Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Lupu, R. E."'
Autor:
Lupu, R. E., Zahnle, Kevin, Marley, Mark S., Schaefer, Laura, Fegley, Bruce, Morley, Caroline, Cahoy, Kerri, Freedman, Richard, Fortney, Jonathan J.
It is now understood that the accretion of terrestrial planets naturally involves giant collisions, the moon-forming impact being a well known example. In the aftermath of such collisions the surface of the surviving planet is very hot and potentiall
Externí odkaz:
http://arxiv.org/abs/1401.1499
Autor:
Bothwell, M. S., Aguirre, J. E., Chapman, S. C., Marrone, D. P., Vieira, J. D., Ashby, M. L. N., Aravena, M., Benson, B. A., Bock, J. J., Bradford, C. M., Brodwin, M., Carlstrom, J., Crawford, T. M., de Breuck, C., Downes, T. P., Fassnacht, C. D., Gonzalez, A. H., Greve, T. R., Gullberg, B., Hezaveh, Y., Holder, G. P., Holzapfel, W. L., Ibar, E., Ivison, R., Kamenetzky, J., Keisler, R., Lupu, R. E., Ma, J., Malkan, M., McIntyre, V., Murphy, E. J., Nguyen, H. T., Reichardt, C. L., Rosenman, M., Spilker, J. S., Stalder, B., Stark, A. A., Strandet, M., Vernet, J., Weiss, A., Welikala, N.
We present observations of SPT-S J053816-5030.8, a gravitationally-lensed dusty star forming galaxy (DSFG) at z = 2.7817, first discovered at millimeter wavelengths by the South Pole Telescope. SPT 0538-50 is typical of the brightest sources found by
Externí odkaz:
http://arxiv.org/abs/1309.3275
Autor:
Pearson, E. A., Eales, S., Dunne, L., Nuevo, J. Gonzalez, Maddox, S., Aguirre, J. E., Baes, M., Baker, A. J., Bourne, N., Bradford, C. M., Clark, C. J. R., Cooray, A., Dariush, A., De Zotti, G., Dye, S., Frayer, D., Gomez, H. L., Harris, A. I., Hopwood, R., Ibar, E., Ivison, R. J., Jarvis, M., Krips, M., Lapi, A., Lupu, R. E., Michałowski, M. J., Rosenman, M., Scott, D., Valiante, E., Valtchanov, I., van der Werf, P., Vieira, J. D.
Upon its completion the Herschel ATLAS (H-ATLAS) will be the largest submillimetre survey to date, detecting close to half-a-million sources. It will only be possible to measure spectroscopic redshifts for a small fraction of these sources. However,
Externí odkaz:
http://arxiv.org/abs/1308.5681
Autor:
Riechers, Dominik A., Bradford, C. M., Clements, D. L., Dowell, C. D., Perez-Fournon, I., Ivison, R. J., Bridge, C., Conley, A., Fu, Hai, Vieira, J. D., Wardlow, J., Calanog, J., Cooray, A., Hurley, P., Neri, R., Kamenetzky, J., Aguirre, J. E., Altieri, B., Arumugam, V., Benford, D. J., Bethermin, M., Bock, J., Burgarella, D., Cabrera-Lavers, A., Chapman, S. C., Cox, P., Dunlop, J. S., Earle, L., Farrah, D., Ferrero, P., Franceschini, A., Gavazzi, R., Glenn, J., Solares, E. A. Gonzalez, Gurwell, M. A., Halpern, M., Hatziminaoglou, E., Hyde, A., Ibar, E., Kovacs, A., Krips, M., Lupu, R. E., Maloney, P. R., Martinez-Navajas, P., Matsuhara, H., Murphy, E. J., Naylor, B. J., Nguyen, H. T., Oliver, S. J., Omont, A., Page, M. J., Petitpas, G., Rangwala, N., Roseboom, I. G., Scott, D., Smith, A. J., Staguhn, J. G., Streblyanska, A., Thomson, A. P., Valtchanov, I., Viero, M., Wang, L., Zemcov, M., Zmuidzinas, J.
Publikováno v:
Nature 496:329-333,2013
Massive present-day early-type (elliptical and lenticular) galaxies probably gained the bulk of their stellar mass and heavy elements through intense, dust-enshrouded starbursts - that is, increased rates of star formation - in the most massive dark
Externí odkaz:
http://arxiv.org/abs/1304.4256
Autor:
Scott, K. S., Lupu, R. E., Aguirre, J. E., Auld, R., Aussel, H., Baker, A. J., Beelen, A., Bock, J., Bradford, C. M., Brisbin, D., Burgarella, D., Carpenter, J. M., Chanial, P., Chapman, S. C., Clements, D. L., Conley, A., Cooray, A., Cox, P., Dowell, C. D., Eales, S., Farrah, D., Franceschini, A., Frayer, D. T., Gavazzi, R., Glenn, J., Griffin, M., Harris, A. I., Ibar, E., Ivison, R. J., Kamenetzky, J., Kim, S., Krips, M., Maloney, P. R., Matsuhara, H., Mortier, A. M. J., Murphy, E. J., Naylor, B. J., Neri, R., Nguyen, H. T., Oliver, S. J., Omont, A., Page, M. J., Papageorgiou, A., Pearson, C. P., Perez-Fournon, I., Pohlen, M., Rawlings, J. I., Raymond, G., Riechers, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Scott, D., Seymour, N., Smith, A. J., Symeonidis, M., Tugwell, K. E., Vaccari, M., Vieira, J. D., Vigroux, L., Wang, L., Wright, G., Zmuidzinas, J.
We report on the redshift measurement and CO line excitation of HERMES J105751.1+573027 (HLSW-01), a strongly lensed submillimeter galaxy discovered in Herschel/SPIRE observations as part of the Herschel Multi-tiered Extragalactic Survey (HerMES). HL
Externí odkaz:
http://arxiv.org/abs/1104.4115
Autor:
Negrello, Mattia, Hopwood, R., De Zotti, G., Cooray, A., Verma, A., Bock, J., Frayer, D. T., Gurwell, M. A., Omont, A., Neri, R., Dannerbauer, H., Leeuw, L. L., Barton, E., Cooke, J., Kim, S., da Cunha, E., Rodighiero, G., Cox, P., Bonfield, D. G., Jarvis, M. J., Serjeant, S., Ivison, R. J., Dye, S., Aretxaga, I., Hughes, D. H., Ibar, E., Bertoldi, F., Valtchanov, I., Eales, S., Dunne, L., Driver, S. P., Auld, R., Buttiglione, S., Cava, A., Grady, C. A., Clements, D. L., Dariush, A., Fritz, J., Hill, D., Hornbeck, J. B., Kelvin, L., Lagache, G., Lopez-Caniego, M., Gonzalez-Nuevo, J., Maddox, S., Pascale, E., Pohlen, M., Rigby, E. E., Robotham, A., Simpson, C., Smith, D. J. B., Temi, P., Thompson, M. A., Woodgate, B. E., York, D. G., Aguirre, J. E., Beelen, A., Blain, A., Baker, A. J., Birkinshaw, M., Blundell, R., Bradford, C. M., Burgarella, D., Danese, L., Dunlop, J. S., Fleuren, S., Glenn, J., Harris, A. I., Kamenetzky, J., Lupu, R. E., Maddalena, R. J., Madore, B. F., Maloney, P. R., Matsuhara, H., Michalowski, M. J., Murphy, E. J., Naylor, B. J., Nguyen, H., Popescu, C., Rawlings, S., Rigopoulou, D., Scott, D., Scott, K. S., Seibert, M., Smail, I., Tuffs, R. J., Vieira, J. D., van der Werf, P. P., Zmuidzinas, J.
Gravitational lensing is a powerful astrophysical and cosmological probe and is particularly valuable at submillimeter wavelengths for the study of the statistical and individual properties of dusty starforming galaxies. However the identification of
Externí odkaz:
http://arxiv.org/abs/1011.1255
Autor:
Lupu, R. E., Scott, K. S., Aguirre, J. E., Aretxaga, I., Auld, R., Barton, E., Beelen, A., Bertoldi, F., Bock, J. J., Bonfield, D., Bradford, C. M., Buttiglione, S., Cava, A., Clements, D. L., Cooke, J., Cooray, A., Dannerbauer, H., Dariush, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Frayer, D., Fritz, J., Glenn, J., Hughes, D. H., Ibar, E., Ivison, R. J., Jarvis, M. J., Kamenetzky, J., Kim, S., Lagache, G., Leeuw, L., Maddox, S., Maloney, P. R., Matsuhara, H., Murphy, E. J., Naylor, B. J., Negrello, M., Nguien, H., Omont, A., Pascale, E., Pohlen, M., Rigby, E., Rodighiero, G., Serjeant, S., Smith, D., Temi, P., Thompson, M., Valtchanov, I., Verma, A., Vieira, J. D., Zmuidzinas, J.
We present new observations from Z-Spec, a broadband 185-305 GHz spectrometer, of five sub-millimeter bright lensed sources selected from the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) science demonstration phase (SDP) catalog. We c
Externí odkaz:
http://arxiv.org/abs/1009.5983
We present the modeling of partial frequency redistribution (PRD) effects for the fluorescent emission lines of molecular hydrogen, the general computational approximations, and the applications to planetary atmospheres, as well as interstellar mediu
Externí odkaz:
http://arxiv.org/abs/0812.2046
Publikováno v:
Astrophys.J. 644 (2006) 981-989
We report the first observation of Ly$\alpha$ pumped molecular hydrogen emission lines in planetary nebulae. The H$_{2}$ emission observed in the ultraviolet spectra of NGC 6853 and NGC 3132 can be explained by excitation of vibrationally hot H$_{2}$
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602547
Autor:
Lupu, R. E., Scott, K. S., Aguirre, J. E., Aretxaga, I., Auld, R., Barton, E., Beelen, A., Bertoldi, F., Bock, J. J., Bonfield, D., Bradford, C. M., Buttiglione, S., Cava, A., Clements, D. L., Cooke, J., Cooray, A., Dannerbauer, H., Dariush, A., De, Zotti G., Dunne, L., Dye, S., Eales, S., Frayer, D., Fritz, J., Glenn, J., Hughes, D. H., Ibar, E., Ivison, R. J., Jarvis, M. J., Kamenetzky, J., Kim, S., Lagache, G., Leeuw, L., Maddox, S., Maloney, P. R., Matsuhara, Hideo
著者人数: 53名
Accepted: 2012-08-13
資料番号: SA1004172000
Accepted: 2012-08-13
資料番号: SA1004172000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2065b1703ffee129f1d0e7141f85b0a4
http://hdl.handle.net/11573/961484
http://hdl.handle.net/11573/961484