DrCarolineClewley

Clewley C, 2016, Troublesome Knowledge in Relativity

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Finoguenov A, Watson MG, Tanaka M, Simpson C, Cirasuolo M, Dunlop JS, Peacock JA, Farrah D, Akiyama M, Ueda Y, Smolčić V, Stewart G, Rawlings S, van BC, Almaini O, Clewley L, Bonfield DG, Jarvis MJ, Barr JM, Foucaud S, McLure RJ, Sekiguchi K, Egami Eet al., 2010, X-ray groups and clusters of galaxies in the Subaru-XMM Deep Field, MNRAS, Vol: 403, Pages: 2063-2076

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Van Breukelen C, Clewley L, 2009, A reliable cluster detection technique using photometric redshifts: introducing the 2TecX algorithm, MNRAS, Vol: 395, Pages: 1845-1856

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Van Breukelen C, Simpson C, Rawlings S, Akiyama M, Bonfield D, Clewley L, Jarvis MJ, Mauch T, Readhead T, Stobbart A, Swinbank M, Watson Met al., 2009, Evidence of a link between the evolution of clusters and their AGN fraction, MNRAS, Vol: 395, Pages: 11-27

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Van Breukelen C, Cotter G, Rawlings S, Readhead T, Bonfield D, Clewley L, Ivison R, Jarvis M, Simpson C, Watson Met al., 2007, Spectroscopic follow-up of a cluster candidate at z = 1.45, MNRAS, Vol: 382, Pages: 971-984

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Clewley L, Van Breukelen C, Bonfield D, 2007, Detecting Galaxy Clusters at 0.1 < z < 2.0

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Swinbank AM, Edge AC, Smail I, Stott JP, Bremer M, Sato Y, Van Breukelen C, Jarvis M, Waddington I, Clewley L, Bergeron J, Cotter G, Dye S, Geach JE, Gonzalez-Solares E, Hirst P, Ivison RJ, Rawlings S, Simpson C, Smith GP, Verma A, Yamada Tet al., 2007, Infrared study of UKIDSS massive supercluster (Swinbank+, 2007), VizieR Online Data Catalog, Vol: 837

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Swinbank AM, Edge AC, Smail I, Stott JP, Bremer M, Sato Y, Van Breukelen C, Jarvis M, Waddington I, Clewley L, Bergeron J, Cotter G, Dye S, Geach JE, Gonzalez-Solares E, Hirst P, Ivison RJ, Rawlings S, Simpson C, Smith GP, Verma A, Yamada Tet al., 2007, The discovery of a massive supercluster at z = 0.9 in the UKIDSS Deep eXtragalactic Survey, MNRAS, Vol: 379, Pages: 1343-1351

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Dunlop J, Akiyama M, Alexander D, Almaini O, Borys C, Bouwens R, Bremer M, Cimatti A, Cirasuolo M, Clewley L, Conselice C, Coppin K, Dalton G, Damen M, Dunne L, Dye S, Eales S, Edge A, Egami E, Fall M, Farrah D, Ferguson H, Finoguenov A, Foucaud S, Franx M, Furusawa H, Huang J, Ibar E, Illingworth G, Ivison R, Jarvis M, Labbe I, Lawrence A, Maddox S, McLure R, Mortier A, Oliver S, Ouchi M, Page M, Papovich C, Quadri R, Rawlings S, Rieke G, Schiminovich D, Sekiguchi K, Serjeant S, Simpson C, Smail I, Stanway E, Taylor A, Watson M, Williams R, Yamada T, Van Breukelen C, van DPet al., 2007, A Spitzer Public Legacy survey of the UKIDSS Ultra Deep Survey

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Van Breukelen C, Clewley L, Bonfield DG, Rawlings S, Jarvis MJ, Barr JM, Foucaud S, Almaini O, Cirasuolo M, Dalton G, Dunlop JS, Edge AC, Hirst P, McLure RJ, Page MJ, Sekiguchi K, Simpson C, Smail I, Watson MGet al., 2006, Galaxy clusters at 0.6 < z < 1.4 in the UKIDSS Ultra Deep Survey Early Data Release, MNRAS, Vol: 373, Pages: L26-L30

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Dye S, Warren SJ, Hambly NC, NJG C, Hodgkin ST, Irwin MJ, Lawrence A, Adamson AJ, Almaini O, Edge AC, Hirst P, Jameson RF, Lucas PW, Van Breukelen C, Bryant J, Casali M, Collins RS, Dalton GB, Davies JI, Davis CJ, Emerson JP, Evans DW, Foucaud S, Gonzales-Solares EA, Hewett PC, Kendall TR, Kerr TH, Leggett SK, Lodieu N, Loveday J, Lewis JR, Mann RG, McMahon RG, Mortlock DJ, Nakajima Y, Pinfield DJ, Rawlings MG, Read MA, Riello M, Sekiguchi K, Smith AJ, ETW S, Varricatt W, Walton NA, Weatherley SJet al., 2006, The UKIRT Infrared Deep Sky Survey Early Data Release, Monthly Notices of the Royal Astronomical Society, Vol: 372, Pages: 1227-1252, ISSN: 0035-8711

This paper defines the UKIRT Infrared Deep Sky Survey (UKIDSS) Early Data Release (EDR). UKIDSS is a set of five large near-infrared surveys being undertaken with the United Kingdom Infrared Telescope Wide Field Camera (WFCAM). The programme began in 2005 May and has an expected duration of 7 yr. Each survey uses some or all of the broad-band filter complement ZY JHK. The EDR is the first public release of data to the European Southern Observatory (ESO) community. All worldwide releases occur after a delay of 18 months from the ESO release. The EDR provides a small sample data set, ∼50 deg2 (about 1 per cent of the whole of UKIDSS), that is a lower limit to the expected quality of future survey data releases. In addition, an EDR+ data set contains all EDR data plus extra data of similar quality, but for areas not observed in all of the required filters (amounting to ∼220 deg2). The first large data release, DR1, will occur in mid-2006. We provide details of the observational implementation, the data reduction, the astrometric and photometric calibration and the quality control procedures. We summarize the data coverage and quality (seeing, ellipticity, photometricity, depth) for each survey and give a brief guide to accessing the images and catalogues from the WFCAM Science Archive.

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Van Breukelen C, Clewley L, Bonfield D, 2006, A new method of detecting high-redshift clusters, ArXiv Astrophysics e-prints

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Jarvis MJ, Van Breukelen C, Venemans BP, Wilman RJet al., 2005, Surveying the High-Redshift Universe with the VIMOS IFU, The Messenger, Vol: 121, Pages: 38-41

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Van Breukelen C, Jarvis MJ, Venemans BP, 2005, The luminosity function of Lyα emitters at 2.3 < z < 4.6 from integral-field spectroscopy, MNRAS, Vol: 359, Pages: 895-905

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Jarvis MJ, Van Breukelen C, Wilman RJ, 2005, The discovery of a type II quasar at z= 1.65 with integral-field spectroscopy, MNRAS, Vol: 358, Pages: L11-L15

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