Search Results - "Baldry, Ivan K."
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The growth of intracluster light in XCS-HSC galaxy clusters from 0.1 < z < 0.5
Published in Monthly notices of the Royal Astronomical Society (01-04-2021)“…ABSTRACT We estimate the intracluster light (ICL) component within a sample of 18 clusters detected in the XMM Cluster Survey (XCS) data using the deep (∼26.8…”
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Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis
Published in Monthly notices of the Royal Astronomical Society (01-04-2012)“…We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital…”
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Galaxy And Mass Assembly (GAMA): deconstructing bimodality – I. Red ones and blue ones
Published in Monthly notices of the Royal Astronomical Society (11-01-2015)“…We measure the mass functions for generically red and blue galaxies, using a z < 0.12 sample of log M* > 8.7 field galaxies from the Galaxy And Mass Assembly…”
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Galaxy And Mass Assembly (GAMA): the stellar mass budget by galaxy type
Published in Monthly notices of the Royal Astronomical Society (01-04-2016)“…We report an expanded sample of visual morphological classifications from the Galaxy and Mass Assembly survey phase two, which now includes 7556 objects…”
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Environment from cross-correlations: connecting hot gas and the quenching of galaxies
Published in Monthly notices of the Royal Astronomical Society (01-08-2020)“…ABSTRACT The observable properties of galaxies depend on both internal processes and the external environment. In terms of the environmental role, we still do…”
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Galaxy pairs in the Sloan Digital Sky Survey – II. The effect of environment on interactions
Published in Monthly notices of the Royal Astronomical Society (21-09-2010)“…We use a sample of close galaxy pairs selected from the Sloan Digital Sky Survey Data Release 4 (SDSS DR4) to investigate in what environments galaxy mergers…”
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The Bimodal Galaxy Color Distribution: Dependence on Luminosity and Environment
Published in The Astrophysical journal (10-11-2004)Get full text
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Constraints on a Universal Stellar Initial Mass Function from Ultraviolet to Near-Infrared Galaxy Luminosity Densities
Published in The Astrophysical journal (10-08-2003)Get full text
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Quantifying the Bimodal Color-Magnitude Distribution of Galaxies
Published in The Astrophysical journal (10-01-2004)“…We analyze the bivariate distribution, in color versus absolute magnitude (u-r vs. M sub(r)), of a low-redshift sample of galaxies from the Sloan Digital Sky…”
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Exploring relations between BCG and cluster properties in the SPectroscopic IDentification of eROSITA Sources survey from 0.05 <z < 0.3
Published in Monthly notices of the Royal Astronomical Society (21-08-2018)“…ABSTRACT We present a sample of 329 low-to intermediate-redshift (0.05 <z< 0.3) brightest cluster galaxies (BCGs) in X-ray-selected clusters from the…”
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The mass–metallicity relation in galaxy clusters: the relative importance of cluster membership versus local environment
Published in Monthly notices of the Royal Astronomical Society (01-07-2009)“…Using a large (14 857), homogenously selected sample of cluster galaxies identified in the Sloan Digital Sky Survey Data Release 4, we investigate the impact…”
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Galaxy and Mass Assembly: FUV, NUV, ugrizYJHK Petrosian, Kron and Sérsic photometry
Published in Monthly notices of the Royal Astronomical Society (01-04-2011)“…In order to generate credible 0.1-2 μm spectral energy distributions, the Galaxy and Mass Assembly (GAMA) project requires many gigabytes of imaging data from…”
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Evolution of star formation in the UKIDSS Ultra Deep Survey field - I. Luminosity functions and cosmic star formation rate out to z = 1.6
Published in Monthly notices of the Royal Astronomical Society (21-07-2013)“…We present new results on the cosmic star formation history in the Subaru/XMM-Newton Deep Survey (SXDS)-Ultra Deep Survey (UDS) field out to z = 1.6. We…”
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Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS
Published in Monthly notices of the Royal Astronomical Society (01-03-2004)“…ABSTRACT We analyse the observed correlation between galaxy environment and Hα emission‐line strength, using volume‐limited samples and group catalogues of 24…”
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Compact galaxies and the size–mass galaxy distribution from a colour-selected sample at 0.04 < z < 0.15 supplemented by ugrizYJHK photometric redshifts
Published in Monthly notices of the Royal Astronomical Society (01-01-2021)“…ABSTRACT The size–mass galaxy distribution is a key diagnostic for galaxy evolution. Massive compact galaxies are potential surviving relics of a high-redshift…”
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Galaxy And Mass Assembly (GAMA): a forensic SED reconstruction of the cosmic star formation history and metallicity evolution by galaxy type
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT We apply the spectral energy distribution (SED) fitting code ProSpect to multiwavelength imaging for ∼7000 galaxies from the GAMA survey at z < 0.06,…”
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Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
Published in Monthly notices of the Royal Astronomical Society (23-04-2022)“…ABSTRACT In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248 682 galaxy spectra,…”
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Galaxy And Mass Assembly (GAMA): mass–size relations of z < 0.1 galaxies subdivided by Sérsic index, colour and morphology
Published in Monthly notices of the Royal Astronomical Society (01-03-2015)“…We use data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01 < z < 0.1 (8399 galaxies in g to Ks bands) to derive the stellar…”
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Galaxy Zoo: the dependence of morphology and colour on environment
Published in Monthly notices of the Royal Astronomical Society (11-03-2009)“…We analyse the relationships between galaxy morphology, colour, environment and stellar mass using data for over 105 objects from Galaxy Zoo, the largest…”
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The galaxy stellar mass function and low surface brightness galaxies from core-collapse supernovae
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)“…Abstract We introduce a method for producing a galaxy sample unbiased by surface brightness and stellar mass, by selecting star-forming galaxies via the…”
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