Zobrazeno 1 - 10
of 551
pro vyhledávání: '"Wild, V"'
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
The role of mass and environment in the build up of the quenched galaxy population since cosmic noon
We conduct the first study of how the relative quenching probability of galaxies depends on environment over the redshift range $0.5 < z < 3$, using data from the UKIDSS Ultra-Deep Survey. By constructing the stellar mass functions for quiescent and
Externí odkaz:
http://arxiv.org/abs/2304.09169
Autor:
van der Wel, A., Noeske, K., Bezanson, R., Pacifici, C., Gallazzi, A., Franx, M., Muñoz-Mateos, J. C., Bell, E. F., Brammer, G., Charlot, S., Chauké, P., Labbé, I., Maseda, M. V., Muzzin, A., Rix, H.-W., Sobral, D., Sande, J. van de, Dokkum, P. G. van, Wild, V., Wolf, C.
The Large Early Galaxy Census (LEGA-C-16) is a Public Spectroscopic Survey of similar to 3200 K-band selected galaxies at redshifts z. =. 0.6 - 1.0 with stellar masses M-* > 10(10) M-circle dot, conducted with VIMOS on ESO's Very Large Telescope. The
Externí odkaz:
http://hdl.handle.net/10150/614714
http://arizona.openrepository.com/arizona/handle/10150/614714
http://arizona.openrepository.com/arizona/handle/10150/614714
Autor:
Carnall, A. C., McLure, R. J., Dunlop, J. S., McLeod, D. J., Wild, V., Cullen, F., Magee, D., Begley, R., Cimatti, A., Donnan, C. T., Hamadouche, M. L., Jewell, S. M., Walker, S.
The extremely rapid assembly of the earliest galaxies during the first billion years of cosmic history is a major challenge for our understanding of galaxy formation physics. The advent of JWST has exacerbated this issue by confirming the existence o
Externí odkaz:
http://arxiv.org/abs/2301.11413
Autor:
Carnall, A. C., McLeod, D. J., McLure, R. J., Dunlop, J. S., Begley, R., Cullen, F., Donnan, C. T., Hamadouche, M. L., Jewell, S. M., Jones, E. W., Pollock, C. L., Wild, V.
We report a robust sample of 10 massive quiescent galaxies at redshift, $z > 3$, selected using the first data from the JWST CEERS programme. Three of these galaxies are at $4 < z < 5$, constituting the best evidence to date for quiescent galaxies si
Externí odkaz:
http://arxiv.org/abs/2208.00986
Autor:
Garilli, B., McLure, R., Pentericci, L., Franzetti, P., Gargiulo, A., Carnall, A., Cucciati, O., Iovino, A., Amorin, R., Bolzonella, M., Bongiorno, A., Castellano, M., Cimatti, A., Cirasuolo, M., Cullen, F., Dunlop, J., Elbaz, D., Finkelstein, S., Fontana, A., Fontanot, F., Fumana, M., Guaita, L., Hartley, W., Jarvis, M., Juneau, S., Maccagni, D., McLeod, D., Nandra, K., Pompei, E., Pozzetti, L., Scodeggio, M., Talia, M., Calabro', A., Cresci, G., Fynbo, J. P. U., Hathi, N. P., Hibon, P., Koekemoer, A. M., Magliocchetti, M., Salvato, M., Vietri, G., Zamorani, G., Almaini, O., Balestra, I., Bardelli, S., Begley, R., Brammer, G., Bell, E. F., Bowler, R. A. A., Brusa, M., Buitrago, F., Caputi, C., Cassata, P., Charlot, S., Citro, A., Cristiani, S., Curtis-Lake, E., Dickinson, M., Fazio, G., Ferguson, H. C., Fiore, F., Franco, M., Georgakakis, A., Giavalisco, M., Grazian, A., Hamadouche, M., Jung, I., Kim, S., Khusanova, Y., Fevre, O. Le, Longhetti, M., Lotz, J., Mannucci, F., Maltby, D., Matsuoka, K., Mendez-Hernandez, H., Mendez-Abreu, J., Mignoli, M., Moresco, M., Nonino, M., Pannella, M., Papovich, C., Popesso, P., Roberts-Borsani, G., Rosario, D. J., Saldana-Lopez, A., Santini, P., Saxena, A., Schaerer, D., Schreiber, C., Stark, D., Tasca, L. A. M., Thomas, R., Vanzella, E., Wild, V., Williams, C., Zucca, E.
Publikováno v:
A&A 647, A150 (2021)
VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 208
Externí odkaz:
http://arxiv.org/abs/2101.07645
Autor:
Maiolino, R., Cirasuolo, M., Afonso, J., Bauer, F. E., Bowler, R., Cucciati, O., Daddi, E., De Lucia, G., Evans, C., Flores, H., Gargiulo, A., Garilli, B., Jablonka, P., Jarvis, M., Kneib, J. -P., Lilly, S., Looser, T., Magliocchetti, M., Man, Z., Mannucci, F., Maurogordato, S., McLure, R. J., Norberg, P., Oesch, P., Oliva, E., Paltani, S., Pappalardo, C., Peng, Y., Pentericci, L., Pozzetti, L., Renzini, A., Rodrigues, M., Royer, F., Serjeant, S., Vanzi, L., Wild, V., Zamorani, G.
Publikováno v:
The Messenger, vol. 180, 2020, p. 24-29
The MOONS instrument possesses an exceptional combination of large multiplexing, high sensitivity, broad simultaneous spectral coverage (from optical to near-infrared bands), large patrol area and high fibre density. These properties provide the unpr
Externí odkaz:
http://arxiv.org/abs/2009.00644
Autor:
Asari, N. Vale, Wild, V., de Amorim, A. L., Werle, A., Zheng, Y., Kennicutt, R., Johnson, B. D., Galametz, M., Pellegrini, E. W., Klessen, R. S., Reissl, S., Glover, S. C. O., Rahner, D.
The H$\alpha$ and H$\beta$ emission line luminosities measured in a single integrated spectrum are affected in non-trivial ways by point-to-point variations in dust attenuation in a galaxy. This work investigates the impact of this variation when est
Externí odkaz:
http://arxiv.org/abs/2007.05544
Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
Autor:
Carnall, A. C., Walker, S., McLure, R. J., Dunlop, J. S., McLeod, D. J., Cullen, F., Wild, V., Amorin, R., Bolzonella, M., Castellano, M., Cimatti, A., Cucciati, O., Fontana, A., Gargiulo, A., Garilli, B., Jarvis, M. J., Pentericci, L., Pozzetti, L., Zamorani, G., Calabro, A., Hathi, N. P., Koekemoer, A. M.
We present a sample of 151 massive ($M_* > 10^{10}\mathrm{M_\odot}$) quiescent galaxies at $2 < z < 5$, based on a sophisticated Bayesian spectral energy distribution fitting analysis of the CANDELS UDS and GOODS-South fields. Our sample includes a r
Externí odkaz:
http://arxiv.org/abs/2001.11975
Autor:
Falcón-Barroso, J., van de Ven, G., Lyubenova, M., Méndez-Abreu, J., Aguerri, J. A. L., García-Lorenzo, B., Bekeraité, S., Sánchez, S. F., Husemann, B., García-Benito, R., Delgado, R. M. González, Mast, D., Walcher, C. J., Zibetti, S., Zhu, L., Barrera-Ballesteros, J. K., Galbany, L., Sánchez-Blázquez, P., Singh, R., Bosch, R. C. E. van den, Wild, V., Bland-Hawthorn, J., Fernandes, R. Cid, de Lorenzo-Cáceres, A., Gallazzi, A., Marino, R. A., Márquez, I., Peletier, R. F., Pérez, E., Pérez, I., Roth, M. M., Rosales-Ortega, F. F., Ruiz-Lara, T., Wisotzki, L., Ziegler, B.
Publikováno v:
A&A 632, A59 (2019)
[Abridged] We present the apparent stellar angular momentum of 300 galaxies across the Hubble sequence, using integral-field spectroscopic data from the CALIFA survey. Adopting the same $\lambda_\mathrm{R}$ parameter previously used to distinguish be
Externí odkaz:
http://arxiv.org/abs/1910.06236