ULAS J123427.52+090754.1 , the SIMBAD biblio

ULAS J123427.52+090754.1 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST22:34:25

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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
2012MNRAS.427.2275B 779       D     X C F     19 31 77 Heavily reddened quasars at z ∼ 2 in the UKIDSS Large Area Survey: a transitional phase in AGN evolution. BANERJI M., McMAHON R.G., HEWETT P.C., et al.
2013MNRAS.429L..55B 55       D     X         2 9 22 Hyperluminous reddened broad-line quasars at z ∼ 2 from the VISTA Hemisphere Survey and WISE All-Sky Survey. BANERJI M., McMAHON R.G., HEWETT P.C., et al.
2014MNRAS.439L..51B 1666 T   A D S   X C F     40 3 17
ULASJ1234+0907: the reddest type 1 quasar at z = 2.5 revealed in the X-ray and far-infrared. 		BANERJI M., FABIAN A.C. and McMAHON R.G.
2014A&A...565A..91F 39           X         1 8 14 Gas reservoir of a hyper-luminous quasar at z = 2.6. FERUGLIO C., BONGIORNO A., FIORE F., et al.
2015A&A...574A..82P 45           X         1 6 77 Galaxy-wide outflows in z ∼ 1.5 luminous obscured quasars revealed through near-IR slit-resolved spectroscopy. PERNA M., BRUSA M., CRESCI G., et al.
2015MNRAS.447.3368B 250       D     X         7 40 68 Heavily reddened type 1 quasars at z > 2 - I. Evidence for significant obscured black hole growth at the highest quasar luminosities. BANERJI M., ALAGHBAND-ZADEH S., HEWETT P.C., et al.
2015MNRAS.453.3932R 78           X         2 67 85 Extremely red quasars from SDSS, BOSS and WISE: classification of optical spectra. ROSS N.P., HAMANN F., ZAKAMSKA N.L., et al.
2016ApJ...823..107F 212       D     X         6 26 21 Infrared spectral energy distribution decomposition of WISE-selected, hyperluminous hot dust-obscured galaxies. FAN L., HAN Y., NIKUTTA R., et al.
2016MNRAS.459..999A 566       D     X C F     13 30 4 Heavily reddened z ∼ 2 Type 1 quasars - II. Hα star formation constraints from SINFONI IFU observations. ALAGHBAND-ZADEH S., BANERJI M., HEWETT P.C., et al.
2017MNRAS.465.4390B 1034     A D S   X C       25 12 33 The discovery of gas-rich, dusty starbursts in luminous reddened quasars at z ∼ 2.5 with ALMA. BANERJI M., CARILLI C.L., JONES G., et al.
2017MNRAS.468.3042M 40           X         1 11 5 Searching for luminous absorbed sources in the WISE AGN catalogue. MOUNTRICHAS G., GEORGANTOPOULOS I., SECREST N.J., et al.
2018MNRAS.474.4528V 41           X         1 33 40 Heavy X-ray obscuration in the most luminous galaxies discovered by WISE. VITO F., BRANDT W.N., STERN D., et al.
2018MNRAS.479.1154B 2545       D     X C F     62 7 5 The interstellar medium properties of heavily reddened quasarsand companions at z∼ 2.5 with ALMA and JVLA. BANERJI M., JONES G.C., WAGG J., et al.
2019MNRAS.487.2594T 260       D     X C F     5 29 ~ [O III] Emission line properties in a new sample of heavily reddened quasars at z > 2. TEMPLE M.J., BANERJI M., HEWETT P.C., et al.
2020MNRAS.492.5280W 428       D     X C F     9 19 ~ A SCUBA-2 850 µm survey of heavily reddened quasars at z ∼ 2. WETHERS C.F., BANERJI M., HEWETT P.C., et al.
2020A&A...637A..84P 17       D               1 32 48 The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies. PENSABENE A., CARNIANI S., PERNA M., et al.
2020MNRAS.495.2652L 388       D     X C       9 16 18 X-ray observations of luminous dusty quasars at z > 2. LANSBURY G.B., BANERJI M., FABIAN A.C., et al.
2021A&A...645A..33B 86           X         2 15 39 The WISSH quasars project. IX. Cold gas content and environment of luminous QSOs at z ∼ 2.4-4.7. BISCHETTI M., FERUGLIO C., PICONCELLI E., et al.
2021MNRAS.503.5583B 2425     A D S   X C       57 5 8 Resolving discs and mergers in z ∼ 2 heavily reddened quasars and their companion galaxies with ALMA. BANERJI M., JONES G.C., CARNIANI S., et al.
2022MNRAS.517.3377S 102       D         F     2 17 6 Red quasars blow out molecular gas from galaxies during the peak of cosmic star formation. STACEY H.R., COSTA T., McKEAN J.P., et al.

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