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WISE J014946.16+235014.6 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST02:47:48 |
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 | 326 | D | X C F | 7 | 36 | 115 | Submillimeter follow-up of WISE-selected hyperluminous galaxies. | WU J., TSAI C.-W., SAYERS J., et al. | |
2013MNRAS.431.1956G | 39 | X | 1 | 71 | 103 | Calibration of the total infrared luminosity of nearby galaxies from Spitzer and Herschel bands. | GALAMETZ M., KENNICUTT R.C., CALZETTI D., et al. | ||
2014ApJ...793....8W | 2439 | K A | D | S X C | 61 | 10 | 17 | Interferometric follow-up of WISE hyper-luminous hot, dust-obscured galaxies. | WU J., BUSSMANN R.S., TSAI C.-W., 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...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 | 297 | D | X | 8 | 26 | 21 | Infrared spectral energy distribution decomposition of WISE-selected, hyperluminous hot dust-obscured galaxies. | FAN L., HAN Y., NIKUTTA R., et al. | |
2018ApJ...856L...5F | 783 | A | D | X C | 19 | 11 | 17 | ALMA detections of CO emission in the most luminous, heavily dust-obscured quasars at z > 3. | FAN L., KNUDSEN K.K., FOGASY J., 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. | ||
2020MNRAS.496.1565P | 43 | X | 1 | 14 | ~ | Cold molecular gas and free-free emission from hot, dust-obscured galaxies at z ∼ 3. | PENNEY J.I., BLAIN A.W., ASSEF R.J., et al. | ||
2021A&A...646A.178S | 1262 | A | D | S X C | 28 | 11 | 8 | Detection of H2O and OH+ in z > 3 hot dust-obscured galaxies. | STANLEY F., KNUDSEN K.K., AALTO S., et al. |
2024ApJ...964...95S | 220 | D | X | 5 | 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. |