ACS-GC 20094946 , the SIMBAD biblio

ACS-GC 20094946 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST09:53:47


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Title First 3 Authors
2007ApJS..172...29H viz 15       D               1 1391 287 The XMM-Newton wide-field survey in the COSMOS field. I. Survey description. HASINGER G., CAPPELLUTI N., BRUNNER H., et al.
2007ApJS..172...70L viz 15       D               2 20803 835 zCOSMOS: a large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field. LILLY S.J., FEVRE O.L., RENZINI A., et al.
2009A&A...497..635C viz 15       D               1 1896 242 The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue. CAPPELLUTI N., BRUSA M., HASINGER G., et al.
2009ApJS..184..158E viz 15       D               1 1767 380 The Chandra COSMOS survey. I. Overview and point source catalog. ELVIS M., CIVANO F., VIGNALI C., et al.
2009ApJS..184..218L viz 15       D               1 10646 500 The zCOSMOS 10k-Bright spectroscopic sample. LILLY S.J., LE BRUN V., MAIER C., et al.
2010A&A...512A..34L viz 15       D               1 548 298 The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS. LUSSO E., COMASTRI A., VIGNALI C., et al.
2010ApJ...716..348B viz 15       D               1 1849 274 The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei. BRUSA M., CIVANO F., COMASTRI A., et al.
2010AJ....140..533G viz 15       D               2 2423 27 Morphologies of radio-, X-ray-, and mid-infrared-selected active galactic nuclei. GRIFFITH R.L. and STERN D.
2011ApJ...742...61S viz 15       D               2 2652 210 Dissecting photometric redshift for active galactic nucleus using XMM- and Chandra-COSMOS samples. SALVATO M., ILBERT O., HASINGER G., et al.
2012ApJS..201...30C viz 15       D               1 1782 201 The Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sources. CIVANO F., ELVIS M., BRUSA M., et al.
2012ApJ...759....6E viz 15       D               1 424 54 Spectral energy distributions of type 1 active galactic nuclei in the COSMOS survey. I. The XMM-COSMOS sample. ELVIS M., HAO H., CIVANO F., et al.
2012MNRAS.427.3103B viz 15       D               1 1737 196 Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies. BONGIORNO A., MERLONI A., BRUSA M., et al.
2013ApJS..206....8M viz 16       D               1 208367 332 A public Ks-selected catalog in the COSMOS/ULTRAVISTA field: photometry, photometric redshifts, and stellar population parameters. MUZZIN A., MARCHESINI D., STEFANON M., et al.
2014MNRAS.438.1288H viz 16       D               1 414 27 Spectral energy distributions of type 1 AGN in XMM-COSMOS - II. Shape evolution. HAO H., ELVIS M., CIVANO F., et al.
2014MNRAS.443.2679B viz 16       D               1 9254 27 The GEEC2 spectroscopic survey of Galaxy groups at 0.8 < z < 1. BALOGH M.L., McGEE S.L., MOK A., et al.
2015ApJ...815...33R viz 16       D               1 814 170 A Hubble diagram for quasars. RISALITI G. and LUSSO E.
2015A&A...584A.106S viz 16       D               2 201 15 Pan-STARRS1 variability of XMM-COSMOS AGN. I. Impact on photometric redshifts. SIMM T., SAGLIA R., SALVATO M., et al.
2016ApJ...817...34M viz 16       D               2 4057 237 The Chandra COSMOS legacy survey: optical/IR identifications. MARCHESI S., CIVANO F., ELVIS M., et al.
2016ApJ...817..160L 17       D               1 59 67 Shadow of a colossus: a z = 2.44 galaxy protocluster detected in 3D LyαForest tomographic mapping of the COSMOS field. LEE K.-G., HENNAWI J.F., WHITE M., et al.
2016ApJ...819...62C viz 16       D               1 4017 337 The Chandra Cosmos Legacy survey: overview and point source catalog. CIVANO F., MARCHESI S., COMASTRI A., 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.
2017MNRAS.471..364B viz 16       D               1 290 1 Inferring Compton-thick AGN candidates at z > 2 with Chandra using the >8 keV rest-frame spectral curvature. BARONCHELLI L., KOSS M., SCHAWINSKI K., et al.
2018MNRAS.475.1288S 16       D               1 150 48 Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations. SCHOLTZ J., ALEXANDER D.M., HARRISON C.M., et al.
2018MNRAS.477.3775B 58       D     X         2 87 8 An Iwasawa-Taniguchi effect for Compton-thick active galactic nuclei. BOORMAN P.G., GANDHI P., BALOKOVIC M., et al.
2018ApJS..237...31L viz 16       D               1 436 83 First data release of the COSMOS Lyα Mapping And Tomography Observations: 3D Lyα forest tomography at 2.05 < z < 2.55. LEE K.-G., KROLEWSKI A., WHITE M., et al.
2019ApJ...878...11Z viz 17       D               1 2465 35 The host-galaxy properties of type 1 versus type 2 active galactic nuclei. ZOU F., YANG G., BRANDT W.N., et al.
2019A&A...627A..33D viz 17       D               1 301 ~ Optically variable AGN in the three-year VST survey of the COSMOS field. DE CICCO D., PAOLILLO M., FALOCCO S., et al.
2020AJ....160...37M viz 17       D               1 193 ~ Effective opacity of the intergalactic medium from galaxy spectra analysis. MONZON J.S., PROCHASKA J.X., LEE K.-G., et al.
2022ApJ...925...34C viz 18       D               1 208670 12 Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey. CUTLER S.E., WHITAKER K.E., MOWLA L.A., et al.
2022A&A...663L...7S viz 18       D               1 127 10 Quasars as high-redshift standard candles. SACCHI A., RISALITI G., SIGNORINI M., et al.
2024ApJ...962...93Z 20       D               1 147 ~ Active Galactic Nuclei and Host Galaxies in COSMOS-Web. I. NIRCam Images, Point-spread-function Models and Initial Results on X-Ray-selected Broad-line AGNs at 0.35 ≲ z ≲ 3.5. ZHUANG M.-Y., LI J. and SHEN Y.

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