Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Dudzeviciute, U."'
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.
Publikováno v:
A&A 691, A299 (2024)
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:
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:
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:
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, Edo, Obreschkow, D.
We exploit the unprecedented depth of integral field data from the KMOS Ultra-deep Rotational Velocity Survey (KURVS) to analyse the strong (H$\alpha$) and forbidden ([NII], [SII]) emission line ratios in 22 main-sequence galaxies at $z\approx1.5$. U
Externí odkaz:
http://arxiv.org/abs/2202.12304
Autor:
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.
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:
http://arxiv.org/abs/2106.05511
Autor:
Stach, S. M., Smail, I., Amvrosiadis, A., Swinbank, A. M., Dudzevičiūtė, U., Geach, J. E., Almaini, O., Birkin, J. E., Chen, Chian-Chou, Conselice, C. J., Cooke, E. A., Coppin, K. E. K., Dunlop, J. S., Farrah, D., Ikarashi, S., Ivison, R. J., Wardlow, J. L.
We present an analysis of the spatial clustering of a large sample of high-resolution, interferometically identified, submillimetre galaxies (SMGs). We measure the projected cross-correlation function of ~350 SMGs in the UKIDSS Ultra Deep-Survey Fiel
Externí odkaz:
http://arxiv.org/abs/2102.12510
Autor:
Cochrane, R. K., Best, P. N., Smail, I., Ibar, E., Swinbank, A. M., Molina, J., Sobral, D., Dudzeviciute, U.
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
Externí odkaz:
http://arxiv.org/abs/2102.07791
Autor:
Gillman, S., Tiley, A. L., Swinbank, A. M., Dudzevičiūtė, U., Sharples, R. M., Smail, Ian, Harrison, C. M., Bunker, Andrew J., Bureau, Martin, Cirasuolo, M., Magdis, Georgios E., Mendel, Trevor, Stott, John P.
We present an analysis of the chemical abundance properties of $\approx$650 star-forming galaxies at $z \approx0.6-1.8$. Using integral-field observations from the $K$-band Multi-Object Spectrograph (KMOS), we quantify the [NII]/H$\alpha$ emission-li
Externí odkaz:
http://arxiv.org/abs/2010.15847
Autor:
Dudzevičiūtė, U., Smail, I., Swinbank, A. M., Lim, C. -F., Wang, W. -H., Simpson, J. M., Ao, Y., Chapman, S. C., Chen, C. -C., Clements, D., Dannerbauer, H., Ho, L. C., Hwang, H. S., Koprowski, M., Lee, C. -H., Scott, D., Shim, H., Shirley, R., Toba, Y.
We analyse the physical properties of 121 SNR $\geq$ 5 sub-millimetre galaxies (SMGs) from the STUDIES 450-$\mu$m survey. We model their UV-to-radio spectral energy distributions using MAGPHYS+photo-$z$ and compare the results to similar modelling of
Externí odkaz:
http://arxiv.org/abs/2010.06605
Autor:
Smail, Ian, Dudzevičiūtė, U., Stach, S. M., Almaini, O., Birkin, J. E., Chapman, S. C., Chen, Chian-Chou, Geach, J. E., Gullberg, B., Hodge, J. A., Ikarashi, S., Ivison, R. J., Scott, D., Simpson, Chris, Swinbank, A. M., Thomson, A. P., Walter, F., Wardlow, J. L., van der Werf, P.
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:
http://arxiv.org/abs/2010.02250