Zobrazeno 1 - 10
of 766
pro vyhledávání: '"F. Arrigoni"'
Autor:
M. Ginolfi, E. Piconcelli, L. Zappacosta, G. C. Jones, L. Pentericci, R. Maiolino, A. Travascio, N. Menci, S. Carniani, F. Rizzo, F. Arrigoni Battaia, S. Cantalupo, C. De Breuck, L. Graziani, K. Knudsen, P. Laursen, V. Mainieri, R. Schneider, F. Stanley, R. Valiante, A. Verhamme
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-15 (2022)
Lyman-alpha emission is one of the observational probes for the high-redshift universe. Here, the authors show several Lyman-alpha emitting companion galaxies around the hot dust-obscured galaxy W0410-091 suggesting that the galaxy evolves in a very
Externí odkaz:
https://doaj.org/article/ea7346be48844af7a9cbe32579f2e85d
Autor:
L. Ferrario, E. Garagiola, C. Gerardi, G. Bellavia, S. Colombo, C. Ticca, C. Rossetti, M. Ciboldi, M. Meroni, A. Vanzulli, A. Rampoldi, T. Bignardi, F. Arrigoni, E. Porazzi, E. Foglia
Publikováno v:
Health Economics Review, Vol 12, Iss 1, Pp 1-10 (2022)
Abstract Background To evaluate the potential benefits of the Magnetic Resonance-guided high intensity Focused Ultrasound (MRgFUS) introduction in the clinical practice, for the treatment of uterine fibroids, in comparison with the standard “conser
Externí odkaz:
https://doaj.org/article/fc9f381073494bc0855e8d0b0ccb1e02
Autor:
Muñoz-Elgueta, N., Battaia, F. Arrigoni, Kauffmann, G., Pakmor, R., Walch, S., Obreja, A., Buhlmann, L.
Publikováno v:
A&A 690, A392 (2024)
Extended [CII] emission on tens of kpc, also known as a [CII] halo, is being currently reported around z$\sim$4-6 star-forming galaxies, especially thanks to the statistics of the ALPINE survey. The [CII] emission is expected to trace dense cold gas
Externí odkaz:
http://arxiv.org/abs/2407.17359
Autor:
Zanella, A., Iani, E., Dessauges-Zavadsky, M., Richard, J., De Breuck, C., Vernet, J., Kohandel, M., Battaia, F. Arrigoni, Bolamperti, A., Calura, F., Chen, C. -C., Devereaux, T., Ferrara, A., Mainieri, V., Pallottini, A., Rodighiero, G., Vallini, L., Vanzella, E.
Observations at UV and optical wavelengths have revealed that galaxies at z~1-4 host star-forming regions, dubbed "clumps", which are believed to form due to the fragmentation of gravitationally unstable, gas-rich disks. However, the detection of the
Externí odkaz:
http://arxiv.org/abs/2402.17837
Autor:
Girdhar, A., Harrison, C. M., Mainieri, V., Aranda, R. Fernández, Alexander, D. M., Battaia, F. Arrigoni, Bianchin, M., Rivera, G. Calistro, Circosta, C., Costa, T., Edge, A. C., Farina, E. P., Kakkad, D., Kharb, P., Molyneux, S. J., Mukherjee, D., Njeri, A., S., Silpa, Venturi, G., Ward, S. R.
We present a study of molecular gas, traced via CO (3-2) from ALMA data, of four z< 0.2, `radio quiet', type 2 quasars (log [L(bol)/(erg/s)] = 45.3 - 46.2; log [L(1.4 GHz)/(W/Hz)] = 23.7 - 24.3). Targets were selected to have extended radio lobes (>=
Externí odkaz:
http://arxiv.org/abs/2311.03453
Autor:
Molyneux, S. J., Rivera, G. Calistro, De Breuck, C., Harrison, C. M., Mainieri, V., Lundgren, A., Kakkad, D., Circosta, C., Girdhar, A., Costa, T., Mullaney, J. R., Kharb, P., Battaia, F. Arrigoni, Farina, E. P., Alexander, D. M., Ward, S. R., S., Silpa, Smit, R.
We present a comprehensive study of the molecular gas properties of 17 Type 2 quasars at $z <$ 0.2 from the Quasar Feedback Survey (L$_{[OIII]}$ > $10^{42.1}$ $\rm ergs^{-1}$), selected by their high [OIII] luminosities and displaying a large diversi
Externí odkaz:
http://arxiv.org/abs/2310.10235
Publikováno v:
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XL-5, Pp 63-70 (2014)
In this paper we address the problem of estimating the attitudes and positions of a set of cameras in an external coordinate system. Starting from a conventional global structure-from-motion pipeline, we present some substantial advances. In order t
Externí odkaz:
https://doaj.org/article/29fa66bcf5b34aa6a0fa7076b8982c8b
Autor:
Stacey, H. R., Battaia, F. Arrigoni
We present deep observations of CO(3-2) from the Cloverleaf lensed quasar-starburst at $z=2.56$. We discover a 4-5 times less massive companion at a projected distance of 33 kpc from the Cloverleaf host galaxy. The galaxies are connected by a bridge
Externí odkaz:
http://arxiv.org/abs/2209.00012
Autor:
Ginolfi, M., Piconcelli, E., Zappacosta, L., Jones, G. C., Pentericci, L., Maiolino, R., Travascio, A., Menci, N., Carniani, S., Rizzo, F., Battaia, F. Arrigoni, Cantalupo, S., De Breuck, C., Graziani, L., Knudsen, K., Laursen, P., Mainieri, V., Schneider, R., Stanley, F., Valiante, R., Verhamme, A.
The phase transition between galaxies and quasars is often identified with the rare population of hyper-luminous, hot dust-obscured galaxies. Galaxy formation models predict these systems to grow via mergers, that can deliver large amounts of gas tow
Externí odkaz:
http://arxiv.org/abs/2208.03248
Autor:
Muñoz-Elgueta, N., Battaia, F. Arrigoni, Kauffmann, G., De Breuck, C., García-Vergara, C., Zanella, A., Farina, E. P., Decarli, R.
Cool gas (T$\sim$10$^{4}$~K) traced by hydrogen Ly$\alpha$ emission is now routinely detected around $z\sim3$ quasars, but little is known about their molecular gas reservoirs. Here, we present an APEX spectroscopic survey of the CO(6-5), CO(7-6) and
Externí odkaz:
http://arxiv.org/abs/2201.11660