[LBX2017] 160 , the SIMBAD biblio

[LBX2017] 160 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST22:40:28

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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
2002ApJS..139..369G viz 349 551 Chandra Deep Field South: the 1 Ms catalog. GIACCONI R., ZIRM A., WANG J., et al.
2003AJ....126..539A viz 960 736 The Chandra Deep Field North Survey. XIII. 2 Ms point-source catalogs. ALEXANDER D.M., BAUER F.E., BRANDT W.N., et al.
2004ApJ...607..721N 215 80 The x-ray-derived cosmological star formation history and the galaxy X-ray luminosity functions in the Chandra Deep Fields North and South. NORMAN C., PTAK A., HORNSCHEMEIER A., et al.
2004ApJS..155...73Z viz 345 104 Photometric redshift of X-ray sources in the Chandra Deep Field-South. ZHENG W., MIKLES V.J., MAINIERI V., et al.
2004ApJS..155..271S viz 15       D               556 542 The Chandra Deep Field-South: Optical spectroscopy. I.. SZOKOLY G.P., BERGERON J., HASINGER G., et al.
2006A&A...451..457T viz 15       D               340 342 X-ray spectral properties of active galactic nuclei in the Chandra Deep Field South. TOZZI P., GILLI R., MAINIERI V., et al.
2006A&A...455..773V viz 108224 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2008ApJ...680..130C viz 15       D               1 1013 61 Mid-infrared properties and color selection for X-Ray-detected active galactic nuclei in the MUSYC Extended Chandra Deep Field-South. CARDAMONE C.N., URRY C.M., DAMEN M., et al.
2008ApJS..179...19L viz 15       D               1 586 273 The Chandra Deep Field-South survey: 2 Ms source catalogs. LUO B., BAUER F.E., BRANDT W.N., et al.
2010ApJS..187..560L viz 15       D               1 469 134 Identifications and photometric redshifts of the 2 Ms Chandra Deep Field-South sources. LUO B., BRANDT W.N., XUE Y.Q., et al.
2010A&A...512A..12B viz 15       D               1 4352 228 The Great Observatories Origins Deep Survey. VLT/VIMOS spectroscopy in the GOODS-South field: part II. BALESTRA I., MAINIERI V., POPESSO P., et al.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2011ApJS..195...10X viz 15       D               1 782 508 The Chandra Deep Field-South survey: 4 Ms source catalogs. XUE Y.Q., LUO B., BRANDT W.N., et al.
2013MNRAS.431..662J 16       D               1 53 17 X-ray detections of submillimetre galaxies: active galactic nuclei versus starburst contribution. JOHNSON S.P., WILSON G.W., WANG Q.D., et al.
2013MNRAS.436.2535J 94       D         F     4 19 18 SATMC: spectral energy distribution analysis through Markov chains. JOHNSON S.P., WILSON G.W., TANG Y., et al.
2014ApJ...796...60H viz 16       D               1 1489 120 CANDELS/GOODS-S, CDFS, and ECDFS : photometric redshifts for normal and X-Ray-detected galaxies. HSU L.-T., SALVATO M., NANDRA K., 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.
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...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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