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Results: 1-17 |
Results: 17

Authors: LILLY S SCHADE D ELLIS R LEFEVRE O BRINCHMANN J TRESSE L ABRAHAM R HAMMER F CRAMPTON D COLLESS M GLAZEBROOK K MALLENORNELAS G BROADHURST T
Citation: S. Lilly et al., HUBBLE-SPACE-TELESCOPE IMAGING OF THE CFRS AND LDSS REDSHIFT SURVEYS - II - STRUCTURAL PARAMETERS AND THE EVOLUTION OF DISK GALAXIES TO Z-SIMILAR-TO-1, The Astrophysical journal, 500(1), 1998, pp. 75-94

Authors: BRINCHMANN J ABRAHAM R SCHADE D TRESSE L ELLIS RS LILLY S LEFEVRE O GLAZEBROOK K HAMMER F COLLESS M CRAMPTON D BROADHURST T
Citation: J. Brinchmann et al., HUBBLE-SPACE-TELESCOPE IMAGING OF THE CFRS AND LDSS REDSHIFT SURVEYS - I - MORPHOLOGICAL PROPERTIES, The Astrophysical journal, 499(1), 1998, pp. 112

Authors: PARKER QA COLLESS M MAMON G
Citation: Qa. Parker et al., THE FLAIR-DENIS REDSHIFT SURVEY, Publications of the Astronomical Society of Australia, 14(1), 1997, pp. 125-126

Authors: SAGLIA RP BERTSCHINGER E BAGGLEY G BURSTEIN D COLLESS M DAVIES RL MCMAHAN RK WEGNER G
Citation: Rp. Saglia et al., THE PECULIAR MOTIONS OF EARLY-TYPE GALAXIES IN 2 DISTANT REGIONS .4. THE PHOTOMETRIC FITTING PROCEDURE, The Astrophysical journal. Supplement series, 109(1), 1997, pp. 79-102

Authors: GRAHAM A COLLESS M
Citation: A. Graham et M. Colless, SOME EFFECTS OF GALAXY STRUCTURE AND DYNAMICS ON THE FUNDAMENTAL PLANE, Monthly Notices of the Royal Astronomical Society, 287(1), 1997, pp. 221-239

Authors: RIX HW GUHATHAKURTA P COLLESS M ING K
Citation: Hw. Rix et al., INTERNAL KINEMATICS OF DISTANT FIELD GALAXIES .1. EMISSION LINEWIDTHSFOR A COMPLETE SAMPLE OF FAINT BLUE GALAXIES AT (Z)SIMILAR-TO-0.25, Monthly Notices of the Royal Astronomical Society, 285(4), 1997, pp. 779-792

Authors: HEYL J COLLESS M ELLIS RS BROADHURST T
Citation: J. Heyl et al., AUTOFIB REDSHIFT SURVEY .2. EVOLUTION OF THE GALAXY LUMINOSITY FUNCTION BY SPECTRAL TYPE, Monthly Notices of the Royal Astronomical Society, 285(3), 1997, pp. 613-634

Authors: WEGNER G COLLESS M BAGGLEY G DAVIES RL BERTSCHINGER E BURSTEIN D MCMAHAN RK SAGLIA RP
Citation: G. Wegner et al., THE PECULIAR MOTIONS OF EARLY-TYPE GALAXIES IN 2 DISTANT REGIONS .1. CLUSTER AND GALAXY SELECTION, The Astrophysical journal. Supplement series, 106(1), 1996, pp. 1-26

Authors: ELLIS RS COLLESS M BROADHURST T HEYL J GLAZEBROOK K
Citation: Rs. Ellis et al., AUTOFIB REDSHIFT SURVEY .1. EVOLUTION OF THE GALAXY LUMINOSITY FUNCTION, Monthly Notices of the Royal Astronomical Society, 280(1), 1996, pp. 235-251

Authors: GRAHAM A LAUER TR COLLESS M POSTMAN M
Citation: A. Graham et al., BRIGHTEST CLUSTER GALAXY PROFILE SHAPES, The Astrophysical journal, 465(2), 1996, pp. 534-547

Authors: COLLESS M DUNN AM
Citation: M. Colless et Am. Dunn, STRUCTURE AND DYNAMICS OF THE COMA CLUSTER, The Astrophysical journal, 458(2), 1996, pp. 435-454

Authors: GLAZEBROOK K ELLIS R COLLESS M BROADHURST T ALLINGTONSMITH J TANVIR N
Citation: K. Glazebrook et al., A FAINT GALAXY REDSHIFT SURVEY TO B=24, Monthly Notices of the Royal Astronomical Society, 273(1), 1995, pp. 157-168

Authors: COLLESS M
Citation: M. Colless, THE ABELL CLUSTER INERTIAL FRAME, The Astronomical journal, 109(5), 1995, pp. 1937-1946

Authors: COLLESS M SCHADE D BROADHURST TJ ELLIS RS
Citation: M. Colless et al., HIGH-RESOLUTION IMAGING OF FAINT BLUE GALAXIES, Monthly Notices of the Royal Astronomical Society, 267(4), 1994, pp. 1108-1120

Authors: COLE S ELLIS R BROADHURST T COLLESS M
Citation: S. Cole et al., THE SPATIAL CLUSTERING OF FAINT GALAXIES, Monthly Notices of the Royal Astronomical Society, 267(3), 1994, pp. 541-547

Authors: SAGLIA RP BERTSCHINGER E BAGGLEY G BURSTEIN D COLLESS M DAVIES RL MCMAHAN RK WEGNER G
Citation: Rp. Saglia et al., THE EFFECTS OF SEEING ON THE PHOTOMETRIC PROPERTIES OF ELLIPTIC GALAXIES, Monthly Notices of the Royal Astronomical Society, 264(4), 1993, pp. 961-974

Authors: COLLESS M BURSTEIN D WEGNER G SAGLIA RP MCMAHAN R DAVIES RL BERTSCHINGER E BAGGLEY G
Citation: M. Colless et al., PHOTOELECTRIC AND CCD PHOTOMETRY OF E AND S0 GALAXIES, Monthly Notices of the Royal Astronomical Society, 262(2), 1993, pp. 475-490
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