Zobrazeno 1 - 10
of 101
pro vyhledávání: '"Abazajian, K"'
Autor:
Keeley, Ryan E., Nierenberg, Anna M., Gilman, Daniel, Gannon, Charles, Birrer, Simon, Treu, Tommaso, Benson, Andrew J., Du, Xiaolong, Abazajian, K. N., Anguita, T., Bennert, V. N., Djorgovski, S. G., Gupta, K. K., Hoenig, S. F., Kusenko, A., Lemon, C., Malkan, M., Motta, V., Moustakas, L. A., Oh, M. S. H., Sluse, D., Stern, D., Wechsler, R. H.
This is the second in a series of papers in which we use JWST MIRI multiband imaging to measure the warm dust emission in a sample of 31 multiply imaged quasars, to be used as a probe of the particle nature of dark matter. We present measurements of
Externí odkaz:
http://arxiv.org/abs/2405.01620
Autor:
Nierenberg, A. M., Keeley, R. E., Sluse, D., Gilman, D., Birrer, S., Treu, T., Abazajian, K. N., Anguita, T., Benson, A. J., Bennert, V. N., Djorgovski, S. G., Du, X., Fassnacht, C. D., Hoenig, S. F., Kusenko, A., Lemon, C., Malkan, M., Motta, V., Moustakas, L. A., Stern, D., Wechsler, R. H.
The flux ratios of gravitationally lensed quasars provide a powerful probe of the nature of dark matter. Importantly, these ratios are sensitive to small-scale structure, irrespective of the presence of baryons. This sensitivity may allow us to study
Externí odkaz:
http://arxiv.org/abs/2309.10101
Gamma-ray observations have revealed strong variability in blazar luminosities in the gamma-ray band over time scales as short as minutes. We show, for the first time, that the correlation of the spectrum with intensity is consistent with the behavio
Externí odkaz:
http://arxiv.org/abs/1709.06535
Akademický článek
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Autor:
Abeysekara, A. U., Alfaro, R., Alvarez, C., Alvarez, J. D., Arceo, R., Arteaga-Velazquez, J. C., Solares, H. A. Ayala, Barber, A. S., Baughman, B. M., Bautista-Elivar, N., Gonzalez, J. Becerra, Belmont, E., BenZvi, S. Y., Berley, D., Rosales, M. Bonilla, Braun, J., Caballero-Lopez, R. A., Caballero-Mora, K. S., Carraminana, A., Castillo, M., Cotti, U., Cotzomi, J., de la Fuente, E., De Leon, C., DeYoung, T., Hernandez, R. Diaz, Diaz-Cruz, L., Diaz-Velez, J. C., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., E., S. F., Fiorino, D. W., Fraija, N., Galindo, A., Garfias, F., Gonzalez, M. M., Goodman, J. A., Grabski, V., Gussert, M., Hampel-Arias, Z., Harding, J. P., Hui, C. M., Huentemeyer, P., Imran, A., Iriarte, A., Karn, P., Kieda, D., Kunde, G. J., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. Leon, Linares, E. C., Linnemann, J. T., Longo, M., Luna-Garcia, R., Marinelli, A., Martinez, H., Martinez, O., Martinez-Castro, J., Matthews, J. A. J., McEnery, J., Torres, E. Mendoza, Miranda-Romagnoli, P., Moreno, E., Mostafa, M., Nellen, L., Newbold, M., Noriega-Papaqui, R., Oceguera-Becerra, T., Patricelli, B., Pelayo, R., Perez-Perez, E. G., Pretz, J., Riviere, C., Rosa-Gonzalez, D., Ryan, J., Salazar, H., Salesa, F., Sandoval, A., Schneider, M., Silich, S., Sinnis, G., Smith, A. J., Woodle, K. Sparks, Springer, R. W., Taboada, I., Toale, P. A., Tollefson, K., Torres, I., Ukwatta, T. N., Villasenor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yodh, G. B., Younk, P. W., Zaborov, D., Zepeda, A., Zhou, H., Abazajian, K. N.
Publikováno v:
Phys. Rev. D 90, 122002 (2014)
The High Altitude Water Cherenkov (HAWC) observatory is a wide field-of-view detector sensitive to gamma rays of 100 GeV to a few hundred TeV. Located in central Mexico at 19 degrees North latitude and 4100 m above sea level, HAWC will observe gamma
Externí odkaz:
http://arxiv.org/abs/1405.1730
Autor:
de Gouvea, A., Pitts, K., Scholberg, K., Zeller, G. P., Alonso, J., Bernstein, A., Bishai, M., Elliott, S., Heeger, K., Hoffman, K., Huber, P., Kaufman, L. J., Kayser, B., Link, J., Lunardini, C., Monreal, B., Morfin, J. G., Robertson, H., Tayloe, R., Tolich, N., Abazajian, K., Akiri, T., Albright, C., Asaadi, J., Babu, K. S, Balantekin, A. B., Barbeau, P., Bass, M., Blake, A., Blondel, A., Blucher, E., Bowden, N., Brice, S. J., Bross, A., Carls, B., Cavanna, F., Choudhary, B., Coloma, P., Connolly, A., Conrad, J., Convery, M., Cooper, R. L., Cowen, D., da Motta, H., de Young, T., Di Lodovico, F., Diwan, M., Djurcic, Z., Dracos, M., Dodelson, S., Efremenko, Y., Ekelof, T., Feng, J. L., Fleming, B., Formaggio, J., Friedland, A., Fuller, G., Gallagher, H., Geer, S., Gilchriese, M., Goodman, M., Grant, D., Gratta, G., Hall, C., Halzen, F., Harris, D., Heffner, M., Henning, R., Hewett, J. L., Hill, R., Himmel, A., Horton-Smith, G., Karle, A., Katori, T., Kearns, E., Kettell, S., Klein, J., Kim, Y., Kim, Y. K., Kolomensky, Yu., Kordosky, M., Kudenko, Yu., Kudryavtsev, V. A., Lande, K., Lang, K., Lanza, R., Lau, K., Lee, H., Li, Z., Littlejohn, B. R., Lin, C. J., Liu, D., Liu, H., Long, K., Louis, W., Luk, K. B., Marciano, W., Mariani, C., Marshak, M., Mauger, C., McDonald, K. T., McFarland, K., McKeown, R., Messier, M., Mishra, S. R., Mosel, U., Mumm, P., Nakaya, T., Nelson, J. K., Nygren, D., Gann, G. D. Orebi, Osta, J., Palamara, O., Paley, J., Papadimitriou, V., Parke, S., Parsa, Z., Patterson, R., Piepke, A., Plunkett, R., Poon, A., Qian, X., Raaf, J., Rameika, R., Ramsey-Musolf, M., Rebel, B., Roser, R., Rosner, J., Rott, C., Rybka, G., Sahoo, H., Sangiorgio, S., Schmitz, D., Shrock, R., Shaevitz, M., Smith, N., Smy, M., Sobel, H., Sorensen, P., Sousa, A., Spitz, J., Strauss, T., Svoboda, R., Tanaka, H. A., Thomas, J., Tian, X., Tschirhart, R., Tully, C., Van Bibber, K., Van de Water, R. G., Vahle, P., Vogel, P., Walter, C. W., Wark, D., Wascko, M., Webber, D., Weerts, H., White, C., White, H., Whitehead, L., Wilson, R. J., Winslow, L., Wongjirad, T, Worcester, E., Yokoyama, M., Yoo, J., Zimmerman, E. D.
This document represents the response of the Intensity Frontier Neutrino Working Group to the Snowmass charge. We summarize the current status of neutrino physics and identify many exciting future opportunities for studying the properties of neutrino
Externí odkaz:
http://arxiv.org/abs/1310.4340
Autor:
Dodelson, S., Honscheid, K., Abazajian, K., Carlstrom, J., Huterer, D., Jain, B., Kim, A., Kirkby, D., Lee, A., Padmanabhan, N., Rhodes, J., Weinberg, D.
The American Physical Society's Division of Particles and Fields initiated a long-term planning exercise over 2012-13, with the goal of developing the community's long term aspirations. The sub-group "Dark Energy and CMB" prepared a series of papers
Externí odkaz:
http://arxiv.org/abs/1309.5386
Autor:
Abazajian, K. N., Arnold, K., Austermann, J., Benson, B. A., Bischoff, C., Bock, J., Bond, J. R., Borrill, J., Calabrese, E., Carlstrom, J. E., Carvalho, C. S., Chang, C. L., Chiang, H. C., Church, S., Cooray, A., Crawford, T. M., Dawson, K. S., Das, S., Devlin, M. J., Dobbs, M., Dodelson, S., Dore, O., Dunkley, J., Errard, J., Fraisse, A., Gallicchio, J., Halverson, N. W., Hanany, S., Hildebrandt, S. R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W. L., Honscheid, K., Hu, W., Hubmayr, J., Irwin, K., Jones, W. C., Kamionkowski, M., Keating, B., Keisler, R., Knox, L., Komatsu, E., Kovac, J., Kuo, C. -L., Lawrence, C., Lee, A. T., Leitch, E., Linder, E., Lubin, P., McMahon, J., Miller, A., Newburgh, L., Niemack, M. D., Nguyen, H., Nguyen, H. T., Page, L., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sehgal, N., Seljak, U., Sievers, J., Silverstein, E., Slosar, A., Smith, K. M., Spergel, D., Staggs, S. T., Stark, A., Stompor, R., Vieregg, A. G., Wang, G., Watson, S., Wollack, E. J., Wu, W. L. K., Yoon, K. W., Zahn, O.
Publikováno v:
Astropart.Phys. 63 (2015) 66-80
This is a report on the status and prospects of the quantification of neutrino properties through the cosmological neutrino background for the Cosmic Frontier of the Division of Particles and Fields Community Summer Study long-term planning exercise.
Externí odkaz:
http://arxiv.org/abs/1309.5383
Autor:
Abazajian, K. N., Arnold, K., Austermann, J., Benson, B. A., Bischoff, C., Bock, J., Bond, J. R., Borrill, J., Buder, I., Burke, D. L., Calabrese, E., Carlstrom, J. E., Carvalho, C. S., Chang, C. L., Chiang, H. C., Church, S., Cooray, A., Crawford, T. M., Crill, B. P., Dawson, K. S., Das, S., Devlin, M. J., Dobbs, M., Dodelson, S., Doré, O., Dunkley, J., Feng, J. L., Fraisse, A., Gallicchio, J., Giddings, S. B., Green, D., Halverson, N. W., Hanany, S., Hanson, D., Hildebrandt, S. R., Hincks, A., Hlozek, R., Holder, G., Holzapfel, W. L., Honscheid, K., Horowitz, G., Hu, W., Hubmayr, J., Irwin, K., Jackson, M., Jones, W. C., Kallosh, R., Kamionkowski, M., Keating, B., Keisler, R., Kinney, W., Knox, L., Komatsu, E., Kovac, J., Kuo, C. -L., Kusaka, A., Lawrence, C., Lee, A. T., Leitch, E., Linde, A., Linder, E., Lubin, P., Maldacena, J., Martinec, E., McMahon, J., Miller, A., Mukhanov, V., Newburgh, L., Niemack, M. D., Nguyen, H., Nguyen, H. T., Page, L., Pryke, C., Reichardt, C. L., Ruhl, J. E., Sehgal, N., Seljak, U., Senatore, L., Sievers, J., Silverstein, E., Slosar, A., Smith, K. M., Spergel, D., Staggs, S. T., Stark, A., Stompor, R., Vieregg, A. G., Wang, G., Watson, S., Wollack, E. J., Wu, W. L. K., Yoon, K. W., Zahn, O., Zaldarriaga, M.
Fluctuations in the intensity and polarization of the cosmic microwave background (CMB) and the large-scale distribution of matter in the universe each contain clues about the nature of the earliest moments of time. The next generation of CMB and lar
Externí odkaz:
http://arxiv.org/abs/1309.5381
Autor:
Abazajian, K. N., Acero, M. A., Agarwalla, S. K., Aguilar-Arevalo, A. A., Albright, C. H., Antusch, S., Arguelles, C. A., Balantekin, A. B., Barenboim, G., Barger, V., Bernardini, P., Bezrukov, F., Bjaelde, O. E., Bogacz, S. A., Bowden, N. S., Boyarsky, A., Bravar, A., Berguno, D. Bravo, Brice, S. J., Bross, A. D., Caccianiga, B., Cavanna, F., Chun, E. J., Cleveland, B. T., Collin, A. P., Coloma, P., Conrad, J. M., Cribier, M., Cucoanes, A. S., D'Olivo, J. C., Das, S., de Gouvea, A., Derbin, A. V., Dharmapalan, R., Diaz, J. S., Ding, X. J., Djurcic, Z., Donini, A., Duchesneau, D., Ejiri, H., Elliott, S. R., Ernst, D. J., Esmaili, A., Evans, J. J., Fernandez-Martinez, E., Figueroa-Feliciano, E., Fleming, B. T., Formaggio, J. A., Franco, D., Gaffiot, J., Gandhi, R., Gao, Y., Garvey, G. T., Gavrin, V. N., Ghoshal, P., Gibin, D., Giunti, C., Gninenko, S. N., Gorbachev, V. V., Gorbunov, D. S., Guenette, R., Guglielmi, A., Halzen, F., Hamann, J., Hannestad, S., Haxton, W., Heeger, K. M., Henning, R., Hernandez, P., Huber, P., Huelsnitz, W., Ianni, A., Ibragimova, T. V., Karadzhov, Y., Karagiorgi, G., Keefer, G., Kim, Y. D., Kopp, J., Kornoukhov, V. N., Kusenko, A., Kyberd, P., Langacker, P., Lasserre, Th., Laveder, M., Letourneau, A., Lhuillier, D., Li, Y. F., Lindner, M., Link, J. M., Littlejohn, B. L., Lombardi, P., Long, K., Lopez-Pavon, J., Louis, W. C., Ludhova, L., Lykken, J. D., Machado, P. A. N., Maltoni, M., Mann, W. A., Marfatia, D., Mariani, C., Matveev, V. A., Mavromatos, N. E., Melchiorri, A., Meloni, D., Mena, O., Mention, G., Merle, A., Meroni, E., Mezzetto, M., Mills, G. B., Minic, D., Miramonti, L., Mohapatra, D., Mohapatra, R. N., Montanari, C., Mori, Y., Mueller, Th. A., Mumm, H. P., Muratova, V., Nelson, A. E., Nico, J. S., Noah, E., Nowak, J., Smirnov, O. Yu., Obolensky, M., Pakvasa, S., Palamara, O., Pallavicini, M., Pascoli, S., Patrizii, L., Pavlovic, Z., Peres, O. L. G., Pessard, H., Pietropaolo, F., Pitt, M. L., Popovic, M., Pradler, J., Ranucci, G., Ray, H., Razzaque, S., Rebel, B., Robertson, R. G. H., Rodejohann, W., Rountree, S. D., Rubbia, C., Ruchayskiy, O., Sala, P. R., Scholberg, K., Schwetz, T., Shaevitz, M. H., Shaposhnikov, M., Shrock, R., Simone, S., Skorokhvatov, M., Sorel, M., Sousa, A., Spergel, D. N., Spitz, J., Stanco, L., Stancu, I., Suzuki, A., Takeuchi, T., Tamborra, I., Tang, J., Testera, G., Tian, X. C., Tonazzo, A., Tunnell, C. D., Van de Water, R. G., Verde, L., Veretenkin, E. P., Vignoli, C., Vivier, M., Vogelaar, R. B., Wascko, M. O., Wilkerson, J. F., Winter, W., Wong, Y. Y. Y., Yanagida, T. T., Yasuda, O., Yeh, M., Yermia, F., Yokley, Z. W., Zeller, G. P., Zhan, L., Zhang, H.
This white paper addresses the hypothesis of light sterile neutrinos based on recent anomalies observed in neutrino experiments and the latest astrophysical data.
Externí odkaz:
http://arxiv.org/abs/1204.5379