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

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00602020" target="_blank" >RIV/67985815:_____/23:00602020 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/23:10475990 RIV/68378271:_____/23:00602020 RIV/61989592:15310/23:73630924

  • Result on the web

    <a href="https://hdl.handle.net/11104/0359240" target="_blank" >https://hdl.handle.net/11104/0359240</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202346927" target="_blank" >10.1051/0004-6361/202346927</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

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

  • Original language description

    Aims. Large-Sized Telescope 1 (LST-1), the prototype for the Large-Sized Telescope at the upcoming Cherenkov Telescope Array Observatory, is concluding its commissioning phase at the Observatorio del Roque de los Muchachos on the island of La Palma. The proximity of LST-1 to the two MAGIC (Major Atmospheric Gamma Imaging Cherenkov) telescopes makes it possible to carry out observations of the same gamma-ray events with both systems. Methods. We describe the joint LST-1+MAGIC analysis pipeline and used simultaneous Crab Nebula observations and Monte Carlo simulations to assess the performance of the three-telescope system. The addition of the LST-1 telescope allows for the recovery of events in which one of the MAGIC images is too dim to survive analysis quality cuts. Results. Thanks to the resulting increase in the collection area and stronger background rejection, we found a significant improvement in sensitivity, allowing for the detection of 30% weaker fluxes in the energy range between 200 GeV and 3 TeV. The spectrum of the Crab Nebula, reconstructed in the energy range between similar to 60 GeV and similar to 10 TeV, is in agreement with previous measurements.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2023

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    680

  • Issue of the periodical within the volume

    Dec

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    21

  • Pages from-to

    A66

  • UT code for WoS article

    001142569000006

  • EID of the result in the Scopus database

    2-s2.0-85181004327