Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Chen, Chian-Chou"'
Autor:
Ramasawmy, Joanna, Klaassen, Pamela D., Cicone, Claudia, Mroczkowski, Tony K., Chen, Chian-Chou, Cornish, Thomas, da Cunha, Elisabete Lima, Hatziminaoglou, Evanthia, Johnstone, Doug, Liu, Daizhong, Perrott, Yvette, Schimek, Alice, Stanke, Thomas, Wedemeyer, Sven
The Atacama Large Aperture Submillimeter Telescope (AtLAST) is a concept for a 50m class single-dish telescope that will provide high sensitivity, fast mapping of the (sub-)millimeter sky. Expected to be powered by renewable energy sources, and to be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95ffc578b4010e84fd5989e307d65a40
Autor:
Iani, E., Zanella, A., Vernet, J., Richard, J., Gronke, M., Harrison, C. M., Arrigoni-Battaia, F., Rodighiero, G., Burkert, A., Behrendt, M., Chen, Chian-Chou, Emsellem, E., Fensch, J., Hibon, P., Hilker, M., Le Floc'h, E., Mainieri, V., Swinbank, A. M., Valentino, F., Vanzella, E., Zwaan, M. A.
Publikováno v:
Iani, E, Zanella, A, Vernet, J, Richard, J, Gronke, M, Harrison, C M, Arrigoni-Battaia, F, Rodighiero, G, Burkert, A, Behrendt, M, Chen, C-C, Emsellem, E, Fensch, J, Hibon, P, Hilker, M, Le Floc'h, E, Mainieri, V, Swinbank, A M, Valentino, F, Vanzella, E & Zwaan, M A 2021, ' Stellar feedback in a clumpy galaxy at z similar to 3.4 ', Monthly Notices of the Royal Astronomical Society, vol. 507, no. 3, pp. 3830-3848 . https://doi.org/10.1093/mnras/stab2376
Giant star-forming regions (clumps) are widespread features of galaxies at z approximate to 1-4. Theory predicts that they can play a crucial role in galaxy evolution, if they survive to stellar feedback for >50 Myr. Numerical simulations show that c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2751::f71ea97dd7e44feb0680d8c3c25aef1c
https://curis.ku.dk/portal/da/publications/stellar-feedback-in-a-clumpy-galaxy-at-z-similar-to-34(c0fa3f3f-23d2-48ea-9959-3f339e7a79a8).html
https://curis.ku.dk/portal/da/publications/stellar-feedback-in-a-clumpy-galaxy-at-z-similar-to-34(c0fa3f3f-23d2-48ea-9959-3f339e7a79a8).html
Autor:
Chen, Chian-Chou, Harrison, C. M., Smail, I., Swinbank, A. M., Turner, O. J., Wardlow, J. L., Brandt, W. N., Calistro Rivera, G., Chapman, S. C., Cooke, E. A., Dannerbauer, H., Dunlop, J. S., Farrah, D., Michałowski, M. J., Schinnerer, E., Simpson, J. M., Thomson, A. P., van der Werf, P. P.
Publikováno v:
Chen, C-C, Harrison, C M, Smail, I, Swinbank, A M, Turner, O J, Wardlow, J L, Brandt, W N, Rivera, G C, Chapman, S C, Cooke, E A, Dannerbauer, H, Dunlop, J S, Farrah, D, Michałowski, M J, Schinnerer, E, Simpson, J M, Thomson, A P & Werf, P P V D 2020, ' Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies ', Astronomy and Astrophysics, vol. 635, A119, pp. 1-15 . https://doi.org/10.1051/0004-6361/201936286
Astronomy & astrophysics, 2020, Vol.635, pp.A119 [Peer Reviewed Journal]
Astronomy & astrophysics, 2020, Vol.635, pp.A119 [Peer Reviewed Journal]
By using data from the Atacama Large Millimeter/submillimeter Array and near-infrared (NIR) integral field spectrographs, including both Spectrograph for INtegral Field Observations in the Near Infrared and K-band Multi Object Spectrograph on the Ver
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::df08c91beaaba527be8dc1e638df223e
https://www.pure.ed.ac.uk/ws/files/213879560/2002.03545v1.pdf
https://www.pure.ed.ac.uk/ws/files/213879560/2002.03545v1.pdf
Autor:
Klitsch, A., Zwaan, M. A., Smail, Ian, Peroux, C., Biggs, A. D., Chen, Chian-Chou, Ivison, R. J., Popping, G., Lagos, C., Bethermin, M., Swinbank, A. M., Hamanowicz, A., Dutta, R.
Measurements of the cosmic far-infrared background (CIB) indicate that emission from many extragalactic phenomena, including star formation and black hole accretion, in the Universe can be obscured by dust. Resolving the CIB to study the population o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1a609d8d030058a97ff29d558aad7917
Autor:
Chen, Chian-Chou, Harrison, C. M., Smail, I., Swinbank, A. M., Turner, O. J., Wardlow, J. L., Brandt, W. N., Rivera, G. Calistro, Chapman, S. C., Cooke, E. A., Dannerbauer, H., Dunlop, J. S., Farrah, D., Micha��owski, M. J., Schinnerer, E., Simpson, J. M., Thomson, A. P., van der Werf, P. P.
Using data from ALMA and near-infrared (NIR) integral field spectrographs including both SINFONI and KMOS on the VLT, we investigate the two-dimensional distributions of H$��$ and rest-frame far-infrared (FIR) continuum in six submillimeter galax
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::282b30a170f36bbe7c3f90330602aca1
Autor:
Chen, Chian-Chou
Star-formation rates (SFRs) are among the most fundamental measurements to galaxy formation models, yet there is still a lack of agreement between measurements made using different methods, expecially when it comes to accounting for dust-obscured SFR
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3792637bf42587dccfdf92bb8c7c4902
Autor:
Cunningham, D. J. M., Chapman, S. C., Aravena, M., De Breuck, C., B��thermin, M., Chen, Chian-Chou, Dong, Chenxing, Gonzalez, A. H., Greve, T. R., Litke, K. C., Ma, J., Malkan, M., Marrone, D. P., Miller, T., Phadke, K. A., Reuter, C., Rotermund, K., Spilker, J. S., Stark, A. A., Strandet, M., Vieira, J. D., Wei��, A.
We present Atacama Compact Array and Atacama Pathfinder Experiment observations of the [N II] 205 $��$m fine-structure line in 40 sub-millimetre galaxies lying at redshifts z = 3 to 6, drawn from the 2500 deg$^2$ South Pole Telescope survey. This
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9ac26fa60f49e937a67593a5ef395b75
Autor:
Rybak, Matus, Rivera, G. Calistro, Hodge, J. A., Smail, Ian, Walter, F., van der Werf, P., da Cunha, E., Chen, Chian-Chou, Dannerbauer, H., Ivison, R. J., Karim, A., Simpson, J. M., Swinbank, A. M., Wardlow, J. L.
We present 0.15-arcsec (1 kpc) resolution ALMA observations of the [CII] 157.74 um line and rest-frame 160-um continuum emission in two z~3 dusty, star-forming galaxies - ALESS 49.1 and ALESS 57.1, combined with resolved CO(3-2) observations. In both
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ea0b403276106290367ec3fac32d0b7
Autor:
Litke, Katrina C., Marrone, Daniel P., Spilker, Justin S., Aravena, Manuel, Bethermin, Matthieu, Chapman, Scott, Chen, Chian-Chou, De Breuck, Carlos, Dong, Chenxing, Gonzalez, Anthony, Greve, Thomas R., Hayward, Christopher C., Hezaveh, Yashar, Jarugula, Sreevani, Ma, Jingzhe, Morningstar, Warren, Narayanan, Desika, Phadke, Kedar, Reuter, Cassie, Vieira, Joaquin, Weiss, Axel, Litke, Katrina, Marrone, Daniel, Spilker, Justin, Breuck, Carlos de, Chen, Chenxing, Greve, Thomas, Hayward, Christopher
Publikováno v:
Litke, K C, Marrone, D P, Spilker, J S, Aravena, M, Béthermin, M, Chapman, S, Chen, C C, Breuck, C D, Dong, C, Gonzalez, A, Greve, T R, Hayward, C C, Hezaveh, Y, Jarugula, S, Ma, J, Morningstar, W, Narayanan, D, Phadke, K, Reuter, C, Vieira, J & Weiss, A 2019, ' Spatially Resolved [C ii] Emission in SPT0346-52: A Hyper-starburst Galaxy Merger at z ~ 5.7 ', Astrophysical Journal, vol. 870, no. 2, 80 . https://doi.org/10.3847/1538-4357/aaf057
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2019, 870 (2), pp.80. ⟨10.3847/1538-4357/aaf057⟩
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2019, 870 (2), pp.80. ⟨10.3847/1538-4357/aaf057⟩
SPT0346-52 is one of the most most luminous and intensely star-forming galaxies in the universe, with L_FIR > 10^13 L_sol and Sigma_SFR ~ 4200 M_sol yr^-1 kpc^-2. In this paper, we present ~0.15'' ALMA observations of the [CII]158micron emission line
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::923cc2749f40f1297668c40e8c72ee9c
https://orbit.dtu.dk/en/publications/715db67a-5888-4454-a809-54e4c2cb0efe
https://orbit.dtu.dk/en/publications/715db67a-5888-4454-a809-54e4c2cb0efe
Autor:
Geach, James E., Banerji, Manda, Bertoldi, Frank, Bethermin, Matthieu, Casey, Caitlin M., Chen, Chian-Chou, Clements, David L., Cicone, Claudia, Combes, Francoise, Conselice, Christopher, Cooray, Asantha, Coppin, Kristen, Daddi, Emanuele, Dannerbauer, Helmut, Dave, Romeel, Doherty, Matthew, Dunlop, James S., Edge, Alastair, Farrah, Duncan, Franco, Maximilien, Fuller, Gary, Garratt, Tracy, Gear, Walter, Greve, Thomas R., Hatziminaoglou, Evanthia, Hayward, Christopher C., Ivison, Rob J., Kawabe, Ryohei, Klaassen, Pamela, Knudsen, Kirsten K., Kohno, Kotaro, Koprowski, Maciej, Lagos, Claudia D. P., Magdis, Georgios E., Magnelli, Benjamin, McGee, Sean L., Michalowski, Michal, Mroczkowski, Tony, Noroozian, Omid, Oliver, Seb, Riechers, Dominik, Rujopakarn, Wiphu, Scott, Douglas, Serjeant, Stephen, Smith, Matthew W. L., Swinbank, Mark, Tamura, Yoichi, van der Werf, Paul, van Kampen, Eelco, Verma, Aprajita, Vieira, Joaquin, Wagg, Jeff, Walter, Fabian, Wang, Lingyu, Wootten, Al, Yun, Min S.
The Sloan Digital Sky Survey (SDSS) was revolutionary because of the extraordinary breadth and ambition of its optical imaging and spectroscopy. We argue that a 'sub-millimeter SDSS' - a sensitive large-area imaging+spectroscopic survey in the sub-mm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54deda2ca49dcbb89f6ee8de7d6c4065