Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Fiolet, N"'
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
Autor:
Omont, A., Neri, R., Cox, P., Lupu, R., Guélin, M., van der Werf, P., Weiß, A., Ivison, R., Negrello, M., Leeuw, L., Lehnert, M., Smail, I., Beelen, A., Aguirre, J. E., Baes, M., Bertoldi, F., Clements, D. L., Cooray, A., Coppin, K., Dannerbauer, H., De Zotti, G., Dye, S., Fiolet, N., Frayer, D., Gavazzi, R., Hughes, D., Jarvis, M., Krips, M., lowski, M. Micha, Murphy, E., Riechers, D., Swinbank, A. M., Temi, P., Vaccari, M., Verma, A., Vieira, J. D., Auld, R., Buttiglione, B., Cava, A., Dariush, A., Dunne, L., Eales, S. A., Fritz, J., Gomez, H., Ibar, E., Maddox, S., Pascale, E., Pohlen, M., Rigby, E., Smith, D., Baker, A. J., Bock, J., Bradford, C. M., Glenn, J., Harris, A. I., Scott, K. S., Zmuidzinas, J.
Publikováno v:
2011 A&A 530, L3
The Herschel survey, H-ATLAS, with its large areal coverage, has recently discovered a number of bright, strongly lensed high-z submillimeter galaxies. The strong magnification makes it possible to study molecular species other than CO, which are oth
Externí odkaz:
http://arxiv.org/abs/1107.4979
Autor:
Stacey, G. J., Hailey-Dunsheath, S., Ferkinhoff, C., Nikola, T., Parshley, S. C., Benford, D. J., Staguhn, J. G., Fiolet, N.
We have detected the 158 {\mu}m [CII] line from 12 galaxies at z~1-2. This is the first survey of this important starformation tracer at redshifts covering the epoch of maximum star-formation in the Universe and quadruples the number of reported high
Externí odkaz:
http://arxiv.org/abs/1009.4216
Autor:
Kovács, A., Omont, A., Beelen, A., Lonsdale, C., Polletta, M., Fiolet, N., Greve, T. R., Borys, C., Cox, P., De Breuck, C., Dole, H., Dowell, C. D., Farrah, D., Lagache, G., Menten, K. M., Bell, T. A., Owen, F.
Publikováno v:
Astrophys.J.717:29-39,2010
We present SHARC-2 350 micron data on 20 luminous z ~ 2 starbursts with S(1.2mm) > 2 mJy from the Spitzer-selected samples of Lonsdale et al. and Fiolet et al. All the sources were detected, with S(350um) > 25 mJy for 18 of them. With the data, we de
Externí odkaz:
http://arxiv.org/abs/1004.0819
Autor:
Yan, Lin, Tacconi, L. ~J., Fiolet, N., Sajina, A., Omont, A., Lutz, D., Zamojski, M., Neri, R., Cox, P., Dasyra, K. ~M.
We present CO observations of 9 ULIRGs at z~2 with S(24\mu m)>1mJy, previously confirmed with the mid-IR spectra in the Spitzer First Look Survey. All targets are required to have accurate redshifts from Keck/GEMINI near-IR spectra. Using the Plateau
Externí odkaz:
http://arxiv.org/abs/1003.2369
Autor:
Fiolet, N., Omont, A., Polletta, M., Owen, F., Berta, S., Shupe, D., Siana, B., Lonsdale, C., Strazzullo, V., Pannella, M., Baker, A. J., Beelen, A., Biggs, A., De Breuck, C., Farrah, D., Ivison, R., Lagache, G., Lutz, D., Tacconi, L. J., Zylka, R.
A complete sample of 33 sources believed to be starbursts ("5.8micron-peakers") was selected in the (0.5 sq. deg.) J1046+56 field with selection criteria F_(24micron)>400muJy, the presence of a redshifted stellar emission peak at 5.8um, and r'(Vega)>
Externí odkaz:
http://arxiv.org/abs/0910.3097
Autor:
Younger, J. D., Omont, A., Fiolet, N., Huang, J. -S., Fazio, G. G., Lai, K., Polletta, M., Rigopoulou, D., Zylka, R.
We present millimetre observations of a sample of 12 high redshift ultraluminous infrared galaxies (ULIRGs) in the Extended Growth Strip (EGS). These objects were initially selected on the basis of their observed mid--IR colours (0.0 < [3.6]-[4.5] <
Externí odkaz:
http://arxiv.org/abs/0812.2476
Autor:
Fiolet, N, Omont, A, Polletta, M, Owen, F, Berta, S, Shupe, D, Siana, B, Lonsdale, C, Strazzullo, V, Pannella, M, Baker, Aj, Beelen, A, Biggs, A, De Breuck, C, Farrah, D, Ivison, R, Lagache, G, Lutz, D, Tacconi, Lj, Zylka, R
Context. Wide-field Spitzer surveys allow identification of thousands of potentially high-z submillimeter galaxies (SMGs) through their bright 24 mu m emission and their mid-IR colors. Aims. We want to determine the average properties of such z simil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::c2492cb7cc7dc36f7795ed34c9590cea
https://hdl.handle.net/11368/2956869
https://hdl.handle.net/11368/2956869
Autor:
Oliver, SJ, 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, DL, Conley, A, Conversi, L, Cooray, A, Dowell, CD, Dubois, EN, 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, González Solares, EA, Griffin, M, Halpern, M, Harwit, M, Hatziminaoglou, E, Heinis, S, Hurley, P, Hwang, HS, Hyde, A, Ibar, E, Ilbert, O, Isaak, K, Ivison, RJ, Lagache, G, Le Floc'h, E, Levenson, L, Faro, BL, Lu, N, Madden, S, Maffei, B, Magdis, G, Mainetti, G, Marchetti, L, Marsden, G, Marshall, J, Mortier, AMJ, Nguyen, HT, O'Halloran, B, Omont, A, Page, MJ, Panuzzo, P, Papageorgiou, A, Patel, H, Pearson, CP, Pérez-Fournon, I, Pohlen, M, Rawlings, JI, Raymond, G, Rigopoulou, D, Riguccini, L, Rizzo, D, Rodighiero, G, Roseboom, IG, Rowan-Robinson, M
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 424(3)
The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme designed to map a set of nested fields totalling ~380deg 2. Fields range in size from 0.01 to ~20deg 2, using the Herschel-Spectral and Photometric Imaging Receiver (SPIRE)
Autor:
Omont, A., Neri, R., Cox, P., Lupu, R., Guélin, M., van der Werf, P., Weiß, A., Ivison, R., Negrello, M., Leeuw, L., Lehnert, M., Smail, I., Verma, A., Baker, A. J., Beelen, A., Aguirre, J. E., Baes, M., Bertoldi, F., Clements, D. L., Cooray, A., Coppin, K., Dannerbauer, H., De Zotti, G., Dye, Simon, Fiolet, N., Frayer, D., Gavazzi, R., Hughes, D., Jarvis, M., Krips, M., Michalowski, M. J., Murphy, E. J., Riechers, D., Serjeant, S., Swinbank, A. M., Temi, P., Vaccari, M., Vieira, J. D., Auld, Robbie Richard, Buttiglione, B., Cava, A., Dariush, Aliakbar, Dunne, L., Eales, Stephen Anthony, Fritz, J., Gomez, Haley Louise, Ibar, E., Maddox, S., Pascale, Enzo, Pohlen, Michael, Rigby, E., Smith, D. J. B., Bock, J., Bradford, C. M., Glenn, J., Scott, K. S., Zmuidzinas, J.
The Herschel survey, H-ATLAS, with its large areal coverage, has recently discovered a number of bright, strongly lensed high-z submillimeter galaxies. The strong magnification makes it possible to study molecular species other than CO, which are oth
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::cec8c8125dc7bc9adf9487709bc972e3
https://orca.cardiff.ac.uk/id/eprint/21847/1/Observation_of_H2O_in_a_strongly_lensed_Herschel-ATLAS_source.pdf
https://orca.cardiff.ac.uk/id/eprint/21847/1/Observation_of_H2O_in_a_strongly_lensed_Herschel-ATLAS_source.pdf