Zobrazeno 1 - 10
of 592
pro vyhledávání: '"Theuns T"'
Autor:
Jara-Ferreira, F., Tissera, P. B., Sillero, E., Rosas-Guevara, Y., Pedrosa, S. E., De Rossi, M. E., Theuns, T., Bignone, L.
The variations in metallicity and spatial patterns within star-forming regions of galaxies result from diverse physical processes unfolding throughout their evolutionary history, with a particular emphasis in recent events. Analysing MaNGA and \texts
Externí odkaz:
http://arxiv.org/abs/2403.06836
Observed and simulated galaxies exhibit correlations between stellar mass, metallicity and morphology. We use the EAGLE cosmological simulation to examine the origin of these correlations for galaxies in the stellar mass range $10^9~\rm{M_\odot} \leq
Externí odkaz:
http://arxiv.org/abs/2203.16326
Autor:
Katsianis, A., Gonzalez, V, Barrientos, D., Yang, X., Lagos, C. D. P., Schaye, J., Camps, P., Trčka, A., Baes, M., Stalevski, M., Blanc, G. A., Theuns, T.
There is a severe tension between the observed star formation rate (SFR) - stellar mass (${\rm M}_{\star}$) relations reported by different authors at $z = 1-4$. In addition, the observations have not been successfully reproduced by state-of-the-art
Externí odkaz:
http://arxiv.org/abs/2001.06025
Autor:
Gillman, S., Tiley, A. L., Swinbank, A. M., Harrison, C. M., Smail, Ian, Dudzevičiūtė, U., Sharples, R. M., Cortese, L., Obreschkow, D., Bower, R. G., Theuns, T., Cirasuolo, M., Fisher, D. B., Glazebrook, K., Ibar, Edo, Mendel, J. Trevor, Sweet, Sarah M.
We present an analysis of the gas dynamics of star-forming galaxies at z~1.5 using data from the KMOS Galaxy Evolution Survey (KGES). We quantify the morphology of the galaxies using $HST$ CANDELS imaging parametrically and non-parametrically. We com
Externí odkaz:
http://arxiv.org/abs/1911.12375
The metallicity of star-forming gas in galaxies from the EAGLE simulations increases with stellar mass. Here we investigate whether the scatter around this relation correlates with morphology and/or stellar kinematics. At redshift $z=0$, galaxies wit
Externí odkaz:
http://arxiv.org/abs/1911.09571
Autor:
Fossati, M., Fumagalli, M., Lofthouse, E. K., D'Odorico, V., Lusso, E., Cantalupo, S., Cooke, R. J., Cristiani, S., Haardt, F., Morris, S. L., Peroux, C., Prichard, L. J., Rafelski, M., Smail, I., Theuns, T.
We present the goals, design, and first results of the MUSE Ultra Deep Field (MUDF) survey, a large programme using the Multi Unit Spectroscopic Explorer (MUSE) instrument at the ESO Very Large Telescope. The MUDF survey is collecting ~ 150 hours on-
Externí odkaz:
http://arxiv.org/abs/1909.04672
Autor:
Gillman, S., Swinbank, A. M., Tiley, A. L., Harrison, C. M., Smail, Ian, Dudzevičiūtė, U., Sharples, R. M., Best, P. N., Bower, R. G., Cochrane, R., Fisher, D., Geach, J. E., Glazebrook, K., Ibar, Edo, Molina, J., Obreschkow, D., Schaller, M., Sobral, D., Sweet, S., Trayford, J. W., Theuns, T.
Publikováno v:
MNRAS 2019,486,175G
We present adaptive optics assisted integral field spectroscopy of 34 star-forming galaxies at $z$ = 0.8-3.3 selected from the HiZELS narrow-band survey. We measure the kinematics of the ionised interstellar medium on $\sim$1 kpc scales, and show tha
Externí odkaz:
http://arxiv.org/abs/1903.05148
Autor:
Lusso, E., Fumagalli, M., Fossati, M., Mackenzie, R., Bielby, R. M., Battaia, F. Arrigoni, Cantalupo, S., Cooke, R., Cristiani, S., Dayal, P., D'Odorico, V., Haardt, F., Lofthouse, E., Morris, S., Peroux, C., Prichard, L., Rafelski, M., Simcoe, R., Swinbank, A. M., Theuns, T.
We present first results from Multi Unit Spectroscopic Explorer (MUSE) observations at the Very Large Telescope in the MUSE Ultra Deep Field (MUDF), a $\approx 1.2\times 1.4$ arcmin$^2$ region for which we are collecting $\approx$200 hours of integra
Externí odkaz:
http://arxiv.org/abs/1903.00483
Autor:
Tiley, Alfred L., Swinbank, A. M., Harrison, C. M., Smail, Ian, Turner, O. J., Schaller, M., Stott, J. P., Sobral, D., Theuns, T., Sharples, R. M., Gillman, S., Bower, R. G., Bunker, A. J., Best, P., Richard, J., Bacon, Roland, Bureau, M., Cirasuolo, M., Magdis, G.
We analyse maps of the spatially-resolved nebular emission of $\approx$1500 star-forming galaxies at $z\approx0.6$-$2.2$ from deep KMOS and MUSE observations to measure the average shape of their rotation curves. We use these to test claims for decli
Externí odkaz:
http://arxiv.org/abs/1811.05982
Autor:
Scholtz, J., Alexander, D. M., Harrison, C. M., Rosario, D. J., McAlpine, S., Mullaney, J. R, Stanley, F., Simpson, J., Theuns, T., Bower, R. G., Hickox, R. C., Santini, P., Swinbank, A. M.
We present sensitive 870$\mu$m continuum measurements from our ALMA programmes of 114 X-ray selected AGN in the CDF-S and COSMOS fields. We use these observations in combination with data from Spitzer and Herschel to construct a sample of 86 X-ray se
Externí odkaz:
http://arxiv.org/abs/1712.02708