no code implementations • 1 Dec 2020 • S. Aune, J. Bortfeldt, F. Brunbauer, C. David, D. Desforge, G. Fanourakis, M. Gallinaro, F. García, I. Giomataris, T. Gustavsson, F. J. Iguaz, M. Kebbiri, K. Kordas, C. Lampoudis, P. Legou, M. Lisowska, J. Liu, M. Lupberger, O. Maillard, I. Manthos, H. Müller, E. Oliveri, T. Papaevangelou, K. Paraschou, M. Pomorski, B. Qi, F. Resnati, L. Ropelewski, D. Sampsonidis, L. Scharenberg, T. Schneider, L. Sohl, M. van Stenis, A. Tsiamis, Y. Tsipolitis, S. E. Tzamarias, A. Utrobicic, R. Veenhof, X. Wang, S. White, Z. Zhang, Y. Zhou
The multi-pad PICOSEC-Micromegas is an improved detector prototype with a segmented anode, consisting of 19 hexagonal pads.
Instrumentation and Detectors High Energy Physics - Experiment
1 code implementation • 31 Mar 2020 • Devansh Agarwal, D. R. Lorimer, M. P. Surnis, X. Pei, A. Karastergiou, G. Golpayegani, D. Werthimer, J. Cobb, M. A. McLaughlin, S. White, W. Armour, D. H. E. MacMahon, A. P. V. Siemion, G. Foster
Depending on the observing mode, this translates to peak flux sensitivities in the range 0. 14--0. 89~Jy.
Instrumentation and Methods for Astrophysics
no code implementations • 30 Mar 2017 • A. S. Trotter, D. E. Reichart, R. E. Egger, J. Stýblová, M. L. Paggen, J. R. Martin, D. A. Dutton, J. E. Reichart, N. D. Kumar, M. P. Maples, B. N. Barlow, T. A. Berger, A. C. Foster, N. R. Frank, F. D. Ghigo, J. B. Haislip, S. A. Heatherly, V. V. Kouprianov, A. P. LaCluyzé, D. A. Moffett, J. P. Moore, J. L. Stanley, S. White
We find that overall, between the late 1950s and late 2010s, Cas A faded at an average rate of $0. 670 \pm 0. 019$ %/yr in L band, consistent with Reichart & Stephens (2000).
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics
