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The evolution of PUCHEROS from a basic to a competitive tool for stellar astrophysics

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00638945" target="_blank" >RIV/67985815:_____/25:00638945 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/25:10512554

  • Result on the web

    <a href="https://hdl.handle.net/11104/0369951" target="_blank" >https://hdl.handle.net/11104/0369951</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/staf1290" target="_blank" >10.1093/mnras/staf1290</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The evolution of PUCHEROS from a basic to a competitive tool for stellar astrophysics

  • Original language description

    We present PUCHEROS+, a new spectrograph developed as an enhanced version of PUCHEROS (Pontificia Universidad Católica High Echelle Resolution Optical Spectrograph), which was the first high-resolution spectrograph built at the Pontificia Universidad Catolica de Chile (UC). With respect to its predecessor, PUCHEROS+ includes a substantial number of improvements, mainly: a new scientific detector, improved objective optics, calibration system, guiding, active thermal control, and remote observing mode. These upgrades convert our early prototype into a much more powerful instrument for science. With a spectral resolution of R=18 000, a spectral range between 400 and 730 nm and an instrument efficiency of about 30 per cent, PUCHEROS+ was tested at the ESO (European Southern Observatory) 1.52-m telescope where it has reached a limiting magnitude of about 12 in V band and radial velocity precision of about 30 m s(-1). The instrument was conceived as a pathfinder for the high-resolution echelle spectrograph PLATOSpec and at the same time, it demonstrates that a compact, relatively low-cost spectrograph can be efficiently employed for long-term monitoring campaigns and as support facility for space missions, in particular if operated remotely at relatively small- or medium-sized telescopes.

  • 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

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2025

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    0035-8711

  • e-ISSN

    1365-2966

  • Volume of the periodical

    542

  • Issue of the periodical within the volume

    3

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    13

  • Pages from-to

    1730-1742

  • UT code for WoS article

    001565128800001

  • EID of the result in the Scopus database

    2-s2.0-105014726975