Zobrazeno 1 - 10
of 81
pro vyhledávání: '"PAVESI R."'
Autor:
Algera, H. S. B., Hodge, J. A., Riechers, D., Murphy, E. J., Pavesi, R., Aravena, M., Daddi, E., Decarli, R., Dickinson, M., Sargent, M., Sharon, C. E., Wagg, J.
The high-frequency radio sky has historically remained largely unexplored due to the typical faintness of sources in this regime, and the modest survey speed compared to observations at lower frequencies. However, high-frequency radio surveys present
Externí odkaz:
http://arxiv.org/abs/2012.08499
Autor:
Gómez-Guijarro, C., Riechers, D. A., Pavesi, R., Magdis, G. E., Leung, T. K. D., Valentino, F., Toft, S., Aravena, M., Chapman, S. C., Clements, D. L., Dannerbauer, H., Oliver, S. J., Pérez-Fournon, I., Valtchanov, I.
Publikováno v:
The Astrophysical Journal, Volume 872, Issue 2, article id. 117, 21 pp. (2019)
ALMA 870$\mu$m continuum imaging has uncovered a population of blends of multiple dusty star-forming galaxies (DSFGs) in sources originally detected with the Herschel Space Observatory. However, their pairwise separations are much smaller that what i
Externí odkaz:
http://arxiv.org/abs/1905.08813
Autor:
Jones, G. C., Carilli, C. L., Shao, Y., Wang, R., Capak, P. L., Pavesi, R., Riechers, D. A., Karim, A., Neeleman, M., Walter, F.
Until recently, determining the rotational properties of galaxies in the early universe (z>4, Universe age <1.5Gyr) was impractical, with the exception of a few strongly lensed systems. Combining the high resolution and sensitivity of ALMA at (sub-)
Externí odkaz:
http://arxiv.org/abs/1709.04954
Autor:
Gallerani, S., Pallottini, A., Feruglio, C., Ferrara, A., Maiolino, R., Vallini, L., Riechers, D. A., Pavesi, R.
We present the first attempt to detect outflows from galaxies approaching the Epoch of Reionization (EoR) using a sample of 9 star-forming ($\rm SFR=31\pm 20~M_{\odot}~yr^{-1}$) $z\sim 5.5$ galaxies for which the [CII]158$\mu$m line has been previous
Externí odkaz:
http://arxiv.org/abs/1604.05714
Autor:
Bulgarelli, A., Argan, A., Barbiellini, G., Basset, M., Chen, A., Di Cocco, G., Foggetta, L., Gianotti, F., Giuliani, A., Longo, F., Mereghetti, S., Monzani, F., Nicolini, L., Pavesi, R., Pellizzoni, A., Pontoni, C., Prest, M., Pucella, G., Tavani, M., Trifoglio, M., Trois, A., Vallazza, E., Vercellone, S.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 2010 614(2):213-226
Akademický článek
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Akademický článek
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Autor:
Walter, F., Carilli, C., Decarli, R., Riechers, D., Aravena, M., Bauer, F., Bertoldi, F., Bolatto, A., Boogaard, L.A., Bouwens, R.J., Burgarella, D., Casey, C., Cooray, A., Cortes, P., Cox, P., Daddi, E., Darling, J., Emonts, B., Lopez, J., Hodge, J.A., Inami, H., Ivison, R., Kovetz, E., Fèvre, O., Magnelli, B., Marrone, D., Murphy, E., Narayanan, D., Novak, M., Oesch, P., Pavesi, R., Santos, T., Sargent, M., Scott, D., Scoville, N., Stacey, G., Wagg, J., Werf, P.P. van der, Uzgil, B., Weiss, A., Yun, M.
Publikováno v:
Bulletin of the American Astronomical Society
Bulletin of the American Astronomical Society, 51(3), 442
Bulletin of the American Astronomical Society, 51(3), 442
One of the last missing pieces in the puzzle of galaxy formation and evolution through cosmic history is a detailed picture of the role of the cold gas supply in the star-formation process. Cold gas is the fuel for star formation, and thus regulates
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c48b2d0487c55fb1bbc12d661b8caf15
https://hdl.handle.net/1887/84559
https://hdl.handle.net/1887/84559
Autor:
Kaasinen, M., Scoville, N., Walter, F., Da Cunha, E., Popping, G., Pavesi, R., Darvish, B., Casey, C., Riechers, D., Glover, S.
Publikováno v:
The Astrophysical Journal
We test the use of long-wavelength dust continuum emission as a molecular gas tracer at high redshift, via a unique sample of a dozen z ∼ 2 galaxies with observations of both the dust continuum and CO(1−0) line emission (obtained with the Atacama
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1874::854fb8f872182263b140810169d1868d
https://hdl.handle.net/21.11116/0000-0005-D0C4-2
https://hdl.handle.net/21.11116/0000-0005-D0C4-2
Autor:
Gallerani, S, Pallottini, A, Feruglio, C, Ferrara, A, Maiolino, R, Vallini, L, Riechers, DA, Pavesi, R
We present the first attempt to detect outflows from galaxies approaching the Epoch of Reionization (EoR) using a sample of 9 star-forming ($\rm SFR=31\pm 20~M_{\odot}~yr^{-1}$) $z\sim 5.5$ galaxies for which the [CII]158$\mu$m line has been previous
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::975aef7d0e2cfd39046b87a808c9ddd4
https://www.repository.cam.ac.uk/handle/1810/275485
https://www.repository.cam.ac.uk/handle/1810/275485