WISE J224607.55-052634.9 , the SIMBAD biblio

WISE J224607.55-052634.9 , the SIMBAD biblio (54 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST05:10:26

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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
2014MNRAS.443..146J 249       D     X C       6 19 41 Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxies. JONES S.F., BLAIN A.W., STERN D., et al.
2015ApJ...804...27A viz 55       D     X         2 118 139 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 viz 211       D     X         6 146 135 The most luminous galaxies discovered by WISE. TSAI C.-W., EISENHARDT P.R.M., WU J., et al.
2016ApJ...816L...6D 1447     A     X C       36 4 59 The strikingly uniform, highly turbulent interstellar medium of the most luminous galaxy in the universe. DIAZ-SANTOS T., ASSEF R.J., BLAIN A.W., et al.
2016ApJ...819..111A 40           X         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 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 212       D     X         6 26 21 Infrared spectral energy distribution decomposition of WISE-selected, hyperluminous hot dust-obscured galaxies. FAN L., HAN Y., NIKUTTA R., et al.
2016MNRAS.458.4383H 39           X         1 23 25 Early science with the Large Millimeter Telescope: observations of extremely luminous high-z sources identified by Planck. HARRINGTON K.C., YUN M.S., CYBULSKI R., et al.
2016MNRAS.459.2014L 39           X         1 7 6 General polytropic self-gravitating cylinder free-fall and accreting mass string with a chain of collapsed objects. LOU Y.-Q. and HU X.-Y.
2016ApJ...827...34O 40           X         1 12 46 Witnessing the birth of the red sequence: ALMA high-resolution imaging of [c II] and dust in two interacting ultra-red starbursts at z = 4.425. OTEO I., IVISON R.J., DUNNE L., et al.
2016MNRAS.463.1291I 43           X         1 2 16 AGN-starburst evolutionary connection: a physical interpretation based on radiative feedback. ISHIBASHI W. and FABIAN A.C.
2017ApJ...835..105R 161           X         4 11 50 NuSTAR observations of WISE J1036+0449, a galaxy at z∼1 obscured by hot dust. RICCI C., ASSEF R.J., STERN D., et al.
2017PASP..129l4101F 40           X         1 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.
2018ApJ...852...96W 82           X         2 11 22 Eddington-limited accretion in z ∼ 2 WISE-selected hot, dust-obscured galaxies. WU J., JUN H.D., ASSEF R.J., et al.
2018ApJ...854..157F 3213 T K A D     X C       79 2 4 The spectral energy distribution of the hyperluminous, Hot dust-obscured galaxy

W2246-0526. 		FAN L., GAO Y., KNUDSEN K.K., et al.
2018ApJ...856L...5F 81           X         2 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 659       D S   X C F     14 33 40 Heavy X-ray obscuration in the most luminous galaxies discovered by WISE. VITO F., BRANDT W.N., STERN D., et al.
2018ApJ...866...92L 40           X         1 89 46 Polar dust, nuclear obscuration, and IR SED diversity in type-1 AGNs. LYU J. and RIEKE G.H.
2018ApJ...868...15T 2994 T K A     X C       73 9 6 Super-Eddington accretion in the WISE-selected extremely luminous infrared galaxy
W2246-0526. 		TSAI C.-W., EISENHARDT P.R.M., JUN H.D., et al.
2018MNRAS.481.4522I 40           X         1 4 2 Variations on a theme of AGN-driven outflows: luminosity evolution and ambient density distribution. ISHIBASHI W. and FABIAN A.C.
2018Sci...362.1034D 5 7 35 The multiple merger assembly of a hyperluminous obscured quasar at redshift 4.6. DIAZ-SANTOS T., ASSEF R.J., BLAIN A.W., et al.
2019A&A...630A..59B viz 17       D               2 51 69 Widespread QSO-driven outflows in the early Universe. BISCHETTI M., MAIOLINO R., CARNIANI S., et al.
2019ApJ...887...74F 41           X         1 6 ~ ALMA reveals a gas-rich, maximum starburst in the hyperluminous, dust-obscured quasar W0533-3401 at z ∼ 2.9. FAN L., KNUDSEN K.K., HAN Y., et al.
2020ApJ...888..110J 42           X         1 15 15 Spectral classification and ionized gas outflows in z ∼ 2 WISE-selected hot dust-obscured galaxies. JUN H.D., ASSEF R.J., BAUER F.E., et al.
2020MNRAS.495.2652L 42           X         1 16 18 X-ray observations of luminous dusty quasars at z > 2. LANSBURY G.B., BANERJI M., FABIAN A.C., et al.
2020MNRAS.496.1565P 41           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.
2020ApJ...897..112A 168           X         4 5 16 Hot dust-obscured galaxies with excess blue light. ASSEF R.J., BRIGHTMAN M., WALTON D.J., et al.
2020ApJ...905...16F 222       D     X         6 26 14 Fast outflows in Hot Dust-Obscured Galaxies detected with Keck/NIRES. FINNERTY L., LARSON K., SOIFER B.T., et al.
2020ApJ...905L..32F 2247 T   A S   X C       52 4 ~ The hyperluminous, dust-obscured quasar
W2246-0526 at z = 4.6: detection of parsec-scale radio activity. 		FAN L., CHEN W., AN T., et al.
2021MNRAS.503L..11E 85           X         2 6 7 A hyperluminous obscured quasar at a redshift of z ≃ 4.3. EFSTATHIOU A., MALEK K., BURGARELLA D., et al.
2021A&A...654A..37D 2065       D     X C       49 10 7 Kinematics and star formation of high-redshift hot dust-obscured quasars as seen by ALMA. DIAZ-SANTOS T., ASSEF R.J., EISENHARDT P.R.M., et al.
2022MNRAS.511.4572A 44           X         1 4 6 A compact symmetric radio source born at one-tenth the current age of the Universe. AN T., WANG A., ZHANG Y., et al.
2022ApJ...929...69L 43           X         1 6 4 Exploring the Radio Spectral Energy Distribution of the Ultraluminous Radio-quiet Quasar SDSS J0100+2802 at Redshift 6.3. LIU Y., WANG R., MOMJIAN E., et al.
2022Natur.604..261F 130           X         3 12 32 A dusty compact object bridging galaxies and quasars at cosmic dawn. FUJIMOTO S., BRAMMER G.B., WATSON D., et al.
2022ApJS..260...49K 17       D               1 87 4 Radio-loud Quasars above Redshift 4: Very Long Baseline Interferometry (VLBI) Imaging of an Extended Sample. KREZINGER M., PERGER K., GABANYI K.E., et al.
2023A&A...673A.116K 131           X         3 13 ~ Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with [C II]. KADE K., KNUDSEN K.K., VLEMMINGS W., et al.
2023A&A...677A..54Z 2115 T   A     X C       47 5 ~ An overdensity of Lyman break galaxies around the hot dust-obscured galaxy
WISE J224607.56-052634.9. 		ZEWDIE D., ASSEF R.J., MAZZUCCHELLI C., et al.
2023ApJ...958..162L 44           X         1 4 ~ Discovery of a Low-redshift Hot Dust-obscured Galaxy. LI G., TSAI C.-W., STERN D., et al.
2024MNRAS.528..499L 18       D               1 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024A&A...682A.166F 3656   K A     X C       81 14 ~ A benchmark for extreme conditions of the multiphase interstellar medium in the most luminous hot dust-obscured galaxy at z = 4.6. FERNANDEZ ARANDA R., DIAZ SANTOS T., HATZIMINAOGLOU E., et al.
2024ApJ...964...95S 332       D     X         8 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.
2024A&A...687A..62F 45           X         1 13 ~ Study of the ∼50 kpc circumgalactic environment around the merger system J2057-0030 at z ∼ 4.6 using ALMA. FUENTEALBA-FUENTES M., LIRA P., DIAZ-SANTOS T., et al.
2024ApJ...971...40L 134           X         3 3 ~ Black Hole Mass and Eddington Ratio Distribution of Hot Dust-obscured Galaxies. LI G., ASSEF R.J., TSAI C.-W., et al.
2024ApJ...972...51L 2822 T   A D     X C       62 4 ~ Lyα Imaging around the Hyperluminous Dust-obscured Quasar

W2246-0526 at z = 4.6. 		LUO Y., FAN L., LIANG Y., et al.
2024MNRAS.534..978M 1003       D     X C F     21 10 ~ CO spectra of the ISM in the Host Galaxies of the most luminous WISE-selected AGNs. MARTIN L.R., BLAIN A.W., DIAZ-SANTOS T., et al.
2025PASJ...77..139I 467           X C       9 15 ~ Detection of the [O I] 63 µm emission line from the z = 6.04 quasar J2054-0005. ISHII N., HASHIMOTO T., FERKINHOFF C., et al.
2025A&A...694A.121Z 1913     A D     X C       41 7 ~ Overdensity of Lyman-break galaxy candidates around hot-dust-obscured galaxies. ZEWDIE D., ASSEF R.J., LAMBERT T., et al.
2025ApJ...981..104L 93           X         2 67 ~ Searching for Low-redshift Hot Dust-obscured Galaxies. LI G., WU J., TSAI C.-W., et al.
2025A&A...695L..15F 1008 T K A     X C       20 1 ~ Spatially resolved dust properties over 50 kpc in a hyperluminous galaxy merger at z = 4.6. FERNANDEZ ARANDA R., DIAZ SANTOS T., HATZIMINAOGLOU E., et al.
2025ApJ...989..230V 1773       S   X C       36 2 ~ Powerful Nuclear Outflows and Circumgalactic Medium Shocks Driven by the Most Luminous Known Obscured Quasar in the Universe. VAYNER A., DIAZ-SANTOS T., EISENHARDT P.R.M., et al.
2025A&A...702A.124A 47           X         1 8 ~ A massive gas outflow outside the line of sight: Imaging polarimetry of the blue excess Hot Dust-Obscured Galaxy W0204-0506. ASSEF R.J., STALEVSKI M., ARMUS L., et al.
2025A&A...702A.174M 47           X         1 15 ~ JWST's PEARLS: A z ≃ 6 quasar in a train-wreck galaxy merger system. MARSHALL M.A., WINDHORST R.A., FERRAMI G., et al.
2025A&A...703A.216H 2127     A S   X C       44 2 ~ Hot Diggity Dog: Simultaneous CO and dust modelling of the most luminous WISE hot dust-obscured galaxy unveils extreme molecular gas excitation. HARRINGTON K.C., FERNANDEZ ARANDA R., BOOGAARD L., et al.
2026A&A...705A..39P 550           X C       10 6 ~ High-z [OI] emission lines: COLDSIM simulations and ALMA observations. PARENTE M., BISCHETTI M., MAIO U., et al.

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