CFRS 22.0576 , the SIMBAD biblio

CFRS 22.0576 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST00:56:00


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Title First 3 Authors
1993ApJ...411..501L 50 119 A deep I-band selected galaxy sample : implications for galaxy evolution. LILLY S.J.
1995ApJ...455...75L viz 14       D               1 438 82 The Canada-France Redshift Survey. III. "Single emission-line" objects, analysis of repeat observations, and spectroscopic identifications in the 1415+52 and 2215+00 fields. LILLY S.J., HAMMER F., LE FEVRE O., et al.
1997ApJ...481...49H viz 411 191 Canada-France Redshift Survey. XIV. Spectral properties of field galaxies up to z=1. HAMMER F., FLORES H., LILLY S.J., et al.
1998ApJ...499..112B viz 340 228 Hubble space telescope imaging of the CFRS and LDSS redshift surveys. I. Morphological properties. BRINCHMANN J., ABRAHAM R., SCHADE D., et al.
2001AJ....122..621V viz 15       D               1 220 14 The evolution of galaxy morphology for galaxies in the Canada-France redshift survey. VAN DEN BERGH S.
2003ApJ...597..730L 67 117 The metallicities of star-forming galaxies at intermediate redshifts 0.47. LILLY S.J., CAROLLO C.M. and STOCKTON A.N.
2005A&A...430..115H viz 174 227 Did most present-day spirals form during the last 8 Gyr? A formation history with violent episodes revealed by panchromatic observations. HAMMER F., FLORES H., ELBAZ D., et al.
2005ApJ...634..849M 39 59 Near-infrared spectroscopy of 0.4 < z < 1.0 CFRS galaxies: oxygen abundances, SFRs, and dust. MAIER C., LILLY S.J., CAROLLO C.M., et al.
2005ApJ...635..260S 1 93 442 The Gemini Deep Deep Survey. VII. The redshift evolution of the mass-metallicity relation. SAVAGLIO S., GLAZEBROOK K., LE BORGNE D., et al.
2006A&A...447..113L 50 43 Significant evolution of the stellar mass-metallicity relation since z ∼ 0.65. LIANG Y.C., HAMMER F. and FLORES H.
2012MNRAS.421.2888R viz 15       D               2 68 25 A decrease of the gas exchanges between galaxies and the intergalactic medium, from 12 to 6 billion years ago. RODRIGUES M., PUECH M., HAMMER F., et al.

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