|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| ULAS J231556.23+014350.3 , the SIMBAD biblio (18 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST03:05:25 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2015MNRAS.447.3368B | 289 | D | X F | 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. | |
| 2016MNRAS.459..999A | 94 | D | F | 3 | 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 | 1192 | A | D | S X C | 29 | 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. |
| 2017ApJ...850..180J | 80 | X | 2 | 19 | 47 | Dynamical characterization of galaxies at z ∼ 4-6 via tilted ring fitting to ALMA [C II] observations. | JONES G.C., CARILLI C.L., SHAO Y., et al. | ||
| 2017A&A...608A..51M | 357 | X C | 8 | 47 | 66 | The WISSH quasars project. III. X-ray properties of hyper-luminous quasars. | MARTOCCHIA S., PICONCELLI E., ZAPPACOSTA L., et al. | ||
| 2018MNRAS.474.4528V | 81 | F | 2 | 33 | 40 | Heavy X-ray obscuration in the most luminous galaxies discovered by WISE. | VITO F., BRANDT W.N., STERN D., et al. | ||
| 2018MNRAS.475.3682W | 458 | D | X F | 11 | 19 | 5 | UV-luminous, star-forming hosts of z ∼ 2 reddened quasars in the Dark Energy Survey. | WETHERS C.F., BANERJI M., HEWETT P.C., et al. | |
| 2018MNRAS.479.1154B | 2986 | D | X C F | 73 | 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. | |
| 2019A&A...630A.118V | 83 | C | 1 | 28 | 69 | The X-ray properties of z > 6 quasars: no evident evolution of accretion physics in the first Gyr of the Universe. | VITO F., BRANDT W.N., BAUER F.E., et al. | ||
| 2020MNRAS.492.5280W | 1045 | D | X C F | 24 | 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 | 223 | D | X | 6 | 16 | 18 | X-ray observations of luminous dusty quasars at z > 2. | LANSBURY G.B., BANERJI M., FABIAN A.C., et al. | |
| 2021MNRAS.503.5583B | 1757 | A | D | S X C | 41 | 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. | |
| 2024MNRAS.528..711G | 45 | X | 1 | 21 | ~ | Accretion and obscuration in merger-dominated luminous red quasars. | GLIKMAN E., LAMASSA S., PICONCELLI E., et al. | ||
| 2024MNRAS.533.2948S | 3521 | A | S X C F | 76 | 2 | ~ | A big red dot: scattered light, host galaxy signatures, and multiphase gas flows in a luminous, heavily reddened quasar at cosmic noon. | STEPNEY M., BANERJI M., TANG S., et al. | |
| 2025ApJ...994...86R | 93 | X | 2 | 22 | ~ | Deciphering the Nature of Virgil: An Obscured Active Galactic Nucleus Lurking within an Apparently Normal Lyα Emitter during Cosmic Reionization. | RINALDI P., PEREZ-GONZALEZ P.G., RIEKE G.H., et al. | ||
| 2026ApJ...999...30C | 50 | X | 1 | 8 | ~ | A z ≃ 0.4 Galaxy Reflecting the High-redshift Little Red Dots: An Extended Starburst with an Overmassive Black Hole. | CHEN X., ICHIKAWA K., AKIYAMA M., et al. |