Zobrazeno 1 - 10
of 1 097
pro vyhledávání: '"Bower, R"'
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:
Masini, A., Hickox, R. C., Carroll, C. M., Aird, J., Alexander, D. M., Assef, R. J., Bower, R., Brodwin, M., Brown, M. J. I., Chatterjee, S., Chen, C. -T. J., Dey, A., DiPompeo, M. A., Duncan, K. J., Eisenhardt, P. R. M., Forman, W. R., Gonzalez, A. H., Goulding, A. D., Hainline, K. N., Jannuzi, B. T., Jones, C., Kochanek, C. S., Kraft, R., Lee, K. -S., Miller, E. D., Mullaney, J., Myers, A. D., Ptak, A., Stanford, A., Stern, D., Vikhlinin, A., Wake, D. A., Murray, S. S.
We present a new, ambitious survey performed with the Chandra X-ray Observatory of the 9.3 deg$^2$ Bo\"otes field of the NOAO Deep Wide-Field Survey. The wide field probes a statistically representative volume of the Universe at high redshift. The Ch
Externí odkaz:
http://arxiv.org/abs/2009.03317
Autor:
Jackson, Thomas M., Rosario, D. J., Alexander, D. M., Scholtz, J., McAlpine, Stuart, Bower, R. G.
In this paper we present data from 72 low redshift, hard X-ray selected AGN taken from the {\it Swift}-BAT 58 month catalogue. We utilise spectral energy distribution fitting to the optical to IR photometry in order to estimate host galaxy properties
Externí odkaz:
http://arxiv.org/abs/2008.05115
Autor:
Stott, J. P., Bielby, R. M., Cullen, F., Burchett, J. N., Tejos, N., Fumagalli, M., Crain, R. A., Morris, S. L., Amos, N., Bower, R. G., Prochaska, J. X.
Publikováno v:
2020, MNRAS, 497, 3083
We demonstrate that the UV brightest quasars at z=1-2 live in overdense environments. This is based on an analysis of deep Hubble Space Telescope WFC3 G141 grism spectroscopy of the galaxies along the lines-of-sight to UV luminous quasars in the reds
Externí odkaz:
http://arxiv.org/abs/2006.07384
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
Autor:
Cooke, E. A., Smail, Ian, Stach, S. M., Swinbank, A. M., Bower, R. G., Chen, Chian-Chou, Koyama, Y., Thomson, A. P.
We analyse 850um continuum observations of eight massive X-ray detected galaxy clusters at z~0.8-1.6 taken with SCUBA-2 on the James Clerk Maxwell Telescope. We find an average overdensity of 850um-selected sources of a factor of 4+/-2 per cluster wi
Externí odkaz:
http://arxiv.org/abs/1904.01582
Autor:
Pawlik, M. M., McAlpine, S., Trayford, J. W., Wild, V., Bower, R., Crain, R. A., Schaller, M., Schaye, J.
About 35 years ago a class of galaxies with unusually strong Balmer absorption lines and weak emission lines was discovered in distant galaxy clusters. These objects, alternatively referred to as post-starburst, E+A or k+a galaxies, are now known to
Externí odkaz:
http://arxiv.org/abs/1903.11050
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:
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:
Tiley, A. L., Bureau, M., Cortese, L., Harrison, C. M., Johnson, H. L., Stott, J. P., Swinbank, A. M., Smail, I., Sobral, D., Bunker, A. J., Glazebrook, K., Bower, R. G., Obreschkow, D., Bryant, J. J., Jarvis, M. J., Bland-Hawthorn, J., Magdis, G., Medling, A. M., Sweet, S. M., Tonini, C., Turner, O. J., Sharples, R. M., Croom, S. M., Goodwin, M., Konstantopoulos, I. S., Lorente, N. P. F., Lawrence, J. S., Mould, J., Owers, M. S., Richards, S. N.
We construct Tully-Fisher relations (TFRs), from large samples of galaxies with spatially-resolved H$\alpha$ emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One Spectroscopic Survey (KROSS) at $z\approx1$. We compare these to
Externí odkaz:
http://arxiv.org/abs/1810.07202