no code implementations • 17 Dec 2020 • Tomoko L. Suzuki, Masato Onodera, Tadayuki Kodama, Emanuele Daddi, Masao Hayashi, Yusei Koyama, Rhythm Shimakawa, Ian Smail, David Sobral, Sandro Tacchella, Ichi Tanaka
We conducted sub-millimeter observations with the Atacama Large Millimeter/sub-millimeter Array (ALMA) of star-forming galaxies at $z\sim3. 3$, whose gas-phase metallicities have been previously measured.
Astrophysics of Galaxies
no code implementations • 8 Oct 2019 • FangXia An, J. M. Simpson, Ian Smail, A. M. Swinbank, Cong Ma, Daizhong Liu, P. Lang, E. Schinnerer, A. Karim, B. Magnelli, S. Leslie, F. Bertoldi, Chian-Chou Chen, J. E. Geach, Y. Matsuda, S. M. Stach, J. L. Wardlow, B. Gullberg, R. J. Ivison, Y. Ao, R. T. Coogan, A. P. Thomson, S. C. Chapman, R. Wang, Wei-Hao Wang, Y. Yang, R. Asquith, N. Bourne, K. Coppin, N. K. Hine, L. C. Ho, H. S. Hwang, Y. Kato, K. Lacaille, A. J. R. Lewis, I. Oteo, J. Scholtz, M. Sawicki, D. Smith
We identify multi-wavelength counterparts to 1, 147 submillimeter sources from the S2COSMOS SCUBA-2 survey of the COSMOS field by employing a recently developed radio$+$machine-learning method trained on a large sample of ALMA-identified submillimeter galaxies (SMGs), including 260 SMGs identified in the AS2COSMOS pilot survey.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
1 code implementation • 18 Sep 2018 • Kevin Lacaille, Scott Chapman, Ian Smail, Charles Steidel, Andrew Blain, James Geach, Anneya Golob, Mark Gurwell, Rob Ivison, Naveen Reddy, Marcin Sawicki
We present James Clerk Maxwell Telescope (JCMT) Submillimetre Common-User Bolometer Array 2 (SCUBA-2) 850 \& 450 $\mu$m observations ($\sigma_{850}\sim0. 5$ mJy, $\sigma_{450}\sim5$ mJy) of the HS1549+19 and HS1700+64 survey fields containing two of the largest known galaxy over-densities at $z=2. 85$ and $2. 30$, respectively.
Astrophysics of Galaxies
1 code implementation • 13 Aug 2018 • Riccardo Pavesi, Chelsea E. Sharon, Dominik A. Riechers, Jacqueline A. Hodge, Roberto Decarli, Fabian Walter, Chris L. Carilli, Emanuele Daddi, Ian Smail, Mark Dickinson, Rob J. Ivison, Mark Sargent, Elisabete da Cunha, Manuel Aravena, Jeremy Darling, Vernesa Smolčić, Nicholas Z. Scoville, Peter L. Capak, Jeff Wagg
We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line deep field targeting CO(1-0) emission from galaxies at $z=1. 95-2. 85$ and CO(2-1) at $z=4. 91-6. 70$.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
