SDSS J021727.74-051720.0 , the SIMBAD biblio

SDSS J021727.74-051720.0 , the SIMBAD biblio (7 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:52:41


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2012ApJ...758...49H 15       D               1 30 22 Comoving space density and obscured fraction of high-redshift active galactic nuclei in the Subaru/XMM-Newton deep survey. HIROI K., UEDA Y., AKIYAMA M., et al.
2014MNRAS.445.3557V 15       D               1 144 72 The hard X-ray luminosity function of high-redshift (3 < z ≲ 5) active galactic nuclei. VITO F., GILLI R., VIGNALI C., et al.
2016MNRAS.457..110M viz 16       D               1 5299 75 A spectroscopic survey of X-ray-selected AGNs in the northern XMM-XXL field. MENZEL M.-L., MERLONI A., GEORGAKAKIS A., et al.
2016MNRAS.457..629C viz 16       D               1 650 33 ZFOURGE catalogue of AGN candidates: an enhancement of 160-µm-derived star formation rates in active galaxies to z = 3.2. COWLEY M.J., SPITLER L.R., TRAN K.-V.H., et al.
2016ApJ...830...51S viz 16       D               1 67525 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.
2022A&A...658A.175P 17       D               1 95 3 XXL-HSC: An updated catalogue of high-redshift (z ≥ 3.5) X-ray AGN in the XMM-XXL northern field. Constraints on the bright end of the soft log N-log S. POULIASIS E., GEORGANTOPOULOS I., RUIZ A., et al.
2022ApJS..259...20H viz 17       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.

goto View the references in ADS