PSO J083.8371+11.8482 , the SIMBAD biblio

PSO J083.8371+11.8482 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST18:34:16


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Title First 3 Authors
2020ApJ...903...34A 2332     A     X C       56 10 27 Probing the nature of high-redshift weak emission line quasars: a young quasar with a starburst host galaxy. ANDIKA I.T., JAHNKE K., ONOUE M., et al.
2022AJ....163..251A 3005     A S   X C       69 10 5 Staring at the Shadows of Archaic Galaxies: Damped Lyα and Metal Absorbers Toward a Young z ∼ 6 Weak-line Quasar. ANDIKA I.T., JAHNKE K., BANADOS E., et al.
2022ApJ...941..106F viz 17       D               1 120 26 The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars. FARINA E.P., SCHINDLER J.-T., WALTER F., et al.
2023A&A...678A.201Z 17       D               1 20 ~ HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars. ZAPPACOSTA L., PICONCELLI E., FIORE F., et al.
2024MNRAS.528..499L 18       D               1 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024MNRAS.534.2062V 18       D               1 72 ~ Characterising the contribution of dust-obscured star formation at ≳ 5 using 18 serendipitously identified [C II] emitters. VAN LEEUWEN I.F., BOUWENS R.J., VAN DER WERF P.P., et al.
2025A&A...693A.157S 19       D               4 22 ~ HYPERION: Broad-band X-ray-to-near-infrared emission of quasars in the first billion years of the Universe. SACCHEO I., BONGIORNO A., PICONCELLI E., et al.
2025ApJ...982...72S 299       D     X         7 12 ~ Direct Evidence for Active Galactic Nuclei Feedback from Fast Molecular Outflows in Reionization-era Quasars. SPILKER J.S., CHAMPAGNE J.B., FAN X., et al.
2026A&A...706A.285C 420       D     X C       8 12 ~ Infrared emission from z ∼ 6.5 quasar host galaxies: a direct estimate of dust physical properties. COSTA M., DECARLI R., POZZI F., et al.

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