Zobrazeno 1 - 10
of 232
pro vyhledávání: '"Furlanetto, C."'
Autor:
Nord, B., Buckley-Geer, E., Lin, H., Diehl, H. T., Helsby, J., Kuropatkin, N., Amara, A., Collett, T., Allam, S., Caminha, G. B., De Bom, C., Desai, S., Dúmet-Montoya, H., da S. Pereira, M. Elidaiana, Finley, D. A., Flaugher, B., Furlanetto, C., Gaitsch, H., Gill, M., Merritt, K. W., More, A., Tucker, D., Saro, A., Rykoff, E. S., Rozo, E., Birrer, S., Abdalla, F. B., Agnello, A., Auger, M., Brunner, R. J., Kind, M. Carrasco, Castander, F. J., Cunha, C. E., da Costa, L. N., Foley, R. J., Gerdes, D. W., Glazebrook, K., Gschwend, J., Hartley, W., Kessler, R., Lagattuta, D., Lewis, G., Maia, M. A. G., Makler, M., Menanteau, F., Niernberg, A., Scolnic, D., Vieira, J. D., Gramillano, R., Abbott, T. M. C., Banerji, M., Benoit-Lévy, A., Brooks, D., Burke, D. L., Capozzi, D., Rosell, A. Carnero, Carretero, J., D’Andrea, C. B., Dietrich, J. P., Doel, P., Evrard, A. E., Frieman, J., Gaztanaga, E., Gruen, D., Honscheid, K., James, D. J., Kuehn, K., Li, T. S., Lima, M., Marshall, J. L., Martini, P., Melchior, P., Miquel, R., Neilsen, E., Nichol, R. C., Ogando, R., Plazas, A. A., Romer, A. K., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Sevilla-Noarbe, I., Smith, R. C., Soares-Santos, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thaler, J., Walker, A. R., Wester, W., Zhang, Y.
We report the observation and confirmation of the first group-and cluster-scale strong gravitational lensing systems found in Dark Energy Survey data. Through visual inspection of data from the Science Verification season, we identified 53 candidate
Externí odkaz:
http://hdl.handle.net/10150/621386
http://arizona.openrepository.com/arizona/handle/10150/621386
http://arizona.openrepository.com/arizona/handle/10150/621386
Autor:
Bom, C. R., Fraga, B. M. O., Dias, L. O., Schubert, P., Valentin, M. Blanco, Furlanetto, C., Makler, M., Teles, K., de Albuquerque, M. Portes, Metcalf, R. Benton
Strong Lensing is a powerful probe of the matter distribution in galaxies and clusters and a relevant tool for cosmography. Analyses of strong gravitational lenses with Deep Learning have become a popular approach due to these astronomical objects' r
Externí odkaz:
http://arxiv.org/abs/2203.09536
Autor:
Schnorr-Müller, A., Trevisan, M., Riffel, R., Chies-Santos, A. L., Furlanetto, C., Ricci, T. V., Lohmann, F. S., Flores-Freitas, R., Mallmann, N. D., Alamo-Martínez, K. A.
We characterized the kinematics, morphology, and stellar population (SP) properties of a sample of massive compact quiescent galaxies (MCGs, $10 \lesssim \log M_\star$/$M_\odot \lesssim 11$ and $r_{\rm e} \sim 1-3 $kpc) in the MaNGA Survey, with the
Externí odkaz:
http://arxiv.org/abs/2104.12737
Autor:
Amvrosiadis, A., Eales, S. A., Negrello, M., Marchetti, L., Smith, M. W. L., Bourne, N., Clements, D. L., De Zotti, G., Dunne, L., Dye, S., Furlanetto, C., Ivison, R. J., Maddox, S., Valiante, E., Baes, M., Baker, A. J., Cooray, A., Crawford, S. M., Frayer, D., Harris, A., Michałowski, M. J., Nayyeri, H., Oliver, S., Riechers, D. A., Serjeant, S., Vaccari, M.
With the advent of wide-area submillimeter surveys, a large number of high-redshift gravitationally lensed dusty star-forming galaxies (DSFGs) has been revealed. Due to the simplicity of the selection criteria for candidate lensed sources in such sur
Externí odkaz:
http://arxiv.org/abs/1801.07282
Autor:
Maddox, S. J., Valiante, E., Cigan, P., Dunne, L., Eales, S., Smith, M. W. L., Dye, S., Furlanetto, C., Ibar, E., de Zotti, G., Millard, J. S., Bourne, N., Gomez, H. L., Ivison, R. J., Scott, D., Valtchanov, I.
The {\it Herschel} Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of 660 deg$^2$ with the PACS and SPIRE cameras in five photometric bands: 100, 160, 250, 350 and 500\mic. This is the second of three papers describing the data releas
Externí odkaz:
http://arxiv.org/abs/1712.07241
Autor:
Bakx, Tom J. L. C., Eales, S. A., Negrello, M., Smith, M. W. L., Valiante, E., Holland, W. S., Baes, M., Bourne, N., Clements, D. L., Dannerbauer, H., De Zotti, G., Dunne, L., Dye, S., Furlanetto, C., Ivison, R. J., Maddox, S., Marchetti, L., Michałowski, M. J., Omont, A., Oteo, I., Wardlow, J. L., van der Werf, P., Yang, C.
We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 square degree H-ATLAS survey. The HerBS sample contains 209 galaxies, selected with a 500 {\mu}m flux density greater than
Externí odkaz:
http://arxiv.org/abs/1709.01514
Autor:
Stanley, F., Alexander, D. M., Harrison, C. M., Rosario, D. J., Wang, L., Aird, J. A., Bourne, N., Dunne, L., Dye, S., Eales, S., Knudsen, K. K., Michalowski, M. J., Valiante, E., De Zotti, G., Furlanetto, C., Ivison, R., Maddox, S., Smith, M. W. L.
We investigate the mean star formation rates (SFRs) in the host galaxies of ~3000 optically selected QSOs from the SDSS survey within the Herschel-ATLAS fields, and a radio-luminous sub-sample, covering the redshift range of z = 0.2-2.5. Using WISE &
Externí odkaz:
http://arxiv.org/abs/1707.05334
Autor:
González-Nuevo, J., Lapi, A., Bonavera, L., Danese, L., de Zotti, G., Negrello, M., Bourne, N., Cooray, A., Dunne, L., Dye, S., Eales, S., Furlanetto, C., Ivison, R. J., Loveday, J., Maddox, S., Smith, M. W. L., Valiante, E.
Publikováno v:
Journal of Cosmology and Astroparticle Physics, Issue 10, article id. 024 (2017)
In this work we measure and study the cross-correlation signal between a foreground sample of GAMA galaxies with spectroscopic redshifts in the range $0.2
Externí odkaz:
http://arxiv.org/abs/1707.03709
Autor:
Maddox, Natasha, Jarvis, M. J., Banerji, M., Hewett, P. C., Bourne, N., Dunne, L., Dye, S., Eales, S., Furlanetto, C., Maddox, S. J., Smith, M. W. L., Valiante, E.
Combining large-area optical quasar surveys with the new far-infrared Herschel-ATLAS Data Release 1, we search for an observational signature associated with the minority of quasars possessing bright far-infrared (FIR) luminosities. We find that FIR-
Externí odkaz:
http://arxiv.org/abs/1706.04789
Autor:
Villanueva, V., Ibar, E., Hughes, T. M., Lara-López, M. A., Dunne, L., Eales, S., Ivison, R. J., Aravena, M., Baes, M., Bourne, N., Cassata, P., Cooray, A., Dannerbauer, H., Davies, L. J. M., Driver, S. P., Dye, S., Furlanetto, C., Herrera-Camus, R., Maddox, S. J., Michalowski, M. J., Molina, J., Riechers, D., Sansom, A. E., Smith, M. W. L., Rodighiero, G., Valiante, E., van der Werf, P.
We present an extragalactic survey using observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to characterise galaxy populations up to $z=0.35$: the Valpara\'iso ALMA Line Emission Survey (VALES). We use ALMA Band-3 CO(1--0) obse
Externí odkaz:
http://arxiv.org/abs/1705.09826