Zobrazeno 1 - 10
of 56
pro vyhledávání: '"U Dudzevičiūtė"'
Autor:
Cheng-Lin Liao, Chian-Chou Chen, Wei-Hao Wang, Ian Smail, Y. Ao, S. C. Chapman, U. Dudzevičiūtė, M. Frias Castillo, Minju M. Lee, Stephen Serjeant, A. M. Swinbank, Dominic J. Taylor, Hideki Umehata, Y. Zhao
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 2, p 226 (2024)
We report the physical properties of the 18 brightest ( S _870 _μ _m = 12.4–19.2 mJy) and not strongly lensed 870 μ m–selected dusty star-forming galaxies (DSFGs), also known as submillimeter galaxies (SMGs), in the COSMOS field. This sample is
Externí odkaz:
https://doaj.org/article/c19a79c85fcb4589b4ef9370bde96cc5
Akademický článek
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Autor:
Juan Molina, David Sobral, Ian Smail, Edo Ibar, A. M. Swinbank, P. N. Best, Cheng Cheng, Rachel Cochrane, U. Dudzevičiūtė
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2021, Vol.503(2), pp.2622-2638 [Peer Reviewed Journal]
Cochrane, R K, Best, P N, Smail, I, Ibar, E, Cheng, C, Swinbank, A M, Molina, J, Sobral, D & Dudzeviciute, U 2021, ' Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 2, pp. 2622-2638 . https://doi.org/10.1093/mnras/stab467
Cochrane, R K, Best, P N, Smail, I, Ibar, E, Cheng, C, Swinbank, A M, Molina, J, Sobral, D & Dudzeviciute, U 2021, ' Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales ', Monthly Notices of the Royal Astronomical Society, vol. 503, no. 2, pp. 2622-2638 . https://doi.org/10.1093/mnras/stab467
We present ~0.15'' spatial resolution imaging of SHiZELS-14, a massive (M*~10^11 M_sol), dusty, star-forming galaxy at z=2.24. Our rest-frame ~1kpc-scale, matched-resolution data comprise four different widely used tracers of star formation: the H-al
Akademický článek
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Autor:
S Gillman, A Puglisi, U Dudzevičiūtė, A M Swinbank, A L Tiley, C M Harrison, J Molina, R M Sharples, R G Bower, M Cirasuolo, Edo Ibar, D Obreschkow
Publikováno v:
Gillman, S, Puglisi, A, Dudzevičiūtė, U, Swinbank, A M, Tiley, A L, Harrison, C M, Molina, J, Sharples, R M, Bower, R G, Cirasuolo, M, Ibar, E & Obreschkow, D 2022, ' The resolved chemical abundance properties within the interstellar medium of star-forming galaxies at z≈1.5 ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 3, pp. 3480–3499 . https://doi.org/10.1093/mnras/stac580
Monthly Notices of the Royal Astronomical Society, 2022, Vol.512(3), pp.3480-3499 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 2022, Vol.512(3), pp.3480-3499 [Peer Reviewed Journal]
We exploit the unprecedented depth of integral field data from the KMOS Ultra-deep Rotational Velocity Survey (KURVS) to analyse the strong (Hα) and forbidden ([N ii], [S ii]) emission line ratios in 22 main-sequence galaxies at $z\, \approx \, 1.5$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a66884fca60fbd2b55c69d1982a5637
https://orbit.dtu.dk/en/publications/8910dc12-e833-4f28-bd8d-f637dd08fab9
https://orbit.dtu.dk/en/publications/8910dc12-e833-4f28-bd8d-f637dd08fab9
Akademický článek
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Autor:
Alfred L. Tiley, Ian Smail, Scott M. Croom, Steven Gillman, A. M. Swinbank, Christopher Harrison, Ray M. Sharples, Danail Obreschkow, U. Dudzevičiūtė, Luca Cortese, Annagrazia Puglisi
Publikováno v:
Tiley, A L, Gillman, S, Cortese, L, Swinbank, A M, Dudzevičiūtė, U, Harrison, C M, Smail, I, Obreschkow, D, Croom, S M, Sharples, R M & Puglisi, A 2021, ' The KMOS galaxy evolution survey (KGES): the angular momentum of star-forming galaxies over the last ≈10 Gyr ', Monthly Notices of the Royal Astronomical Society, vol. 506, pp. 323–342 . https://doi.org/10.1093/mnras/stab1692
Monthly Notices of the Royal Astronomical Society, 2021, Vol.506(1), pp.323-342 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 2021, Vol.506(1), pp.323-342 [Peer Reviewed Journal]
We present the KMOS Galaxy Evolution Survey (KGES), a $K$-band Multi-Object Spectrograph (KMOS) study of the H$\alpha$ and [NII] emission from 288 $K$ band-selected galaxies at $1.2 \lesssim z \lesssim 1.8$, with stellar masses in the range $\log_{10
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c68284389fdbeddbd2821537f70f696c
http://arxiv.org/abs/2106.05511
http://arxiv.org/abs/2106.05511
Autor:
Axel Weiss, Fang Xia An, Andrew Blain, Duncan Farrah, Douglas Scott, U. Dudzevičiūtė, James Dunlop, Michał J. Michałowski, J. M. Simpson, Bitten Gullberg, P. van der Werf, Omar Almaini, S. M. Stach, V. Arumugam, E. A. Cooke, Jacqueline Hodge, Takamitsu Miyaji, Scott Chapman, Julie Wardlow, Dale D. Kocevski, A. M. Swinbank, James E. Geach, C. J. Conselice, Chian-Chou Chen, E. da Cunha, Alasdair Thomson, Rob Ivison, Kristen Coppin, Ian Smail
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2019, Vol.487(4), pp.4648-4668 [Peer Reviewed Journal]
We present the catalogue and properties of sources in AS2UDS, an 870-$\mu$m continuum survey with the Atacama Large Millimetre/sub-millimetre Array (ALMA) of 716 single-dish sub-millimetre sources detected in the UKIDSS/UDS field by the SCUBA-2 Cosmo
Publikováno v:
Proceedings of the International Astronomical Union. 15:274-279
The spatial distribution of the dust and stars contains crucial information about the evolutionary pathways of galaxies. We present results of our study combing high-resolution ALMA and HST observations of z ∼ 2 bright sub-millimeter galaxies (SMGs
Autor:
A. M. Swinbank, Fabian Walter, Rob Ivison, Jacqueline Hodge, Douglas Scott, Jack Birkin, Julie Wardlow, Alasdair Thomson, U. Dudzevičiūtė, Chian-Chou Chen, S. M. Stach, Ian Smail, Omar Almaini, Chris Simpson, P. van der Werf, S. Ikarashi, James E. Geach, B. Gullberg, Scott Chapman
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2021, Vol.502(3), pp.3426-3435 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 502(3), 3426-3435
Monthly Notices of the Royal Astronomical Society, 502(3), 3426-3435
We analyse a robust sample of 30 near-infrared-faint (K>25.3, 5 sigma) submillimetre galaxies selected across a 0.96 deg^2 field, to investigate their properties and the cause of their lack of detectable optical/near-infrared emission. Our analysis e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2415029926375a6e5d10a8e65d86738f
https://doi.org/10.1093/mnras/stab283
https://doi.org/10.1093/mnras/stab283