other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
WISE J085929.94+482302.3 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST02:48:37 |
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...756...96W | 171 | D | X F | 4 | 36 | 115 | Submillimeter follow-up of WISE-selected hyperluminous galaxies. | WU J., TSAI C.-W., SAYERS J., et al. | |
2015ApJ...804...27A | 16 | D | 1 | 118 | 139 | Half of the most luminous quasars may be obscured: investigating the nature of WISE-selected hot dust-obscured galaxies. | ASSEF R.J., EISENHARDT P.R.M., STERN D., et al. | ||
2015ApJ...805...90T | 16 | D | 3 | 146 | 135 | The most luminous galaxies discovered by WISE. | TSAI C.-W., EISENHARDT P.R.M., WU J., et al. | ||
2016ApJ...819..111A | 83 | C | 1 | 12 | 45 | Hot dust obscured galaxies with excess blue light: dual AGN or single AGN under extreme conditions? | ASSEF R.J., WALTON D.J., BRIGHTMAN M., et al. | ||
2016ApJ...822L..32F | 100 | D | F | 3 | 18 | 80 | The most luminous heavily obscured quasars have a high merger fraction: morphological study of WISE-selected hot dust-obscured galaxies. | FAN L., HAN Y., FANG G., et al. | |
2016ApJ...823..107F | 16 | D | 5 | 26 | 21 | Infrared spectral energy distribution decomposition of WISE-selected, hyperluminous hot dust-obscured galaxies. | FAN L., HAN Y., NIKUTTA R., et al. | ||
2017PASP..129l4101F | 219 | D | X | 6 | 11 | 5 | The SCUBA-2 850 µm follow-up of WISE-selected, luminous dust-obscured quasars. | FAN L., JONES S.F., HAN Y., et al. | |
2018MNRAS.474.4528V | 17 | D | 2 | 33 | 40 | Heavy X-ray obscuration in the most luminous galaxies discovered by WISE. | VITO F., BRANDT W.N., STERN D., et al. | ||
2020ApJ...905...16F | 358 | D | X | 9 | 26 | 14 | Fast outflows in Hot Dust-Obscured Galaxies detected with Keck/NIRES. | FINNERTY L., LARSON K., SOIFER B.T., et al. |