Analysis techniques and performance of the Domino Ring Sampler version 4 based readout for the MAGIC telescopes

Bibcode
2013nimpa.723..109s
DOI
10.1016/j.nima.2013.05.014
Sitarek, Julian; Gaug, Markus; Mazin, Daniel; Paoletti, Riccardo; Tescaro, D.
Referencia bibliográfica

Nuclear Instruments and Methods in Physics Research A, Volume 723, p. 109-120.

Fecha de publicación:
9
2013
Número de autores
5
Número de autores del IAC
1
Número de citas
21
Número de citas referidas
14
Descripción
Recently the readout of the MAGIC telescopes has been upgraded to a new system based on the Domino Ring Sampler version 4 chip. We present the analysis techniques and the signal extraction performance studies of this system. We study the behavior of the baseline, the noise, the cross-talk, the linearity and the time resolution. We investigate also the optimal signal extraction. In addition we show some of the analysis techniques specific to the readout based on the Domino Ring Sampler version 2 chip, previously used in the MAGIC II telescope.
Tipo
Con árbitro

Te puede interesar

  • Con árbitro
    A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3
    We report on deep SCUBA-2 observations at 850 $\mu$m and NOrthern Extended Millimetre Array (NOEMA) spectroscopic measurements at 2 mm of the environment surrounding the luminous, massive (M * ≈ 2 × 10 11 M ⊙) Herschel-selected source HerBS-70. This source was revealed by previous NOEMA observations to be a binary system of dusty star-forming
    Bakx, Tom J. L. C. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024MNRAS.530.4578B
    Número de citas
    0
  • Con árbitro
    Overmassive Black Holes at Cosmic Noon: Linking the Local and the High-redshift Universe
    We report for the first time a sample of 12 supermassive black holes (SMBHs) hosted by low-mass galaxies at cosmic noon, i.e., in a redshift range consistent with the peak of star formation history: z ∼ 1–3. These black holes are 2 orders of magnitude too massive for the stellar content of their hosts when compared with the local relation for
    Mezcua, Mar et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024ApJ...966L..30M
    Número de citas
    0
  • Con árbitro
    The tidal deformation and atmosphere of WASP-12 b from its phase curve★
    Context. Ultra-hot Jupiters present a unique opportunity to understand the physics and chemistry of planets, their atmospheres, and interiors at extreme conditions. WASP-12 b stands out as an archetype of this class of exoplanets, with a close-in orbit around its star that results in intense stellar irradiation and tidal effects. Aims: The goals
    Akinsanmi, B. et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024A&A...685A..63A
    Número de citas
    0