ZFOURGE CDFS 24788 , the SIMBAD biblio

ZFOURGE CDFS 24788 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST13:48:12


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Title First 3 Authors
2011ApJ...743..146C viz 15       D               1 4132 61 Active and passive galaxies at z ∼ 2: rest-frame optical morphologies with WFC3. CAMERON E., CAROLLO C.M., OESCH P.A., et al.
2014ApJ...793..101T viz 16       D               1 120 15 No more active galactic nuclei in clumpy disks than in smooth galaxies at z ∼ 2 in CANDELS/3D-HST. TRUMP J.R., BARRO G., JUNEAU S., 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.
2014ApJ...796...64C viz 16       D               1 91 20 Hubble Space Telescope emission line galaxies at z ∼ 2: the Lyα escape fraction. CIARDULLO R., ZEIMANN G.R., GRONWALL C., 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.
2016ApJ...817...10G viz 16       D               1 259 10 Young, star-forming galaxies and their local counterparts: the evolving relationship of mass-SFR-metallicity since z ∼ 2.1. GRASSHORN GEBHARDT H.S., ZEIMANN G.R., CIARDULLO 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.
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.

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