Zobrazeno 1 - 10
of 141
pro vyhledávání: '"Smee, S."'
Autor:
Arnquist, I., Avalos, N., Bailly, P., Baxter, D., Bertou, X., Bogdan, M., Bourgeois, C., Brandt, J., Cadiou, A., Castello-Mor, N., Chavarria, A. E., Conde, M., Cuevas-Zepeda, J., Dastgheibi-Fard, A., De Dominicis, C., Deligny, O., Desani, R., Dhellot, M., Duarte-Campderros, J., Estrada, E., Florin, D., Gadola, N., Gaior, R., Gkougkousis, E. -L., Sanchez, J. Gonzalez, Hope, S., Hossbach, T., Huehn, M., Kallander, M., Kilminster, B., Iddir, L., Lantero-Barreda, A., Lawson, I., Lebbolo, H., Lee, S., Leray, P., Selvon, A. Letessier, Lin, H., Loaiza, P., Lopez-Virto, A., Martin, D., McGuire, K. J., Milleto, T., Mitra, P., Martin, D. Moya, Munagavalasa, S., Norcini, D., Overman, C., Paul, S., Peterson, D., Piers, A., Pochon, O., Privitera, P., Reynet, D., Roach, B. A., Robmann, P., Roehnelt, R., Settimo, M., Smee, S., Smida, R., Stillwell, B., Van Wechel, T., Traina, M., Vilar, R., Vollhardt, A., Warot, G., Wolf, D., Yajur, R., Zopounidis, J-P.
The DArk Matter In CCDs at Modane (DAMIC-M) experiment is designed to search for light dark matter (m$_{\chi}$<10\,GeV/c$^2$) at the Laboratoire Souterrain de Modane (LSM) in France. DAMIC-M will use skipper charge-coupled devices (CCDs) as a kg-scal
Externí odkaz:
http://arxiv.org/abs/2407.17872
Autor:
Wilson, J. C., Hearty, F. R., Skrutskie, M. F., Majewski, S. R., Holtzman, J. A., Eisenstein, D., Gunn, J., Blank, B., Henderson, C., Smee, S., Nelson, M., Nidever, D., Arns, J., Barkhouser, R., Barr, J., Beland, S., Bershady, M. A., Blanton, M. R., Brunner, S., Burton, A., Carey, L., Carr, M., Colque, J. P., Crane, J., Damke, G. J., Davidson Jr., J. W., Dean, J., Di Mille, F., Don, K. W., Ebelke, G., Evans, M., Fitzgerald, G., Gillespie, B., Hall, M., Harding, A., Harding, P., Hammond, R., Hancock, D., Harrison, C., Hope, S., Horne, T., Karakla, J., Lam, C., Leger, F., MacDonald, N., Maseman, P., Matsunari, J., Melton, S., Mitcheltree, T., O'Brien, T., O'Connell, R. W., Patten, A., Richardson, W., Rieke, G., Rieke, M., Roman-Lopes, A., Schiavon, R. P., Sobeck, J. S., Stolberg, T., Stoll, R., Tembe, M., Trujillo, J. D., Uomoto, A., Vernieri, M., Walker, E., Weinberg, D. H., Young, E., Anthony-Brumfield, B., Bizyaev, D., Breslauer, B., De Lee, N., Downey, J., Halverson, S., Huehnerhoff, J., Klaene, M., Leon, E., Long, D., Mahadevan, S., Malanushenko, E., Nguyen, D. C., Owen, R., Sanchez-Gallego, J. R., Sayres, C., Shane, N., Shectman, S. A., Shetrone, M., Skinner, D., Stauffer, F., Zhao, B.
We describe the design and performance of the near-infrared (1.51--1.70 micron), fiber-fed, multi-object (300 fibers), high resolution (R = lambda/delta lambda ~ 22,500) spectrograph built for the Apache Point Observatory Galactic Evolution Experimen
Externí odkaz:
http://arxiv.org/abs/1902.00928
Autor:
Madec, F., Fur, A. Le, Mignant, D. Le, Dohlen, K., Barrette, R., Belhadi, M., Pascal, S., Smee, S., Gunn, J., Merrer, J. Le, Lorred, M., Jaquet, M., Balard, P., Blanchard, P., Thao, W., Roman, F., Lapere, V., Gabriel, JF, Loomis, C., Golebiowski, M., Hart, M., Oliveira, L., Oliveira, A., Tamura, N., Shimono, A.
The Prime Focus Spectrograph (PFS) of the Subaru Measurement of Images and Redshifts (SuMIRe) project for Subaru telescope consists in four identical spectrographs fed by 600 fibers each. Each spectrograph is composed by an optical entrance unit that
Externí odkaz:
http://arxiv.org/abs/1608.01287
Autor:
Vives, S., Mignant, D. Le, Gunn, J. E., Smee, S., de Oliveira, L. Souza, Tamura, N., Sugai, H., Barkhouser, R., Bozier, A., Carr, M. A., de Oliveira, A. Cesar, Ferrand, D., Golebiowski, M., Hart, M., Hope, S., Jaquet, M., Madec, F., Pascal, S., Pegot-Ogier, T., de Arruda, M. Vittal
The Prime Focus Spectrograph (PFS) is a new facility instrument for Subaru Telescope which will be installed in around 2017. It is a multi-object spectrograph fed by about 2400 fibers placed at the prime focus covering a hexagonal field-of-view with
Externí odkaz:
http://arxiv.org/abs/1408.2827
Autor:
Harris, H. C., Hansen, B. M. S., Liebert, J., Berk, D. E. Vanden, Anderson, S. F., Knapp, G. R., Fan, X., Margon, B., Munn, J. A., Nichol, R. C., Pier, J. R., Schneider, D. P., Smith, J. A., Winget, D. E., York, D. G., Anderson Jr, J. E., Brinkmann, J., Burles, S., Chen, B., Connolly, A. J., Csabai, I., Frieman, J. A., Gunn, J. E., Hennessy, G. S., Hindsley, R. B., Ivezic, Z., Kent, S., Lamb, D. Q., Lupton, R. H., Newberg, H. J., Schlegel, D. J., Smee, S., Strauss, M. A., Thakar, A. R., Uomoto, A., Yanny, B.
Publikováno v:
Astrophys.J. 549 (2001) L109-L113
Early data taken during commissioning of the SDSS have resulted in the discovery of a very cool white dwarf. It appears to have stronger collision induced absorption from molecular hydrogen than any other known white dwarf, suggesting it has a cooler
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101021
Autor:
Henderson, S., Abraham, W., Aleksandrov, A., Allen, C., Alonso, J., Anderson, D., Arenius, D., Arthur, T., Assadi, S., Ayers, J., Bach, P., Badea, V., Battle, R., Beebe-Wang, J., Bergmann, B., Bernardin, J., Bhatia, T., Billen, J., Birke, T., Bjorklund, E., Blaskiewicz, M., Blind, B., Blokland, W., Bookwalter, V., Borovina, D., Bowling, S., Bradley, J., Brantley, C., Brennan, J., Brodowski, J., Brown, S., Brown, R., Bruce, D., Bultman, N., Cameron, P., Campisi, I., Casagrande, F., Catalan-Lasheras, N., Champion, M., Chen, Z., Cheng, D., Cho, Y., Christensen, K., Chu, C., Cleaves, J., Connolly, R., Cote, T., Cousineau, S., Crandall, K., Creel, J., Crofford, M., Cull, P., Cutler, R., Dabney, R., Dalesio, L., Daly, E., Damm, R., Danilov, V., Davino, D., Davis, K., Dawson, C., Day, L., Deibele, C., Delayen, J., DeLong, J., Demello, A., DeVan, W., Digennaro, R., Dixon, K., Dodson, G., Doleans, M., Doolittle, L., Doss, J., Drury, M., Elliot, T., Ellis, S., Error, J., Fazekas, J., Fedotov, A., Feng, P., Fischer, J., Fox, W., Fuja, R., Funk, W., Galambos, J., Ganni, V., Garnett, R., Geng, X., Gentzlinger, R., Giannella, M., Gibson, P., Gillis, R., Gioia, J., Gordon, J., Gough, R., Greer, J., Gregory, W., Gribble, R., Grice, W., Gurd, D., Gurd, P., Guthrie, A., Hahn, H., Hardek, T., Hardekopf, R., Harrison, J., Hatfield, D., He, P., Hechler, M., Heistermann, F., Helus, S., Hiatt, T., Hicks, S., Hill, J., Hoff, L., Hoff, M., Hogan, J., Holding, M., Holik, P., Holmes, J., Holtkamp, N., Hovater, C., Howell, M., Hseuh, H., Huhn, A., Hunter, T., Ilg, T., Jackson, J., Jain, A., Jason, A., Jeon, D., Johnson, G., Jones, A., Joseph, S., Justice, A., Kang, Y., Kasemir, K., Keller, R., Kersevan, R., Kerstiens, D., Kesselman, M., Kim, S., Kneisel, P., Kravchuk, L., Kuneli, T., Kurennoy, S., Kustom, R., Kwon, S., Ladd, P., Lambiase, R., Lee, Y.Y., Leitner, M., Leung, K.-N., Lewis, S., Liaw, C., Lionberger, C., Lo, C.C., Long, C., Ludewig, H., Ludvig, J., Luft, P., Lynch, M., Ma, H., MacGill, R., Macha, K., Madre, B., Mahler, G., Mahoney, K., Maines, J., Mammosser, J., Mann, T., Marneris, I., Marroquin, P., Martineau, R., Matsumoto, K., McCarthy, M., McChesney, C., McGahern, W., McGehee, P., Meng, W., Merz, B., Meyer, R., Jr., Meyer, R., Sr., Miller, B., Mitchell, R., Mize, J., Monroy, M., Munro, J., Murdoch, G., Musson, J., Nath, S., Nelson, R., O׳Hara, J., Olsen, D., Oren, W., Oshatz, D., Owens, T., Pai, C., Papaphilippou, I., Patterson, N., Patterson, J., Pearson, C., Pelaia, T., Pieck, M., Piller, C., Plawski, T., Plum, M., Pogge, J., Power, J., Powers, T., Preble, J., Prokop, M., Pruyn, J., Purcell, D., Rank, J., Raparia, D., Ratti, A., Reass, W., Reece, K., Rees, D., Regan, A., Regis, M., Reijonen, J., Rej, D., Richards, D., Richied, D., Rode, C., Rodriguez, W., Rodriguez, M., Rohlev, A., Rose, C., Roseberry, T., Jr., Rowton, L., Roybal, W., Rust, K., Salazer, G., Sandberg, J., Saunders, J., Schenkel, T., Schneider, W., Schrage, D., Schubert, J., Severino, F., Shafer, R., Shea, T., Shishlo, A., Shoaee, H., Sibley, C., Sims, J., Smee, S., Smith, J., Smith, K., Spitz, R., Staples, J., Stein, P., Stettler, M., Stirbet, M., Stockli, M., Stone, W., Stout, D., Stovall, J., Strelo, W., Strong, H., Sundelin, R., Syversrud, D., Szajbler, M., Takeda, H., Tallerico, P., Tang, J., Tanke, E., Tepikian, S., Thomae, R., Thompson, D., Thomson, D., Thuot, M., Treml, C., Tsoupas, N., Tuozzolo, J., Tuzel, W., Vassioutchenko, A., Virostek, S., Wallig, J., Wanderer, P., Wang, Y., Wang, J.G., Wangler, T., Warren, D., Wei, J., Weiss, D., Welton, R., Weng, J., Weng, W-T., Wezensky, M., White, M., Whitlatch, T., Williams, D., Williams, E., Wilson, K., Wiseman, M., Wood, R., Wright, P., Wu, A., Ybarrolaza, N., Young, K., Young, L., Yourd, R., Zachoszcz, A., Zaltsman, A., Zhang, S., Zhang, W., Zhang, Y., Zhukov, A.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 1 November 2014 763:610-673
Autor:
Persson, S. E., Murphy, D. C., Smee, S., Birk, C., Monson, A. J., Uomoto, A., Koch, E., Shectman, S., Barkhouser, R., Orndorff, J., Hammond, R., Harding, A., Scharfstein, G., Kelson, D., Marshall, J., McCarthy, P. J.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2013 . 125(928), 654-682.
Externí odkaz:
https://www.jstor.org/stable/10.1086/671164
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2011 01. 123(899), 87-106.
Externí odkaz:
https://www.jstor.org/stable/10.1086/658238
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.