Zobrazeno 1 - 10
of 2 958
pro vyhledávání: '"B. lo"'
Autor:
L. Brunasso, F. Ascanio, B. Lo Duca, A.M. Fimognari, L. Grippi, A. Odierna, D.G. Iacopino, V. Fiorenza
Publikováno v:
Brain and Spine, Vol 1, Iss , Pp 100351- (2021)
Externí odkaz:
https://doaj.org/article/abac77fb42d948be8ac2368510726b03
Publikováno v:
Kidney International Reports, Vol 1, Iss 4, Pp S16-S17 (2016)
Externí odkaz:
https://doaj.org/article/4e8172a58d4e43038e3e32ee70db6a3c
Autor:
Shirley, R., Duncan, K., Varillas, M. C. Campos, Hurley, P. D., Malek, K., Roehlly, Y., Smith, M. W. L., Aussel, H., Bakx, T., Buat, V., Burgarella, D., Christopher, N., Duivenvoorden, S., Eales, S., Efstathiou, A., Solares, E. A. Gonzalez, Griffin, M., Jarvis, M., Faro, B. Lo, Marchetti, L., McCheyne, I., Papadopoulos, A., Penner, K., Pons, E., Prescott, M., Rigby, E., Rottgering, H., Saxena, A., Scudder, J., Vaccari, M., Wang, L., Oliver, S. J.
We present the Herschel Extragalactic Legacy Project (HELP). This project collates, curates, homogenises, and creates derived data products for most of the premium multi-wavelength extragalactic data sets. The sky boundaries for the first data releas
Externí odkaz:
http://arxiv.org/abs/2105.05659
Autor:
Faro, B. Lo, Buat, V., Roehlly, Y., Álvarez-Márquez, J., Burgarella, D., Silva, L., Efstathiou, A.
In this work we investigate the far-UV to NIR shape of the dust attenuation curve of a sample of IR selected dust obscured (U)LIRGs at z$\sim$2. The spectral energy distributions (SEDs) are fitted with CIGALE, a physically-motivated spectral synthesi
Externí odkaz:
http://arxiv.org/abs/1707.09805
Autor:
Álvarez-Márquez, J., Burgarella, D., Heinis, S., Buat, V., Faro, B. Lo, Béthermin, M., López-Fortín, C. E., Cooray, A., Farrah, D., Hurley, P., Ibar, E., Ilbert, O., Koekemoer, A. M., Lemaux, B. C., Pérez-Fournon, I., Rodighiero, G., Salvato, M., Scott, D., Taniguchi, Y., Vieira, J. D., Wang, L.
Publikováno v:
A&A 587, A122 (2016)
We explore from a statistical point of view the far-infrared (far-IR) and sub-millimeter (sub-mm) properties of a large sample of LBGs (22,000) at z~3 in the COSMOS field. The large number of galaxies allows us to split it in several bins as a functi
Externí odkaz:
http://arxiv.org/abs/1512.04120
Autor:
Laporte, N., Pérez-Fournon, I., Calanog, J. A., Cooray, A., Wardlow, J. L., Bock, J., Bridge, C., Burgarella, D., Bussmann, R. S., Cabrera-Lavers, A., Casey, C. M., Clements, D. L., Conley, A., Dannerbauer, H., Farrah, D., Fu, H., Gavazzi, R., González-Solares, E. A., Ivison, R. J., Faro, B. Lo, Ma, B., Magdis, G., Marques-Chaves, R., Martínez-Navajas, P., Oliver, S. J., Osage, W. A., Riechers, D., Rigopoulou, D., Scott, D., Streblyanska, A., Vieira, J. D.
We describe the search for Lyman-break galaxies (LBGs) near the sub-millimeter bright starburst galaxy HFLS3 at $z$$=$6.34 and a study on the environment of this massive galaxy during the end of reionization.We performed two independent selections of
Externí odkaz:
http://arxiv.org/abs/1504.04534
We complement our previous analysis of a sample of z~1-2 luminous and ultra-luminous infrared galaxies ((U)LIRGs), by adding deep VLA radio observations at 1.4 GHz to a large data-set from the far-UV to the sub-mm, including Spitzer and Herschel data
Externí odkaz:
http://arxiv.org/abs/1412.3458
Autor:
Rossi, A., Piranomonte, S., Savaglio, S., Palazzi, E., Michałowski, M. J., Klose, S., Hunt, L. K., Amati, L., Elliott, J., Greiner, J., Guidorzi, C., Japelj, J., Kann, D. A., Faro, B. Lo, Guelbenzu, A. Nicuesa, Schulze, S., Vergani, S. D., Arnold, L. A., Covino, S., D'Elia, V., Ferrero, P., Filgas, R., Goldoni, P., Yoldaş, A. Küpcü, Borgne, D. Le, Pian, E., Schady, P., Stratta, G.
Publikováno v:
A&A 572, A47 (2014)
Long-duration gamma-ray bursts (LGRBs) are produced by the collapse of very massive stars. Due to the short lifetime of their progenitors, LGRBs pinpoint star-forming galaxies. We present here a multi-band search for the host galaxy of the long dark
Externí odkaz:
http://arxiv.org/abs/1409.0017
Autor:
Faro, B. Lo, Franceschini, A., Vaccari, M., Silva, L., Rodighiero, G., Berta, S., Bock, J., Burgarella, D., Buat, V., Cava, A., Clements, D. L., Cooray, A., Farrah, D., Feltre, A., Solares, E. A. González, Hurley, P., Lutz, D., Magdis, G., Magnelli, B., Marchetti, L., Oliver, S. J., Page, M. J., Popesso, P., Pozzi, F., Rigopoulou, D., Rowan-Robinson, M., Roseboom, I. G., Scott, Douglas, Smith, A. J., Symeonidis, M., Wang, L., Wuyts, S.
We combine far-infrared photometry from Herschel (PEP/HERMES) with deep mid-infrared spectroscopy from Spitzer to investigate the nature and the mass assembly history of a sample of 31 Luminous and Ultraluminous Infrared Galaxies at z~1 and 2 selecte
Externí odkaz:
http://arxiv.org/abs/1211.6116
Autor:
HerMES Collaboration, Oliver, S. J., Bock, J., Altieri, B., Amblard, A., Arumugam, V., Aussel, H., Babbedge, T., Beelen, A., Béthermin, M., Blain, A., Boselli, A., Bridge, C., Brisbin, D., Buat, V., Burgarella, D., Castro-Rodríguez, N., Cava, A., Chanial, P., Cirasuolo, M., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dowell, C. D., Dubois, E. N., Dwek, E., Dye, S., Eales, S., Elbaz, D., Farrah, D., Feltre, A., Ferrero, P., Fiolet, N., Fox, M., Franceschini, A., Gear, W., Giovannoli, E., Glenn, J., Gong, Y., Solares, E. A. González, Griffin, M., Halpern, M., Harwit, M., Hatziminaoglou, E., Heinis, S., Hurley, P., Hwang, H. S., Hyde, A., Ibar, E., Ilbert, O., Isaak, K., Ivison, R. J., Lagache, G., Floc'h, E. Le, Levenson, L., Faro, B. Lo, Lu, N., Madden, S., Maffei, B., Magdis, G., Mainetti, G., Marchetti, L., Marsden, G., Marshall, J., Mortier, A. M. J., Nguyen, H. T., O'Halloran, B., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Patel, H., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rawlings, J. I., Raymond, G., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Portal, M. Sánchez, Schulz, B., Scott, Douglas, Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vieira, J. D., Viero, M., Vigroux, L., Wang, L., Ward, R., Wardlow, J., Wright, G., Xu, C. K., Zemcov, M.
The Herschel Multi-tiered Extragalactic Survey, HerMES, is a legacy program designed to map a set of nested fields totalling ~380 deg^2. Fields range in size from 0.01 to ~20 deg^2, using Herschel-SPIRE (at 250, 350 and 500 \mu m), and Herschel-PACS
Externí odkaz:
http://arxiv.org/abs/1203.2562