GOODS J221743.08+001508.3 , the SIMBAD biblio

GOODS J221743.08+001508.3 , the SIMBAD biblio (17 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST01:31:41

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		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.
1996AJ....112..839C 1 386 1520 New insight on Galaxy formation and evolution from Keck spectroscopy of the Hawaii deep fields. COWIE L.L., SONGAILA A., HU E.M., 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.
2001ApJ...550..570H 2 15 111 Luminous compact galaxies at intermediate redshifts: progenitors of bulges of massive spirals? HAMMER F., GRUEL N., THUAN T.X., et al.
2002MNRAS.333..633A 124 19 Restrictions to the galaxy evolutionary models from the Hawaiian Deep Fields SSA13 and SSA22. AGUERRI J.A.L. and TRUJILLO I.
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.
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.
2006A&A...448..893L viz         O           148 34 Spectrophotometric properties of galaxies at intermediate redshifts (z ∈ [0.2-1.0]). I. Sample description, photometric properties and spectral measurements. LAMAREILLE F., CONTINI T., LE BORGNE J.-F., et al.
2006A&A...448..907L         O           129 33 Spectrophotometric properties of galaxies at intermediate redshifts (z ∈ [0.2-1.0]). II. The Luminosity - Metallicity relation. LAMAREILLE F., CONTINI T., BRINCHMANN J., et al.
2006A&A...455..107F viz 1 48 173 3D spectroscopy with VLT/GIRAFFE. I. The true Tully Fisher relationship at z ∼ 0.6. FLORES H., HAMMER F., PUECH M., et al.
2006A&A...455..119P 1 20 45 3D spectroscopy with VLT/GIRAFFE. II. Are luminous compact galaxies merger remnants? PUECH M., HAMMER F., FLORES H., et al.
2008A&A...484..173P 15       D               1 72 128 IMAGES. III. The evolution of the near-infrared Tully-Fisher relation over the last 6 Gyr. PUECH M., FLORES H., HAMMER F., et al.
2009A&A...495...53L viz 15       D               1 19223 81 Physical properties of galaxies and their evolution in the VIMOS VLT deep survey. I. The evolution of the mass-metallicity relation up to z ∼ 0.9. LAMAREILLE F., BRINCHMANN J., CONTINI T., et al.
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.
2013A&A...559A..14L viz 16       D               1 37850 306 The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z ∼ 6.7 selected with 17.5 ≤ iAB≤ 24.75. LE FEVRE O., CASSATA P., CUCCIATI O., et al.
2018A&A...611A..53J viz 16       D               1 24519 3 Automated reliability assessment for spectroscopic redshift measurements. JAMAL S., LE BRUN V., LE FEVRE O., et al.

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