[MBR2003] CDFS-H 1424 , the SIMBAD biblio

[MBR2003] CDFS-H 1424 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST22:12:38

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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
2003A&A...403..493M viz 4820 24 H-band observations of the Chandra Deep Field South. MOY E., BARMBY P., RIGOPOULOU D., et al.
2008ApJS..179..114M viz 15       D               1 523 107 The VLA 1.4 GHz survey of the Extended Chandra Deep Field-South: first data release. MILLER N.A., FOMALONT E.B., KELLERMANN K.I., et al.
2012ApJS..203...15B viz 15       D               1 894 38 The sub-mJy radio population of the E-CDFS: optical and infrared counterpart identification. BONZINI M., MAINIERI V., PADOVANI P., et al.
2013ApJS..205...13M viz 16       D               1 894 109 The Very Large Array 1.4 GHz survey of the Extended Chandra Deep Field South: second data release. MILLER N.A., BONZINI M., FOMALONT E.B., et al.
2013MNRAS.436.3759B viz 16       D               1 885 125 The sub-mJy radio sky in the Extended Chandra Deep Field-South: source population. BONZINI M., PADOVANI P., MAINIERI V., 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.
2015MNRAS.453.1079B viz 16       D               1 781 30 Star formation properties of sub-mJy radio sources. BONZINI M., MAINIERI V., PADOVANI P., 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.
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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