Zobrazeno 1 - 10
of 876
pro vyhledávání: '"Tasca L"'
Autor:
Devereaux, T., Cassata, P., Ibar, E., Accard, C., Guillaume, C., Béthermin, M., Dessauges-Zavadsky, M., Faisst, A., Jones, G. C., Zanella, A., Bardelli, S., Boquien, M., D'Onghia, E., Giavalisco, M., Ginolfi, M., Gobat, R., Hayward, C. C., Koekemoer, A. M., Lemaux, B., Magdis, G., Mendez-Hernandez, H., Molina, J., Pozzi, F., Romano, M., Tasca, L., Vergani, D., Zamorani, G., Zucca, E.
Publikováno v:
A&A 686, A156 (2024)
Context: From redshift 6 to redshift $\approx$ 4 galaxies grow rapidly from low mass galaxies towards the more mature massive galaxies we see at the cosmic noon. Growth via gas accretion and mergers undoubtedly shape this evolution - however, there c
Externí odkaz:
http://arxiv.org/abs/2311.11493
Autor:
Béthermin, M., Accard, C., Guillaume, C., Dessauges-Zavadsky, M., Ibar, E., Cassata, P., Devereaux, T., Faisst, A., Freundlich, J., Jones, G. C., Kraljic, K., Algera, H., Amorin, R. O., Bardelli, S., Boquien, M., Buat, V., Donghia, E., Dubois, Y., Ferrara, A., Fudamoto, Y., Ginolfi, M., Guillard, P., Giavalisco, M., Gruppioni, C., Gururajan, G., Hathi, N., Hayward, C. C., Koekemoer, A. M., Lemaux, B. C., Magdis, G. E., Molina, J., Narayanan, D., Mayer, L., Pozzi, F., Rizzo, F., Romano, M., Tasca, L., Theulé, P., Vergani, D., Vallini, L., Zamorani, G., Zanella, A., Zucca, E.
The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density ($\Sigma_{\rm gas}$-$\Sigma_{\rm SFR}$) is essential to understand star formation processes in galaxies. So far, it has been measured up to z~2.5 in
Externí odkaz:
http://arxiv.org/abs/2311.08474
Autor:
Méndez-Hernández, H., Cassata, P., Ibar, E., Amorín, R, Aravena, M., Bardelli, S., Cucciati, O., Garilli, B., Giavalisco, M., Guaita, L., Hathi, N., Koekemoer, A., Brun, V. Le, Lemaux, B. C., Maccagni, D., Ribeiro, B., Tasca, L., Tejos, N., Thomas, R., Tresse, L., Vergani, D., Zamorani, G., Zucca, E.
Publikováno v:
A&A 666, A56 (2022)
The circumgalactic medium (CGM) is the location where the interplay between large-scale outflows and accretion onto galaxies occurs. Metals in different ionization states flowing between the circumgalactic and intergalactic mediums are affected by la
Externí odkaz:
http://arxiv.org/abs/2206.08923
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:
Hammer, F., Morris, S., Cuby, J. G., Kaper, L., Steinmetz, M., Afonso, J., Barbuy, B., Bergin, E., Finogenov, A., Gallego, J., Kassin, S., Miller, C., Ostlin, G., Penterricci, L., Schaerer, D., Ziegler, B., Chemla, F., Dalton, G., De Frondat, F., Evans, C., Mignant, D. Le, Puech, M., Rodrigues, M., Sanchez-Janssen, R., Taburet, S., Tasca, L., Yang, Y. B., Zanchetta, S., Dohlen, K., Dubbeldam, M., Hadi, K. El, Janssen, A., Kelz, A., Larrieu, M., Lewis, I., MacIntosh, M., Morris, T., Navarro, R., Seifert, W.
The powerful combination of the cutting-edge multi-object spectrograph MOSAIC with the world largest telescope, the ELT, will allow us to probe deeper into the Universe than was possible. MOSAIC is an extremely efficient instrument in providing spect
Externí odkaz:
http://arxiv.org/abs/2011.03549
Autor:
Yan, Lin, Sajina, A., Loiacono, F., Lagache, G., Bèthermin, M., Faisst, A., Ginolfi, M., Fèvre, O. Le, Gruppioni, C., Capak, P. L., Cassata, P., Schaerer, D., Silverman, J. D., Bardelli, S., Dessauges-Zavadsky, M., Cimatti, A., Hathi, N. P., Lemaux, B. C., Ibar, E., Jones, G. C., Koekemoer, A. M., Oesch, P. A., Talia, M., Pozzi, F., Riechers, D. A., Tasca, L. A., Toft, S., Vallini, L., Vergani, D., Zamorani, G., Zucca, E.
We present the [CII]158$\mu$m line luminosity functions (LFs) at $z\sim4-6$ using the ALMA observations of 118 sources, which are selected to have UV luminosity $M_{1500A}<-20.2$ and optical spectroscopic redshifts in COSMOS and ECDF-S. Of the 118 ta
Externí odkaz:
http://arxiv.org/abs/2006.04835
Autor:
Faisst, A. L., Schaerer, D., Lemaux, B. C., Oesch, P. A., Fudamoto, Y., Cassata, P., Bethermin, M., Capak, P. L., Fevre, O. Le, Silverman, J. D., Yan, L., Ginolfi, M., Koekemoer, A. M., Morselli, L., Amorin, R., Bardelli, S., Boquien, M., Brammer, G., Cimatti, A., Dessauges-Zavadsky, M., Fujimoto, S., Gruppioni, C., Hathi, N. P., Hemmati, S., Ibar, E., Jones, G. C., Khusanova, Y., Loiacono, F., Pozzi, F., Talia, M., Tasca, L. A. M., Riechers, D. A., Rodighiero, G., Romano, M., Scoville, N., Toft, S., Vallini, L., Vergani, D., Zamorani, G., Zucca, E.
We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey - the first large multi-wavelength survey which aims at characterizing the gas and dust properti
Externí odkaz:
http://arxiv.org/abs/1912.01621
Autor:
Gargiulo, A., Cucciati, O., Garilli, B., Scodeggio, M., Bolzonella, M., Zamorani, G., De Lucia, G., Krywult, J., Guzzo, L., Granett, B. R., de la Torre, S., Abbas, U., Adami, C., Arnouts, S., Bottini, D., Cappi, A., Franzetti, P., Fritz, A., Haines, C., Hawken, A. J., Iovino, A., Brun, V. Le, Fèvre, O. Le, Maccagni, D., Małek, K., Marulli, F., Moutard, T., Polletta, M., Pollo, A., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., Coupon, J., Ilbert, O., Moscardini, L., Peacock, J. A.
Publikováno v:
A&A 631, A15 (2019)
We use the statistics of the VIPERS survey to investigate the relation between the surface mean stellar mass density Sigma=Mstar/(2*pi*Re^2) of massive passive galaxies (MPGs, Mstar>10^11 Msun) and their environment in the redshift range 0.5
Externí odkaz:
http://arxiv.org/abs/1909.05094
Autor:
Khusanova, Y., Fèvre, O. Le, Cassata, P., Cucciati, O., Lemaux, B. C., Tasca, L. A. M., Thomas, R., Garilli, B., Brun, V. Le, Maccagni, D., Pentericci, L., Zamorani, G., Amorín, R., Bardelli, S., Castellano, M., Cassarà, L. P., Cimatti, A., Giavalisco, M., Hathi, N. P., Ilbert, O., Koekemoer, A. M., Marchi, F., Pforr, J., Ribeiro, B., Schaerer, D., Tresse, L., Vergani, D., Zucca, E.
Publikováno v:
A&A 634, A97 (2020)
We establish a robust statistical description of the star-forming galaxy population at the end of cosmic HI reionization ($5.0\le{}z\le6.6$) from a large sample of 52 galaxies with spectroscopically confirmed redshifts from the VIMOS UltraDeep Survey
Externí odkaz:
http://arxiv.org/abs/1903.01884
Autor:
Adami, C., Giles, P., Koulouridis, E., Pacaud, F., Caretta, C. A., Pierre, M., Eckert, D., Ramos-Ceja, M. E., Gastaldello, F., Fotopoulou, S., Guglielmo, V., Lidman, C., Sadibekova, T., Iovino, A., Maughan, B., Chiappetti, L., Alis, S., Altieri, B., Baldry, I., Bottini, D., Birkinshaw, M., Bremer, M., Brown, M., Cucciati, O., Driver, S., Elmer, E., Ettori, S., Evrard, A. E., Faccioli, L., Granett, B., Grootes, M., Guzzo, L., Hopkins, A., Horellou, C., Lef, J. P., Liske, J., Malek, K., Marulli, F., Maurogordato, S., Owers, M., Paltani, S., Poggianti, B., Polletta, M., Plionis, M., Pollo, A., Pompei, E., Ponman, T., Rapetti, D., Ricci, M., Robotham, A., Tuffs, R., Tasca, L., Valtchanov, I., Vergani, D., Wagner, G., Willis, J., consortium, the XXL
In the currently debated context of using clusters of galaxies as cosmological probes, the need for well-defined cluster samples is critical. The XXL Survey has been specifically designed to provide a well characterised sample of some 500 X-ray detec
Externí odkaz:
http://arxiv.org/abs/1810.03849