An extended [CII] halo around a massive star-forming galaxy at z = 5.3

Autor: Trystan S Lambert, A Posses, M Aravena, J Gónzalez-López, R J Assef, T Díaz-Santos, D Brisbin, R Decarli, R Herrera-Camus, J Mejía, C Ricci

High-redshift observations are often biased towards massive and bright galaxies that are not necessarily representative of the full population. In order to accurately study galaxy evolution and mass assembly at these redshifts, observations of ``norm

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d3a36a61d91fe56a33a3aaaf1d058170

Imaging Polarization of the Blue-Excess Hot Dust-Obscured Galaxy WISE J011601.41-050504.0

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

NuSTAR observations of WISE J1036+0449, a galaxy at z ∼ 1 obscured by hot dust

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

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

HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift

Autor: M. P. Viero, L. Moncelsi, R. F. Quadri, V. Arumugam, R. J. Assef, M. Béthermin, J. Bock, C. Bridge, C. M. Casey, A. Conley, A. Cooray, D. Farrah, J. Glenn, S. Heinis, E. Ibar, S. Ikarashi, R. J. Ivison, K. Kohno, G. Marsden, S. J. Oliver, I. G. Roseboom, B. Schulz, D. Scott, P. Serra, M. Vaccari, J. D. Vieira, L. Wang, J. Wardlow, G. W. Wilson, M. S. Yun, M. Zemcov

Publikováno v: The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2013, 779 (1), ⟨10.1088/0004-637X/779/1/32⟩
The Astrophysical Journal, 2013, 779 (1), ⟨10.1088/0004-637X/779/1/32⟩
Astrophysical Journal, vol 779, iss 1
Viero, MP; Moncelsi, L; Quadri, RF; Arumugam, V; Assef, RJ; Béthermin, M; et al.(2013). HerMES: The contribution to the cosmic infrared background from galaxies selected by mass and redshift. Astrophysical Journal, 779(1). doi: 10.1088/0004-637X/779/1/32. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/7ns3595f

We quantify the fraction of the cosmic infrared background (CIB) that originates from galaxies identified in the UV/optical/near-infrared by stacking 81,250 (~35.7 arcmin^2) K-selected sources (K_AB < 24.0), split according to their rest-frame U - V

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdc6b0822adebdadb601c1ff64071298
https://doi.org/10.1088/0004-637X/779/1/32

The Contribution of Galaxies to the 3.4 μm Cosmic Infrared Background as Measured Using WISE.

Autor: S. E. Lake, E. L. Wright, R. J. Assef, T. H. Jarrett, S. Petty, S. A. Stanford, C.-W. Tsai

Publikováno v: Astrophysical Journal; 12/20/2019, Vol. 887 Issue 2, p1-1, 1p