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Akademický článek
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Autor:
Adams, C. B., Benbow, W., Brill, A., Buckley, J. H., Christiansen, J. L., Falcone, A., Feng, Q., Finley, J. P., Foote, G. M., Fortson, L., Furniss, A., Giuri, C., Hanna, D., Hassan, T., Hervet, O., Holder, J., Hona, B., Humensky, T. B., Jin, W., Kaaret, P., Kleiner, T. K., Kumar, S., Lang, M. J., Lundy, M., Maier, G., Moriarty, P., Mukherjee, R., Rosillo, M. Nievas, O'Brien, S., Park, N., Patel, S., Pfrang, K., Pohl, M., Prado, R. R., Pueschel, E., Quinn, J., Ragan, K., Reynolds, P. T., Ribeiro, D., Roache, E., Ryan, J. L., Santander, M., Weinstein, A., Williams, D. A., Williamson, T. J.
Publikováno v:
Astronomy and astrophysics 658, A83 (2022). doi:10.1051/0004-6361/202142275
Astronomy and astrophysics 658, A83 (2022). doi:10.1051/0004-6361/202142275
Context. The response of imaging air Cherenkov telescopes to incident $γ$-ray-initiated showers in the atmosphere changes as the telescopes age due to exposure to light
Context. The response of imaging air Cherenkov telescopes to incident $γ$-ray-initiated showers in the atmosphere changes as the telescopes age due to exposure to light
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ddad9cf1b1690e8c39c5d2b71d1c98d3
https://bib-pubdb1.desy.de/record/474671
https://bib-pubdb1.desy.de/record/474671
Autor:
Euclid Collaboration, Borlaff, A. S., Gómez-Alvarez, P., Altieri, B., Marcum, P. M., Vavrek, R., Laureijs, R., Kohley, R., Buitrago, F., Cuillandre, J. -C., Duc, P. -A., Gaspar Venancio, L. M., Amara, A., Andreon, S., Auricchio, N., Azzollini, R., Baccigalupi, C., Balaguera-Antolínez, A., Baldi, M., Bardelli, S., Bender, R., Biviano, A., Bodendorf, C., Bonino, D., Bozzo, E., Branchini, E., Brescia, M., Brinchmann, J., Burigana, C., Cabanac, R., Camera, S., Candini, G. P., Capobianco, V., Cappi, A., Carbone, C., Carretero, J., Carvalho, C. S., Casas, S., Castander, F. J., Castellano, M., Castignani, G., Cavuoti, S., Cimatti, A., Cledassou, R., Colodro-Conde, C., Congedo, G., Conselice, C. J., Conversi, L., Copin, Y., Corcione, L., Coupon, J., Courtois, H. M., Cropper, M., Da Silva, A., Degaudenzi, H., Di Ferdinando, D., Douspis, M., Dubath, F., Duncan, C. A. J., Dupac, X., Dusini, S., Ealet, A., Fabricius, M., Farina, M., Farrens, S., Ferreira, P. G., Ferriol, S., Finelli, F., Flose-Reimberg, P., Fosalba, P., Frailis, M., Franceschi, E., Fumana, M., Galeotta, S., Ganga, K., Garilli, B., Gillis, B., Giocoli, C., Gozaliasl, G., Graciá-Carpio, J., Grazian, A., Grupp, F., Haugan, S. V. H., Holmes, W., Hormuth, F., Jahnke, K., Keihanen, E., Kermiche, S., Kiessling, A., Kilbinger, M., Kirkpatrick, C. C., Kitching, T., Knapen, J. H., Kubik, B., Kümmel, M., Kunz, M., Kurki-Suonio, H., Liebing, P., Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Mainetti, G., Maino, D., Mansutti, O., Marggraf, O., Markovic, K., Martinelli, M., Martinet, N., Martínez-Delgado, D., Marulli, F., Massey, R., Maturi, M., Maurogordato, S., Medinaceli, E., Mei, S., Meneghetti, M., Merlin, E., Metcalf, R. B., Meylan, G., Moresco, M., Morgante, G., Moscardini, L., Munari, E., Nakajima, R., Neissner, C., Niemi, S. M., Nightingale, J. W., Nucita, A., Padilla, C., Paltani, S., Pasian, F., Patrizii, L., Pedersen, K., Percival, W. J., Pettorino, V., Pires, S., Poncet, M., Popa, L., Potter, D., Pozzetti, L., Raison, F., Rebolo, R., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rosset, C., Rossetti, E., Saglia, R., Sánchez, A. G., Sapone, D., Sauvage, M., Schneider, P., Scottez, V., Secroun, A., Seidel, G., Serrano, S., Sirignano, C., Sirri, G., Skottfelt, J., Stanco, L., Starck, J. L., Sureau, F., Tallada-Crespí, P., Taylor, A. N., Tenti, M., Tereno, I., Teyssier, R., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E. A., Valenziano, L., Valiviita, J., Vassallo, T., Viel, M., Wang, Y., Weller, J., Whittaker, L., Zacchei, A., Zamorani, G., Zucca, E.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
Universidad de Nebrija
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 657, pp.A92. ⟨10.1051/0004-6361/202141935⟩
Astronomy & Astrophysics, 657:A92
Astronomy & astrophysics, 657:A92. EDP Sciences
Universidad de Nebrija
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 657, pp.A92. ⟨10.1051/0004-6361/202141935⟩
Astronomy & Astrophysics, 657:A92
Astronomy & astrophysics, 657:A92. EDP Sciences
Full list of authors: Borlaff, A. S.; Gómez-Alvarez, P.; Altieri, B.; Marcum, P. M.; Vavrek, R.; Laureijs, R.; Kohley, R.; Buitrago, F.; Cuillandre, J. -C.; Duc, P. -A.; Gaspar Venancio, L. M.; Amara, A.; Andreon, S.; Auricchio, N.; Azzollini, R.; B
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::87afbea55c8d6dbd6dc20c915b23827d
https://hdl.handle.net/11587/467398
https://hdl.handle.net/11587/467398
Autor:
A. Zaslavsky, I. Mann, J. Soucek, A. Czechowski, D. Píša, J. Vaverka, N. Meyer-Vernet, M. Maksimovic, E. Lorfèvre, K. Issautier, K. Rackovic Babic, S. D. Bale, M. Morooka, A. Vecchio, T. Chust, Y. Khotyaintsev, V. Krasnoselskikh, M. Kretzschmar, D. Plettemeier, M. Steller, Š. Štverák, P. Trávníček, A. Vaivads
Publikováno v:
Astronomy & Astrophysics, 656, pp. 1-13
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 656, pp.A30. ⟨10.1051/0004-6361/202140969⟩
Astronomy & Astrophysics, 656, 1-13
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 656, pp.A30. ⟨10.1051/0004-6361/202140969⟩
Astronomy & Astrophysics, 656, 1-13
Impacts of dust grains on spacecraft are known to produce typical impulsive signals in the voltage waveform recorded at the terminals of electric antennas. Such signals are routinely detected by the Time Domain Sampler (TDS) system of the Radio and P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9bbe14d5148e1f07405d892dfe14b63
Autor:
Jordi Portell, Ulrich Bastian, Alex Bombrun, Nicholas Rowell, Nigel Hambly, Michael Davidson, M. Riello, C. Crowley, A. Mora, F. van Leeuwen, U. Lammers, F. De Angeli, M. Biermann, C. Fabricius, J. Castañeda, Lennart Lindegren, Jose M Hernandez, G. Gracia, Anthony G. A. Brown, D. W. Evans, D. Busonero
Publikováno v:
Astronomy and Astrophysics, 649
Digital.CSIC. Repositorio Institucional del CSIC
instname
Rowell, N, Davidson, M, Lindegren, L, Leeuwen, F V, Castañeda, J, Fabricius, C, Bastian, U, Hambly, N C, Hernández, J, Bombrun, A, Evans, D W, Angeli, F D, Riello, M, Busonero, D, Crowley, C, Mora, A, Lammers, U, Gracia, G, Portell, J, Biermann, M & Brown, A G A 2021, ' Gaia Early Data Release 3 : Modelling and calibration of Gaia's point and line spread functions ', Astronomy and Astrophysics, vol. 649, A11, pp. 1-22 . https://doi.org/10.1051/0004-6361/202039448
Digital.CSIC. Repositorio Institucional del CSIC
instname
Rowell, N, Davidson, M, Lindegren, L, Leeuwen, F V, Castañeda, J, Fabricius, C, Bastian, U, Hambly, N C, Hernández, J, Bombrun, A, Evans, D W, Angeli, F D, Riello, M, Busonero, D, Crowley, C, Mora, A, Lammers, U, Gracia, G, Portell, J, Biermann, M & Brown, A G A 2021, ' Gaia Early Data Release 3 : Modelling and calibration of Gaia's point and line spread functions ', Astronomy and Astrophysics, vol. 649, A11, pp. 1-22 . https://doi.org/10.1051/0004-6361/202039448
Rowell, N., et al.
[Context] The unprecedented astrometric precision of the Gaia mission relies on accurate estimates of the locations of sources in the Gaia data stream. This is ultimately performed by point spread function (PSF) fitting, which
[Context] The unprecedented astrometric precision of the Gaia mission relies on accurate estimates of the locations of sources in the Gaia data stream. This is ultimately performed by point spread function (PSF) fitting, which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54c9874d3da888e6078d3a9a4e06a989
https://hdl.handle.net/1887/3250901
https://hdl.handle.net/1887/3250901
Autor:
Martin J. Dyer, P. Kerry, A. J. Brown, D. I. Sahman, Naidu Bezawada, T. Gamble, Enric Palle, Tim Morris, Pablo Rodríguez-Gil, T. Muñoz-Darias, Leander Mehrgan, C Miller, D. Ives, Jim M. Wild, Elmé Breedt, T. Shahbaz, J. Casares, Antonio Cabrera-Lavers, S. P. Littlefair, David Lunney, Manuel A. P. Torres, D. Garcia-Alvarez, Ingrid Pelisoli, Cornelis M. Dubbeldam, Richard Ashley, V. S. Dhillon, Martin Black, S D Dixon, Xiaofeng Gao, Steven G. Parsons, Romano L. M. Corradi, J. Stegmeier, Richard Wilson, R D Domínguez, M. J. Green, David Henry, T. R. Marsh, James Osborn, A. de Ugarte Postigo
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2021, Vol.507(1), pp.350-366 [Peer Reviewed Journal]
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Full list of authors: Dhillon, V. S.; Bezawada, N.; Black, M.; Dixon, S. D.; Gamble, T.; Gao, X.; Henry, D. M.; Kerry, P.; Littlefair, S. P.; Lunney, D. W.; Marsh, T. R.; Miller, C.; Parsons, S. G.; Ashley, R. P.; Breedt, E.; Brown, A.; Dyer, M. J.;
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::42ce69ddb90e8cce3910f64695fb13ea
Autor:
Dmitry Khangulyan, Diego F. Torres, E. de Oña Wilhelmi, Enrique Mestre, Fabio Acero, Roberta Zanin
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly notices of the Royal Astronomical Society 509(1), 337-346 (2020). doi:10.1093/mnras/staa3599
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly notices of the Royal Astronomical Society 509(1), 337-346 (2020). doi:10.1093/mnras/staa3599
Digital.CSIC. Repositorio Institucional del CSIC
instname
Monthly Notices of the Royal Astronomical Society, 2021, 501 (1), pp.337-346. ⟨10.1093/mnras/staa3599⟩
Monthly notices of the Royal Astronomical Society 509(1), 337 - 346 (2020). doi:10.1093/mnras/staa3599
Since 2009, several rapid and bright flares have been observed at high energies (>100 MeV) from the direction of the Crab Nebula. Several hypo
Since 2009, several rapid and bright flares have been observed at high energies (>100 MeV) from the direction of the Crab Nebula. Several hypo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f50b44cc3d65148c8c2187acedbb08eb
https://hal.archives-ouvertes.fr/hal-03070605
https://hal.archives-ouvertes.fr/hal-03070605
Autor:
Adam, R, Ade, PAR, Aghanim, N, Arnaud, M, Aumont, J, Baccigalupi, C, Banday, AJ, Barreiro, RB, Bartlett, JG, Bartolo, N, Battaner, E, Benabed, K, Benoit-Lévy, A, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bonaldi, A, Bonavera, L, Bond, JR, Borrill, J, Bouchet, FR, Boulanger, F, Bracco, A, Bucher, M, Burigana, C, Butler, RC, Calabrese, E, Cardoso, J-F, Catalano, A, Challinor, A, Chamballu, A, Chary, R-R, Chiang, HC, Christensen, PR, Clements, DL, Colombi, S, Colombo, LPL, Combet, C, Couchot, F, Coulais, A, Crill, BP, Curto, A, Cuttaia, F, Danese, L, Davies, RD, Davis, RJ, de Bernardis, P, de Zotti, G, Delabrouille, J, Delouis, J-M, Désert, F-X, Dickinson, C, Diego, JM, Dolag, K, Dole, H, Donzelli, S, Doré, O, Douspis, M, Ducout, A, Dunkley, J, Dupac, X, Efstathiou, G, Elsner, F, Enßlin, TA, Eriksen, HK, Falgarone, E, Finelli, F, Forni, O, Frailis, M, Fraisse, AA, Franceschi, E, Frejsel, A, Galeotta, S, Galli, S, Ganga, K, Ghosh, T, Giard, M, Giraud-Héraud, Y, Gjerløw, E, González-Nuevo, J, Górski, KM, Gratton, S, Gregorio, A, Gruppuso, A, Guillet, V, Hansen, FK, Hanson, D, Harrison, DL, Helou, G, Henrot-Versillé, S, Hernández-Monteagudo, C, Herranz, D, Hivon, E, Hobson, M, Holmes, WA, Huffenberger, KM, Hurier, G, Jaffe, AH, Jaffe, TR, Jewell, J
The six parameters of the standard ΛCDM model have best-fit values derived from the Planck temperature power spectrum that are shifted somewhat from the best-fit values derived from WMAP data. These shifts are driven by features in the Planck temper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::be0b28e0718bac6260a5fe6ab31478a8
https://escholarship.org/uc/item/3475d58t
https://escholarship.org/uc/item/3475d58t