Search

Your search keyword '"Abe, S"' showing total 21 results
Start Over Author "Abe, S" Publisher edp sciences
21 results on '"Abe, S"'

1. Insights into the broadband emission of the TeV blazar Mrk 501 during the first X-ray polarization measurements.

Author

MAGIC Collaboration, Abe, S., Abhir, J., Acciari, V. A., Aguasca-Cabot, A., Agudo, I., Aniello, T., Ansoldi, S., Antonelli, L. A., Arbet Engels, A., Arcaro, C., Asano, K., Babić, A., Baquero, A., Barres de Almeida, U., Barrio, J. A., Batković, I., Bautista, A., Baxter, J., and Becerra González, J.

Subjects
*X-rays, *CRAB Nebula, *ELECTRON distribution, *BREWSTER'S angle, *GAMMA ray bursts, *OPTICAL polarization, *BL Lacertae objects, *LINEAR polarization, *SYNCHROTRONS
Abstract

Aims. We present the first multiwavelength study of Mrk 501 that contains simultaneous very-high-energy (VHE) γ-ray observations and X-ray polarization measurements from the Imaging X-ray Polarimetry Explorer (IXPE). Methods. We used radio-to-VHE data from a multiwavelength campaign carried out between March 1, 2022, and July 19, 2022 (MJD 59639 to MJD 59779). The observations were performed by MAGIC, Fermi-LAT, NuSTAR, Swift (XRT and UVOT), and several other instruments that cover the optical and radio bands to complement the IXPE pointings. We characterized the dynamics of the broadband emission around the X-ray polarization measurements through its multiband fractional variability and correlations, and compared changes observed in the polarization degree to changes seen in the broadband emission using a multi-zone leptonic scenario. Results. During the IXPE pointings, the VHE state is close to the average behavior, with a 0.2–1 TeV flux of 20%–50% of the emission of the Crab Nebula. Additionally, it shows low variability and a hint of correlation between VHE γ-rays and X-rays. Despite the average VHE activity, an extreme X-ray behavior is measured for the first two IXPE pointings, taken in March 2022 (MJD 59646 to 59648 and MJD 59665 to 59667), with a synchrotron peak frequency > 1 keV. For the third IXPE pointing, in July 2022 (MJD 59769 to 59772), the synchrotron peak shifts toward lower energies and the optical/X-ray polarization degrees drop. All three IXPE epochs show an atypically low Compton dominance in the γ-rays. The X-ray polarization is systematically higher than at lower energies, suggesting an energy stratification of the jet. While during the IXPE epochs the polarization angles in the X-ray, optical, and radio bands align well, we find a clear discrepancy in the optical and radio polarization angles in the middle of the campaign. Such results further support the hypothesis of an energy-stratified jet. We modeled broadband spectra taken simultaneous to the IXPE pointings, assuming a compact zone that dominates in the X-rays and the VHE band, and an extended zone stretching farther downstream in the jet that dominates the emission at lower energies. NuSTAR data allow us to precisely constrain the synchrotron peak and therefore the underlying electron distribution. The change between the different states observed in the three IXPE pointings can be explained by a change in the magnetization and/or the emission region size, which directly connects the shift in the synchrotron peak to lower energies with the drop in the polarization degree. [ABSTRACT FROM AUTHOR]

Published
2024
Full Text
View/download PDF

2. Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data

Author

Abe, H., primary, Abe, K., additional, Abe, S., additional, Acciari, V. A., additional, Aguasca-Cabot, A., additional, Agudo, I., additional, Alvarez Crespo, N., additional, Aniello, T., additional, Ansoldi, S., additional, Antonelli, L. A., additional, Aramo, C., additional, Arbet-Engels, A., additional, Arcaro, C., additional, Artero, M., additional, Asano, K., additional, Aubert, P., additional, Baack, D., additional, Babić, A., additional, Baktash, A., additional, Bamba, A., additional, Baquero Larriva, A., additional, Baroncelli, L., additional, Barres de Almeida, U., additional, Barrio, J. A., additional, Batković, I., additional, Baxter, J., additional, Becerra González, J., additional, Bednarek, W., additional, Bernardini, E., additional, Bernardos, M. I., additional, Bernete Medrano, J., additional, Berti, A., additional, Besenrieder, J., additional, Bhattacharjee, P., additional, Biederbeck, N., additional, Bigongiari, C., additional, Biland, A., additional, Bissaldi, E., additional, Blanch, O., additional, Bonnoli, G., additional, Bordas, P., additional, Bošnjak, Ž., additional, Bulgarelli, A., additional, Burelli, I., additional, Burmistrov, L., additional, Buscemi, M., additional, Busetto, G., additional, Campoy Ordaz, A., additional, Cardillo, M., additional, Caroff, S., additional, Carosi, A., additional, Carosi, R., additional, Carrasco, M. S., additional, Carretero-Castrillo, M., additional, Cassol, F., additional, Castro-Tirado, A. J., additional, Cauz, D., additional, Cerasole, D., additional, Ceribella, G., additional, Chai, Y., additional, Cheng, K., additional, Chiavassa, A., additional, Chikawa, M., additional, Chytka, L., additional, Cifuentes, A., additional, Cikota, S., additional, Colombo, E., additional, Contreras, J. L., additional, Cornelia, A., additional, Cortina, J., additional, Costantini, H., additional, Covino, S., additional, D’Amico, G., additional, D’Elia, V., additional, Da Vela, P., additional, Dalchenko, M., additional, Dazzi, F., additional, De Angelis, A., additional, de Bony de Lavergne, M., additional, De Lotto, B., additional, De Lucia, M., additional, de Menezes, R., additional, Del Peral, L., additional, Del Popolo, A., additional, Deleglise, G., additional, Delfino, M., additional, Delgado Mendez, C., additional, Delgado Mengual, J., additional, della Volpe, D., additional, Dellaiera, M., additional, Depaoli, D., additional, Di Piano, A., additional, Di Pierro, F., additional, Di Pilato, A., additional, Di Tria, R., additional, Di Venere, L., additional, Dominik, R. M., additional, Dominis Prester, D., additional, Donini, A., additional, Dorner, D., additional, Doro, M., additional, Díaz, C., additional, Eisenberger, L., additional, Elsässer, D., additional, Emery, G., additional, Escudero, J., additional, Fallah Ramazani, V., additional, Fariña, L., additional, Fattorini, A., additional, Ferrara, G., additional, Ferrarotto, F., additional, Fiasson, A., additional, Foffano, L., additional, Font, L., additional, Freixas Coromina, L., additional, Fröse, S., additional, Fukami, S., additional, Fukazawa, Y., additional, Garcia López, R. J., additional, Garcia, E., additional, Garczarczyk, M., additional, García López, R. J., additional, Gasbarra, C., additional, Gasparrini, D., additional, Gasparyan, S., additional, Gaug, M., additional, Geyer, D., additional, Giesbrecht Paiva, J. G., additional, Giglietto, N., additional, Giordano, F., additional, Gliwny, P., additional, Godinović, N., additional, Grau, R., additional, Green, D., additional, Green, J. G., additional, Gunji, S., additional, Günther, P., additional, Hackfeld, J., additional, Hadasch, D., additional, Hahn, A., additional, Hashiyama, K., additional, Hassan, T., additional, Hayashi, K., additional, Heckmann, L., additional, Heller, M., additional, Herrera Llorente, J., additional, Hirotani, K., additional, Hoffmann, D., additional, Horns, D., additional, Houles, J., additional, Hrabovsky, M., additional, Hrupec, D., additional, Hui, D., additional, Hütten, M., additional, Iarlori, M., additional, Imazawa, R., additional, Inada, T., additional, Inome, Y., additional, Ioka, K., additional, Iori, M., additional, Iotov, R., additional, Ishio, K., additional, Jacquemont, M., additional, Jiménez Martínez, I., additional, Jobst, E., additional, Jormanainen, J., additional, Jurysek, J., additional, Kagaya, M., additional, Karas, V., additional, Katagiri, H., additional, Kataoka, J., additional, Kerszberg, D., additional, Kluge, G. W., additional, Kobayashi, Y., additional, Kohri, K., additional, Kong, A., additional, Kouch, P. M., additional, Kubo, H., additional, Kushida, J., additional, Lainez, M., additional, Lamanna, G., additional, Lamastra, A., additional, Le Flour, T., additional, Leone, F., additional, Lindfors, E., additional, Linhoff, L., additional, Linhoff, M., additional, Lombardi, S., additional, Longo, F., additional, Loporchio, S., additional, Lorini, A., additional, Lozano Bahilo, J., additional, Luque-Escamilla, P. L., additional, Lyard, E., additional, Láinez Lezáun, M., additional, López-Coto, R., additional, López-Moya, M., additional, López-Oramas, A., additional, Machado de Oliveira Fraga, B., additional, Majumdar, P., additional, Makariev, M., additional, Mandat, D., additional, Maneva, G., additional, Manganaro, M., additional, Mangano, S., additional, Mang, N., additional, Manicò, G., additional, Mannheim, K., additional, Mariotti, M., additional, Marquez, P., additional, Marsella, G., additional, Martinez, O., additional, Martínez, G., additional, Martínez, M., additional, Martí, J., additional, Mas-Aguilar, A., additional, Maurin, G., additional, Mazin, D., additional, Menchiari, S., additional, Mender, S., additional, Mestre Guillen, E., additional, Micanovic, S., additional, Miceli, D., additional, Miener, T., additional, Miranda, J. M., additional, Mirzoyan, R., additional, Mizuno, T., additional, Mićanović, S., additional, Molero González, M., additional, Molina, E., additional, Mondal, H. A., additional, Montaruli, T., additional, Monteiro, I., additional, Moralejo, A., additional, Morcuende, D., additional, Morselli, A., additional, Moya, V., additional, Muraishi, H., additional, Murase, K., additional, Nagataki, S., additional, Nakamori, T., additional, Nanci, C., additional, Neronov, A., additional, Neustroev, V., additional, Nickel, L., additional, Nievas Rosillo, M., additional, Nigro, C., additional, Nikolić, L., additional, Nilsson, K., additional, Nishijima, K., additional, Njoh Ekoume, T., additional, Noda, K., additional, Nosek, D., additional, Nozaki, S., additional, Ohishi, M., additional, Ohtani, Y., additional, Oka, T., additional, Okumura, A., additional, Orito, R., additional, Otero-Santos, J., additional, Paiano, S., additional, Palatiello, M., additional, Paneque, D., additional, Pantaleo, F. R., additional, Paoletti, R., additional, Paredes, J. M., additional, Pavletić, L., additional, Pech, M., additional, Pecimotika, M., additional, Peresano, M., additional, Persic, M., additional, Pfeiffle, F., additional, Pietropaolo, E., additional, Pihet, M., additional, Pirola, G., additional, Plard, C., additional, Podobnik, F., additional, Poireau, V., additional, Polo, M., additional, Pons, E., additional, Prada Moroni, P. G., additional, Prandini, E., additional, Prast, J., additional, Principe, G., additional, Priyadarshi, C., additional, Prouza, M., additional, Rando, R., additional, Rhode, W., additional, Ribó, M., additional, Rico, J., additional, Righi, C., additional, Rizi, V., additional, Rodriguez Fernandez, G., additional, Rodríguez Frías, M. D., additional, Sahakyan, N., additional, Saito, T., additional, Sakurai, S., additional, Sanchez, D. A., additional, Satalecka, K., additional, Sato, M., additional, Sato, Y., additional, Saturni, F. G., additional, Savchenko, V., additional, Schleicher, B., additional, Schmidt, K., additional, Schmuckermaier, F., additional, Schubert, J. L., additional, Schussler, F., additional, Schweizer, T., additional, Sciaccaluga, A., additional, Siegert, T., additional, Silvia, R., additional, Sitarek, J., additional, Sliusar, V., additional, Sobczynska, D., additional, Spolon, A., additional, Stamerra, A., additional, Strišković, J., additional, Strom, D., additional, Strzys, M., additional, Suda, Y., additional, Suutarinen, S., additional, Šarić, T., additional, Tajima, H., additional, Takahashi, H., additional, Takahashi, M., additional, Takata, J., additional, Takeishi, R., additional, Tam, P. H. T., additional, Tanaka, S. J., additional, Tateishi, D., additional, Tavecchio, F., additional, Temnikov, P., additional, Terada, Y., additional, Terauchi, K., additional, Terzić, T., additional, Teshima, M., additional, Tluczykont, M., additional, Tokanai, F., additional, Torres, D. F., additional, Tosti, L., additional, Travnicek, P., additional, Truzzi, S., additional, Tutone, A., additional, Ubach, S., additional, Vacula, M., additional, Vallania, P., additional, van Scherpenberg, J., additional, Vazquez Acosta, M., additional, Ventura, S., additional, Verguilov, V., additional, Viale, I., additional, Vigliano, A., additional, Vigorito, C. F., additional, Visentin, E., additional, Vitale, V., additional, Voutsinas, G., additional, Vovk, I., additional, Vuillaume, T., additional, Vázquez Acosta, M., additional, Walter, R., additional, Wei, Z., additional, Will, M., additional, Yamamoto, T., additional, Yamazaki, R., additional, Yoshida, T., additional, Yoshikoshi, T., additional, and Zywucka, N., additional

Published
2023
Full Text
View/download PDF

3. Star tracking for pointing determination of Imaging Atmospheric Cherenkov Telescopes. Application to the Large-Sized Telescope of the Cherenkov Telescope Array

Author

Abe, K., primary, Abe, S., additional, Aguasca-Cabot, A., additional, Agudo, I., additional, Alvarez Crespo, N., additional, Antonelli, L. A., additional, Aramo, C., additional, Arbet-Engels, A., additional, Cornelia, A., additional, Artero, M., additional, Asano, K., additional, Aubert, P., additional, Baktash, A., additional, Bamba, A., additional, Baquero Larriva, A., additional, Baroncelli, L., additional, Barres de Almeida, U., additional, Barrio, J. A., additional, Batkovic, I., additional, Baxter, J., additional, Becerra González, J., additional, Bernardini, E., additional, Bernardos, M. I., additional, Bernete Medrano, J., additional, Berti, A., additional, Bhattacharjee, P., additional, Biederbeck, N., additional, Bigongiari, C., additional, Bissaldi, E., additional, Blanch, O., additional, Bonnoli, G., additional, Bordas, P., additional, Bulgarelli, A., additional, Burelli, I., additional, Burmistrov, L., additional, Buscemi, M., additional, Cardillo, M., additional, Caroff, S., additional, Carosi, A., additional, Cassol, F., additional, Cauz, D., additional, Ceribella, G., additional, Chai, Y., additional, Cheng, K., additional, Chiavassa, A., additional, Chikawa, M., additional, Chytka, L., additional, Cifuentes, A., additional, Contreras, J. L., additional, Cortina, J., additional, Costantini, H., additional, Dalchenko, M., additional, De Angelis, A., additional, de Bony de Lavergne, M., additional, De Lotto, B., additional, de Menezes, R., additional, Deleglise, G., additional, Delgado, C., additional, Delgado Mengual, J., additional, della Volpe, D., additional, Dellaiera, M., additional, Di Piano, A., additional, Di Pierro, F., additional, Di Tria, R., additional, Di Venere, L., additional, Díaz, C., additional, Dominik, R. M., additional, Dominis Prester, D., additional, Donini, A., additional, Dorner, D., additional, Doro, M., additional, Elsässer, D., additional, Emery, G., additional, Escudero, J., additional, Fallah Ramazani, V., additional, Ferrara, G., additional, Ferrarotto, F., additional, Fiasson, A., additional, Freixas Coromina, L., additional, Fröse, S., additional, Fukami, S., additional, Fukazawa, Y., additional, Garcia, E., additional, Garcia López, R., additional, Gasbarra, C., additional, Gasparrini, D., additional, Geyer, D., additional, Giesbrecht Paiva, J., additional, Giglietto, N., additional, Giordano, F., additional, Giro, E., additional, Gliwny, P., additional, Godinovic, N., additional, Grau, R., additional, Green, D., additional, Green, J., additional, Gunji, S., additional, Günther, P., additional, Hackfeld, J., additional, Hadasch, D., additional, Hahn, A., additional, Hashiyama, K., additional, Hassan, T., additional, Hayashi, K., additional, Heckmann, L., additional, Heller, M., additional, Herrera Llorente, J., additional, Hirotani, K., additional, Hoffmann, D., additional, Horns, D., additional, Houles, J., additional, Hrabovsky, M., additional, Hrupec, D., additional, Hui, D., additional, Hütten, M., additional, Iarlori, M., additional, Imazawa, R., additional, Inada, T., additional, Inome, Y., additional, Ioka, K., additional, Iori, M., additional, Ishio, K., additional, Jacquemont, M., additional, Jimenez Martinez, I., additional, Jurysek, J., additional, Kagaya, M., additional, Karas, V., additional, Katagiri, H., additional, Kataoka, J., additional, Kerszberg, D., additional, Kobayashi, Y., additional, Kohri, K., additional, Kong, A., additional, Kubo, H., additional, Kushida, J., additional, Lainez, M., additional, Lamanna, G., additional, Lamastra, A., additional, Le Flour, T., additional, Linhoff, M., additional, Longo, F., additional, López-Coto, R., additional, López-Oramas, A., additional, Loporchio, S., additional, Lorini, A., additional, Luque-Escamilla, P. L., additional, Majumdar, P., additional, Makariev, M., additional, Mandat, D., additional, Manganaro, M., additional, Manicò, G., additional, Mannheim, K., additional, Mariotti, M., additional, Marquez, P., additional, Marsella, G., additional, Martí, J., additional, Martinez, O., additional, Martínez, G., additional, Martínez, M., additional, Mas-Aguilar, A., additional, Maurin, G., additional, Mazin, D., additional, Mestre Guillen, E., additional, Micanovic, S., additional, Miceli, D., additional, Miener, T., additional, Miranda, J. M., additional, Mirzoyan, R., additional, Mizuno, T., additional, Molero Gonzalez, M., additional, Molina, E., additional, Montaruli, T., additional, Monteiro, I., additional, Moralejo, A., additional, Morcuende, D., additional, Morselli, A., additional, Muraishi, H., additional, Murase, K., additional, Nagataki, S., additional, Nakamori, T., additional, Nickel, L., additional, Nievas, M., additional, Nishijima, K., additional, Noda, K., additional, Nosek, D., additional, Nozaki, S., additional, Ohishi, M., additional, Ohtani, Y., additional, Oka, T., additional, Okumura, A., additional, Orito, R., additional, Otero-Santos, J., additional, Palatiello, M., additional, Paneque, D., additional, Pantaleo, F. R., additional, Paoletti, R., additional, Paredes, J. M., additional, Pech, M., additional, Pecimotika, M., additional, Peresano, M., additional, Pfeiffle, F., additional, Pietropaolo, E., additional, Pirola, G., additional, Plard, C., additional, Podobnik, F., additional, Poireau, V., additional, Polo, M., additional, Pons, E., additional, Prandini, E., additional, Prast, J., additional, Principe, G., additional, Priyadarshi, C., additional, Prouza, M., additional, Rando, R., additional, Rhode, W., additional, Ribó, M., additional, Rizi, V., additional, Rodriguez Fernandez, G., additional, Saito, T., additional, Sakurai, S., additional, Sanchez, D. A., additional, Šarić, T., additional, Sato, Y., additional, Saturni, F. G., additional, Schleicher, B., additional, Schmuckermaier, F., additional, Schubert, J. L., additional, Schussler, F., additional, Schweizer, T., additional, Sato, M., additional, Siegert, T., additional, Silvia, R., additional, Sitarek, J., additional, Sliusar, V., additional, Spolon, A., additional, Strišković, J., additional, Strzys, M., additional, Suda, Y., additional, Tajima, H., additional, Takahashi, H., additional, Takahashi, M., additional, Takata, J., additional, Takeishi, R., additional, Tam, P. H. T., additional, Tanaka, S. J., additional, Tateishi, D., additional, Temnikov, P., additional, Terada, Y., additional, Terauchi, K., additional, Terzic, T., additional, Teshima, M., additional, Tluczykont, M., additional, Tokanai, F., additional, Torres, D. F., additional, Travnicek, P., additional, Truzzi, S., additional, Tutone, A., additional, Vacula, M., additional, Vallania, P., additional, van Scherpenberg, J., additional, Vázquez Acosta, M., additional, Viale, I., additional, Vigliano, A., additional, Vigorito, C. F., additional, Vitale, V., additional, Voutsinas, G., additional, Vovk, I., additional, Vuillaume, T., additional, Walter, R., additional, Wei, Z., additional, Will, M., additional, Yamamoto, T., additional, Yamazaki, R., additional, Yoshida, T., additional, Yoshikoshi, T., additional, and Zywucka, N., additional

Published
2023
Full Text
View/download PDF

4. Multi-year characterisation of the broad-band emission from the intermittent extreme BL Lac 1ES 2344+514.

Author

Abe, H., Abe, S., Acciari, V. A., Agudo, I., Aniello, T., Ansoldi, S., Antonelli, L. A., Arbet Engels, A., Arcaro, C., Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., Barres de Almeida, U., Batković, I., Baxter, J., Becerra González, J., Bernardini, E., and Bernete, J.

Subjects
*SPECTRAL energy distribution, *X-ray spectra, *HARD X-rays, *BL Lacertae objects
Abstract

Aims. The BL Lac 1ES 2344+514 is known for temporary extreme properties characterised by a shift of the synchrotron spectral energy distribution (SED) peak energy νsynch, p above 1 keV. While those extreme states have only been observed during high flux levels thus far, additional multi-year observing campaigns are required to achieve a coherent picture. Here, we report the longest investigation of the source from radio to very high energy (VHE) performed so far, focussing on a systematic characterisation of the intermittent extreme states. Methods. We organised a monitoring campaign covering a 3-year period from 2019 to 2021. More than ten instruments participated in the observations in order to cover the emission from radio to VHE. In particular, sensitive X-ray measurements by XMM-Newton, NuSTAR, and AstroSat took place simultaneously with multi-hour MAGIC observations, providing an unprecedented constraint of the two SED components for this blazar. Results. While our results confirm that 1ES 2344+514 typically exhibits νsynch, p > 1 keV during elevated flux periods, we also find periods where the extreme state coincides with low flux activity. A strong spectral variability thus happens in the quiescent state, and is likely caused by an increase in the electron acceleration efficiency without a change in the electron injection luminosity. On the other hand, we also report a strong X-ray flare (among the brightest for 1ES 2344+514) without a significant shift of νsynch, p. During this particular flare, the X-ray spectrum is among the softest of the campaign. It unveils complexity in the spectral evolution, where the common harder-when-brighter trend observed in BL Lacs is violated. By combining Swift-XRT and Swift-UVOT measurements during a low and hard X-ray state, we find an excess of the UV flux with respect to an extrapolation of the X-ray spectrum to lower energies. This UV excess implies that at least two regions significantly contribute to the infrared/optical/ultraviolet/X-ray emission. Using the simultaneous MAGIC, XMM-Newton, NuSTAR, and AstroSat observations, we argue that a region possibly associated with the 10 GHz radio core may explain such an excess. Finally, we investigate a VHE flare, showing an absence of simultaneous variability in the 0.3−2 keV band. Using time-dependent leptonic modelling, we show that this behaviour, in contradiction to single-zone scenarios, can instead be explained by a two-component model. [ABSTRACT FROM AUTHOR]

Published
2024
Full Text
View/download PDF

5. Multiwavelength study of the galactic PeVatron candidate LHAASO J2108+5157

Author

Abe, S., primary, Aguasca-Cabot, A., additional, Agudo, I., additional, Alvarez Crespo, N., additional, Antonelli, L. A., additional, Aramo, C., additional, Arbet-Engels, A., additional, Artero, M., additional, Asano, K., additional, Aubert, P., additional, Baktash, A., additional, Bamba, A., additional, Baquero Larriva, A., additional, Baroncelli, L., additional, Barres de Almeida, U., additional, Barrio, J. A., additional, Batkovic, I., additional, Baxter, J., additional, Becerra González, J., additional, Bernardini, E., additional, Bernardos, M. I., additional, Bernete Medrano, J., additional, Berti, A., additional, Bhattacharjee, P., additional, Biederbeck, N., additional, Bigongiari, C., additional, Bissaldi, E., additional, Blanch, O., additional, Bordas, P., additional, Buisson, C., additional, Bulgarelli, A., additional, Burelli, I., additional, Buscemi, M., additional, Cardillo, M., additional, Caroff, S., additional, Carosi, A., additional, Cassol, F., additional, Cauz, D., additional, Ceribella, G., additional, Chai, Y., additional, Cheng, K., additional, Chiavassa, A., additional, Chikawa, M., additional, Chytka, L., additional, Cifuentes, A., additional, Contreras, J. L., additional, Cortina, J., additional, Costantini, H., additional, D’Amico, G., additional, Dalchenko, M., additional, De Angelis, A., additional, de Bony de Lavergne, M., additional, De Lotto, B., additional, de Menezes, R., additional, Deleglise, G., additional, Delgado, C., additional, Delgado Mengual, J., additional, della Volpe, D., additional, Dellaiera, M., additional, Di Piano, A., additional, Di Pierro, F., additional, Di Tria, R., additional, Di Venere, L., additional, Díaz, C., additional, Dominik, R. M., additional, Dominis Prester, D., additional, Donini, A., additional, Dorner, D., additional, Doro, M., additional, Elsässer, D., additional, Emery, G., additional, Escudero, J., additional, Fallah Ramazani, V., additional, Ferrara, G., additional, Fiasson, A., additional, Freixas Coromina, L., additional, Fröse, S., additional, Fukami, S., additional, Fukazawa, Y., additional, Garcia, E., additional, Garcia López, R., additional, Gasparrini, D., additional, Geyer, D., additional, Giesbrecht Paiva, J., additional, Giglietto, N., additional, Giordano, F., additional, Giro, E., additional, Gliwny, P., additional, Godinovic, N., additional, Grau, R., additional, Green, D., additional, Green, J., additional, Gunji, S., additional, Hackfeld, J., additional, Hadasch, D., additional, Hahn, A., additional, Hashiyama, K., additional, Hassan, T., additional, Hayashi, K., additional, Heckmann, L., additional, Heller, M., additional, Herrera Llorente, J., additional, Hirotani, K., additional, Hoffmann, D., additional, Horns, D., additional, Houles, J., additional, Hrabovsky, M., additional, Hrupec, D., additional, Hui, D., additional, Hütten, M., additional, Imazawa, R., additional, Inada, T., additional, Inome, Y., additional, Ioka, K., additional, Iori, M., additional, Ishio, K., additional, Iwamura, Y., additional, Jacquemont, M., additional, Jimenez Martinez, I., additional, Jurysek, J., additional, Kagaya, M., additional, Karas, V., additional, Katagiri, H., additional, Kataoka, J., additional, Kerszberg, D., additional, Kobayashi, Y., additional, Kong, A., additional, Kubo, H., additional, Kushida, J., additional, Lainez, M., additional, Lamanna, G., additional, Lamastra, A., additional, Le Flour, T., additional, Linhoff, M., additional, Longo, F., additional, López-Coto, R., additional, López-Moya, M., additional, López-Oramas, A., additional, Loporchio, S., additional, Lorini, A., additional, Luque-Escamilla, P. L., additional, Majumdar, P., additional, Makariev, M., additional, Mandat, D., additional, Manganaro, M., additional, Manicò, G., additional, Mannheim, K., additional, Mariotti, M., additional, Marquez, P., additional, Marsella, G., additional, Martí, J., additional, Martinez, O., additional, Martínez, G., additional, Martínez, M., additional, Marusevec, P., additional, Mas-Aguilar, A., additional, Maurin, G., additional, Mazin, D., additional, Mestre Guillen, E., additional, Micanovic, S., additional, Miceli, D., additional, Miener, T., additional, Miranda, J. M., additional, Mirzoyan, R., additional, Mizuno, T., additional, Molero Gonzalez, M., additional, Molina, E., additional, Montaruli, T., additional, Monteiro, I., additional, Moralejo, A., additional, Morcuende, D., additional, Morselli, A., additional, Mrakovcic, K., additional, Murase, K., additional, Nagai, A., additional, Nakamori, T., additional, Nickel, L., additional, Nievas, M., additional, Nishijima, K., additional, Noda, K., additional, Nosek, D., additional, Nozaki, S., additional, Ohishi, M., additional, Ohtani, Y., additional, Okazaki, N., additional, Okumura, A., additional, Orito, R., additional, Otero-Santos, J., additional, Palatiello, M., additional, Paneque, D., additional, Pantaleo, F. R., additional, Paoletti, R., additional, Paredes, J. M., additional, Pavletić, L., additional, Pech, M., additional, Pecimotika, M., additional, Pietropaolo, E., additional, Pirola, G., additional, Podobnik, F., additional, Poireau, V., additional, Polo, M., additional, Pons, E., additional, Prandini, E., additional, Prast, J., additional, Priyadarshi, C., additional, Prouza, M., additional, Rando, R., additional, Rhode, W., additional, Ribó, M., additional, Rizi, V., additional, Rodriguez Fernandez, G., additional, Saito, T., additional, Sakurai, S., additional, Sanchez, D. A., additional, Šarić, T., additional, Saturni, F. G., additional, Scherpenberg, J., additional, Schleicher, B., additional, Schmuckermaier, F., additional, Schubert, J. L., additional, Schussler, F., additional, Schweizer, T., additional, Seglar Arroyo, M., additional, Sitarek, J., additional, Sliusar, V., additional, Spolon, A., additional, Strišković, J., additional, Strzys, M., additional, Suda, Y., additional, Sunada, Y., additional, Tajima, H., additional, Takahashi, M., additional, Takahashi, H., additional, Takata, J., additional, Takeishi, R., additional, Tam, P. H. T., additional, Tanaka, S. J., additional, Tateishi, D., additional, Temnikov, P., additional, Terada, Y., additional, Terauchi, K., additional, Terzic, T., additional, Teshima, M., additional, Tluczykont, M., additional, Tokanai, F., additional, Torres, D. F., additional, Travnicek, P., additional, Truzzi, S., additional, Tutone, A., additional, Uhlrich, G., additional, Vacula, M., additional, Vázquez Acosta, M., additional, Verguilov, V., additional, Viale, I., additional, Vigliano, A., additional, Vigorito, C. F., additional, Vitale, V., additional, Voutsinas, G., additional, Vovk, I., additional, Vuillaume, T., additional, Walter, R., additional, Will, M., additional, Yamamoto, T., additional, Yamazaki, R., additional, Yoshida, T., additional, Yoshikoshi, T., additional, Zywucka, N., additional, Balbo, M., additional, Eckert, D., additional, and Tramacere, A., additional

Published
2023
Full Text
View/download PDF

6. MAGIC observations provide compelling evidence of hadronic multi-TeV emission from the putative PeVatron SNR G106.3+2.7.

Author

MAGIC Collaboration, Abe, H., Abe, S., Acciari, V. A., Agudo, I., Aniello, T., Ansoldi, S., Antonelli, L. A., Arbet Engels, A., Arcaro, C., Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., Barres de Almeida, U., Barrio, J. A., Batković, I., Baxter, J., and Becerra González, J.

Subjects
PARTICLE emissions, THRESHOLD energy, HADRONIC atoms, SUPERNOVA remnants, MAGIC, PARTICLE acceleration, COSMIC ray showers, COSMIC rays
Abstract

Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capable of accelerating cosmic rays (CRs) to ~ PeV energies. However, conclusive observational evidence for this has not yet been found. The SNR G106.3+2.7, detected at 1–100 TeV energies by different γ-ray facilities, is one of the most promising PeVatron candidates. This SNR has a cometary shape, which can be divided into a head and a tail region with different physical conditions. However, in which region the 100 TeV emission is produced has not yet been identified because of the limited position accuracy and/or angular resolution of existing observational data. Additionally, it remains unclear as to whether the origin of the γ-ray emission is leptonic or hadronic. Aims. With the better angular resolution provided by new MAGIC data compared to earlier γ-ray datasets, we aim to reveal the acceleration site of PeV particles and the emission mechanism by resolving the SNR G106.3+2.7 with 0.1° resolution at TeV energies. Methods. We observed the SNR G106.3+2.7 using the MAGIC telescopes for 121.7 h in total – after quality cuts – between May 2017 and August 2019. The analysis energy threshold is ~0.2 TeV, and the angular resolution is 0.07−0.1°. We examined the γ-ray spectra of different parts of the emission, whilst benefitting from the unprecedented statistics and angular resolution at these energies provided by our new data. We also used measurements at other wavelengths such as radio, X-rays, GeV γ-rays, and 10 TeV γ-rays to model the emission mechanism precisely. Results. We detect extended γ-ray emission spatially coincident with the radio continuum emission at the head and tail of SNR G106.3+2.7. The fact that we detect a significant γ-ray emission with energies above 6.0 TeV from only the tail region suggests that the emissions above 10 TeV detected with air shower experiments (Milagro, HAWC, Tibet ASγ and LHAASO) are emitted only from the SNR tail. Under this assumption, the multi-wavelength spectrum of the head region can be explained with either hadronic or leptonic models, while the leptonic model for the tail region is in contradiction with the emission above 10 TeV and X-rays. In contrast, the hadronic model could reproduce the observed spectrum at the tail by assuming a proton spectrum with a cutoff energy of ~1 PeV for that region. Such high-energy emission in this middle-aged SNR (4−10 kyr) can be explained by considering a scenario where protons escaping from the SNR in the past interact with surrounding dense gases at present. Conclusions. The γ-ray emission region detected with the MAGIC telescopes in the SNR G106.3+2.7 is extended and spatially coincident with the radio continuum morphology. The multi-wavelength spectrum of the emission from the tail region suggests proton acceleration up to ~PeV, while the emission mechanism of the head region could either be hadronic or leptonic. [ABSTRACT FROM AUTHOR]

Published
2023
Full Text
View/download PDF

7. Tokai Radioactive Ion Accelerator Complex (TRIAC)

Author

Watanabe, Y. X., Arai, S., Arakaki, Y., Fuchi, Y., Hirayama, Y., Imai, N., Ishiyama, H., Jeong, S. C., Kawakami, H., Miyatake, H., Niki, K., Nomura, T., Okada, M., Oyaizu, M., Tanaka, M. H., Tomizawa, M., Yoshikawa, N., Abe, S., Hanashima, S., Hashimoto, T., Ichikawa, S., Ikezoe, H., Ishii, T., Ishizaki, N., Kabumoto, H., Katayama, I., Koizumi, M., Matsuda, M., Mitsuoka, S., Nakanoya, T., Nishio, K., Ohuchi, I., Osa, A., Sato, T. K., Takeuchi, S., Tayama, H., and Tsukihashi, Y.

Published
2007
Full Text
View/download PDF

11. The formation of open fractures in cohesive materials, results of scaled analogue and numerical modelling on fault zone porosity development

Author

Urai J.L., Abe S., van Gent H, and Holland M.

Subjects
Physics, QC1-999
Abstract

We compare analogue and numerical models of dilatational fractures at low confining stress. These structures form an effective conduit for fluid flow in the field, but are difficult to model since they form in cohesive materials at low stresses. We use a truly cohesive powder for the analogue models and a Discrete Element Model (DEM) with brittle-elastic bonds for the numerical modelling. We show that despite variations in the model type, small differences in the location of initial fractures and the way these structures link-up to control the evolution of the model, the observed structures are robust. Three structural zones develop where different fault types dominate. In 3D numerical models we show an increase of the porosity on the fault zone with increasing deformation. The progradation direction is shown to be controlled by the position of the fracture. The combination of analogue models with cohesive powder and DEMs with internal cohesion is an excellent tool to study the evolution of open fractures.

Published
2010
Full Text
View/download PDF

14. MAGNETIC PROPERTY OF SmAg1-xInx

Author

Yagasaki, K., primary, Wauke, T., additional, Kaneko, T., additional, Miura, S., additional, Abe, S., additional, Fujii, H., additional, and Kadena, Y., additional

Published
1988
Full Text
View/download PDF

16. MAGNETIC PROPERTIES OF Cr2S3

Author

Yuzuri, M., primary, Kaneko, T., additional, Tsushima, T., additional, Miura, S., additional, Abe, S., additional, Kido, G., additional, and Nakagawa, N., additional

Published
1988
Full Text
View/download PDF

21. Implant-type tissue-engineered cartilage derived from human auricular chondrocyte may maintain cartilaginous property even under osteoinductive condition.

Author

Saka N, Watanabe Y, Abe S, Yajima A, and Kawano H

Abstract

Introduction: There is a growing need for chondrocyte implantation for reconstructing cartilage defect. However, ossification of the implanted cartilage is a challenging problem. Implant-type tissue-engineered cartilage from human auricular chondrocytes is a three-dimensional implant type cartilage using PLLA as a scaffold for chondrocytes. Although there is a study which evaluated the ossification of this cartilage in subcutaneous area, there is no study which clarify the possibility of ossification in osteoinductive surroundings. The purpose of this study was to elucidate the possibility of the ossification of implant-type tissue-engineered cartilage using human auricular chondrocyte in an osteoinductive environment., Methods: Human chondrocytes were harvested from ear cartilage. After dispersion by enzyme digestion, they were put into either a poly-L-lactic acid (PLLA) or poly lactic-co-glycolic acid (PLGA) scaffold, with collagen gel. Implant-type tissue-engineered cartilage was interposed between pieces of human iliac bone harvested from the same donor and implanted subcutaneously in nude rats. Scaffold without chondrocytes was used as a control. After 1, 3, and 6 months, ossification and cartilage formation were evaluated by X-ray, hematoxylin-eosin (HE) stain and toluidine blue (TB) stain., Results: There was no ossification of implant-type cartilage using human chondrocytes, even under osteoinductive conditions. HE staining showed that perichondrium formed around the constructs and chondrocytes were observed 6months after the implantation. TB staining showed metachromasia in every sample, with the area of metachromasia increasing over time, suggesting maturation of the cartilage., Conclusions: In conclusion, adjacent iliac bone had no apparent effect on the maturation of cartilage in implant-type tissue-engineered cartilage. Cartilage retention and maturation even in the presence of iliac bone could have been due to a scarcity of mesenchymal stem cells in the bone and surrounding area., (© N. Saka et al., published by EDP Sciences, 2019.)

Published
2019
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results