Relative stability of two laser frequency combs for routine operation on HARPS and FOCES

Bibcode
2016SPIE.9908E..64P
DOI
10.1117/12.2231434
Probst, R. A.; Lo Curto, Gaspare; Ávila, Gerardo; Brucalassi, Anna; Canto Martins, Bruno L.; de Castro Leão, Izan; Esposito, M.; González Hernández, J. I.; Grupp, Frank; Hänsch, Theodor W.; Holzwarth, Ronald; Kellermann, Hanna; Kerber, Florian; Mandel, Olaf; Manescau, Antonio; Pasquini, Luca; Pozna, Eszter; Rebolo, R.; Renan de Medeiros, José; Stark, Sebastian P.; Steinmetz, Tilo; Suárez Mascareño, A.; Udem, Thomas; Urrutia, Josefina; Wu, Yuanjie
Referencia bibliográfica

Proceedings of the SPIE, Volume 9908, id. 990864 16 pp. (2016).

Fecha de publicación:
8
2016
Número de autores
25
Número de autores del IAC
4
Número de citas
17
Número de citas referidas
16
Descripción
We report on the installation of a laser frequency comb (LFC) at the HARPS spectrograph, which we characterize relative to a second LFC that we had brought to HARPS for testing. This allowed us for the first time to probe the relative stability of two independent astronomical LFCs over an extended wavelength range. Both LFCs covered the spectral range of HARPS at least from 460 to 690 nm. After optimization of the fiber coupling to HARPS to suppress modal noise, a relative stability of the two LFCs in the low cm/s range was obtained. In combination with the results of our four earlier LFC test campaigns on HARPS, the available data now cover a time span of more than six years.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Convection, rotation, and magnetic activity of solar-like stars from asteroseismology
    During the last decade, our understanding of stellar physics and evolution has undergone a tremendous revolution thanks to asteroseismology. Space missions such as CoRoT, Kepler, K2, and TESS have already been observing millions of stars providing high-precision photometric data. With these data, it is possible to study the convection of stars
    Mathur, Savita

    Fecha de publicación:

    0
    2024
    Bibcode
    2024IAUS..365..195M
    Número de citas
    0
  • Sin árbitro
    Tales of stellar & binary co-evolution, told by stellar oscillations
    Stellar binarity and stellar oscillations are mostly seen and studied as two separate phenomena. Sometimes, one process is even complicating the analysis of the other beyond the liking of one or the other research community. However, the complete picture painted by the physical constraints provided by the combination of both processes represents a
    Beck, Paul G.

    Fecha de publicación:

    10
    2024
    Bibcode
    2024bss..confE..35B
    Número de citas
    0
  • Sin árbitro
    The Multimodal Universe: 100 TB of Machine Learning Ready Astronomical Data
    We present the Multimodal Universe, a new framework collating over 100 TB of multimodal astronomical data for its first release, spanning images, spectra, time series, tabular and hyper-spectral data. This unified collection enables a wide variety of machine learning (ML) applications and research across astronomical domains. The dataset brings
    Angeloudi, Eirini et al.

    Fecha de publicación:

    12
    2024
    Bibcode
    2024RNAAS...8..301A
    Número de citas
    0