Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Naylor, B. J."'
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:
Bradford, C. M., Bolatto, A. D., Maloney, P. R., Aguirre, J. E., Bock, J. J., Glenn, J., Kamenetzky, J., Lupu, R., Matsuhara, H., Murphy, E. J., Naylor, B. J., Nguyen, H. T., Scott, K., Zmuidzinas, J.
We present the rest-frame 200--320 \mm\ spectrum of the z=3.91 quasar \apm, obtained with Z-Spec at the Caltech Submillimeter Observatory. In addition to the \jeight\ to \jthirteen\ CO rotational transitions which dominate the CO cooling, we find six
Externí odkaz:
http://arxiv.org/abs/1106.4301
Autor:
Gavazzi, R., Cooray, A., Conley, A., Aguirre, J. E., Amblard, A., Auld, R., Beelen, A., Blain, A., Blundell, R., Bock, J., Bradford, C. M., Bridge, C., Brisbin, D., Burgarella, D., Chanial, P., Chapin, E., Christopher, N., Clements, D. L., Cox, P., Djorgovski, S. G., Dowell, C. D., Eales, S., Earle, L., Ellsworth-Bowers, T. P., Farrah, D., Franceschini, A., Fu, H., Glenn, J., Solares, E. A. González, Griffin, M., Gurwell, M. A., Halpern, M., Ibar, E., Ivison, R. J., Jarvis, M., Kamenetzky, J., Kim, S., Krips, M., Levenson, L., Lupu, R., Mahabal, A., Maloney, P. D., Maraston, C., Marchetti, L., Marsden, G., Matsuhara, H., Mortier, A. M. J., Murphy, E., Naylor, B. J., Neri, R., Nguyen, H. T., Oliver, S. J., Omont, A., Page, M. J., Papageorgiou, A., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rangwala, N., Rawlings, J. I., Raymond, G., Riechers, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Schulz, B., Scott, Douglas, Scott, K. S., Serra, P., Seymour, N., Shupe, D. L., Smith, A. J., Symeonidis, M., Tugwell, K. E., Vaccari, M., Valiante, E., Valtchanov, I., Verma, A., Vieira, J. D., Vigroux, L., Wang, L., Wardlow, J., Wiebe, D., Wright, G., Xu, C. K., Zeimann, G., Zemcov, M., Zmuidzinas, J.
We present the results of a gravitational lensing analysis of the bright $\zs=2.957$ sub-millimeter galaxy (SMG), HERMES J105751.1+573027 found in {\it Herschel}/SPIRE Science Demonstration Phase data from the Herschel Multi-tiered Extragalactic Surv
Externí odkaz:
http://arxiv.org/abs/1104.4119
Autor:
Conley, A., Cooray, A., Vieira, J. D., Solares, E. A. González, Kim, S., Aguirre, J. E., Amblard, A., Auld, R., Baker, A. J., Beelen, A., Blain, A., Blundell, R., Bock, J., Bradford, C. M., Bridge, C., Brisbin, D., Burgarella, D., Carpenter, J. M., Chanial, P., Chapin, E., Christopher, N., Clements, D. L., Cox, P., Djorgovski, S. G., Dowell, C. D., Eales, S., Earle, L., Ellsworth-Bowers, T. P., Farrah, D., Franceschini, A., Frayer, D., Fu, H., Gavazzi, R., Glenn, J., Griffin, M., Gurwell, M. A., Halpern, M., Ibar, E., Ivison, R. J., Jarvis, M., Kamenetzky, J., Krips, M., Levenson, L., Lupu, R., Mahabal, A., Maloney, P. D., Maraston, C., Marchetti, L., Marsden, G., Matsuhara, H., Mortier, A. M. J., Murphy, E., Naylor, B. J., Neri, R., Nguyen, H. T., Oliver, S. J., Omont, A., Page, M. J., Papageorgiou, A., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rangwala, N., Rawlings, J. I., Raymond, G., Riechers, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Schulz, B., Scott, Douglas, Scott, K., Serra, P., Seymour, N., Shupe, D. L., Smith, A. J., Symeonidis, M., Tugwell, K. E., Vaccari, M., Valiante, E., Valtchanov, I., Verma, A., Viero, M. P., Vigroux, L., Wang, L., Wiebe, D., Wright, G., Xu, C. K., Zeimann, G., Zemcov, M., Zmuidzinas, J.
Publikováno v:
ApJ, 732, L35 (2011)
We report the discovery of a bright ($f(250\mum) > 400$ mJy), multiply-lensed submillimeter galaxy \obj\ in {\it Herschel}/SPIRE Science Demonstration Phase data from the HerMES project. Interferometric 880\mum\ Submillimeter Array observations resol
Externí odkaz:
http://arxiv.org/abs/1104.4113
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:
Kamenetzky, J., Glenn, J., Maloney, P. R., Aguirre, J. E., Bock, J. J., Bradford, C. M., Earle, L., Inami, H., Matsuhara, H., Murphy, E. J., Naylor, B. J., Nguyen, H. T., Zmuidzinas, J.
We present a 190-307 GHz broadband spectrum obtained with Z-Spec of NGC 1068 with new measurements of molecular rotational transitions. After combining our measurements with those previously published and considering the specific geometry of this Sey
Externí odkaz:
http://arxiv.org/abs/1102.3915
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
Autor:
Ikarashi, S., Kohno, K., Aguirre, J. E., Aretxaga, I., Arumugam, V., Austermann, J. E., Bock, J. J., Bradford, C. M., Cirasuolo, M., Earle, L., Ezawa, H., Furusawa, H., Furusawa, J., Glenn, J., Hatsukade, B., Hughes, D. H., Iono, D., Ivison, R. J., Johnson, S., Kamenetzky, J., Kawabe, R., Lupu, R., Maloney, P., Matsuhara, H., Mauskopf, P. D., Motohara, K., Murphy, E. J., Nakajima, K., Nakanishi, K., Naylor, B. J., Nguyen, H. T., Perera, T. A., Scott, K. S., Shimasaku, K., Takagi, T., Takata, T., Tamura, Y., Tanaka, K., Tsukagoshi, T., Wilner, D. J., Wilson, G. W., Yun, M. S., Zmuidzinas, J.
We report the detection of an extremely bright ($\sim$37 mJy at 1100 $\mu$m and $\sim$91 mJy at 880 $\mu$m) submillimeter galaxy (SMG), AzTEC-ASTE-SXDF1100.001 (hereafter referred to as SXDF1100.001 or Orochi), discovered in 1100 $\mu$m observations
Externí odkaz:
http://arxiv.org/abs/1009.1455
Autor:
Naylor, B. J., Bradford, C. M., Aguirre, J. E., Bock, J. J., Earle, L., Glenn, J., Inami, H., Kamenetzky, J., Maloney, P. R., Matsuhara, H., Nguyen, H. T., Zmuidzinas, J.
We present a three-pointing study of the molecular gas in the starburst nucleus of M82 based on 190 - 307 GHz spectra obtained with Z-Spec at the Caltech Submillimeter Observatory. We present intensity measurements, detections and upper limits, for 2
Externí odkaz:
http://arxiv.org/abs/1006.1964