Zobrazeno 1 - 10
of 29
pro vyhledávání: '"H. D. Jun"'
Autor:
R. J. Assef, F. E. Bauer, A. W. Blain, M. Brightman, T. Díaz-Santos, P. R. M. Eisenhardt, H. D. Jun, D. Stern, C.-W. Tsai, D. J. Walton, J. W. Wu
We report on VLT/FORS2 imaging polarimetry observations in the $R_{\rm special}$ band of WISE J011601.41-050504.0 (W0116-0505), a heavily obscured hyper-luminous quasar at $z=3.173$ classified as a Hot, Dust-Obscured Galaxy (Hot DOG) based on its mid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45a7197d5c89dfd7338640d256885f9b
Publikováno v:
2018 XIII International Conference on Electrical Machines (ICEM).
Loss and efficiency evaluation of induction motors (IMs) by summation of losses is based on sinusoidal drive. There are more and more cases of driving induction motors by a complete drive module (CDM). When the induction motor is driven by the conver
Autor:
D. Stern, Roberto J. Assef, C. W. Tsai, Jingwen Wu, Tanio Díaz-Santos, Hanae Inami, Andrew Blain, K. Dibert, F. Leclercq, H. D. Jun, George B. Lansbury, Manuel Aravena, Peter Eisenhardt
Publikováno v:
Science
Science, 2018, 362, pp.1034-1036. ⟨10.1126/science.aap7605⟩
Science, 2018, 362, pp.1034-1036. ⟨10.1126/science.aap7605⟩
Galaxy mergers and gas accretion from the cosmic web drove the growth of galaxies and their central black holes at early epochs. We report spectroscopic imaging of a multiple merger event in the most luminous known galaxy, WISE J224607.56-052634.9 (W
Autor:
C. Ricci, R. J. Assef, D. Stern, R. Nikutta, D. M. Alexander, D. Asmus, D. R. Ballantyne, F. E. Bauer, A. W. Blain, S. Boggs, P. G. Boorman, W. N. Brandt, M. Brightman, C. S. Chang, C.-T. J. Chen, F. E. Christensen, A. Comastri, W. W. Craig, T. Díaz-Santos, P. R. Eisenhardt, D. Farrah, P. Gandhi, C. J. Hailey, F. A. Harrison, H. D. Jun, M. J. Koss, S. LaMassa, G. B. Lansbury, C. B. Markwardt, M. Stalevski, F. Stanley, E. Treister, C.-W. Tsai, D. J. Walton, J. W. Wu, L. Zappacosta, W. W. Zhang
Publikováno v:
Ricci, C, Assef, R J, Stern, D, Nikutta, R, Alexander, D M, Asmus, D, Ballantyne, D R, Bauer, F E, Blain, A W, Boggs, S, Boorman, P G, Brandt, W N, Brightman, M, Chang, C S, Chen, C-T J, Christensen, F E, Comastri, A, Craig, W W, Díaz-Santos, T, Eisenhardt, P R, Farrah, D, Gandhi, P, Hailey, C J, Harrison, F A, Jun, H D, Koss, M J, LaMassa, S, Lansbury, G B, Markwardt, C B, Stalevski, M, Stanley, F, Treister, E, Tsai, C-W, Walton, D J, Wu, J W, Zappacosta, L & Zhang, W W 2017, ' NuSTAR observations of WISE J1036+0449, a galaxy at z ∼ 1 obscured by hot dust ', Astrophysical Journal, vol. 835, no. 1, 105 . https://doi.org/10.3847/1538-4357/835/1/105
Astrophysical journal, 2017, Vol.835(1), pp.105 [Peer Reviewed Journal]
ASTROPHYSICAL JOURNAL
Astrophysical journal, 2017, Vol.835(1), pp.105 [Peer Reviewed Journal]
ASTROPHYSICAL JOURNAL
Hot, Dust-Obscured Galaxies (Hot DOGs), selected from the WISE all sky infrared survey, host some of the most powerful Active Galactic Nuclei (AGN) known, and might represent an important stage in the evolution of galaxies. Most known Hot DOGs are at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fafdb4a58761c5b306cb06a1f0f26eda
https://orbit.dtu.dk/en/publications/8ed6a27b-5887-450d-b13d-5a7e4e12efb6
https://orbit.dtu.dk/en/publications/8ed6a27b-5887-450d-b13d-5a7e4e12efb6
Autor:
Roberto J. Assef, Armin Rest, D. Stern, C. L. Waters, Peter Eisenhardt, H. D. Jun, J. L. Prieto, H. Flewelling, Roc M. Cutri, Nick Kaiser, Matthew J. Graham, R. P. Kudritzki
Publikováno v:
The Astrophysical Journal. 866:26
Recently Assef et al.(2018) presented two catalogs of AGN candidates over 30,093 deg^2 selected from the Wide-field Infrared Survey Explorer (WISE) observations. From their most reliable sample, Assef et al. (2018) identified 45 AGN candidates with t
Autor:
D. N. Burrows, J. A. Kennea, G. Ghisellini, V. Mangano, B. Zhang, K. L. Page, M. Eracleous, P. Romano, T. Sakamoto, A. D. Falcone, J. P. Osborne, S. Campana, A. P. Beardmore, A. A. Breeveld, M. M. Chester, R. Corbet, S. Covino, J. R. Cummings, P. D'Avanzo, V. D'Elia, P. Esposito, P. A. Evans, D. Fugazza, J. M. Gelbord, K. Hiroi, S. T. Holland, K. Y. Huang, M. Im, G. Israel, Y. Jeon, Y.-B. Jeon, H. D. Jun, N. Kawai, J. H. Kim, H. A. Krimm, F. E. Marshall, null P. Mészáros, H. Negoro, N. Omodei, W.-K. Park, J. S. Perkins, M. Sugizaki, H.-I. Sung, G. Tagliaferri, E. Troja, Y. Ueda, Y. Urata, R. Usui, L. A. Antonelli, S. D. Barthelmy, G. Cusumano, P. Giommi, A. Melandri, M. Perri, J. L. Racusin, B. Sbarufatti, M. H. Siegel, N. Gehrels
Publikováno v:
Nature. 476(7361)
Massive black holes are believed to reside at the centres of most galaxies. They can be- come detectable by accretion of matter, either continuously from a large gas reservoir or impulsively from the tidal disruption of a passing star, and conversion
Publikováno v:
World Environmental and Water Resources Congress 2008.
In this paper the hazard rates of the cast iron 6 inch (about 150 mm) pipes of a study area are modeled by implementing the proportional hazards modeling approach for consecutive pipe failures. A methodology of identifying individual pipes according
Publikováno v:
World Environmental and Water Resources Congress 2008.
In sewer layout design, most developed models are designed to determine pipe diameter, slope and overall layout to minimize the least cost for the design rainfall. However, these models cannot consider the superposition effect of runoff hydrographs e
Publikováno v:
World Environmental & Water Resources Congress 2008; 2008, p1-10, 10p
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