WISE J014946.16+235014.6 , the SIMBAD biblio

WISE J014946.16+235014.6 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST02:47:48


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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 viz 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 viz 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.

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