EIS-DEEP CDFS-3 Ks 1 74 , the SIMBAD biblio

EIS-DEEP CDFS-3 Ks 1 74 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST16:59:32

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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
2002A&A...392..395C viz 546 166 The K20 survey. III. Photometric and spectroscopic properties of the sample. CIMATTI A., MIGNOLI M., DADDI E., et al.
2003A&A...403..493M viz 4820 24 H-band observations of the Chandra Deep Field South. MOY E., BARMBY P., RIGOPOULOU D., et al.
2003ApJ...595..685G viz 233 30 Hubble Space Telescope imaging in the Chandra Deep Field-South. III. Quantitative morphology of the 1 million second Chandra counterparts and comparison with the field population. GROGIN N.A., KOEKEMOER A.M., SCHREIER E.J., et al.
2005A&A...437..883M viz 15       D               1 546 208 The K20 survey. VII. The spectroscopic catalogue: Spectral properties and evolution of the galaxy population. MIGNOLI M., CIMATTI A., ZAMORANI G., et al.
2006A&A...449..951G viz 1278 302 The GOODS-MUSIC sample: a multicolour catalog of near-IR selected galaxies in the GOODS-South field. GRAZIAN A., FONTANA A., DE SANTIS C., et al.
2006A&A...452..119O viz 3542 8 ESO imaging survey: infrared observations of CDF-S and HDF-S. OLSEN L.F., MIRALLES J.-M., DA COSTA L., et al.
2009PASJ...61..177B viz 15       D               1 258 10 Deep 15 mu.m AKARI observations in the CDFS: Estimating dust luminosities for a MIR-selected sample and for Lyman Break Galaxies and the evolution of Ldust/LUV with the redshift. BURGARELLA D., BUAT V., TAKEUCHI T.T., et al.
2011A&A...533A.119E viz 15       D               1 3965 926 GOODS-Herschel: an infrared main sequence for star-forming galaxies. ELBAZ D., DICKINSON M., HWANG H.S., et al.
2012MNRAS.425.2116C viz 15       D               1 7382 55 The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS spectroscopic survey of the Chandra Deep Field-South. COOPER M.C., YAN R., DICKINSON M., et al.
2014ApJS..214...24S viz 16       D               1 66903 733 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al.
2015AJ....149..178M viz 16       D               1 1020 31 A WFC3 grism emission line redshift catalog in the GOODS-South field. MORRIS A.M., KOCEVSKI D.D., TRUMP J.R., et al.
2016ApJS..225...27M viz 16       D               1 19341 548 The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ∼ 100,000 galaxies. MOMCHEVA I.G., BRAMMER G.B., VAN DOKKUM P.G., et al.
2016ApJ...830...51S viz 16       D               1 67524 168 The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al.
2016A&A...594A..77D viz 4 15 70 Flat rotation curves and low velocity dispersions in KMOS star-forming galaxies at z ∼ 1. DI TEODORO E.M., FRATERNALI F. and MILLER S.H.
2017MNRAS.467.1965H viz 16       D               1 590 79 The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z ~= 0.9 galaxies. HARRISON C.M., JOHNSON H.L., SWINBANK A.M., et al.
2018MNRAS.475.5133R viz 16       D               1 11242 2 Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ∼ 1.5. RODRIGUES M., PUECH M., FLORES H., et al.
2021MNRAS.500.4229G 88               F     1 12 17 The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z ≃ 0.6-1.8. GILLMAN S., TILEY A.L., SWINBANK A.M., et al.
2021MNRAS.503.1753S viz 17       D               1 345 10 Flat rotation curves of z ∼ 1 star-forming galaxies. SHARMA G., SALUCCI P., HARRISON C.M., et al.
2022A&A...659A..40S viz 18       D               1 225 9 Observational evidence of evolving dark matter profiles at z ≤ 1. SHARMA G., SALUCCI P. and VAN DE VEN G.

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