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The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts (2016)
Journal Article
Serjeant, S., Geach, J. E., Dunlop, J. S., Halpern, M., Smail, I., van der Werf, P., …Zemcov, M. (2017). The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts. Monthly Notices of the Royal Astronomical Society, 465(2), 1789-1806. https://doi.org/10.1093/mnras/stw2721

We present a catalogue of ∼3000 submillimetre sources detected (≥3.5σ) at 850 μm over ∼5 deg2 surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 Cosmology Legacy Survey (S2CLS). This is the largest survey of its kind at 850 μm, incr... Read More about The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts.

Faint submillimeter galaxies identified through their optical/near-infrared colors: 1. Spatial clustering and halo masses (2016)
Journal Article
Chen (陳建州), C., Smail, I., Swinbank, A., Simpson, J. M., Almaini, O., Conselice, C. J., …Wilkinson, A. (2016). Faint submillimeter galaxies identified through their optical/near-infrared colors: 1. Spatial clustering and halo masses. Astrophysical Journal, 831(1), https://doi.org/10.3847/0004-637X/831/1/91

The properties of submillimeter galaxies (SMGs) that are fainter than the confusion limit of blank-field single-dish surveys (S850  2 mJy) are poorly constrained. Using a newly developed color selection technique, Optical-Infrared Triple Color (OIRT... Read More about Faint submillimeter galaxies identified through their optical/near-infrared colors: 1. Spatial clustering and halo masses.

Galaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELS (2016)
Journal Article
Simmons, B., Lintott, C., Willett, K. W., Masters, K. L., Kartaltepe, J. S., Häußler, B., …Wiklind, T. (2017). Galaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELS. Monthly Notices of the Royal Astronomical Society, 464(4), doi:10.1093/mnras/stw2587

We present quantified visual morphologies of approximately 48 000 galaxies observed in three Hubble Space Telescope legacy fields by the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) and classified by participants in the Ga... Read More about Galaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELS.

The evolution of galaxy number density at z < 8 and its implications (2016)
Journal Article
Conselice, C. J., Wilkinson, A., Duncan, K., & Mortlock, A. (2016). The evolution of galaxy number density at z < 8 and its implications. Astrophysical Journal, 830(2), doi:10.3847/0004-637X/830/2/83

The evolution of the number density of galaxies in the universe, and thus also the total number of galaxies, is a fundamental question with implications for a host of astrophysical problems including galaxy evolution and cosmology. However there has... Read More about The evolution of galaxy number density at z < 8 and its implications.

Exploring the progenitors of brightest cluster galaxies at z ∼ 2 (2016)
Journal Article
Zhao, D., Conselice, C. J., Aragón-Salamanca, A., Almaini, O., Hartley, W. G., Lani, C., …Old, L. (2017). Exploring the progenitors of brightest cluster galaxies at z ∼ 2. Monthly Notices of the Royal Astronomical Society, 464(2), doi:10.1093/mnras/stw2406

We present a new method for tracing the evolution of brightest cluster galaxies (BCGs) from z ∼ 2 to z ∼ 0. We conclude on the basis of semi-analytical models that the best method to select BCG progenitors at z ∼ 2 is a hybrid environmental density a... Read More about Exploring the progenitors of brightest cluster galaxies at z ∼ 2.

The impact of protocluster environments at z = 1.6 (2016)
Journal Article
Hatch, N. A., Cooke, E. A., Muldrew, S. I., Hartley, W. G., Almaini, O., Conselice, C. J., & Simpson, C. (2017). The impact of protocluster environments at z = 1.6. Monthly Notices of the Royal Astronomical Society, 464(1), 876-884. https://doi.org/10.1093/mnras/stw2359

We investigate the effects of dense environments on galaxy evolution by examining how the properties of galaxies in the z = 1.6 protocluster Cl 0218.3−0510 depend on their location. We determine galaxy properties using spectral energy distribution fi... Read More about The impact of protocluster environments at z = 1.6.

Mass assembly and morphological transformations since z∼ 3 from CANDELS (2016)
Journal Article
Huertas-Company, M., Bernardi, M., Pérez-González, P., Ashby, M., Barro, G., Conselice, C. J., …Shankar, F. (2016). Mass assembly and morphological transformations since z∼ 3 from CANDELS. Monthly Notices of the Royal Astronomical Society, 462(4), doi:10.1093/mnras/stw1866

We quantify the evolution of the stellar mass functions (SMFs) of star-forming and quiescent galaxies as a function of morphology from z ∼ 3 to the present. Our sample consists of ∼50 000 galaxies in the CANDELS fields (∼880 arcmin2), which we divide... Read More about Mass assembly and morphological transformations since z∼ 3 from CANDELS.

The formation of bulges, discs and two-component galaxies in the CANDELS Survey at z < 3 (2016)
Journal Article
Margalef-Bentabol, B., Conselice, C. J., Mortlock, A., Hartley, W., Duncan, K., Ferguson, H. C., …Primack, J. R. (2016). The formation of bulges, discs and two-component galaxies in the CANDELS Survey at z < 3. Monthly Notices of the Royal Astronomical Society, 461(3), doi:10.1093/mnras/stw1451

We examine a sample of 1495 galaxies in the CANDELS fields to determine the evolution of two-component galaxies, including bulges and discs, within massive galaxies at the epoch 1 < z < 3 when the Hubble sequence forms. We fit all of our galaxies’ li... Read More about The formation of bulges, discs and two-component galaxies in the CANDELS Survey at z < 3.

HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster (2016)
Journal Article
Fabian, A., Walker, S., Russell, H., Pinto, C., Canning, R., Salome, P., …Reynolds, C. (in press). HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster. Monthly Notices of the Royal Astronomical Society, 461(1), doi:10.1093/mnras/stw1350

Narrow-band HST imaging has resolved the detailed internal structure of the 10 kpc diameter H α+[N II] emission line nebulosity in NGC4696, the central galaxy in the nearby Centaurus cluster, showing that the dusty, molecular, filaments have a width... Read More about HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster.

The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation (2016)
Journal Article
Ownsworth, J. R., Conselice, C. J., Mundy, C. J., Mortlock, A., Hartley, W. G., Duncan, K., & Almaini, O. (2016). The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation. Monthly Notices of the Royal Astronomical Society, 461(1), doi:10.1093/mnras/stw1207

Due to significant galaxy contamination and impurity in stellar mass selected samples (up to 95 per cent from z = 0–3), we examine the star formation history, quenching time-scales, and structural evolution of galaxies using a constant number density... Read More about The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation.

The Dark Energy Survey: more than dark energy – an overview (2016)
Journal Article
Abbott, T., Abdalla, F., Aleksic, J., Allam, S., Amara, A., Bacon, D., …Conselice, C. J. (2016). The Dark Energy Survey: more than dark energy – an overview. Monthly Notices of the Royal Astronomical Society, 460(2), doi:10.1093/mnras/stw641

This overview paper describes the legacy prospect and discovery potential of the Dark Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the DES early data. DES is using a wide-field camera (DECam) on the 4 m Blanco T... Read More about The Dark Energy Survey: more than dark energy – an overview.

A mature galaxy cluster at z= 1.58 around the radio galaxy 7C 1753+6311 (2016)
Journal Article
Cooke, E. A., Hatch, N. A., Stern, D., Rettura, A., Brodwin, M., Galametz, A., …Jarvis, M. (2016). A mature galaxy cluster at z= 1.58 around the radio galaxy 7C 1753+6311. Astrophysical Journal, 816(2), doi:10.3847/0004-637X/816/2/83

We report on the discovery of a z = 1.58 mature cluster around the high-redshift radio galaxy 7C 1753+6311, first identified in the Clusters Around Radio-loud active galactic nuclei survey. Two-thirds of the excess galaxies within the central 1 Mpc l... Read More about A mature galaxy cluster at z= 1.58 around the radio galaxy 7C 1753+6311.

Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment (2015)
Journal Article
Zhao, D., Aragón-Salamanca, A., & Conselice, C. J. (2015). Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment. Monthly Notices of the Royal Astronomical Society, 453(4), doi:10.1093/mnras/stv1940

Using a sample of 425 nearby brightest cluster galaxies (BCGs) from von der Linden et al., we study the relationship between their internal properties (stellar masses, structural parameters and morphologies) and their environment. More massive BCGs t... Read More about Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment.

The formation history of massive cluster galaxies as revealed by CARLA (2015)
Journal Article
Conselice, C. J., Hatch, N. A., Cooke, E. A., Cooke, E. A., Hatch, N. A., Rettura, A., …Stanford, S. A. (2015). The formation history of massive cluster galaxies as revealed by CARLA. Monthly Notices of the Royal Astronomical Society, 452(3), 2318-2336. https://doi.org/10.1093/mnras/stv1413

© 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. We use a sample of 37 of the densest clusters and protoclusters across 1.3 ≤ z ≤ 3.2 from the Clusters Around Radio-Loud AGN (CARLA) survey to study... Read More about The formation history of massive cluster galaxies as revealed by CARLA.

Galaxy And Mass Assembly (GAMA): end of survey report and data release 2 (2015)
Journal Article
Liske, J., Baldry, I., Driver, S., Tuffs, R., Alpaslan, M., Andrae, E., …Wright, A. (2015). Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. Monthly Notices of the Royal Astronomical Society, 452(2), https://doi.org/10.1093/mnras/stv1436

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 (split among five survey regions) down to a limiting magnitude of r < 19.8 mag, we have collect... Read More about Galaxy And Mass Assembly (GAMA): end of survey report and data release 2.

The link between morphology and structure of brightest cluster galaxies: automatic identification of cDs (2015)
Journal Article
Zhao, D., Aragón-Salamanca, A., & Conselice, C. J. (2015). The link between morphology and structure of brightest cluster galaxies: automatic identification of cDs. Monthly Notices of the Royal Astronomical Society, 448(3), doi:10.1093/mnras/stv190

We study a large sample of 625 low-redshift brightest cluster galaxies (BCGs) and link their morphologies to their structural properties. We derive visual morphologies and find that ∼57 per cent of the BCGs are cD galaxies, ∼13 per cent are elliptica... Read More about The link between morphology and structure of brightest cluster galaxies: automatic identification of cDs.

The SCUBA-2 cosmology legacy survey: ALMA resolves the rest-frame far-infrared emission of sub-millemeter galaxies (2015)
Journal Article
Conselice, C., Simpson, J., Smail, I., Swinbank, A., Almaini, O., Blain, A., …van der Werf, P. (2015). The SCUBA-2 cosmology legacy survey: ALMA resolves the rest-frame far-infrared emission of sub-millemeter galaxies. Astrophysical Journal, 799(1), 81. https://doi.org/10.1088/0004-637x/799/1/81

We present high-resolution (0’’.3) Atacama Large Millimeter Array 870 μm imaging of 52 sub-millimeter galaxies (SMGs) in the Ultra Deep Survey field to investigate the size and morphology of the sub-millimeter (sub-mm) emission on 2–10 kpc scales. We... Read More about The SCUBA-2 cosmology legacy survey: ALMA resolves the rest-frame far-infrared emission of sub-millemeter galaxies.

Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sersic index, colour and morphology (2015)
Journal Article
Lange, R., Driver, S. P., Robotham, A. S., Kelvin, L. S., Graham, A. W., Alpaslan, M., …Wilkins, S. M. (2015). Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sersic index, colour and morphology. Monthly Notices of the Royal Astronomical Society, 447(3), 2603-2630. doi:10.1093/mnras/stu2467

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 mass–half-light radius relations for various divisions of ‘early’- and ‘late’-type samples. We fin... Read More about Galaxy And Mass Assembly (GAMA): mass-size relations of z < 0.1 galaxies subdivided by Sersic index, colour and morphology.


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