Zobrazeno 1 - 10
of 3 203
pro vyhledávání: '"Zotti, P."'
Autor:
Bonato, Matteo, Leisawitz, David, De Zotti, Gianfranco, Sommovigo, Laura, Shivaei, Irene, Urry, C. Megan, Farrah, Duncan, Spencer, Locke, Ricketti, Berke V., Rana, Hannah, Aalto, Susanne, Sanders, David B., Mundy, Lee G.
Far-infrared (FIR) surveys are critical to probing the co-evolution of black holes and galaxies, since of order half the light from accreting black holes and active star formation is emitted in the rest-frame infrared over $0.5\lesssim z \lesssim 10$
Externí odkaz:
http://arxiv.org/abs/2411.01216
Autor:
Bakx, T. J. L. C., Amvrosiadis, A., Bendo, G. J., Algera, H. S. B., Serjeant, S., Bonavera, L., Borsato, E., Chen, X., Cox, P., González-Nuevo, J., Hagimoto, M., Harrington, K. C., Ivison, R. J., Kamieneski, P., Marchetti, L., Riechers, D. A., Tsukui, T., van der Werf, P. P., Yang, C., Zavala, J. A., Andreani, P., Berta, S., Cooray, A. R., De Zotti, G., Eales, S., Ikeda, R., Knudsen, K. K., Mitsuhashi, I., Negrello, M., Neri, R., Omont, A., Scott, D., Tamura, Y., Temi, P., Urquhart, S. A.
We use the Atacama Large sub/Millimetre Array (ALMA) to efficiently observe spectral lines across Bands 3, 4, 5, 6, 7, and 8 at high-resolution (0.5" - 0.1") for 16 bright southern Herschel sources at $1.5 < z < 4.2$. With only six and a half hours o
Externí odkaz:
http://arxiv.org/abs/2410.16351
Autor:
Papp, Eszter, Vattay, Gabor, Romero-Muniz, Carlos, Zotti, Linda A., Fereiro, Jerry A., Sheves, Mordechai, Cahen, David
The finding that electronic conductance across ultra-thin protein films between metallic electrodes remains nearly constant from room temperature to just a few degrees Kelvin has posed a challenge. We show that a model based on a generalized Landauer
Externí odkaz:
http://arxiv.org/abs/2407.17982
Autor:
Bonato, Matteo, Baronchelli, Ivano, Casasola, Viviana, De Zotti, Gianfranco, Trobbiani, Leonardo, Ruli, Erlis, Tailor, Vidhi, Bianchi, Simone
We exploit the DustPedia sample of galaxies within approximately 40 Mpc, selecting 388 sources, to investigate the correlations between IR luminosity (L$_{\rm IR}$), the star formation rate (SFR), and the CO(1-0) luminosity (L$_{\rm CO}$) down to muc
Externí odkaz:
http://arxiv.org/abs/2407.10801
Autor:
De Zotti, G., Bonato, M., Giulietti, M., Massardi, M., Negrello, M., Algera, H. S. B., Delhaize, J.
We argue that the difference in infrared-to-radio luminosity ratio between local and high-redshift star-forming galaxies reflects {the alternative physical conditions} -- including magnetic field configurations -- of the dominant population of star-f
Externí odkaz:
http://arxiv.org/abs/2407.04825
We investigate the constraints provided by the Euclid space observatory on the physical properties of dusty star forming galaxies (DSFGs) at z>~1.5 detected in wide area sub millimetre surveys with Herschel. We adopt a physical model for the high z p
Externí odkaz:
http://arxiv.org/abs/2404.11551
Autor:
Borsato, Edoardo, Marchetti, Lucia, Negrello, Mattia, Corsini, Enrico Maria, Wake, David, Amvrosiadis, Aristeidis, Baker, Andrew, Bakx, Tom, Beelen, Alexandre, Berta, Stefano, Clements, David, Cooray, Asantha, Cox, Pierre, Dannerbauer, Helmut, de Zotti, Gianfranco, Dye, Simon, Eales, Stephen, Enia, Andrea, Farrah, Duncan, Gonzalez-Nuevo, Joaquin, Hughes, David, Ismail, Diana, Jin, Shuowen, Lapi, Andrea, Lehnert, Matthew, Neri, Roberto, Pérez-Fournon, Ismael, Rodighiero, Giulia, Scott, Douglas, Serjeant, Stephen, Stanley, Flora, Urquhart, Sheona, van der Werf, Paul, Vaccari, Mattia, Wang, Lingyu, Yang, Chentao, Young, Anthony
We have carried out HST snapshot observations at 1.1 $\mu$m of 281 candidate strongly lensed galaxies identified in the wide-area extragalactic surveys conducted with the Herschel space observatory. Our candidates comprise systems with flux densities
Externí odkaz:
http://arxiv.org/abs/2311.01158
In this paper we extend the Tiered Radio Extragalactic Continuum Simulation (T-RECS) to include HI emission. The HI T-RECS model is based on the most recent HI mass function estimates, combined with prescriptions to convert HI mass to total integrate
Externí odkaz:
http://arxiv.org/abs/2305.10175
Autor:
Hagimoto, M., Bakx, T. J. L. C., Serjeant, S., Bendo, G. J., Urquhart, S. A., Eales, S., Harrington, K. C., Tamura, Y., Umehata, H., Berta, S., Cooray, A. R., Cox, P., De Zotti, G., Lehnert, M. D., Riechers, D. A., Scott, D., Temi, P., van der Werf, P. P., Yang, C., Amvrosiadis, A., Andreani, P. M., Baker, A. J., Beelen, A., Borsato, E., Buat, V., Butler, K. M., Dannerbauer, H., Dunne, L., Dye, S., Enia, A. F. M., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Ivison, R. J., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Neri, R., Omont, A., Perez-Fournon, I., Sedgwick, C., Smith, M. W. L., Stanley, F., Verma, A., Vlahakis, C., Ward, B., Weiner, C., Weiss, A., Young, A. J.
We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 to 4.6 detected by the Atacama Large Millimetre/submillimetre Array. These lines include a total of 156 CO, [C I], and H2O emission lines
Externí odkaz:
http://arxiv.org/abs/2303.04830
Autor:
Bendo, G. J., Urquhart, S. A., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M. D., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., González-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Jones, B. M., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Pérez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., van der Werf, P., Verma, A., Vlahakis, C., Weiß, A., Yang, C., Young, A. J.
We present 101 and 151 GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500 micron flux densities >80 mJy and 250-500 micron colours consistent with z > 2, most of which are expected to be gravitationally lensed o
Externí odkaz:
http://arxiv.org/abs/2301.02584