COSMOS 859900 , the SIMBAD biblio

COSMOS 859900 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST04:51:30


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Title First 3 Authors
2012ApJ...755..169M viz 15       D               1 144 86 Evolution of the quasar luminosity function over 3 < z < 5 in the COSMOS survey field. MASTERS D., CAPAK P., SALVATO M., et al.
2012ApJ...760..128M viz 15       D               1 235 51 Lyα emission from high-redshift sources in COSMOS. MALLERY R.P., MOBASHER B., CAPAK P., 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.
2013A&A...556A..55I viz 16       D               1 259207 819 Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA. ILBERT O., McCRACKEN H.J., LE FEVRE O., et al.
2015ApJ...815...57U viz 16       D               1 306 7 A correlation between Lyα spectral line profile and rest-frame UV morphology. U V., HEMMATI S., DARVISH B., et al.
2016ApJ...819...24W viz 16       D               1 796 79 A survey of luminous high-redshift quasars with SDSS and WISE. I. Target selection and optical spectroscopy. WANG F., WU X.-B., FAN X., et al.
2018ApJ...858...77H viz 16       D               1 7945 125 The DEIMOS 10k spectroscopic survey catalog of the COSMOS field. HASINGER G., CAPAK P., SALVATO M., et al.
2019MNRAS.490.2542P viz 17       D               1 2245 ~ Unveiling the weak radio quasar population at z≥4. PERGER K., FREY S., GABANYI K.E., 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.
2022ApJS..259...20H viz 18       D               1 1042 83 GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. HARIKANE Y., ONO Y., OUCHI M., et al.

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