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Wyszukujesz frazę "Brown, A." wg kryterium: Autor


Tytuł:
Direct and moderation effects on U.S. apparel manufacturers’ engagement in network ties
Autorzy:
Brown, David A.
Engel-Enright, Carol
Miller, Nancy J.
Wydawca:
Cognitione Foundation for the Dissemination of Knowledge and Science
Cytata wydawnicza:
Miller, N. J., Engel-Enright, C., & Brown, D. A. (2021). Direct and moderation effects on U.S. apparel manufacturers’ engagement in network ties. Journal of Entrepreneurship, Management and Innovation, 17(3), 67-113. https://doi.org/10.7341/20211733
Opis:
PURPOSE: Firms do not continue and prosper purely on their own individual endeavors, as each firm is influenced by the activities of others, and thus direct and indirect relationships shape the firm’s strategic management. These relationships form the tactics by which knowledge and other strategically important resources are accessed and created. Forming and maintaining ties among members of a network have been the subject of numerous research studies in the social, economic, and business literature. Our work is framed by the resource-based view of the firm perspective along with social capital theory and its shared constructs in network theory. Prior findings suggest that networking ties are strategic actions generated for firm growth and continuance. The ties may be short-term or develop into long-term relationships. The intent of this research is to fill some of the gaps in interorganizational networking strategy by analyzing five antecedents that have been suggested in the literature as individually associated with entrepreneurs’ engagement in network ties. In this way, our work provides another research avenue for examining networking’s contribution to strategic management. We hypothesized positive connections to entrepreneurs’ engagement in network ties from antecedents involving the firm’s knowledge absorptive capacity, business goals, entrepreneurial orientation, social interactions, and support from their environment. METHODOLOGY: In our quantitative approach, we tested our proposed macrolevel direct and moderating connections through an online survey of 125 U.S. apparel manufacturing firms. The apparel manufacturing sector in the U.S., as in many countries, has struggled with multiple disrupting factors contributing to the sector’s decline in firm continuance. FINDINGS: The results from OLS regression analyses support our hypothesized connections in that each of the five antecedents significantly contributed to entrepreneurs’ engagement in network ties; however, when all five were collectively examined only absorptive capacity, social interaction, and business goals were significant (R2 = 0.58). Further examination of moderation effects found the entrepreneurs’ perceptions of a supportive environment to modify both entrepreneurial orientation and business goals. RESEARCH AND PRACTICAL IMPLICATIONS: The effects of a supportive environment on business goals’ relationship with network ties were greater when perceptions of a supportive environment decreased, while the effects of a supportive environment on entrepreneurship orientation’s relationship with network ties were greater when perceptions of a supportive environment increased suggesting further study of U.S. entrepreneurs’ perceptions of their environments. Entrepreneurs’ interested in building domestic and international supply chain ties may find network ties provide one solution for adapting the firm’s resources for global competitiveness. Future studies may direct attention to other industry sectors or countries for replication with larger sample sizes as we recognize the limitations to generalizability and scale refinement due to our limited sample size. ORIGINALITY AND VALUE: The examination of five constructs to shed light on how an organization’s decisions may relate to engaging in networks and provides theoretical as well as practical implications that contribute to the larger organizational system framework.
Dostawca treści:
Repozytorium Centrum Otwartej Nauki
Artykuł
Tytuł:
TeV flaring activity of the AGN PKS 0625–354 in November 2018
Autorzy:
Schüssler, F.
Holch, T. L.
Batzofin, R.
Mehta, A.
Holler, M.
Niemiec, J.
Barnard, J.
Fontaine, G.
Wierzcholska, A.
Lenain, J.-P.
Aharonian, F.
Kostunin, D.
Lang, R. G.
de Ona Wilhelmi, E.
Ren, H.
Streil, K.
Giavitto, G.
Caroff, S.
Ohm, S.
Glawion, D.
O’Brien, P.
Khatoon, R.
Kasai, E.
Sanchez, D. A.
Takahashi, T.
Sasaki, M.
Leitl, F.
Spencer, S.
Barbosa Martins, V.
Ait Benkhali, F.
Punch, M.
Brose, R.
Reimer, O.
Boisson, C.
Casanova, S.
Bradascio, F.
Katarzyński, K.
Venter, C.
Chibueze, O.
Kluźniak, W.
Bernlöhr, K.
Bulik, T.
Böttcher, M.
Brun, F.
Panny, S.
Cerruti, M.
Veh, J.
van Eldik, C.
Borowska, J.
Schutte, H. M.
Stawarz, Łukasz
Hinton, J. A.
Salzmann, H.
Bylund, T.
Rudak, B.
Bolmont, J.
Reimer, A.
Joshi, V.
Bi, B.
de Naurois, M.
Suzuki, H.
Moulin, E.
Kosack, K.
Wagner, S. J.
Zargaryan, D.
Chand, T.
Mitchell, A.
Gabici, S.
Funk, S.
Chen, A.
Baktash, A.
Steinmassl, S.
Olivera-Nieto, L.
Breuhaus, M.
Dmytriiev, A.
Chandra, S.
Davids, I. D.
Ernenwein, J.-P.
Ostrowski, Michał
Doroshenko, V.
Khélifi, B.
Le Stum, S.
Jamrozy, Marek
Shapopi, J. N. S.
Cotter, G.
Mackey, J.
Moderski, R.
Leuschner, F.
Ghafourizadeh, S.
Einecke, S.
Becherini, Y.
Quirrenbach, A.
Cecil, R.
Aschersleben, J.
Specovius, A.
Tanaka, T.
Damascene Mbarubucyeye, J.
Meyer, M.
Jung-Richardt, I.
Chibueze, J.
Bruno, B.
Haerer, L.
Backes, M.
Prokhorov, D. A.
Djuvsland, J.
Vecchi, M.
Żywucka, N.
Horns, D.
Grolleron, G.
Marx, R.
Glicenstein, J. F.
Reichherzer, P.
Zouari, S.
Goswami, P.
Rieger, F.
Berge, D.
Lemière, A.
Parsons, R. D.
Pühlhofer, G.
Celic, J.
Brown, A.
Ashkar, H.
de Bony de Lavergne, M.
Luashvili, A.
Egberts, K.
Sol, H.
Montanari, A.
Sushch, I.
Jankowsky, F.
Burger-Scheidlin, C.
Glombitza, J.
Füßling, M.
Pita, S.
Sahakian, V.
Zdziarski, A. A.
Zech, A.
Steenkamp, R.
Zacharias, M.
Komin, Nu.
Opis:
Most γ-ray detected active galactic nuclei are blazars with one of their relativistic jets pointing towards the Earth. Only a few objects belong to the class of radio galaxies or misaligned blazars. Here, we investigate the nature of the object PKS 0625−354, its γ-ray flux and spectral variability and its broad-band spectral emission with observations from H.E.S.S., Fermi-LAT, Swift-XRT, and UVOT taken in November 2018. The H.E.S.S. light curve above 200 GeV shows an outburst in the first night of observations followed by a declining flux with a halving time scale of 5.9 h. The γγ-opacity constrains the upper limit of the angle between the jet and the line of sight to ∼10°. The broad-band spectral energy distribution shows two humps and can be well fitted with a single-zone synchrotron self Compton emission model. We conclude that PKS 0625−354, as an object showing clear features of both blazars and radio galaxies, can be classified as an intermediate active galactic nuclei. Multi-wavelength studies of such intermediate objects exhibiting features of both blazars and radio galaxies are sparse but crucial for the understanding of the broad-band emission of γ-ray detected active galactic nuclei in general.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Very-high-energy γ-ray emission from young massive star clusters in the Large Magellanic Cloud
Autorzy:
Schutte, H. M.
Rowell, G.
Montanari, A.
Marx, R.
Kundu, A.
Glicenstein, J. F.
Żywucka, N.
Jamrozy, Marek
Pühlhofer, G.
Martins, V. Barbosa
Benkhali, F. Ait
Ostrowski, Michał
Brown, A.
Böttcher, M.
Le Stum, S.
Leuschner, F.
Chibueze, O.
Ren, H.
Sushch, I.
Aschersleben, J.
White, R.
de Bony de Lavergne, M.
Mackey, J.
Kluźniak, W.
Renaud, M.
Mitchell, A.
Reimer, A.
Reville, B.
Vecchi, M.
de Naurois, M.
Lenain, J.-P.
Cristofari, P.
Ravikularaman, S.
Chandra, S.
Reimer, O.
Funk, S.
Horns, D.
Filipovic, M.
Sahakian, V.
Lang, R. G.
Egberts, K.
Casanova, S.
Moghadam, M. O.
Brose, R.
Hofmann, W.
Lemoine-Goumard, M.
Feijen, K.
Tsirou, M.
Schüssler, F.
Batzofin, R.
Ruiz-Velasco, E.
Mehta, A.
Borowska, J.
Wagner, S. J.
Bernlöhr, K.
Kosack, K.
Rudak, B.
Santangelo, A.
Spencer, S.
Zdziarski, A. A.
Jankowsky, F.
Bruno, B.
Cotter, G.
Khatoon, R.
Celic, J.
Jung-Richardt, I.
Katarzyński, K.
Brun, F.
Einecke, S.
Dmytriiev, A.
Devin, J.
Panny, S.
Chibueze, J.
Steppa, C.
Hinton, J. A.
Rieger, F.
Ashkar, H.
Heß, B.
Cerruti, M.
Lemière, A.
Sasaki, M.
Chand, T.
Stawarz, Łukasz
Niemiec, J.
Bolmont, J.
de Ona Wilhelmi, E.
Backes, M.
Berge, D.
Venter, C.
Pensec, U.
Aharonian, F.
Terrier, R.
Tsuji, N.
Khélifi, B.
Moderski, R.
Taylor, A. M.
Chen, A.
Becherini, Y.
Regeard, M.
Haerer, L.
Huang, Zhiqiu
Zacharias, M.
Marandon, V.
Peron, G.
Burger-Scheidlin, C.
Holch, T. L.
Sabri, K.
Gabici, S.
Vink, J.
Kostunin, D.
Djuvsland, J.
Grolleron, G.
Wierzcholska, A.
Djannati-Ataï, A.
Moulin, E.
Steinmassl, S.
van Eldik, C.
Martí-Devesa, G.
Ohm, S.
Olivera-Nieto, L.
Kasai, E.
Streil, K.
Zech, A.
Gallant, Y. A.
Komin, Nu.
Salzmann, H.
Schäfer, J.
Fontaine, G.
Mohrmann, L.
Quirrenbach, A.
Glombitza, J.
Sol, H.
Opis:
The Tarantula Nebula in the Large Magellanic Cloud is known for its high star formation activity. At its center lies the young massive star cluster R136, providing a significant amount of the energy that makes the nebula shine so brightly at many wavelengths. Recently, young massive star clusters have been suggested to also efficiently produce very high-energy cosmic rays, potentially beyond PeV energies. Here, we report the detection of very-high-energy γ-ray emission from the direction of R136 with the High Energy Stereoscopic System, achieved through a multicomponent, likelihood-based modeling of the data. This supports the hypothesis that R136 is indeed a very powerful cosmic-ray accelerator. Moreover, from the same analysis, we provide an updated measurement of the γ-ray emission from 30 Dor C, the only superbubble detected at TeV energies presently. The γ-ray luminosity above 0.5 TeV of both sources is (2–3) × 10$^{35}$ erg s$^{−1}$. This exceeds by more than a factor of 2 the luminosity of HESS J1646−458, which is associated with the most massive young star cluster in the Milky Way, Westerlund 1. Furthermore, the γ-ray emission from each source is extended with a significance of >3σ and a Gaussian width of about 30 pc. For 30 Dor C, a connection between the γ-ray emission and the nonthermal X-ray emission appears likely. Different interpretations of the γ-ray signal from R136 are discussed.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
H.E.S.S. programme searching for VHE gamma rays associated with FRBs
Autorzy:
Schüssler, F.
Batzofin, R.
Mehta, A.
Holler, M.
Niemiec, J.
Fontaine, G.
Santangelo, A.
Lenain, J.-P.
Aharonian, F.
Kostunin, D.
Ren, H.
de Ona Wilhelmi, E.
Regeard, M.
Khatoon, R.
Kasai, E.
Wierzcholska, Alicja
Takahashi, T.
Sasaki, M.
Spencer, S.
Steppa, C.
Schäfer, J.
Barbosa Martins, V.
Sharma, A.
Punch, M.
Brose, R.
Reimer, O.
Boisson, C.
Casanova, S.
Huang, Zhiqiu
Wach, T.
Bradascio, F.
Katarzyński, K.
Venter, C.
Chibueze, O.
Kluźniak, W.
Bernlöhr, K.
Böttcher, M.
Brun, F.
Panny, S.
Cerruti, M.
Marandon, V.
van Eldik, C.
Borowska, J.
Sabri, K.
Stawarz, Łukasz
Salzmann, H.
Rudak, B.
Bolmont, J.
Kerszberg, D.
Schutte, H.M.
Parsons, R.D.
Escañuela Nieves, C.
Jaitly, A.
de Naurois, M.
Moulin, E.
Kosack, K.
Żywucka-Hejzner, Natalia
Chand, T.
Mitchell, A.
Archaryya, A.
Lang, R.G.
Gabici, S.
Funk, S.
Ravikularaman, S.
Chen, A.
Steinmassl, S.
Olivera-Nieto, L.
Tsirou, M.
Dmytriiev, A.
Heß, B.
Chandra, S.
Ernenwein, J.-P.
Ostrowski, Michał
Moghadam, M.O.
Djannati-Ataï, A.
Kundu, A.
Khélifi, B.
Le Stum, S.
Jamrozy, Marek
Mackey, J.
Moderski, R.
Einecke, S.
O'Brien, P.
Becherini, Y.
Quirrenbach, A.
Aschersleben, J.
Tanaka, T.
Rowell, G.
Damascene Mbarubucyeye, J.
Meyer, M.
Jung-Richardt, I.
Chibueze, J.
Bruno, B.
Lemoine-Goumard, M.
Pensec, U.
Backes, M.
Djuvsland, J.
Vecchi, M.
Filipovic, M.
Horns, D.
Malyshev, D.
Zdziarski, A.A.
Grolleron, G.
Glicenstein, J.F.
Marx, R.
Rieger, F.
Berge, D.
Lemière, A.
de Assis Scarpin, J.
Pühlhofer, G.
Celic, J.
Brown, A.
Ashkar, H.
de Bony de Lavergne, M.
Hofmann, W.
Luashvili, A.
Egberts, K.
Wagner, S.J.
Shapopi, J.N.S.
Panter, M.
Jankowsky, F.
Burger-Scheidlin, C.
Glombitza, J.
Holch, T.L.
Pita, S.
Sahakian, V.
Reville, B.
Zech, A.
Steenkamp, R.
Komin, Nu.
Opis:
Fast Radio Bursts (FRBs) are highly energetic, extremely short-lived bursts of radio flashes. Despite extensive research, the exact cause of these outbursts remains speculative. The high luminosity, short duration, and high dispersion measure of these events suggest they result from extreme, high-energy extragalactic sources, such as highly magnetized and rapidly spinning neutron stars known as magnetars. The number of detected FRBs, including repeating ones, has grown rapidly in recent years. Except for FRB 20200428D, and FRB-like radio burst that is associated to Galactic magnetar SGR 1935+2154, no multi-wavelength counterpart to any FRB has been detected yet. The High Energy Stereoscopic System (H.E.S.S.) telescope has developed a program to follow up FRBs searching for their gamma-ray counterparts, helping to uncover the nature of FRBs and FRB sources. This paper provides an overview of the searches for FRB sources conducted by H.E.S.S., including follow-up observations and simultaneous multi-wavelength campaigns with radio and X-ray observatories. Among the FRB sources observed by H.E.S.S., nine are localized with redshifts ranging between 0.11 and 0.492 from 2015 to 2022. No significant very high energy (VHE) emission was detected during these observations. We report constraints on the VHE luminosity ranging from 10$^{44}$ erg s$^{-1}$ and 10$^{48}$ erg s$^{-1}$, placing limits on the FRB's region persistent VHE emission and potential FRB afterglow emission across timescales from hours to years.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
The Cherenkov Telescope Array potential for the study of young supernova remnants
Autorzy:
Rovero, A. C.
Huovelin, J.
Siejkowski, H.
Majumdar, P.
Hrupec, D.
Baushev, A.
Garcia, B.
Lucarelli, F.
Katz, U.
Orito, R.
Bulik, T.
Weinstein, A.
Nievas, M.
Hrabovsky, M.
Kubo, H.
Gaug, M.
Ohishi, M.
Kaufmann, S.
Di Giulio, C.
Mirabal, N.
Nosek, D.
Szanecki, M.
Dournaux, J.-L.
Komin, N.
Maccarone, M. C.
Ebr, J.
Nunio, F.
Yoshikoshi, T.
Bonardi, A.
Egberts, K.
Fontaine, G.
Lee, W. H.
Pech, M.
Kluźniak, W.
De Lotto, B.
Pareschi, G.
Lamanna, G.
Lenain, J.-P.
Kocot, J.
Persic, M.
Moulin, E.
Carr, J.
Chudoba, J.
Lohse, T.
Tibolla, O.
Meagher, K.
de los Reyes Lopez, R.
Hörandel, J.
Wilhelm, A.
Lombardi, S.
Nishijima, K.
Ong, R. A.
Romano, P.
Vallania, P.
Khélifi, B.
Fesquet, M.
Telezhinsky, I.
Jamrozy, Marek
de la Calle, I.
Rodriguez Fernandez, G.
Szepieniec, T.
Pohl, M.
Ohm, S.
Di Girolamo, T.
Palatka, M.
Font, L.
De Palma, F.
Mazziotta, M. N.
Giordano, F.
Acharya, B. S.
Di Pierro, F.
Stefanik, S.
Fleischhack, H.
Rainò, S.
Chadwick, P.
Kaaret, P. E.
Berge, D.
Wagner, S. J.
Becker Tjus, J.
Maier, G.
Morselli, A.
Gonzalez, M. M.
Wakely, S. P.
Giuliani, A.
Dwarkadas, V.
Niemiec, J.
Grabarczyk, T.
Caraveo, P.
Barrio, J. A.
Wierzcholska, Alicja
Rudak, B.
Busetto, G.
Contreras, J. L.
Burton, M.
Tovmassian, G.
Gargano, F.
Hassan, T.
Cotter, G.
Prouza, M.
Vigorito, C.
Bohacova, M.
Fuessling, M.
Brown, A.
Babic, A.
van Eldik, C.
Sillanpää, A.
Carosi, R.
Stolarczyk, T.
Aramo, C.
De Franco, A.
Malaguti, G.
Mandat, D.
Humensky, T. B.
López-Coto, R.
Wojcik, P.
Travnicek, P.
Kushida, J.
Janecek, P.
Quirrenbach, A.
Shayduk, M.
Vercellone, S.
Dazzi, F.
Garrido, D.
Otte, N.
López-Oramas, A.
Garcia López, R.
Connaughton, V.
Conforti, V.
Förster, A.
Godinovic, N.
Tejedor, L. A.
Bugaev, V.
Giglietto, N.
Trzeciak, M.
Schovanek, P.
Tibaldo, L.
Teshima, M.
Garczarczyk, M.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
The H.E.S.S. extragalactic sky survey with the first decade of observations
Autorzy:
Rowell, G.
Montanari, A.
Marx, R.
Kundu, A.
Glicenstein, J. F.
Goswami, P.
Sanchez, D. A.
Völk, H. J.
Jamrozy, Marek
Pühlhofer, G.
Suzuki, H.
Ostrowski, Michał
Brown, A.
Böttcher, M.
Le Stum, S.
Leuschner, F.
Chibueze, O.
Ren, H.
Aschersleben, J.
Bradascio, F.
de Bony de Lavergne, M.
Mackey, J.
Fegan, S.
Mitchell, A.
Reimer, A.
Reville, B.
Vecchi, M.
de Naurois, M.
Lenain, J.-P.
Cristofari, P.
Ravikularaman, S.
Chandra, S.
Reimer, O.
O’Brien, P.
Funk, S.
Bulik, T.
Horns, D.
Sahakian, V.
Lang, R. G.
Egberts, K.
Casanova, S.
Żywucka-Hejzner, Natalia
Holler, M.
Brose, R.
Hofmann, W.
Tanaka, T.
Ait Benkhali, F.
Lemoine-Goumard, M.
Tsirou, M.
Takahashi, T.
Schüssler, F.
Batzofin, R.
Ruiz-Velasco, E.
Mehta, A.
Sharma, A.
Borowska, J.
Wagner, S. J.
Bernlöhr, K.
Kosack, K.
Rudak, B.
Santangelo, A.
Spencer, S.
Zdziarski, A. A.
Boisson, C.
Jankowsky, F.
Shapopi, J. N. S.
Bruno, B.
Davids, I. D.
Luashvili, A.
Cotter, G.
Khatoon, R.
Celic, J.
Katarzyński, K.
Brun, F.
Einecke, S.
Dmytriiev, A.
Mbarubucyeye, J. D.
Devin, J.
Panny, S.
Chibueze, J.
Steppa, C.
Hinton, J. A.
Rieger, F.
Ashkar, H.
Heß, B.
Wierzcholska, Alicja
Cerruti, M.
Barbosa Martins, V.
Lemière, A.
Sasaki, M.
Chand, T.
Jardin-Blicq, A.
Stawarz, Łukasz
Niemiec, J.
Bolmont, J.
de Ona Wilhelmi, E.
Backes, M.
Berge, D.
Venter, C.
Pensec, U.
Aharonian, F.
Terrier, R.
Thakur, A.
Malyshev, D.
Khélifi, B.
Steenkamp, R.
Moderski, R.
Taylor, A. M.
Chen, A.
Becherini, Y.
Regeard, M.
Haerer, L.
Huang, Zhiqiu
Zacharias, M.
Marandon, V.
Bouyahiaoui, M.
Burger-Scheidlin, C.
Holch, T. L.
Gabici, S.
Vink, J.
Kostunin, D.
Djuvsland, J.
Grolleron, G.
Steinmassl, S.
van Eldik, C.
Martí-Devesa, G.
Olivera-Nieto, L.
Bylund, T.
Kasai, E.
Wach, T.
Zech, A.
Komin, Nu.
Salzmann, H.
Reis, I.
Schäfer, J.
Punch, M.
Fontaine, G.
Mohrmann, L.
Quirrenbach, A.
Glombitza, J.
Sol, H.
Panter, M.
Opis:
The results of the first extragalactic gamma-ray survey by the High Energy Stereoscopic System (H.E.S.S.) are presented. The survey comprises 2720 hours of very high-energy gamma-ray observations of the extragalactic sky, recorded with H.E.S.S. from 2004 up to the end of 2012. These data have been re-analysed using a common consistent set of up-to-date data calibration and analysis tools. From this analysis, a list of 23 detected objects, predominantly blazars, was obtained. This catalogue was assessed in terms of the source class populations that it contains. The level of source parameter bias for the blazar sources, probed by this observational dataset, was evaluated using Monte-Carlo simulations. Spectral results obtained with the H.E.S.S. data were compared with the Fermi-LAT catalogues to present the full gamma-ray picture of the detected objects. Lastly, this unique dataset was used to assess the contribution of BL Lacertae objects and flat-spectrum radio quasars to the extragalactic gamma-ray background light at several hundreds of gigaelectronvolts. These results are accompanied by the release of the high-level data to the astrophysical community.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Discovery of very-high-energy $\gamma$-ray emission from the vicinity of PSR J1913+1011 with HESS
Autorzy:
Hermann, G.
Fontaine, G.
Lohse, T.
Moderski, R.
Ward, M.
Braun, I.
Rudak, B.
Superina, G.
Hauser, D.
Latham, I. J.
Shalchi, A.
Brown, A. M.
Farnier, C.
Egberts, K.
Rosier-Lees, S.
Maurin, G.
Boutelier, T.
Domainko, W.
Heinzelmann, G.
O'C. Drury, L.
Stegmann, C.
Clapson, A. C.
Bulik, T.
van Eldik, C.
Beilicke, M.
Panter, M.
Terrier, R.
Akhperjanian, A. G.
Pedaletti, G.
Ripken, J.
Kerschhaggl, M.
Venter, C.
Santangelo, A.
Funk, Seb.
Dickinson, H. J.
Pühlhofer, G.
Schöck, F.
Marcowith, A.
Steenkamp, R.
Hoppe, S.
Hofmann, W.
Horns, D.
Bazer-Bachi, A. R.
de Naurois, M.
Aharonian, F.
Büsching, I.
Boisson, C.
Schröder, R.
Hauser, M.
Dalton, M.
Martineau-Huynh, O.
Stawarz, Łukasz
Vivier, M.
Füßling, M.
Moulin, E.
Schwanke, U.
de Jager, O. C.
Zech, A.
Nolan, S. J.
Jacholkowska, A.
Lenain, J.-P.
Nedbal, D.
Ostrowski, Michał
Tavernet, J.-P.
de Oña Wilhelmi, E.
Katarzyński, K.
Rayner, S. M.
Behera, B.
Costamante, L.
Ohm, S.
Rolland, L.
Raubenheimer, B. C.
Spangler, D.
Holleran, M.
Kosack, K.
Volpe, F.
Bühler, R.
Gallant, Y. A.
Hoffmann, A.
Dyks, J.
Glicenstein, J. F.
Olive, J.-P.
Punch, M.
Renaud, M.
Henri, G.
Borrel, V.
Fiasson, A.
Feinstein, F.
Dubois, F.
Bolz, O.
Degrange, B.
Rowell, G.
Pita, S.
Rob, L.
Maurin, D.
Lemoine-Goumard, M.
Jung, I.
Ruppel, J.
McComb, T. J. L.
Wagner, S. J.
Keogh, D.
Brion, E.
Völk, H. J.
Espigat, P.
Sahakian, V.
Khélifi, B.
Raue, M.
Osborne, J. L.
Bernlöhr, K.
Goret, P.
Coignet, G.
Dubus, G.
Martin, J. M.
Schwarzburg, S.
Chounet, L.-M.
Kendziorra, E.
Lemière, A.
Schwemmer, S.
Cornils, R.
Petrucci, P.-O.
Zdziarski, A. A.
Carrigan, S.
Masterson, C.
Benbow, W.
Hadjichristidis, C.
Sol, H.
Djannati-Ataï, A.
Giebels, B.
Orford, K. J.
Vialle, J. P.
Chadwick, P. M.
Glück, B.
Vasileiadis, G.
Komin, Nu.
Lamanna, G.
Barres de Almeida, U.
Tam, P. H.
Schlickeiser, R.
Vincent, P.
Hinton, J. A.
Pelletier, G.
Reimer, O.
Förster, A.
Emmanoulopoulos, D.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
HESS very-high-energy gamma-ray sources without identified counterparts
Autorzy:
Ward, M.
Rowell, G.
Akhperjanian, A. G.
Glicenstein, J. F.
Völk, H. J.
Martin, J. M.
Schröder, R.
Petrucci, P.-O.
Pühlhofer, G.
de Jager, O. C.
Raue, M.
Pita, S.
Vasileiadis, G.
Bolz, O.
Ostrowski, Michał
Coignet, G.
Renaud, M.
Barres de Almeida, U.
Pelletier, G.
Kerschhaggl, M.
Kendziorra, E.
Raubenheimer, B. C.
de Naurois, M.
Keogh, D.
Schöck, F.
Lenain, J.-P.
Martineau-Huynh, O.
Dyks, J.
Shalchi, A.
Jung, I.
Osborne, J. L.
Dalton, M.
Hadjichristidis, C.
Funk, S.
Costamante, L.
Bulik, T.
Spangler, D.
Vialle, J. P.
Horns, D.
Sahakian, V.
Egberts, K.
Hofmann, W.
Lamanna, G.
Lemoine-Goumard, M.
Schwemmer, S.
Farnier, C.
Dubois, F.
Glück, B.
Schlickeiser, R.
Vincent, P.
Degrange, B.
Wagner, S. J.
Bernlöhr, K.
Tam, P. H.
Kosack, K.
Rudak, B.
Santangelo, A.
Büsching, I.
Zdziarski, A. A.
Boisson, C.
Behera, B.
Cornils, R.
Rosier-Lees, S.
Bazer-Bachi, A. R.
Bühler, R.
Katarzyński, K.
Ripken, J.
Domainko, W.
Hoffmann, A.
Hinton, J. A.
Feinstein, F.
Lemière, A.
Braun, I.
Boutelier, T.
Masterson, C.
Vivier, M.
Stawarz, Łukasz
Carrigan, S.
Ranchon, S.
Lohse, T.
Dickinson, H. J.
O'C. Drury, L.
Hauser, M.
Venter, C.
Henri, G.
Nedbal, D.
Ruppel, J.
Aharonian, F.
Chounet, L.-M.
Terrier, R.
Rolland, L.
Khélifi, B.
Goret, P.
Moderski, R.
Pedaletti, G.
Steenkamp, R.
Nolan, S. J.
Emmanoulopoulos, D.
Clapson, A. C.
Stegmann, C.
Fiasson, A.
Brown, A. M.
Hauser, D.
Volpe, F.
Giebels, B.
Heinzelmann, G.
Marcowith, A.
Olive, J.-P.
Djannati-Ataï, A.
Moulin, E.
Förster, A.
Espigat, P.
McComb, T. J. L.
van Eldik, C.
Orford, K. J.
Schwanke, U.
Ohm, S.
Zech, A.
Borrel, V.
Dubus, G.
Beilicke, M.
Gallant, Y. A.
Komin, Nu.
Rob, L.
Latham, I. J.
Benbow, W.
Chadwick, P. M.
Punch, M.
Brion, E.
Füßling, M.
Maurin, G.
Rayner, S. M.
Holleran, M.
Fontaine, G.
Jacholkowska, A.
de Oña Wilhelmi, E.
Superina, G.
Hermann, G.
Tavernet, J.-P.
Maurin, D.
Sol, H.
Hoppe, S.
Schwarzburg, S.
Panter, M.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł

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