[LBX2017] 670 , the SIMBAD biblio

[LBX2017] 670 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST11:30:22


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Title First 3 Authors
2008ApJ...682..985W viz 227 271 FIREWORKS U38-to-24 µm photometry of the GOODS Chandra Deep Field-South: multiwavelength catalog and total infrared properties of distant Ks-selected galaxies. WUYTS S., LABBE I., FORSTER SCHREIBER N.M., et al.
2012ApJ...744..181Z 15       D               1 46 25 Internal structure of protocluster galaxies: accelerated structural evolution in overdense environments? ZIRM A.W., TOFT S. and TANAKA M.
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.
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.
2017ApJS..228....2L viz 16       D               1 1061 334 The Chandra Deep Field-South survey: 7 Ms source catalogs. LUO B., BRANDT W.N., XUE Y.Q., 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.
2019ApJ...877....5L viz 17       D               1 439 2 Piercing through highly obscured and Compton-thick AGNs in the Chandra Deep Fields. I. X-ray spectral and long-term variability analyses. LI J., XUE Y., SUN M., et al.
2019ApJ...887...23B viz 17       D               1 942 ~ A submillimeter perspective on the GOODS fields (SUPER GOODS). IV. The submillimeter properties of X-ray sources in the CDF-S. BARGER A.J., COWIE L.L., BAUER F.E., et al.
2020MNRAS.492.1887G viz 17       D               1 792 ~ Physical properties of the CDFS X-ray sources through fitting spectral energy distributions. GUO X., GU Q., DING N., et al.

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