Radio to γ-ray observations of 3C 454.3:1993-1995

Bibcode
1997AIPC..410.1423A
DOI
10.1063/1.53955
Aller, M. F.; Marscher, A. P.; Hartman, R. C.; Aller, H. D.; Aller, M. C.; Balonek, T. J.; Begelman, M. C.; Chiaberge, M.; Clements, S. D.; Collmar, W.; de Francesco, G.; Gear, W. K.; Georganopoulos, M.; Ghisellini, G.; Glass, I. S.; González-Pérez, J. N.; Heinämäki, P.; Herter, M.; Hooper, E. J.; Hughes, P. A.; Johnson, W. N.; Katajainen, S.; Kidger, M. R.; Kraus, A.; Lanteri, L.; Lawrence, G. F.; Lichti, G. G.; Lin, Y. C.; Madejski, G. M.; McNaron-Brown, K.; Moore, E. M.; Mukherjee, R.; Nair, A. D.; Nilsson, K.; Peila, A.; Pierkowski, D. B.; Pohl, M.; Pursimo, T.; Raiteri, C. M.; Reich, W.; Robson, E. I.; Sillanpää, A.; Sikora, M.; Smith, A. G.; Steppe, H.; Stevens, J.; Takalo, L. O.; Teräsranta, H.; Tornikoski, M.; Valtaoja, E.; von Montigny, C.; Villata, M.; Wagner, S.; Wichmann, R.; Witzel, A.
Referencia bibliográfica

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1423-1427 (1997).

Fecha de publicación:
5
1997
Número de autores
55
Número de autores del IAC
2
Número de citas
6
Número de citas referidas
5
Descripción
Results from a multiwaveband study of the γ-ray-bright compact radio source 3C 454.3 are presented.
Tipo
Sin árbitro
Fuentes de rayos gamma
Estallidos de rayos gamma

Te puede interesar

  • Sin árbitro
    Workshop summary: Kaons@CERN 2023

    Kaon physics is at a turning point - while the rare-kaon experiments NA62 and KOTO are in full swing, the end of their lifetime is approaching and the future experimental landscape needs to be defined. With HIKE, KOTO-II and LHCb-Phase-II on the table and under scrutiny, it is a very good moment in time to take stock and contemplate about the

    Anzivino, G. et al.

    Fecha de publicación:

    4
    2024
    Bibcode
    2024EPJC...84..377A
    Número de citas
    0
  • Sin árbitro
    First light and results for atmospheric characterization with The Near Infra-Red Planet Searcher (NIRPS)

    NIRPS is a new fiber-fed high spectral resolution (~80k) spectrograph assisted by adaptive optics installed on the 3.6m telescope of ESO at LaSilla, Chile. Operated simultaneously with HARPS, NIRPS covers the Y, J, and H bands. The commissioning phase demonstrated high stability for time-series observations along precise radial velocities reaching

    Allart, Romain et al.

    Fecha de publicación:

    4
    2024
    Bibcode
    2024ESS.....562419A
    Número de citas
    0
  • Sin árbitro
    Nodal Precession of a Hot Jupiter Transiting the Edge of a Late A-Type Star TOI-1518

    TOI-1518b, a hot Jupiter around a late A-type star, is one of the few planetary systems that transit the edge of the stellar surface (the impact parameter b~0.9) among hot Jupiters around hot stars (Cabot et al. 2021). The host star's high rotation speed (Vsini s~85 km s -1) and the planet's nearly polar orbit (λ~120 deg) may cause a nodal

    Watanabe, Noriharu et al.

    Fecha de publicación:

    4
    2024
    Bibcode
    2024ESS.....561705W
    Número de citas
    0