Search Results - "Wilkins, S. M."
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Discovery and properties of ultra-high redshift galaxies (9 < z < 12) in the JWST ERO SMACS 0723 Field
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT We present a reduction and analysis of the James Webb Space Telescope (JWST) SMACS 0723 field using new post-launch calibrations to conduct a search…”
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Galaxy And Mass Assembly: accurate panchromatic photometry from optical priors using lambdar
Published in Monthly notices of the Royal Astronomical Society (21-07-2016)“…We present the Lambda Adaptive Multi-Band Deblending Algorithm in R (lambdar), a novel code for calculating matched aperture photometry across images that are…”
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Galaxy And Mass Assembly (GAMA): curation and reanalysis of 16.6k redshifts in the G10/COSMOS region
Published in Monthly notices of the Royal Astronomical Society (11-02-2015)“…We discuss the construction of the Galaxy And Mass Assembly (GAMA) 10h region (G10) using publicly available data in the Cosmic Evolution Survey region…”
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The ultraviolet colours and dust attenuation of Lyman-break galaxies
Published in Monthly notices of the Royal Astronomical Society (21-02-2013)“…Using galform, a semi-analytical model of galaxy formation in the Λ cold dark matter cosmology, we study the rest-frame ultraviolet (UV) colours of Lyman-break…”
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Galaxy And Mass Assembly: the G02 field, Herschel–ATLAS target selection and data release 3
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…Abstract We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic redshift and multiwavelength…”
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Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function to z = 0.1 from the r-band selected equatorial regions
Published in Monthly notices of the Royal Astronomical Society (01-09-2017)“…Abstract We derive the low-redshift galaxy stellar mass function (GSMF), inclusive of dust corrections, for the equatorial Galaxy And Mass Assembly (GAMA) data…”
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Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass
Published in Monthly notices of the Royal Astronomical Society (11-11-2014)“…We use a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift sample to fully describe the stellar mass dependence of close pairs and…”
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Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies
Published in Monthly notices of the Royal Astronomical Society (01-09-2015)“…The modification of star formation (SF) in galaxy interactions is a complex process, with SF observed to be both enhanced in major mergers and suppressed in…”
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Red, redder, reddest: SCUBA-2 imaging of colour-selected Herschel sources
Published in Monthly notices of the Royal Astronomical Society (11-06-2018)“…Abstract High-redshift, luminous, dusty star-forming galaxies (DSFGs) constrain the extremity of galaxy formation theories. The most extreme are discovered…”
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Galaxy And Mass Assembly (GAMA): bivariate functions of Hα star-forming galaxies
Published in Monthly notices of the Royal Astronomical Society (01-02-2015)“…We present bivariate luminosity and stellar mass functions of Hα star-forming galaxies drawn from the Galaxy And Mass Assembly (GAMA) survey. While optically…”
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11
Discovery and properties of ultra-high redshift galaxies ($9<z<12$) in the JWST ERO SMACS 0723 Field
Published 03-01-2023“…We present a reduction and analysis of the \textit{James Webb Space Telescope} (JWST) SMACS~0723 field using new post-launch calibrations to conduct a search…”
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12
ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields
Published 22-10-2024“…We present a set of photometric catalogs primarily aimed at providing the community with a comprehensive database for the study of galaxy populations in the…”
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The emergence of passive galaxies in the early Universe
Published 11-05-2021“…A&A 652, A30 (2021) The emergence of passive galaxies in the early Universe results from the interplay among the processes responsible for their rapid assembly…”
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Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
Published in Monthly notices of the Royal Astronomical Society (11-09-2015)“…The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectroscopic surveys of low redshift galaxies. Covering an area of ∼286 deg2…”
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GALAXY AND MASS ASSEMBLY (GAMA): MID-INFRARED PROPERTIES AND EMPIRICAL RELATIONS FROM WISE
Published in The Astrophysical journal (20-02-2014)“…The Galaxy And Mass Assembly (GAMA) survey furnishes a deep redshift catalog that, when combined with the Wide-field Infrared Survey Explorer (WISE), allows us…”
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CEERS MIRI Imaging: Data Reduction and Quality Assessment
Published in Astrophysical journal. Letters (01-10-2023)“…Abstract The Cosmic Evolution Early Release Science Survey (CEERS), targeting the Extended Groth Strip extragalactic field, is one of the James Webb Space…”
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Temperature dependence of chiral discrimination in supercritical fluid chromatography and high-performance liquid chromatography
Published in Journal of Chromatography A (21-04-1995)“…Chiral separations of related compounds within a series of potassium channel activator (KCA) analogues were compared by supercritical fluid chromatography…”
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18
Red, redder, reddest: SCUBA-2 imaging of colour-selected \textit{Herschel} sources
Published 22-01-2018“…High-redshift, luminous, dusty star forming galaxies (DSFGs) constrain the extremity of galaxy formation theories. The most extreme are discovered through…”
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Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3
Published 24-11-2017“…Mon.Not.Roy.Astron.Soc. 474 (2018) 3875-3888 We describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic…”
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20
Interpreting high [O III]/Hbeta ratios with maturing starbursts
Published 18-08-2014“…Star forming galaxies at high redshift show ubiquitously high ionization parameters, as measured by the ratio of optical emission lines. We demonstrate that…”
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