The structure and evolution of a forming galaxy cluster at z = 1.62

J. Conselice, C.; G. Hartley, W.; A. Cooke, E.; I. Muldrew, S.; A. Hatch, N.; Hatch, Nina A.; Muldrew, Stuart I.; Cooke, Elizabeth A.; Hartley, William G.; Almaini, O.; J. Simpson, C.; Conselice, Christopher J.

doi:10.1093/mnras/stw602

The SCUBA-2 Cosmology Legacy Survey: 850 ?m 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 ?m 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), https://doi.org/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 SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field (2016)
Journal Article
Wilkinson, A., Almaini, O., Chen, C. C., Smail, I., Arumugam, V., Blain, A., …Wild, V. (2017). The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field. Monthly Notices of the Royal Astronomical Society, 464(2), 1380-1392. https://doi.org/10.1093/mnras/stw2405

© 2016 The Authors. Submillimetre galaxies (SMGs) are among the most luminous dusty galaxies in the Universe, but their true nature remains unclear; are SMGs the progenitors of the massive elliptical galaxies we see in the local Universe, or are they... Read More about The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field.

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), 1393-1414. https://doi.org/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.

The evolution of post-starburst galaxies from z=2 to 0.5 (2016)
Journal Article
Wild, V., Almaini, O., Dunlop, J., Simpson, C., Rowlands, K., Bowler, R., …McLure, R. (2016). The evolution of post-starburst galaxies from z=2 to 0.5. Monthly Notices of the Royal Astronomical Society, 463(1), 832-844. https://doi.org/10.1093/mnras/stw1996

We present the evolution in the number density and stellar mass functions of photometrically selected post-starburst galaxies in the UKIDSSUltraDeep Survey,with redshifts of 0.5

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), https://doi.org/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 identification of post-starburst galaxies at z?1 using multiwavelength photometry: a spectroscopic verification (2016)
Journal Article
Maltby, D. T., Almaini, O., Wild, V., Hatch, N. A., Hartley, W. G., Simpson, C., …Cirasuolo, M. (2016). The identification of post-starburst galaxies at z∼1 using multiwavelength photometry: a spectroscopic verification. Monthly Notices of the Royal Astronomical Society: Letters, 459(1), Article L114-L118. https://doi.org/10.1093/mnrasl/slw057

Despite decades of study, we still do not fully understand why some massive galaxies abruptly switch off their star formation in the early Universe, and what causes their rapid transition to the red sequence. Post-starburst galaxies provide a rare op... Read More about The identification of post-starburst galaxies at z?1 using multiwavelength photometry: a spectroscopic verification.

The SCUBA-2 Cosmology Legacy Survey: multiwavelength counterparts to 103 submillimeter galaxies in the UKIDSS-UDS field (2016)
Journal Article
Chen, C., Smail, I., Ivison, R. J., Arumugam, V., Almaini, O., Conselice, C. J., …Zavala, J. A. (2016). The SCUBA-2 Cosmology Legacy Survey: multiwavelength counterparts to 103 submillimeter galaxies in the UKIDSS-UDS field. Astrophysical Journal, 820(2), 82. https://doi.org/10.3847/0004-637x/820/2/82

We present multiwavelength identifications for the counterparts of 1088 submillimeter sources detected at 850 μm in the SCUBA-2 Cosmology Legacy Survey study of the UKIRT Infrared Deep Sky Survey-Ultra-Deep Survey (UDS) field. By utilizing an Atacama... Read More about The SCUBA-2 Cosmology Legacy Survey: multiwavelength counterparts to 103 submillimeter galaxies in the UKIDSS-UDS field.

The structure and evolution of a forming galaxy cluster at z = 1.62 (2016)
Journal Article
J. Conselice, C., G. Hartley, W., A. Cooke, E., I. Muldrew, S., A. Hatch, N., Hatch, N. A., …Conselice, C. J. (2016). The structure and evolution of a forming galaxy cluster at z = 1.62. Monthly Notices of the Royal Astronomical Society, 459(1), 387-401. https://doi.org/10.1093/mnras/stw602

We present a comprehensive picture of the Cl0218.3-0510 protocluster at $z=1.623$ across 10 co-moving Mpc. Using filters that tightly bracket the Balmer and 4000 Angstrom breaks of the protocluster galaxies we obtain precise photometric redshifts res... Read More about The structure and evolution of a forming galaxy cluster at z = 1.62.

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