Zobrazeno 1 - 10
of 763
pro vyhledávání: '"Swinbank, A. M."'
Autor:
Dutta, Rajeshwari, Fumagalli, Michele, Fossati, Matteo, Rafelski, Marc, Revalski, Mitchell, Battaia, Fabrizio Arrigoni, D'Odorico, Valentina, Peroux, Celine, Prichard, Laura J., Swinbank, A. M.
We characterize, for the first time, the average extended emission in multiple lines ([OII], [OIII], and Hbeta) around a statistical sample of 560 galaxies at z~0.25-0.85. By stacking the Multi Unit Spectroscopic Explorer (MUSE) 3D data from two larg
Externí odkaz:
http://arxiv.org/abs/2409.02182
Autor:
Klutse, D. Y., Hilton, M., Heywood, I., Smail, I., Swinbank, A. M., Knowles, K., Sikhosana, S. P.
We present the first detailed radio study of the galaxy cluster XMMXCS J2215.9-1738 at $z$ = 1.46 using MeerKAT $L$-band (1.3 GHz) observations. We combine our radio observation with archival optical and infrared data to investigate the star formatio
Externí odkaz:
http://arxiv.org/abs/2407.03667
Autor:
Gillman, Steven, Smail, Ian, Gullberg, Bitten, Swinbank, A. M., Vijayan, Aswin P., Lee, Minju, Brammer, Gabe, Dudzevičiūtė, U., Greve, Thomas R., Almaini, Omar, Brinch, Malte, Chapman, Scott C., Chen, Chian-Chou, Ikarashi, Soh, Matsuda, Yuichi, Wang, Wei-Hao, Walter, Fabian, van der Werf, Paul P.
We present an analysis of the JWST NIRCam and MIRI morphological properties of 80 massive ($\log_{10}(M_\ast[M_{\odot}])$=11.2$\pm$0.1) dusty star-forming galaxies at $z$$=$2.7$^{+1.2}_{-0.7}$, identified as sub-millimetre galaxies (SMGs) by ALMA, th
Externí odkaz:
http://arxiv.org/abs/2406.03544
Autor:
Castillo, Marta Frias, Rybak, Matus, Hodge, Jacqueline A., Van der Werk, Paul, Smail, Ian, Butterworth, Joshua, Jansen, Jasper, Topkaras, Theodoros, Chen, Chian-Chou, Chapman, Scott C., Weiss, Axel, Algera, Hiddo, Birkin, Jack E., da Cunha, Elisabete, Chen, Jianhang, Dannerbauer, Helmut, Jiménez-Andrade, E. F., Ikarashi, Soh, Liao, Cheng-Lin, Murphy, Eric J., Swinbank, A. M., Walter, Fabian, Rivera, Gabriela Calistro, Ivison, R. J., Lagos, Claudia del P.
The CO(1--0) and [\ion{C}{1}](1--0) emission lines are well-established tracers of cold molecular gas mass in local galaxies. At high redshift, where the interstellar medium (ISM) is likely to be denser, there have been limited direct comparisons of
Externí odkaz:
http://arxiv.org/abs/2404.05596
Autor:
Amvrosiadis, A., Wardlow, J. L., Birkin, J. E., Smail, I., Swinbank, A. M., Nightingale, J., Bertoldi, F., Brandt, W. N., Casey, C. M., Chapman, S. C., Chen, C. -C., Cox, P., da Cunha, E., Dannerbauer, H., Dudzevičiūtė, U., Gullberg, B., Hodge, J. A., Knudsen, K. K., Menten, K., Walter, F., van der Werf, P.
We present a new method for modelling the kinematics of galaxies from interferometric observations by performing the optimization of the kinematic model parameters directly in visibility-space instead of the conventional approach of fitting velocity
Externí odkaz:
http://arxiv.org/abs/2312.08959
Autor:
Smail, Ian, Dudzeviciute, Ugne, Gurwell, Mark, Fazio, Giovanni G., Willner, S. P., Swinbank, A. M., Arumugam, Vinodiran, Summers, Jake, Cohen, Seth H., Jansen, Rolf A., Windhorst, Rogier A., Meena, Ashish, Zitrin, Adi, Keel, William C., Coe, Dan, Conselice, Christopher J., D'Silva, Jordan C. J., Driver, Simon P., Frye, Brenda, Grogin, Norman A., Koekemoer, Anton M., Marshall, Madeline A., Nonino, Mario, Pirzkal, Nor, Robotham, Aaron, Rutkowski, Michael J., Ryan Jr., Russell E., Tompkins, Scott, Willmer, Christopher N. A., Yan, Haojing, Broadhurst, Thomas J., Cheng, Cheng, Diego, Jose M., Kamieneski, Patrick, Yun, Min
We present a multi-wavelength analysis using SMA, JCMT, NOEMA, JWST, HST, and SST of two dusty strongly star-forming galaxies, 850.1 and 850.2, seen through the massive cluster lens A1489. These SMA-located sources both lie at z=4.26 and have bright
Externí odkaz:
http://arxiv.org/abs/2306.16039
Autor:
Dunlop, J. S., McLure, R. J., Biggs, A. D., Geach, J. E., Michałowski, M. J., Ivison, R. J., Rujopakarn, W., van Kampen, E., Kirkpatrick, A., Pope, A., Scott, D., Swinbank, A. M., Targett, T. A., Aretxaga, I., Austermann, J. E., Best, P. N., Bruce, V. A., Chapin, E. L., Charlot, S., Cirasuolo, M., Coppin, K., Ellis, R. S., Finkelstein, S. L., Hayward, C. C., Hughes, D. H., Ibar, E., Jagannathan, P., Khochfar, S., Koprowski, M. P., Narayanan, D., Nyland, K., Papovich, C., Peacock, J. A., Rieke, G. H., Robertson, B., Vernstrom, T., Werf, P. P. van der, Wilson, G. W., Yun, M.
We present the results of the first, deep Atacama Large Millimeter Array ( ALMA) imaging covering the full similar or equal to 4.5 arcmin(2) of the Hubble Ultra Deep Field ( HUDF) imaged with Wide Field Camera 3/IR on HST. Using a 45-pointing mosaic,
Externí odkaz:
http://hdl.handle.net/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
Autor:
Rujopakarn, W., Dunlop, J. S., Rieke, G. H., Ivison, R. J., Cibinel, A., Nyland, K., Jagannathan, P., Silverman, J. D., Alexander, D. M., Biggs, A. D., Bhatnagar, S., Ballantyne, D. R., Dickinson, M., Elbaz, D., Geach, J. E., Hayward, C. C., Kirkpatrick, A., McLure, R. J., Michałowski, M. J., Miller, N. A., Narayanan, D., Owen, F. N., Pannella, M., Papovich, C., Pope, A., Rau, U., Robertson, B. E., Scott, D., Swinbank, A. M., Werf, P. van der, Kampen, E. van, Weiner, B. J., Windhorst, R. A.
We present; 0 4 resolution extinction-independent distributions of star formation and dust in 11 star-forming galaxies (SFGs) at z. =. 1.3-3.0. These galaxies are selected from sensitive blank-field surveys of the 2 x 2' Hubble Ultra-Deep Field at gi
Externí odkaz:
http://hdl.handle.net/10150/624030
http://arizona.openrepository.com/arizona/handle/10150/624030
http://arizona.openrepository.com/arizona/handle/10150/624030
Autor:
Birkin, Jack E., Puglisi, A., Swinbank, A. M., Smail, Ian, An, Fang Xia, Chapman, S. C., Chen, Chian-Chou, Conselice, C. J., Dudzevičiūtė, U., Farrah, D., Gullberg, B., Matsuda, Y., Schinnerer, E., Scott, D., Wardlow, J. L., van der Werf, P.
We present spatially resolved kinematics of 27 ALMA-identified dust-obscured star-forming galaxies (DSFGs) at $z\sim$1.3-2.6, as traced by H$\alpha$ emission using VLT/KMOS near-infrared integral field spectroscopy from the "KMOS-ALMA Observations of
Externí odkaz:
http://arxiv.org/abs/2301.05720
Autor:
Hyun, Minhee, Im, Myungshin, Smail, Ian R., Cotton, William D., Birkin, Jack E., Kikuta, Satoshi, Shim, Hyunjin, Willmer, Christopher N. A., Condon, James J., Windhorst, Rogier A., Cohen, Seth H., Jansen, Rolf A., Ly, Chun, Matsuda, Yuichi, Fazio, Giovanni G., Swinbank, A. M., Yan, Haojing
Publikováno v:
ApJS 264 19 (2023)
The James Webb Space Telescope Time-Domain Field (JWST-TDF) is an $\sim$14$'$ diameter field near the North Ecliptic Pole that will be targeted by one of the JWST Guaranteed Time Observations programs. Here, we describe our James Clerk Maxwell Telesc
Externí odkaz:
http://arxiv.org/abs/2301.02786