Zobrazeno 1 - 10
of 3 585
pro vyhledávání: '"Mcleod, D."'
The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
Autor:
Carnall, A. C., Cullen, F., McLure, R. J., McLeod, D. J., Begley, R., Donnan, C. T., Dunlop, J. S., Shapley, A. E., Rowlands, K., Almaini, O., Arellano-Córdova, K. Z., Barrufet, L., Cimatti, A., Ellis, R. S., Grogin, N. A., Hamadouche, M. L., Illingworth, G. D., Koekemoer, A. M., Leung, H. -H., Lovell, C. C., Pérez-González, P. G., Santini, P., Stanton, T. M., Wild, V.
We report ultra-deep, medium-resolution spectroscopic observations for 4 quiescent galaxies with log$_{10}(M_*/\mathrm{M_\odot})>11$ at $3 < z < 5$. These data were obtained with JWST NIRSpec as part of the Early eXtragalactic Continuum and Emission
Externí odkaz:
http://arxiv.org/abs/2405.02242
Autor:
Stanton, T. M., Cullen, F., McLure, R. J., Shapley, A. E., Arellano-Córdova, K. Z., Begley, R., Amorín, R., Barrufet, L., Calabrò, A., Carnall, A. C., Cirasuolo, M., Dunlop, J. S., Donnan, C. T., Hamadouche, M. L., Liu, F. -Y., McLeod, D. J., Pentericci, L., Pozzetti, L., Sanders, R. L., Scholte, D., Topping, M. W.
We present determinations of the gas-phase and stellar metallicities of a sample of 65 star-forming galaxies at $z \simeq 3.5$ using rest-frame far-ultraviolet (FUV) spectroscopy from the VANDELS survey in combination with follow-up rest-frame optica
Externí odkaz:
http://arxiv.org/abs/2405.00774
Autor:
Barrufet, L., Oesch, P., Marques-Chaves, R., Arellano-Cordova, K., Baggen, J. F. W., Carnall, A. C., Cullen, F., Dunlop, J. S., Gottumukkala, R., Fudamoto, Y., Illingworth, G. D., Magee, D., McLure, R. J., McLeod, D. J., Michałowski, M. J., Stefanon, M., van Dokkum, P. G., Weibel, A.
The advent of the JWST has revolutionised our understanding of high-redshift galaxies. In particular, the NIRCam instrument on-board JWST has revealed a population of Hubble Space Telescope (HST)-dark galaxies that had previously evaded optical detec
Externí odkaz:
http://arxiv.org/abs/2404.08052
Autor:
Koprowski, M. P., Wijesekera, J. V., Dunlop, J. S., McLeod, D. J., Michałowski, M. J., Lisiecki, K., McLure, R. J.
We present a new determination of the star-forming main sequence (MS), obtained through stacking 100k K-band-selected galaxies in the far-IR Herschel and James Clerk Maxwell Telescope (JCMT) imaging. By fitting the dust emission curve to the stacked
Externí odkaz:
http://arxiv.org/abs/2403.06575
Autor:
Donnan, C. T., McLure, R. J., Dunlop, J. S., McLeod, D. J., Magee, D., Arellano-Córdova, K. Z., Barrufet, L., Begley, R., Bowler, R. A. A., Carnall, A. C., Cullen, F., Ellis, R. S., Fontana, A., Illingworth, G. D., Grogin, N. A., Hamadouche, M. L., Koekemoer, A. M., Liu, F. -Y., Mason, C., Santini, P., Stanton, T. M.
We present a new determination of the evolving galaxy UV luminosity function (LF) over the redshift range $8.5
Externí odkaz:
http://arxiv.org/abs/2403.03171
Autor:
Varadaraj, R. G., Bowler, R. A. A., Jarvis, M. J., Adams, N. J., Choustikov, N., Koekemoer, A. M., Carnall, A. C., McLeod, D. J., Dunlop, J. S., Donnan, C. T., Grogin, N. A.
We use data from the JWST Public Release IMaging for Extragalactic Research (PRIMER) survey to measure the size scaling relations of 1668 rest-frame UV-bright Lyman-break galaxies (LBGs) at $z=3-5$ with stellar masses $\mathrm{log}_{10}(M_{\star}/M_{
Externí odkaz:
http://arxiv.org/abs/2401.15971
Autor:
Cullen, F., McLeod, D. J., McLure, R. J., Dunlop, J. S., Donnan, C. T., Carnall, A. C., Keating, L. C., Magee, D., Arellano-Cordova, K. Z., Bowler, R. A. A., Begley, R., Flury, S. R., Hamadouche, M. L., Stanton, T. M.
We present an analysis of the ultraviolet (UV) continuum slopes ($\beta$) for a sample of $172$ galaxy candidates at $8 < z_{\mathrm{phot}} < 16$ selected from a combination of JWST NIRCam imaging and COSMOS/UltraVISTA ground-based near-infrared imag
Externí odkaz:
http://arxiv.org/abs/2311.06209
Autor:
Talia, M., Schreiber, C., Garilli, B., Pentericci, L., Pozzetti, L., Zamorani, G., Cullen, F., Moresco, M., Calabrò, A., Castellano, M., Fynbo, J. P. U., Guaita, L., Marchi, F., Mascia, S., McLure, R., Mignoli, M., Pompei, E., Vanzella, E., Bongiorno, A., Vietri, G., Amorín, R. O., Bolzonella, M., Carnall, A. C., Cimatti, A., Cresci, G., Cristiani, S., Cucciati, O., Dunlop, J. S., Fontanot, F., Franzetti, P., Gargiulo, A., Hamadouche, M. L., Hathi, N. P., Hibon, P., Iovino, A., Koekemoer, A. M., Mannucci, F., McLeod, D. J., Saldana-Lopez, A.
Publikováno v:
A&A 678, A25 (2023)
VANDELS is a deep spectroscopic survey, performed with the VIMOS instrument at VLT, aimed at studying in detail the physical properties of high-redshift galaxies. VANDELS targeted about 2100 sources at 1
Externí odkaz:
http://arxiv.org/abs/2309.14436
Autor:
Begley, R., Cullen, F., McLure, R. J., Shapley, A. E., Dunlop, J. S., Carnall, A. C., McLeod, D. J., Donnan, C. T., Hamadouche, M. L., Stanton, T. M.
We present a study of the connection between the escape fraction of Lyman-alpha (Ly$\alpha$) and Lyman-continuum (LyC) photons within a sample of N=152 star-forming galaxies selected from the VANDELS survey at $3.85
Externí odkaz:
http://arxiv.org/abs/2306.03916
Autor:
McLeod, D. J., Donnan, C. T., McLure, R. J., Dunlop, J. S., Magee, D., Begley, R., Carnall, A. C., Cullen, F., Ellis, R. S., Hamadouche, M. L., Stanton, T. M.
We present a new determination of the evolving galaxy UV luminosity function (LF) over the redshift range $9.5250$ arcmin$^2$) data set of JWST NIRCam near-infrared imaging assembled from thirteen public JWST surveys.
Externí odkaz:
http://arxiv.org/abs/2304.14469