Zobrazeno 1 - 10
of 267
pro vyhledávání: '"D. Staszak"'
Autor:
H. Agakishiev, M. M. Aggarwal, Z. Ahammed, A. V. Alakhverdyants, I. Alekseev, J. Alford, B. D. Anderson, C. D. Anson, D. Arkhipkin, G. S. Averichev, J. Balewski, D. R. Beavis, N. K. Behera, R. Bellwied, M. J. Betancourt, R. R. Betts, A. Bhasin, A. K. Bhati, H. Bichsel, J. Bielcik, J. Bielcikova, B. Biritz, L. C. Bland, W. Borowski, J. Bouchet, E. Braidot, A. V. Brandin, A. Bridgeman, S. G. Brovko, E. Bruna, S. Bueltmann, I. Bunzarov, T. P. Burton, X. Z. Cai, H. Caines, M. Calderón de la Barca Sánchez, D. Cebra, R. Cendejas, M. C. Cervantes, Z. Chajecki, P. Chaloupka, S. Chattopadhyay, H. F. Chen, J. H. Chen, J. Y. Chen, L. Chen, J. Cheng, M. Cherney, A. Chikanian, K. E. Choi, W. Christie, P. Chung, M. J. M. Codrington, R. Corliss, J. G. Cramer, H. J. Crawford, S. Dash, A. Davila Leyva, L. C. De Silva, R. R. Debbe, T. G. Dedovich, A. A. Derevschikov, R. Derradi de Souza, L. Didenko, P. Djawotho, S. M. Dogra, X. Dong, J. L. Drachenberg, J. E. Draper, J. C. Dunlop, L. G. Efimov, M. Elnimr, J. Engelage, G. Eppley, M. Estienne, L. Eun, O. Evdokimov, R. Fatemi, J. Fedorisin, A. Feng, R. G. Fersch, P. Filip, E. Finch, V. Fine, Y. Fisyak, C. A. Gagliardi, D. R. Gangadharan, A. Geromitsos, F. Geurts, P. Ghosh, Y. N. Gorbunov, A. Gordon, O. Grebenyuk, D. Grosnick, S. M. Guertin, A. Gupta, W. Guryn, B. Haag, O. Hajkova, A. Hamed, L-X. Han, J. W. Harris, J. P. Hays-Wehle, M. Heinz, S. Heppelmann, A. Hirsch, E. Hjort, G. W. Hoffmann, D. J. Hofman, B. Huang, H. Z. Huang, T. J. Humanic, L. Huo, G. Igo, P. Jacobs, W. W. Jacobs, C. Jena, F. Jin, J. Joseph, E. G. Judd, S. Kabana, K. Kang, J. Kapitan, K. Kauder, H. Ke, D. Keane, A. Kechechyan, D. Kettler, D. P. Kikola, J. Kiryluk, A. Kisiel, V. Kizka, A. G. Knospe, D. D. Koetke, T. Kollegger, J. Konzer, I. Koralt, L. Koroleva, W. Korsch, L. Kotchenda, V. Kouchpil, P. Kravtsov, K. Krueger, M. Krus, L. Kumar, P. Kurnadi, M. A. C. Lamont, J. M. Landgraf, S. LaPointe, J. Lauret, A. Lebedev, R. Lednicky, J. H. Lee, W. Leight, M. J. LeVine, C. Li, L. Li, N. Li, W. Li, X. Li, Y. Li, Z. M. Li, M. A. Lisa, F. Liu, H. Liu, J. Liu, T. Ljubicic, W. J. Llope, R. S. Longacre, W. A. Love, Y. Lu, E. V. Lukashov, X. Luo, G. L. Ma, Y. G. Ma, D. P. Mahapatra, R. Majka, O. I. Mall, L. K. Mangotra, R. Manweiler, S. Margetis, C. Markert, H. Masui, H. S. Matis, Yu. A. Matulenko, D. McDonald, T. S. McShane, A. Meschanin, R. Milner, N. G. Minaev, S. Mioduszewski, A. Mischke, M. K. Mitrovski, B. Mohanty, M. M. Mondal, B. Morozov, D. A. Morozov, M. G. Munhoz, M. Naglis, B. K. Nandi, T. K. Nayak, P. K. Netrakanti, L. V. Nogach, S. B. Nurushev, G. Odyniec, A. Ogawa, null Oh, null Ohlson, V. Okorokov, E. W. Oldag, D. Olson, M. Pachr, B. S. Page, S. K. Pal, Y. Pandit, Y. Panebratsev, T. Pawlak, H. Pei, T. Peitzmann, C. Perkins, W. Peryt, S. C. Phatak, P. Pile, M. Planinic, M. A. Ploskon, J. Pluta, D. Plyku, N. Poljak, A. M. Poskanzer, B. V. K. S. Potukuchi, C. B. Powell, D. Prindle, N. K. Pruthi, P. R. Pujahari, J. Putschke, H. Qiu, R. Raniwala, S. Raniwala, R. L. Ray, R. Redwine, R. Reed, H. G. Ritter, J. B. Roberts, O. V. Rogachevskiy, J. L. Romero, A. Rose, L. Ruan, J. Rusnak, N. R. Sahoo, S. Sakai, I. Sakrejda, T. Sakuma, S. Salur, J. Sandweiss, E. Sangaline, A. Sarkar, J. Schambach, R. P. Scharenberg, A. M. Schmah, N. Schmitz, T. R. Schuster, J. Seele, J. Seger, I. Selyuzhenkov, P. Seyboth, E. Shahaliev, M. Shao, M. Sharma, S. S. Shi, Q. Y. Shou, E. P. Sichtermann, F. Simon, R. N. Singaraju, M. J. Skoby, N. Smirnov, H. M. Spinka, B. Srivastava, T. D. S. Stanislaus, D. Staszak, S. G. Steadman, J. R. Stevens, R. Stock, M. Strikhanov, B. Stringfellow, A. A. P. Suaide, M. C. Suarez, N. L. Subba, M. Sumbera, X. M. Sun, Y. Sun, Z. Sun, B. Surrow, D. N. Svirida, T. J. M. Symons, A. Szanto de Toledo, J. Takahashi, A. H. Tang, Z. Tang, L. H. Tarini, T. Tarnowsky, D. Thein, J. H. Thomas, J. Tian, A. R. Timmins, D. Tlusty, M. Tokarev, V. N. Tram, S. Trentalange, R. E. Tribble, null Tribedy, O. D. Tsai, T. Ullrich, D. G. Underwood, G. Van Buren, G. van Nieuwenhuizen, J. A. Vanfossen, Jr., R. Varma, G. M. S. Vasconcelos, A. N. Vasiliev, F. Videbæk, Y. P. Viyogi, S. Vokal, M. Wada, M. Walker, F. Wang, G. Wang, H. Wang, J. S. Wang, Q. Wang, X. L. Wang, Y. Wang, G. Webb, J. C. Webb, G. D. Westfall, C. Whitten Jr., H. Wieman, S. W. Wissink, R. Witt, W. Witzke, Y. F. Wu, null Xiao, W. Xie, H. Xu, N. Xu, Q. H. Xu, W. Xu, Y. Xu, Z. Xu, L. Xue, Y. Yang, P. Yepes, K. Yip, I-K. Yoo, M. Zawisza, H. Zbroszczyk, W. Zhan, J. B. Zhang, S. Zhang, W. M. Zhang, X. P. Zhang, Y. Zhang, Z. P. Zhang, J. Zhao, C. Zhong, W. Zhou, X. Zhu, Y. H. Zhu, R. Zoulkarneev, Y. Zoulkarneeva
Publikováno v:
Chinese Physics C. 45:044002
Dihadron azimuthal correlations containing a high transverse momentum ( ) trigger particle are sensitive to the properties of the nuclear medium created at RHIC through the strong interactions occurring between the traversing parton and the medium, i
Akademický článek
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Autor:
Ralph Bird, Q. Feng, Marita Krause, Martin Pohl, M. J. Lang, J. Tyler, Matteo Cerruti, J. H. Buckley, A. N. Otte, Amy Furniss, I. Telezhinsky, E. Roache, Jamie Holder, M. P. Connolly, Wystan Benbow, N. Kelley-Hoskins, P. Kaaret, Olivier Hervet, Alex Geringer-Sameth, Karlen Shahinyan, B. Zitzer, J. Grube, M. Buchovecky, G. H. Sembroski, F. Krennrich, S. McArthur, N. H. Park, David Kieda, C. B. Rulten, P. Kar, Etienne Bourbeau, T. T.Y. Lin, N. Håkansson, Henrike Fleischhack, J. V. Tucci, A. Popkow, C. A. Johnson, M. Kertzman, Sinéad M. Griffin, R. Mukherjee, P. Moriarty, S. P. Wakely, Karen Byrum, R. A. Ong, Lucy Fortson, A. Weinstein, Marcos Santander, B. Hummensky, M. K. Daniel, John L. Quinn, T. Brantseg, E. Pueschel, David A. Williams, Gordon T. Richards, P. T. Reynolds, K. Ragan, Daniel Nieto, Moritz Hütten, A. Archer, D. Staszak, S. Trepanier, Jodi Christiansen, P. Wilcox, I. Sadeh, Wei Cui, Savvas M. Koushiappas, A. W. Smith, J. P. Finley, S. Archambault, D. S. Hanna, V. Bugaev, S. O'Brien, G. Hughes
Publikováno v:
ResearcherID
Physical review / D 95(8), 082001 (2017). doi:10.1103/PhysRevD.95.082001
Physical review / D 95(8), 082001 (2017). doi:10.1103/PhysRevD.95.082001
We present constraints on the annihilation cross section of WIMP dark matter based on the joint statistical analysis of four dwarf galaxies with VERITAS. These results are derived from an optimized photon weighting statistical technique that improves
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79918d62ce54c4c29eb764302ae4b536
http://arxiv.org/abs/1703.04937
http://arxiv.org/abs/1703.04937
Autor:
Q. Feng, P. T. Reynolds, C. A. Johnson, Wystan Benbow, A. Popkow, J. P. Finley, D. S. Hanna, B. Zitzer, Manel Errando, S. Kumar, D. B. Kieda, Karlen Shahinyan, Daniel Nieto, Henrike Fleischhack, Gernot Maier, Lucy Fortson, Moritz Hütten, David A. Williams, S. O'Brien, J. Tyler, M. Pohl, P. Kaaret, R. A. Ong, Thomas Weisgarber, Nahee Park, S. McArthur, J. H. Buckley, G. H. Sembroski, I. Sadeh, P. Wilcox, I. Telezhinsky, Jamie Holder, John L. Quinn, E. Pueschel, M. Buchovecky, P. Moriarty, P. Kar, A. N. Otte, S. Trepanier, Patrick Slane, A. J.R. Weinstein, A. Wilhelm, Ralph Bird, M. P. Connolly, D. Staszak, K. Ragan, Wei Cui, A. Archer, Gordon T. Richards, M. J. Lang, Marcos Santander, E. Roache, A. D. Falcone, Etienne Bourbeau, S. Archambault, Reshmi Mukherjee, Dwarkadas, N. Kelley-Hoskins, Bugaev, Matteo Cerruti, Amy Furniss, Sinéad M. Griffin, M. Kertzman, A. McCann, S. P. Wakely, Marita Krause
Publikováno v:
The astrophysical journal / 1 836(1), 23 (2017). doi:10.3847/1538-4357/836/1/23
The astrophysical journal 836(1), 23 (2017). doi:10.3847/1538-4357/836/1/23
High-energy gamma-ray emission from supernova remnants (SNRs) has provided a unique perspective for studies of Galactic cosmic-ray acceleration. Tycho's SNR is a particu
High-energy gamma-ray emission from supernova remnants (SNRs) has provided a unique perspective for studies of Galactic cosmic-ray acceleration. Tycho's SNR is a particu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e33653b6b262a5d23b665f021188b6c1
http://hdl.handle.net/10379/10282
http://hdl.handle.net/10379/10282
Autor:
G. H. Gillanders, A. Weinstein, Martin Pohl, M. Kertzman, S. McArthur, Sinéad M. Griffin, Wystan Benbow, O. Hervet, P. Moriarty, Henrike Fleischhack, Q. Feng, A. Popkow, John L. Quinn, P. Kaaret, M. J. Lang, D. S. Hanna, David Kieda, Gordon T. Richards, Lucy Fortson, R. A. Ong, Ralph Bird, P. T. Reynolds, J. P. Finley, Wei Cui, J. V. Cardenzana, E. Pueschel, Maria Krause, David A. Williams, M. Buchovecky, C. A. Johnson, N. H. Park, Daniel Nieto, E. Roache, L. Ciupik, A. Bouvier, Gernot Maier, Abraham D. Falcone, M. K. Daniel, S. P. Wakely, A. N. Otte, Karlen Shahinyan, S. Archambault, S. O'Brien, K. Ragan, I. Telezhinsky, Jamie Holder, Matteo Cerruti, Amy Furniss, M. P. Connolly, G. Hughes, Etienne Bourbeau, B. Zitzer, A. Archer, T. T.Y. Lin, G. H. Sembroski, T. B. Humensky, Moritz Hütten, Manel Errando, I. Sadeh, R. Mukherjee, D. Staszak, S. Trepanier, P. Wilcox, V. Bugaev, C. Rulten, P. Kar
Publikováno v:
Astroparticle physics 91, 34-43 (2017). doi:10.1016/j.astropartphys.2017.03.001
ResearcherID
ResearcherID
Astroparticle physics 91, 34 - 43 (2017). doi:10.1016/j.astropartphys.2017.03.001
Imaging atmospheric Cherenkov telescopes (IACTs) are equipped with sensitive photomultiplier tube (PMT) cameras. Exposure to high levels of background illumination
Imaging atmospheric Cherenkov telescopes (IACTs) are equipped with sensitive photomultiplier tube (PMT) cameras. Exposure to high levels of background illumination
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10c20ac15401aaf7f24e0ad4d61a021f
Very high energy observations of the binaries V 404 CYG AND 4U 0115+634 during giant X-Ray outbursts
Autor:
Wystan Benbow, Daniel Nieto, D. Staszak, Sanjay Kumar, P. Kaaret, A. Flinders, K. Ragan, Gernot Maier, S. Griffin, Matteo Cerruti, I. Telezhinsky, David Kieda, Jamie Holder, S. P. Wakely, P. Moriarty, John L. Quinn, Karen Byrum, N. Kelley-Hoskins, R. Mukherjee, A. Furniss, T. B. Humensky, R. A. Ong, Wei Cui, E. Pueschel, M. Fernandez-Alonso, S. Schlenstedt, O. Hervet, Q. Feng, E. Roache, D. S. Hanna, P. Wilcox, M. P. Connolly, A. C. Rovero, N. H. Park, Gordon T. Richards, M. Kertzman, J. H. Buckley, Abraham D. Falcone, C. A. Johnson, V. Bugaev, Karlen Shahinyan, David A. Williams, E. Bourbeau, H. Fleischhack, Ralph Bird, T. T.Y. Lin, Julien Rousselle, P. T. Reynolds, I. Sadeh, M. Hütten, P. Kar, M. J. Lang, A. Popkow, J. Tyler, J. Grube, Manel Errando, A. Archer, Stephan O'Brien, G. H. Sembroski, Lucy Fortson, Martin Pohl, M. Buchovecky, J. P. Finley, Maria Krause, A. Wilhelm
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The astrophysical journal / 1 831(1), 113 (2016). doi:10.3847/0004-637X/831/1/113
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The astrophysical journal / 1 831(1), 113 (2016). doi:10.3847/0004-637X/831/1/113
Transient X-ray binaries produce major outbursts in which the X-ray flux can increase over the quiescent level by factors as large as $10^7$. The low-mass X-ray binary V 404 Cyg and the high-mass system 4U 0115+634 underwent such major outbursts in J
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c3b61a0c4652450671d35e3d67c46fa
http://iopscience.iop.org/article/10.3847/0004-637X/831/1/113/meta
http://iopscience.iop.org/article/10.3847/0004-637X/831/1/113/meta
Autor:
A. N. Otte, Geza Gyuk, E. Roache, M. P. Connolly, J. V. Tucci, Gernot Maier, S. P. Wakely, Abraham D. Falcone, Karlen Shahinyan, Wystan Benbow, N. Håkansson, Anna Barnacka, P. T. Reynolds, R. A. Ong, John L. Quinn, Ralph Bird, S. T. Griffiths, K. Sweeney, I. Telezhinsky, Jamie Holder, S. Federici, Martin Pohl, N. H. Park, J. Millis, J. Dumm, B. Zitzer, G. H. Sembroski, J. Grube, P. Kar, S. Godambe, Manel Errando, M. Kertzman, R. Welsing, M. J. Lang, L. C. Reyes, S. Kumar, K. Berger, Hugh Dickinson, D. S. Hanna, Xuhui Chen, Matteo Cerruti, Amy Furniss, Wei Cui, Henric Krawczynski, Y. Khassen, A. McCann, Q. Feng, A. O'Faolain de Bhroithe, David A. Williams, P. Kaaret, Lucy Fortson, D. Staszak, A. Popkow, Vladimir Vassiliev, H. Prokoph, Matthias Beilicke, J. S. Perkins, E. Pueschel, Markus Böttcher, J. Tyler, A. Wilhelm, A. Varlotta, A. Archer, J. V. Cardenzana, C. A. Johnson, E. Collins-Hughes, G. Hughes, David Kieda, Jodi Christiansen, J. D. Eisch, J. P. Finley, G. H. Gillanders, T. J. N. Nelson, S. McArthur, S. Griffin, K. Meagher, Jean-Francois Rajotte, S. Archambault, L. Ciupik, K. Ragan, V. Bugaev, H. Fleischhack, J. H. Buckley, A. W. Smith, A. S Madhavan, Gordon T. Richards, B. Behera, Daniel Nieto, P. Moriarty
Publikováno v:
Monthly notices of the Royal Astronomical Society 461(1), 202-208 (2016). doi:10.1093/mnras/stw1319
The BL Lacertae object 1ES 1440+122 was observed in the energy range from 85 GeV to 30 TeV by the VERITAS array of imaging atmospheric Cherenkov telescopes. The observations, taken between 2008 May and 2010 June and totalling 53 hours, resulted in th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f16e491e849e59ba81f8ff41771b06c7
http://hdl.handle.net/10379/10278
http://hdl.handle.net/10379/10278
Autor:
M. Buchovecky, Q. Feng, J. Grube, I. Telezhinsky, Jamie Holder, S. O'Brien, P. T. Reynolds, A. McCann, P. Fortin, Ralph Bird, Hugh Dickinson, Wystan Benbow, Anushka Udara Abeysekara, S. Archambault, Reshmi Mukherjee, A. Archer, D. Staszak, Martin Pohl, A. N. Otte, K. Meagher, S. McArthur, E. Pueschel, Maria Krause, O. M. Weiner, D. J. Fegan, Karen Byrum, J. D. Eisch, Abraham D. Falcone, Daniel Nieto, A. Weinstein, Karlen Shahinyan, S. Vincent, G. H. Gillanders, N. H. Park, D. S. Hanna, L. Ciupik, David A. Williams, N. Håkansson, Henrike Fleischhack, P. Kaaret, J. V. Cardenzana, J. V. Tucci, M. J. Lang, Moritz Hütten, Gernot Maier, John L. Quinn, N. Kelley-Hoskins, C. A. Johnson, K. Ragan, Geza Gyuk, Lucy Fortson, S. P. Wakely, R. A. Ong, David Kieda, F. Krennrich, Sinéad M. Griffin, J. Tyler, Matteo Cerruti, J. H. Buckley, Amy Furniss, Gordon T. Richards, E. Roache, P. Moriarty, J. P. Finley, G. Ratliff, Xuhui Chen, J. S. Perkins, Jodi Christiansen, T. B. Humensky, G. H. Sembroski, B. Zitzer, Manel Errando, S. Kumar, T. T.Y. Lin, A. Popkow, M. Kertzman, A. O'Faolain de Bhroithe, Wei Cui, A. Petrashyk, P. Kar, Marcos Santander
Publikováno v:
The astrophysical journal / 2 818(2), L33 (2016). doi:10.3847/2041-8205/818/2/L33
The astrophysical journal / 2 818(2), L33(2016). doi:10.3847/2041-8205/818/2/L33
The F-type star KIC 8462852 has recently been identified as an exceptional target for search for extraterrestrial intelligence (SETI) observations. We describe an a
The F-type star KIC 8462852 has recently been identified as an exceptional target for search for extraterrestrial intelligence (SETI) observations. We describe an a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7a98e95157da53ba9eb5251b82ed951
http://hdl.handle.net/10379/10075
http://hdl.handle.net/10379/10075
A search for very high energy gamma rays from the missing link binary pulsar J1023+0038 with VERITAS
Autor:
Wystan Benbow, John L. Quinn, A. Petrashyk, M. J. Lang, P. Kar, O. M. Weiner, Jonathan Biteau, J. P. Finley, B. Zitzer, N. Håkansson, Henrike Fleischhack, David Kieda, A. W. Smith, A. Flinders, Q. Feng, Abraham D. Falcone, Gordon T. Richards, E. Roache, Karlen Shahinyan, E. Pueschel, Geza Gyuk, S. Vincent, Nahee Park, A. Varlotta, N. Kelley-Hoskins, T. B. Humensky, Maria Krause, P. Moriarty, K. L. Byrum, Wei Cui, J. Grube, P. Kaaret, J. V. Cardenzana, J. D. Eisch, S. McArthur, A. McCann, Xuhui Chen, V. Bugaev, L. Ciupik, S. Archambault, Reshmi Mukherjee, Daniel Nieto, A. O'Faolain de Bhroithe, Sinéad M. Griffin, A. Popkow, E. Aliu, Maria Chernyakova, Lucy Fortson, J. Tyler, Matteo Cerruti, Moritz Hütten, J. H. Buckley, R. A. Ong, A. N. Otte, Amy Furniss, Marcos Santander, M. Kertzman, Martin Pohl, S. P. Wakely, P. Fortin, V. Pelassa, C. B. Rulten, Ralph Bird, G. H. Sembroski, A. Loo, K. Meagher, Hugh Dickinson, Mallory S. E. Roberts, M. Buchovecky, M. P. Connolly, D. Pandel, P. T. Reynolds, A. J.R. Weinstein, C. A. Johnson, J. V. Tucci, Gernot Maier, A. Wilhelm, D. Staszak, K. Ragan, I. Telezhinsky, Jamie Holder, David A. Williams, Thanh Huy Nguyen, A. Archer, G. H. Gillanders
Publikováno v:
The astrophysical journal / 1 831(2), 193 (2016). doi:10.3847/0004-637X/831/2/193
The binary millisecond radio pulsar PSR J1023+0038 exhibits many characteristics similar to the gamma-ray binary system PSR B1259--63/LS 2883, making it an ideal candidate for the study of high-energy non-thermal emission. It has been the subject of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1f4e9ba7f7c97358443d77d00e1791d
https://bib-pubdb1.desy.de/record/316601
https://bib-pubdb1.desy.de/record/316601