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| FIRST J160357.3+274552 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST02:55:05 |
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...756...96W | 93 | D | F | 3 | 36 | 115 | Submillimeter follow-up of WISE-selected hyperluminous galaxies. | WU J., TSAI C.-W., SAYERS J., et al. | |
| 2014MNRAS.443..146J | 210 | D | X C | 5 | 19 | 41 | Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxies. | JONES S.F., BLAIN A.W., STERN D., et al. | |
| 2015MNRAS.448.3325J | 39 | X | 1 | 41 | 27 | Submillimetre observations of WISE/radio-selected AGN and their environments. | JONES S.F., BLAIN A.W., LONSDALE C., 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. | ||
| 2016MNRAS.455.2058F | 551 | A | D | X C F | 13 | 13 | 3 | Four hot DOGs in the microwave. | FREY S., PARAGI Z., GABANYI K.E., et al. |
| 2016ApJ...822L..32F | 96 | 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. | ||
|
2017MNRAS.468..196T
|
16 | D | 1 | 46259 | 2 | The invisible AGN catalogue: a mid-infrared-radio selection method for optically faint active galactic nuclei. | TRUEBENBACH A.E. and DARLING J. | ||
| 2024ApJ...964...95S | 287 | D | X | 7 | 44 | ~ | Physical Properties of Hyperluminous, Dust-obscured Quasars at z ∼ 3: Multiwavelength Spectral Energy Distribution Analysis and Cold Gas Content Revealed by ALMA. | SUN W., FAN L., HAN Y., et al. |
