The evolution of PUCHEROS from a basic to a competitive tool for stellar astrophysics
Identifikátory výsledku
Kód výsledku v 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>
Nalezeny alternativní kódy
RIV/00216208:11320/25:10512554
Výsledek na webu
<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>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
The evolution of PUCHEROS from a basic to a competitive tool for stellar astrophysics
Popis výsledku v původním jazyce
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.
Název v anglickém jazyce
The evolution of PUCHEROS from a basic to a competitive tool for stellar astrophysics
Popis výsledku anglicky
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.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2025
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
e-ISSN
1365-2966
Svazek periodika
542
Číslo periodika v rámci svazku
3
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
13
Strana od-do
1730-1742
Kód UT WoS článku
001565128800001
EID výsledku v databázi Scopus
2-s2.0-105014726975