Zobrazeno 1 - 10
of 61
pro vyhledávání: '"Hills, R. E."'
Autor:
White, S. M., Iwai, K., Phillips, N. M., Hills, R. E., Hirota, A., Yagoubov, P., Siringo, G., Shimojo, M., Bastian, T. S., Hales, A. S., Sawada, T., Asayama, S., Sugimoto, M., Marson, R. G., Kawasaki, W., Muller, E., Nakazato, T., Sugimoto, K., Brajsa, R., Skokic, I., Barta, M., Kim, S., Remijan, A., de Gregorio, I., Corder, S. A., Hudson, H. S., Loukitcheva, M., Chen, B., De Pontieu, B., Fleishmann, G. D., Gary, D. E., Kobelski, A., Wedemeyer, S., Yan, Y.
The Atacama Large Millimeter-submillimeter Array (ALMA) radio telescope has commenced science observations of the Sun starting in late 2016. Since the Sun is much larger than the field of view of individual ALMA dishes, the ALMA interferometer is una
Externí odkaz:
http://arxiv.org/abs/1705.04766
Autor:
Shimojo, M., Bastian, T. S., Hales, A. S., White, S. M., Iwai, K., Hills, R. E., Hirota, A., Phillips, N. M., Sawada, T., Yagoubov, P., Siringo, G., Asayama, S., Sugimoto, M., Brajsa, R., Skokic, I., Barta, M., Kim, S., de Gregorio, I., Corder, S. A., Hudson, H. S., Wedemeyer, S., Gary, D. E., De Pontieu, B., Loukitcheva, M., Fleishman, G. D., Chen, B., Kobelski, A., Yan, Y.
Publikováno v:
Solar Physics Vol. 292: 87. (2017)
Observations of the Sun at millimeter and submillimeter wavelengths offer a unique probe into the structure, dynamics, and heating of the chromosphere; the structure of sunspots; the formation and eruption of prominences and filaments; and energetic
Externí odkaz:
http://arxiv.org/abs/1704.03236
Autor:
Partnership, ALMA, Fomalont, E. B., Vlahakis, C., Corder, S., Remijan, A., Barkats, D., Lucas, R., Hunter, T. R., Brogan, C. L., Asaki, Y., Matsushita, S., Dent, W. R. F., Hills, R. E., Phillips, N., Richards, A. M. S., Cox, P., Amestica, R., Broguiere, D., Cotton, W., Hales, A. S., Hiriart, R., Hirota, A., Hodge, J. A., Impellizzeri, C. M. V., Kern, J., Kneissl, R., Liuzzo, E., Marcelino, N., Marson, R., Mignano, A., Nakanishi, K., Nikolic, B., Perez, J. E., Pérez, L. M., Toledo, I., Aladro, R., Butler, B., Cortes, J., Cortes, P., Dhawan, V., Di Francesco, J., Espada, D., Galarza, F., Garcia-Appadoo, D., Guzman-Ramirez, L., Humphreys, E. M., Jung, T., Kameno, S., Laing, R. A., Leon, S., Mangum, J., Marconi, G., Nagai, H., Nyman, L. -A., Radiszcz, M., Rodón, J. A., Sawada, T., Takahashi, S., Tilanus, R. P. J., van Kempen, T., Vilaro, B. Vila, Watson, L. C., Wiklind, T., Gueth, F., Tatematsu, K., Wootten, A., Castro-Carrizo, A., Chapillon, E., Dumas, G., de Gregorio-Monsalvo, I., Francke, H., Gallardo, J., Garcia, J., Gonzalez, S., Hibbard, J. E., Hill, T., Kaminski, T., Karim, A., Krips, M., Kurono, Y., Lopez, C., Martin, S., Maud, L., Morales, F., Pietu, V., Plarre, K., Schieven, G., Testi, L., Videla, L., Villard, E., Whyborn, N., Zwaan, M. A., Alves, F., Andreani, P., Avison, A., Barta, M., Bedosti, F., Bendo, G. J., Bertoldi, F., Bethermin, M., Biggs, A., Boissier, J., Brand, J., Burkutean, S., Casasola, V., Conway, J., Cortese, L., Dabrowski, B., Davis, T. A., Trigo, M. Diaz, Fontani, F., Franco-Hernandez, R., Fuller, G., Madrid, R. Galvan, Giannetti, A., Ginsburg, A., Graves, S. F., Hatziminaoglou, E., Hogerheijde, M., Jachym, P., Serra, I. Jimenez, Karlicky, M., Klaasen, P., Kraus, M., Kunneriath, D., Lagos, C., Longmore, S., Leurini, S., Maercker, M., Magnelli, B., Vidal, I. Marti, Massardi, M., Maury, A., Muehle, S., Muller, S., Muxlow, T., O'Gorman, E., Paladino, R., Petry, D., Pineda, J., Randall, S., Richer, J. S., Rossetti, A., Rushton, A., Rygl, K., Monge, A. Sanchez, Schaaf, R., Schilke, P., Stanke, T., Schmalzl, M., Stoehr, F., Urban, S., van Kampen, E., Vlemmings, W., Wang, K., Wild, W., Yang, Y., Iguchi, S., Hasegawa, T., Saito, M., Inatani, J., Mizuno, N., Asayama, S., Kosugi, G., Morita, K. -I., Chiba, K., Kawashima, S., Okumura, S. K., Ohashi, N., Ogasawara, R., Sakamoto, S., Noguchi, T., Huang, Y. -D., Liu, S. -Y., Kemper, F., Koch, P. M., Chen, M. -T., Chikada, Y., Hiramatsu, M., Iono, D., Shimojo, M., Komugi, S., Kim, J., Lyo, A. -R., Muller, E., Herrera, C., Miura, R. E., Ueda, J., Chibueze, J., Su, Y. -N., Trejo-Cruz, A., Wang, K. -S., Kiuchi, H., Ukita, N., Sugimoto, M., Kawabe, R., Hayashi, M., Miyama, S., Ho, P. T. P., Kaifu, N., Ishiguro, M., Beasley, A. J., Bhatnagar, S., Braatz III, J. A., Brisbin, D. G., Brunetti, N., Carilli, C., Crossley, J. H., D'Addario, L., Meyer, J. L. Donovan, Emerson, D. T., Evans, A. S., Fisher, P., Golap, K., Griffith, D. M., Hale, A. E., Halstead, D., Hardy, E. J., Hatz, M. C., Holdaway, M., Indebetouw, R., Jewell, P. R., Kepley, A. A., Kim, D. -C., Lacy, M. D., Leroy, A. K., Liszt, H. S., Lonsdale, C. J., Matthews, B., McKinnon, M., Mason, B. S., Moellenbrock, G., Moullet, A., Myers, S. T., Ott, J., Peck, A. B., Pisano, J., Radford, S. J. E., Randolph, W. T., Venkata, U. Rao, Rawlings, M. G., Rosen, R., Schnee, S. L., Scott, K. S., Sharp, N. K., Sheth, K., Simon, R. S., Tsutsumi, T., Wood, S. J.
Publikováno v:
The Astrophysical Journal Letters, volume 808, issue 1, article id. L1, 11 pp. (2015)
A major goal of the Atacama Large Millimeter/submillimeter Array (ALMA) is to make accurate images with resolutions of tens of milliarcseconds, which at submillimeter (submm) wavelengths requires baselines up to ~15 km. To develop and test this capab
Externí odkaz:
http://arxiv.org/abs/1504.04877
Autor:
Partnership, ALMA, Vlahakis, C., Hunter, T. R., Hodge, J. A., Pérez, L. M., Andreani, P., Brogan, C. L., Cox, P., Martin, S., Zwaan, M., Matsushita, S., Dent, W. R. F., Impellizzeri, C. M. V., Fomalont, E. B., Asaki, Y., Barkats, D., Hills, R. E., Hirota, A., Kneissl, R., Liuzzo, E., Lucas, R., Marcelino, N., Nakanishi, K., Phillips, N., Richards, A. M. S., Toledo, I., Aladro, R., Broguiere, D., Cortes, J. R., Cortes, P. C., Espada, D., Galarza, F., Garcia-Appadoo, D., Guzman-Ramirez, L., Hales, A. S., Humphreys, E. M., Jung, T., Kameno, S., Laing, R. A., Leon, S., Marconi, G., Mignano, A., Nikolic, B., Nyman, L. -A., Radiszcz, M., Remijan, A., Rodón, J. A., Sawada, T., Takahashi, S., Tilanus, R. P. J., Vilaro, B. Vila, Watson, L. C., Wiklind, T., Ao, Y., Di Francesco, J., Hatsukade, B., Hatziminaoglou, E., Mangum, J., Matsuda, Y., van Kampen, E., Wootten, A., de Gregorio-Monsalvo, I., Dumas, G., Francke, H., Gallardo, J., Garcia, J., Gonzalez, S., Hill, T., Iono, D., Kaminski, T., Karim, A., Krips, M., Kurono, Y., Lonsdale, C., Lopez, C., Morales, F., Plarre, K., Videla, L., Villard, E., Hibbard, J. E., Tatematsu, K.
Publikováno v:
The Astrophysical Journal Letters, Volume 808, Issue 1, article id. L4, 10 pp. (2015)
We present initial results of very high resolution Atacama Large Millimeter/submillimeter Array (ALMA) observations of the $z$=3.042 gravitationally lensed galaxy HATLAS J090311.6+003906 (SDP.81). These observations were carried out using a very exte
Externí odkaz:
http://arxiv.org/abs/1503.02652
Atacama Large Millimeter/submillimeter Array (ALMA) will be the world largest mm/submm interferometer, and currently the Early Science is ongoing, together with the commissioning and science verification (CSV). Here we present a study of the temporal
Externí odkaz:
http://arxiv.org/abs/1210.5306
Autor:
Buckle, J. V., Hills, R. E., Smith, H., Dent, W. R. F., Bell, G., Curtis, E. I., Dace, R., Gibson, H., Graves, S. F., Leech, J., Richer, J. S., Williamson, R., Withington, S., Yassin, G., Bennett, R., Hastings, P., Laidlaw, I., Lightfoot, J. F., Burgess, T., Dewdney, P. E., Hovey, G., Willis, A. G., Redman, R., Wooff, B., Berry, D. S., Cavanagh, B., Davis, G. R., Dempsey, J., Friberg, P., Jenness, T., Kackley, R., Rees, N. P., Tilanus, R., Walther, C., Zwart, W., Klapwijk, T. M., Kroug, M., Zijlstra, T.
This paper describes a new Heterodyne Array Receiver Programme (HARP) and Auto-Correlation Spectral Imaging System (ACSIS) that have recently been installed and commissioned on the James Clerk Maxwell Telescope (JCMT). The 16-element focal-plane arra
Externí odkaz:
http://arxiv.org/abs/0907.3610
Autor:
Consortium, AMI, Zwart, J. T. L., Barker, R. W., Biddulph, P., Bly, D., Boysen, R. C., Brown, A. R., Clementson, C., Crofts, M., Culverhouse, T. L., Czeres, J., Dace, R. J., Davies, M. L., D'Alessandro, R., Doherty, P., Duggan, K., Ely, J. A., Felvus, M., Feroz, F., Flynn, W., Franzen, T. M. O., Geisbüsch, J., Génova-Santos, R., Grainge, K. J. B., Grainger, W. F., Hammett, D., Hills, R. E., Hobson, M. P., Holler, C. M., Hurley-Walker, N., Jilley, R., Jones, M. E., Kaneko, T., Kneissl, R., Lancaster, K., Lasenby, A. N., Marshall, P. J., Newton, F., Norris, O., Northrop, I., Odell, D. M., Pober, J. C., Pooley, G. G., Quy, V., Rodríguez-Gonzálvez, C., Saunders, R. D. E., Scaife, A. M., Schofield, J., Scott, P. F., Shaw, C., Shimwell, T. W., Smith, H., Taylor, A. C., Titterington, D. J., Velić, M., Waldram, E. M., West, S., Wood, B. A., Yassin, G.
The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz, with very high sensitivity to angular scales 30''-10'. The telescope is aimed principally at Sunyaev-Zel'dovich imaging
Externí odkaz:
http://arxiv.org/abs/0807.2469
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 384: 1207-1210 (2008)
We present the antenna design for a radio interferometer, the Arcminute Microkelvin Imager, together with its beam pattern measurement. Our aim was to develop a low-cost system with high aperture efficiency and low ground-spill across the frequency r
Externí odkaz:
http://arxiv.org/abs/0712.0911
Autor:
Ward-Thompson, D., Di Francesco, J., Hatchell, J., Hogerheijde, M. R., Bastien, P., Basu, S., Bonnell, I., Bowey, J., Brunt, C., Buckle, J., Butner, H., Cavanagh, B., Chrysostomou, A., Curtis, E., Davis, C. J., Dent, W. R. F., van Dishoeck, E., Edmunds, M. G., Fich, M., Fiege, J., Fissel, L., Friberg, P., Friesen, R., Frieswijk, W., Fuller, G. A., Gosling, A., Graves, S., Greaves, J. S., Helmich, F., Hills, R. E., Holland, W. S., Houde, M., Jayawardhana, R., Johnstone, D., Joncas, G., Kirk, H., Kirk, J. M., Knee, L. B. G., Matthews, B., Matthews, H., Matzner, C., Moriarty-Schieven, G. H., Naylor, D., Nutter, D., Padman, R., Plume, R., Rawlings, J. M. C., Redman, R. O., Reid, M., Richer, J. S., Shipman, R., Simpson, R. J., Spaans, M., Stamatellos, D., Tsanis, Y., Viti, S., Weferling, B., White, G. J., Whitworth, A. P., Wouterloot, J., Yates, J., Zhu, M.
This paper describes a James Clerk Maxwell Telescope (JCMT) legacy survey that has been awarded roughly 500 hrs of observing time to be carried out from 2007 to 2009. In this survey we will map with SCUBA-2 (Submillimetre Common User Bolometer Array
Externí odkaz:
http://arxiv.org/abs/0707.0169
We describe phase-retrieval holography measurements of the 100-m diameter Green Bank Telescope using astronomical sources and an astronomical receiver operating at a wavelength of 7 mm. We use the technique with parameterization of the aperture in te
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612249