribution (SED) package that encapsulates the best practices for SED methodologies in a number of astrophysical domain…
Star-Forming, Rotating Spheroidal Galaxies in the GAMA and SAMI Surveys
Amanda J. Moffett, Steven Phillipps, Aaron S. G. Robotham +23
The Galaxy And Mass Assembly (GAMA) survey has morphologically identified a class of "Little Blue Spheroid" (LBS) galaxies whose relationship to other classes of galaxies we now ex…
On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
Rogier A. Windhorst, M. Alpaslan, S. Andrews +44
Recent near-IR power-spectra and panchromatic Extragalactic Background Light measurements provide upper limits on the near-IR surface brightness (SB>31 mag/arcsec^2) that may come…
Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
L. J. M. Davies, A. S. G. Robotham, C. del P. Lagos +16
Recently a number of studies have found a similarity between the passive fraction of central and satellite galaxies when controlled for both stellar and halo mass. These results su…
The Causes of the Red Sequence, the Blue Cloud, the Green Valley and the Green Mountain
Stephen Eales, Maarten Baes, Nathan Bourne +23
The galaxies found in optical surveys fall in two distinct regions of a diagram of optical colour versus absolute magnitude: the red sequence and the blue cloud with the green vall…
Galaxy And Mass Assembly (GAMA): impact of the group environment on galaxy star formation
S. Barsanti, M. S. Owers, S. Brough +9
We explore how the group environment may affect the evolution of star-forming galaxies. We select 1197 Galaxy And Mass Assembly (GAMA) groups at and analyze t…
Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3
I. K. Baldry, J. Liske, M. J. I. Brown +39
We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic redshift and multi-wavelength photometric survey in three equator…
Galaxy And Mass Assembly (GAMA): Accurate Panchromatic Photometry from Optical Priors using LAMBDAR
A. H. Wright, A. S. G. Robotham, N. Bourne +26
We present the Lambda Adaptive Multi-Band Deblending Algorithm in R (LAMBDAR), a novel code for calculating matched aperture photometry across images that are neither pixel- nor PS…
Galaxy And Mass Assembly (GAMA): the wavelength-dependent sizes and profiles of galaxies revealed by MegaMorph
Benedetta Vulcani, Steven P. Bamford, Boris Häußler +14
We investigate the relationship between colour and structure within galaxies using a large, volume-limited sample of bright, low-redshift galaxies with optical to near-infrared ima…
Galaxy and Mass Assembly (GAMA): The evolution of bias in the radio source population to z ~ 1.5
S. N. Lindsay, M. J. Jarvis, M. G. Santos +8
We present a large-scale clustering analysis of radio galaxies in the Very Large Array (VLA) Faint Images of the Radio Sky at Twenty-cm (FIRST) survey over the Galaxy And Mass Asse…
Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing
J. González-Nuevo, A. Lapi, M. Negrello +25
We report a highly significant () spatial correlation between galaxies with mJy detected in the equatorial fields of the \textsl{Herschel} Astrophysica…
Galaxy And Mass Assembly (GAMA): Resolving the role of environment in galaxy evolution
S. Brough, S. Croom, R. Sharp +18
We present observations of 18 galaxies from the Galaxy And Mass Assembly (GAMA) survey made with the SPIRAL optical integral field unit (IFU) on the Anglo-Australian Telescope. The…
Herschel-ATLAS/GAMA: a difference between star-formation rates in strong-line and weak-line radio galaxies
M. J. Hardcastle, J. H. Y. Ching, J. S. Virdee +25
We have constructed a sample of radio-loud objects with optical spectroscopy from the Galaxy and Mass Assembly (GAMA) project over the Herschel-ATLAS Phase 1 fields. Classifying th…
Galaxy and Mass Assembly (GAMA): FUV, NUV, ugrizYJHK Petrosian, Kron and Sèrsic photometry
David T. Hill, Lee S. Kelvin, Simon P. Driver +33
In order to generate credible 0.1-2 μm SEDs, the GAMA project requires many Gigabytes of imaging data from a number of instruments to be re-processed into a standard format. In thi…
The Herschel-ATLAS: Evolution of the 250um luminosity function out to z=0.5
S. Dye, L. Dunne, S. Eales +65
We have determined the luminosity function of 250um-selected galaxies detected in the ~14 sq.deg science demonstration region of the Herschel-ATLAS project out to a redshift of z=0…