Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Fournon, I. Perez"'
Autor:
Greenslade, J., Aguilar, E., Clements, D. L., Dannerbauer, H., Cheng, T., Petitpas, G., Yang, C., Messias, H., Oteo, I., Farrah, D., Michalowski, M. J., Fournon, I. Perez, Aretxaga, I., Yun, M. S., Eales, S., Dunne, L., Cooray, A., Andreani, P., Hughes, D. H., Velazquez, M., Sanchez-Arguelles, D., Ponthieu, N.
Dusty star-forming galaxies (DSFGs) detected at $z > 4$ provide important examples of the first generations of massive galaxies. However, few examples with spectroscopic confirmation are currently known, with Hershel struggling to detect significant
Externí odkaz:
http://arxiv.org/abs/1910.03512
Autor:
Fernández-Ontiveros, J. A., Armus, L., Baes, M., Bernard-Salas, J., Bolatto, A. D., Braine, J., Ciesla, L., De Looze, I., Egami, E., Fischer, J., Giard, M., González-Alfonso, E., Granato, G. L., Gruppioni, C., Imanishi, M., Ishihara, D., Kaneda, H., Madden, S., Malkan, M., Matsuhara, H., Matsuura, M., Nagao, T., Najarro, F., Nakagawa, T., Onaka, T., Oyabu, S., Pereira-Santaella, M., Fournon, I. Pérez, Roelfsema, P., Santini, P., Silva, L., Smith, J. -D. T., Spinoglio, L., van der Tak, F., Wada, T., Wu, R.
The physical processes driving the chemical evolution of galaxies in the last $\sim 11\, \rm{Gyr}$ cannot be understood without directly probing the dust-obscured phase of star-forming galaxies and active galactic nuclei. This phase, hidden to optica
Externí odkaz:
http://arxiv.org/abs/1710.02150
Autor:
Elbaz, D., Hwang, H. S., Magnelli, B., Daddi, E., Aussel, H., Altieri, B., Amblard, A., Andreani, P., Arumugam, V., Auld, R., Babbedge, T., Berta, S., Blain, A., Bock, J., Bongiovanni, A., Boselli, A., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Cepa, J., Chanial, P., Chary, R. -R., Cimatti, A., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dickinson, M., Dominguez, H., Dowell, C. D., Dunlop, J. S., Dwek, E., Eales, S., Farrah, D., Schreiber, N. Forster, Fox, M., Franceschini, A., Gear, W., Genzel, R., Glenn, J., Griffin, M., Gruppioni, C., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Lagache, G., Borgne, D. Le, Floc'h, E. Le, Levenson, L., Lu, N., Lutz, D., Madden, S., Maffei, B., Magdis, G., Mainetti, G., Maiolino, R., Marchetti, L., Mortier, A. M. J., Nguyen, H. T., Nordon, R., O'Halloran, B., Okumura, K., Oliver, S. J., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Fournon, I. Perez, Garcıa, A. M. Perez, Poglitsch, A., Pohlen, M., Popesso, P., Pozzi, F., Rawlings, J. I., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Saintonge, A., Sanchez-Portal, M., Santini, P., Sauvage, M., Schulz, B., Scott, Douglas, Seymour, N., Shao, L., Shupe, D. L., Smith, A. J., Stevens, J. A., Sturm, E., Symeonidis, M., Tacconi, L., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vieira, J., Vigroux, L., Wang, L., Ward, R., Wright, G., Xu, C. K., Zemcov, M.
The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the spectral energ
Externí odkaz:
http://arxiv.org/abs/1005.2859
Autor:
Schulz, B., Pearson, C. P., Clements, D. L., Altieri, B., Amblard, A., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Blain, A., Bock, J., Boselli, A., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Chanial, P., Conley, A., Conversi, L., Cooray, A., Dowell, C. D., Dwek, E., Eales, S., Elbaz, D., Fox, M., Franceschini, A., Gear, W., Giovannoli, E., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Marsden, G., Mortier, A. M. J., Nguyen, H. T., O'Halloran, B., Oliver, S. J., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Fournon, I. Perez, Pohlen, M., Rangwala, N., Rawlings, J., Raymond, G., Rigopoulou, D., Rizzo, D., Roseboom, I. G., Rowan-Robinson, M., Portal, M. Sanchez, Scott, Douglas, Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K. E., Vaccari, M., Valiante, E., Valtchanov, I., Vigroux, L., Wang, L., Ward, R., Wright, G., Xu, C. K., Zemcov, M.
We present colours of sources detected with the Herschel/SPIRE instrument in deep extragalactic surveys of the Lockman Hole, Spitzer-FLS, and GOODS-N fields in three photometric bands at 250, 350 and 500 micrometers. We compare these with expectation
Externí odkaz:
http://arxiv.org/abs/1005.2396
Autor:
Magnelli, B., Lutz, D., Berta, S., Altieri, B., Andreani, P., Aussel, H., Castaneda, H., Cava, A., Cepa, J., Cimatti, A., Daddi, E., Dannerbauer, H., Dominguez, H., Elbaz, D., Schreiber, N. Forster, Genzel, R., Grazian, A., Gruppioni, C., Magdis, G., Maiolino, R., Nordon, R., Fournon, I. Perez, Garcia, I. Perez, Poglitsch, A., Popesso, P., Pozzi, F., Riguccini, L., Rodighiero, G., Saintonge, A., Santini, P., Sanchez-Portal, M., Shao, L., Sturm, E., Tacconi, L., Valtchanov, I., Wieprecht, E., Wiezorrek, E.
We use deep observations obtained with the Photodetector Array Camera and Spectrometer (PACS) onboard the Herschel space observatory to study the far-infrared (FIR) properties of submm and optically faint radio galaxies (SMGs and OFRGs). From literat
Externí odkaz:
http://arxiv.org/abs/1005.1154
Autor:
Snellen, I., Schilizzi, R. T., Bremer, M. N., de Bruyn, A. G., Miley, G. K., Rottgering, H. J. A., McMahon, R. G., Fournon, I. Perez
A sample of 47 faint Gigahertz Peaked Spectrum (GPS) radio sources selected from the Westerbork Northern Sky Survey (WENSS, Rengelink et al. 1997), has been imaged in the optical and near infrared, resulting in an identification fraction of 87%. The
Externí odkaz:
http://arxiv.org/abs/astro-ph/9809069