Zobrazeno 51 - 60
of 14 144
pro vyhledávání: '"Smith, N. A."'
Autor:
Foley, R. J., Alexander, K. D., Andreoni, I., Arcavi, I., Auchettl, K., Barnes, J., Baym, G., Bellm, E. C., Beloborodov, A. M., Blagorodnova, N., Blakeslee, J. P., Brady, P. R., Branchesi, M., Brown, J. S., Butler, N., Cantiello, M., Chornock, R., Cook, D. O., Cooke, J., Coppejans, D. L., Corsi, A., Couch, S. M., Coughlin, M. W., Coulter, D. A., Cowperthwaite, P. S., Dietrich, T., Dimitriadis, G., Drout, M. R., Elias, J. H., Farr, B., Fernandez, R., Filippenko, A. V., Fong, W., Fragos, T., Frail, D. A., Freedman, W. L., Fryer, C. L., Golkhou, V. Z., Hiramatsu, D., Hjorth, J., Horesh, A., Hosseinzadeh, G., Hotokezaka, K., Howell, D. A., Hung, T., Jones, D. O., Kalogera, V., Kasen, D., Kerzendorf, W. E., Kilpatrick, C. D., Kirshner, R. P., Krisciunas, K., Lattimer, J. M., Lazzati, D., Levan, A. J., MacFadyen, A. I., Maeda, K., Mandel, I., Mandel, K. S., Margalit, B., Margutti, R., McIver, J., Metzger, B. D., Mooley, K., Moriya, T., Murguia-Berthier, A., Narayan, G., Nicholl, M., Nissanke, S., Nomoto, K., O'Meara, J. M., O'Shaughnessy, R., O'Connor, E., Palmese, A., Pan, Y. -C., Pankow, C., Paterson, K., Perley, D. A., Perna, R., Piro, A. L., Pritchard, T. A., Quataert, E., Radice, D., Ramirez-Ruiz, E., Reddy, S., Rest, A., Riess, A. G., Rodriguez, C. L., Rojas-Bravo, C., Rossi, E. M., Rosswog, S., Ruiz, M., Shapiro, S. L., Shoemaker, D. H., Siebert, M. R., Siegel, D. M., Siellez, K., Smith, N., Soares-Santos, M., Suntzeff, N. B., Surman, R., Tanaka, M., Tanvir, N. R., Terreran, G., Valenti, S., Villar, V. A., Wang, L., Webb, S. A., Wheeler, J. C., Williams, P. K. G., Woosley, S., Zaldarriaga, M., Zevin, M.
As of today, we have directly detected exactly one source in both gravitational waves (GWs) and electromagnetic (EM) radiation, the binary neutron star merger GW170817, its associated gamma-ray burst GRB170817A, and the subsequent kilonova SSS17a/AT
Externí odkaz:
http://arxiv.org/abs/1903.04553
Autor:
Azzi, P., Farry, S., Nason, P., Tricoli, A., Zeppenfeld, D., Khalek, R. Abdul, Alimena, J., Andari, N., Bella, L. Aperio, Armbruster, A. J., Baglio, J., Bailey, S., Bakos, E., Bakshi, A., Baldenegro, C., Balli, F., Barker, A., Barter, W., de Blas, J., Blekman, F., Bloch, D., Bodek, A., Boonekamp, M., Boos, E., Sola, J. D. Bossio, Cadamuro, L., Camarda, S., Campanario, F., Campanelli, M., Campbell, J. M., Cao, Q. -H., Cavaliere, V., Cerri, A., Chahal, G. S., Chargeishvili, B., Charlot, C., Chen, S. -L., Chen, T., Cieri, L., Ciuchini, M., Corcella, G., Cotogno, S., Covarelli, R., Cruz-Martinez, J. M., Czakon, M., Dainese, A., Dang, N. P., Darmé, L., Dawson, S., De la Torre, H., Deile, M., Deliot, F., Demers, S., Denner, A., Derue, F., Di Ciaccio, L., Di Clemente, W. K., Damiani, D. Dominguez, Dudko, L., Durglishvili, A., Dünser, M., Ebadi, J., De Faria, R. B. Ferreira, Ferrera, G., Ferroglia, A., Figy, T. M., Finelli, K. D., Fiolhais, M. C. N., Franco, E., Frederix, R., Fuks, B., Galhardo, B., Gao, J., Gaunt, J. R., Gehrmann, T., Ridder, A. Gehrmann-De, Giljanovic, D., Giuli, F., Glover, E. W. N., Goodsell, M. D., Gouveia, E., Govoni, P., Goy, C., Grazzini, M., Grohsjean, A., Grosse-Oetringhaus, J. F., Gunnellini, P., Gwenlan, C., Harland-Lang, L. A., Harrison, P. F., Heinrich, G., Helsens, C., Herndon, M., Hindrichs, O., Hirschi, V., Hoang, A., Hoepfner, K., Hogan, J. M., Huss, A., Jahn, S., Jain, Sa., Jones, S. P., Jung, A. W., Jung, H., Kallweit, S., Kar, D., Karlberg, A., Kasemets, T., Kerner, M., Khandoga, M. K., Khanpour, H., Khatibi, S., Khukhunaishvili, A., Kieseler, J., Kretzschmar, J., Kroll, J., Kryshen, E., Lang, V. S., Lechner, L., Lee, C. A., Leigh, M., Lelas, D., Les, R., Lewis, I. M., Li, B., Li, Q., Li, Y., Lidrych, J., Ligeti, Z., Lindert, J. M., Liu, Y., Lohwasser, K., Long, K., Lontkovskyi, D., Majumder, G., Mancini, M., Mandrik, P., Mangano, M. L., Marchesini, I., Mayer, C., Mazumdar, K., McFayden, J. A., Lagarelhos, P. M. Mendes Amaral Torres, Meyer, A. B., Mikhalcov, S., Mishima, S., Mitov, A., Najafabadi, M. Mohammadi, Llácer, M. Moreno, Mulders, M., Myska, M., Narain, M., Nisati, A., Nitta, T., Onofre, A., Griso, S. Pagan, Pagani, D., Cortezon, E. Palencia, Papanastasiou, A., Pedro, K., Pellen, M., Perfilov, M., Perrozzi, L., Petersen, B. A., Pierini, M., Pires, J., Pleier, M. -A., Plätzer, S., Potamianos, K., Pozzorini, S., Price, A. C., Rauch, M., Re, E., Reina, L., Reuter, J., Robens, T., Rojo, J., Royon, C., Saito, S., Savin, A., Sawant, S., Schneider, B., Schoefbeck, R., Schoenherr, M., Schäfer-Siebert, H., Seidel, M., Selvaggi, M., Shears, T., Silvestrini, L., Sjodahl, M., Skovpen, K., Smith, N., Spitzbart, D., Starovoitov, P., Suster, C. J. E., Tan, P., Taus, R., Teague, D., Terashi, K., Terron, J., Uplap, S., Veloso, F., Verzetti, M., Vesterinen, M. A., Vladimirov, V. E., Volkov, P., Vorotnikov, G., Milosavljevic, M. Vranjes, Vranjes, N., Vryonidou, E., Walker, D., Wiesemann, M., Wu, Y., Xu, T., Yacoob, S., Yazgan, E., Zahreddine, J., Zanderighi, G., Zaro, M., Zenaiev, O., Della Porta, G. Zevi, Zhang, C., Zhang, W., Zhu, H. L., Zlebcik, R., Zubair, F. N.
The successful operation of the Large Hadron Collider (LHC) and the excellent performance of the ATLAS, CMS, LHCb and ALICE detectors in Run-1 and Run-2 with $pp$ collisions at center-of-mass energies of 7, 8 and 13 TeV as well as the giant leap in p
Externí odkaz:
http://arxiv.org/abs/1902.04070
Autor:
Ajaj, R., Amaudruz, P. -A., Araujo, G. R., Baldwin, M., Batygov, M., Beltran, B., Bina, C. E., Bonatt, J., Boulay, M. G., Broerman, B., Bueno, J. F., Burghardt, P. M., Butcher, A., Cai, B., Cavuoti, S., Chen, M., Chen, Y., Cleveland, B. T., Cranshaw, D., Dering, K., DiGioseffo, J., Doria, L., Duncan, F. A., Dunford, M., Erlandson, A., Fatemighomi, N., Fiorillo, G., Florian, S., Flower, A., Ford, R. J., Gagnon, R., Gallacher, D., Garcés, E. A., Garg, S., Giampa, P., Goeldi, D., Golovko, V. V., Gorel, P., Graham, K., Grant, D. R., Hallin, A. L., Hamstra, M., Harvey, P. J., Hearns, C., Joy, A., Jillings, C. J., Kamaev, O., Kaur, G., Kemp, A., Kochanek, I., Kuźniak, M., Langrock, S., La Zia, F., Lehnert, B., Li, X., Lidgard, J., Lindner, T., Litvinov, O., Lock, J., Longo, G., Majewski, P., McDonald, A. B., McElroy, T., McGinn, T., McLaughlin, J. B., Mehdiyev, R., Mielnichuk, C., Monroe, J., Nadeau, P., Nantais, C., Ng, C., Noble, A. J., O'Dwyer, E., Ouellet, C., Pasuthip, P., Peeters, S. J. M., Piro, M. -C., Pollmann, T. R., Rand, E. T., Rethmeier, C., Retière, F., Seeburn, N., Singhrao, K., Skensved, P., Smith, B., Smith, N. J. T., Sonley, T., Soukup, J., Stainforth, R., Stone, C., Strickland, V., Sur, B., Tang, J., Vázquez-Jáuregui, E., Veloce, L., Viel, S., Walding, J., Waqar, M., Ward, M., Westerdale, S., Willis, J., Zuñiga-Reyes, A.
Publikováno v:
Phys. Rev. D 100, 022004 (2019)
DEAP-3600 is a single-phase liquid argon (LAr) direct-detection dark matter experiment, operating 2 km underground at SNOLAB (Sudbury, Canada). The detector consists of 3279 kg of LAr contained in a spherical acrylic vessel. This paper reports on the
Externí odkaz:
http://arxiv.org/abs/1902.04048
Publikováno v:
Phys. Rev. A 100, 013853 (2019)
Optical interferometers with suspended mirrors are the archetype of all current audio-frequency gravitational-wave detectors. The radiation pressure interaction between the motion of the mirror and the circulating optical field in such interferometer
Externí odkaz:
http://arxiv.org/abs/1812.10184
Autor:
Doctor, Z., Kessler, R., Herner, K., Palmese, A., Soares-Santos, M., Annis, J., Brout, D., Holz, D. E., Sako, M., Rest, A., Cowperthwaite, P., Berger, E., Foley, R. J., Conselice, C. J., Gill, M. S. S., Allam, S., Balbinot, E., Butler, R. E., Chen, H. -Y., Chornock, R., Cook, E., Diehl, H. T., Farr, B., Fong, W., Frieman, J., Fryer, C., García-Bellido, J., Margutti, R., Marshall, J. L., Matheson, T., Metzger, B. D., Nicholl, M., Paz-Chinchón, F., Salim, S., Sauseda, M., Secco, L. F., Smith, N., Smith, R. C., Vivas, A. K., Tucker, D. L., Abbott, T. M. C., Avila, S., Bechtol, K., Bertin, E., Brooks, D., Buckley-Geer, E., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., D'Andrea, C. B., da Costa, L. N., De Vicente, J., Desai, S., Doel, P., Flaugher, B., Fosalba, P., Gaztanaga, E., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gutierrez, G., Hartley, W. G., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kent, S., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Menanteau, F., Miller, C. J., Miquel, R., Neilsen, E., Nord, B., Ogando, R. L. C., Plazas, A. A., Roodman, A., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Walker, A. R., Wester, W.
Publikováno v:
The Astrophysical Journal Letters, Volume 873, Issue 2, article id. L24, 9 pp. (2019)
Binary black hole (BBH) mergers found by the LIGO and Virgo detectors are of immense scientific interest to the astrophysics community, but are considered unlikely to be sources of electromagnetic emission. To test whether they have rapidly fading op
Externí odkaz:
http://arxiv.org/abs/1812.01579
Autor:
Dimitriadis, G., Foley, R. J., Rest, A., Kasen, D., Piro, A. L., Polin, A., Jones, D. O., Villar, A., Narayan, G., Coulter, D. A., Kilpatrick, C. D., Pan, Y. -C., Rojas-Bravo, C., Fox, O. D., Jha, S. W., Nugent, P. E., Riess, A. G., Scolnic, D., Drout, M. R., Barentsen, G., Dotson, J., Gully-Santiago, M., Hedges, C., Cody, A. M., Barclay, T., Howell, S., Garnavich, P., Tucker, B. E., Shaya, E., Mushotzky, R., Olling, R. P., Margheim, S., Zenteno, A., Coughlin, J., Van Cleve, J. E., Cardoso, J. Vinicius de Miranda, Larson, K. A., McCalmont-Everton, K. M., Peterson, C. A., Ross, S. E., Reedy, L. H., Osborne, D., McGinn, C., Kohnert, L., Migliorini, L., Wheaton, A., Spencer, B., Labonde, C., Castillo, G., Beerman, G., Steward, K., Hanley, M., Larsen, R., Gangopadhyay, R., Kloetzel, R., Weschler, T., Nystrom, V., Moffatt, J., Redick, M., Griest, K., Packard, M., Muszynski, M., Kampmeier, J., Bjella, R., Flynn, S., Elsaesser, B., Chambers, K. C., Flewelling, H. A., Huber, M. E., Magnier, E. A., Waters, C. Z., Schultz, A. S. B., Bulger, J., Lowe, T. B., Willman, M., Smartt, S. J., Smith, K. W., Points, S., Strampelli, G. M., Brimacombe, J., Chen, P., Munoz, J. A., Mutel, R. L., Shields, J., Vallely, P. J., Villanueva Jr, S., Li, W., Wang, X., Zhang, J., Lin, H., Mo, J., Zhao, X., Sai, H., Zhang, X., Zhang, K., Zhang, T., Wang, L., Baron, E., DerKacy, J. M., Li, L., Chen, Z., Xiang, D., Rui, L., Huang, F., Li, X., Hosseinzadeh, G., Howell, D. A., Arcavi, I., Hiramatsu, D., Burke, J., Valenti, S., Tonry, J. L., Denneau, L., Heinze, A. N., Weiland, H., Stalder, B., Vinko, J., Sarneczky, K., Pa, A., Bodi, A., Bognar, Zs., Csak, B., Cseh, B., Csornyei, G., Hanyecz, O., Ignacz, B., Kalup, Cs., Konyves-Toth, R., Kriskovics, L., Ordasi, A., Rajmon, I., Sodor, A., Szabo, R., Szakats, R., Zsidi, G., Williams, S. C., Nordin, J., Cartier, R., Frohmaier, C., Galbany, L., Gutierrez, C. P., Hook, I., Inserra, C., Smith, M., Sand, D. J., Andrews, J. E., Smith, N., Bilinski, C.
We present an exquisite, 30-min cadence Kepler (K2) light curve of the Type Ia supernova (SN Ia) 2018oh (ASASSN-18bt), starting weeks before explosion, covering the moment of explosion and the subsequent rise, and continuing past peak brightness. The
Externí odkaz:
http://arxiv.org/abs/1811.10061
Autor:
Li, W., Wang, X., Vinkó, J., Mo, J., Hosseinzadeh, G., Sand, D. J., Zhang, J., Lin, H., Zhang, T., Wang, L., Chen, Z., Xiang, D., Rui, L., Huang, F., Li, X., Zhang, X., Li, L., Baron, E., Derkacy, J. M., Zhao, X., Sai, H., Zhang, K., Howell, D. A., McCully, C., Arcavi, I., Valenti, S., Hiramatsu, D., Burke, J., Rest, A., Garnavich, P., Tucker, B. E., Narayan, G., Shaya, E., Margheim, S., Zenteno, A., Villar, A., Dimitriadis, G., Foley, R. J., Pan, Y. -C., Coulter, D. A., Fox, O. D., Jha, S. W., Jones, D. O., Kasen, D. N., Kilpatrick, C. D., Piro, A. L., Riess, A. G., Rojas-Bravo, C., Shappee, B. J., Holoien, T. W. -S., Stanek, K. Z., Drout, M. R., Auchettl, K., Kochanek, C. S., Brown, J. S., Bose, S., Bersier, D., Brimacombe, J., Chen, P., Dong, S., Holmbo, S., Muñoz, J. A., Mutel, R. L., Post, R. S., Prieto, J. L., Shields, J., Tallon, D., Thompson, T. A., Vallely, P. J., Villanueva Jr., S., Smartt, S. J., Smith, K. W., Chambers, K. C., Flewelling, H. A., Huber, M. E., Magnier, E. A., Waters, C. Z., Schultz, A. S. B., Bulger, J., Lowe, T. B., Willman, M., Sárneczky, K., Pál, A., Wheeler, J. C., Bódi, A., Bognár, Zs., Csák, B., Cseh, B., Csörnyei, G., Hanyecz, O., Ignácz, B., Kalup, Cs., Könyves-Tóth, R., Kriskovics, L., Ordasi, A., Rajmon, I., Sódor, A., Szabó, R., Szakáts, R., Zsidi, G., Milne, P., Andrews, J. E., Smith, N., Bilinski, C., Brown, P. J., Nordin, J., Williams, S. C., Galbany, L., Palmerio, J., Hook, I. M., Inserra, C., Maguire, K., Cartier, Régis, Razza, A., Gutiérrez, C. P., Hermes, J. J., Reding, J. S., Kaiser, B. C., Tonry, J. L., Heinze, A. N., Denneau, L., Weiland, H., Stalder, B., Barentsen, G., Dotson, J., Barclay, T., Gully-Santiago, M., Hedges, C., Cody, A. M., Howell, S., Coughlin, J., Van Cleve, J. E., Cardoso, J. Vinícius de Miranda, Larson, K. A., McCalmont-Everton, K. M., Peterson, C. A., Ross, S. E., Reedy, L. H., Osborne, D., McGinn, C., Kohnert, L., Migliorini, L., Wheaton, A., Spencer, B., Labonde, C., Castillo, G., Beerman, G., Steward, K., Hanley, M., Larsen, R., Gangopadhyay, R., Kloetzel, R., Weschler, T., Nystrom, V., Moffatt, J., Redick, M., Griest, K., Packard, M., Muszynski, M., Kampmeier, J., Bjella, R., Flynn, S., Elsaesser, B.
Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting constraints o
Externí odkaz:
http://arxiv.org/abs/1811.10056
Autor:
Trilling, DE, Mommert, M, Hora, JL, Farnocchia, D, Chodas, P, Giorgini, J, Smith, HA, Carey, S, Lisse, CM, Werner, M, McNeill, A, Chesley, SR, Emery, JP, Fazio, G, Fernandez, YR, Harris, A, Marengo, M, Mueller, M, Roegge, A, Smith, N, Weaver, HA, Meech, K, Micheli, M
Publikováno v:
Published in the Astronomical Journal, 156, 261 (2018)
1I/`Oumuamua is the first confirmed interstellar body in our Solar System. Here we report on observations of `Oumuamua made with the Spitzer Space Telescope on 2017 November 21--22 (UT). We integrated for 30.2~hours at 4.5 micron (IRAC channel 2). We
Externí odkaz:
http://arxiv.org/abs/1811.08072
Autor:
Smith, N. Ammon1 (AUTHOR) nsmith@glenmary.org
Publikováno v:
Religions. Nov2023, Vol. 14 Issue 11, p1393. 9p.
Akademický článek
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