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
18
Número de citas referidas
17
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
    joshspeagle/dynesty: v3.0.0
    This is major release with several infrastructural changes that will make future development of dynesty easier, as well as significant speedups. The release also deprecated some rarely used options. Major refactor of the code that makes it easier to add new samplers. Major speedup of the uniform sampler when sampling in parallel You can now provide
    Koposov, Sergey et al.

    Fecha de publicación:

    10
    2025
    Bibcode
    2025zndo..17268284K
    Número de citas
    1
  • Sin árbitro
    (163) Erigone, (302) Clarissa, and (752) Sulamitis as seen with JWST's NIRSpec
    Primitive asteroids in the Main Belt possess one of the most pristine inventories of materials in the Solar System. Main Belt primitive asteroids are particularly interesting due to clear evidence of phyllosilicates, i.e., silicates that have encountered liquid water and undergone chemical alteration. Since asteroids are thought to be likely
    Harvison, Brittany et al.

    Fecha de publicación:

    9
    2025
    Bibcode
    2025epsc.conf.1004H
    Número de citas
    0
  • Sin árbitro
    NEOMIR: project statut of ESA's space-based infrared mission for NEO detection and early warning
    To warn about potential asteroid or comet impacts, we must first observe and discover these objects through dedicated NEO surveys. Most current and planned surveys are ground-based and use visible light, but they face limitations like weather dependency, limited sky visibility, difficulty detecting at low galactic latitudes, and inability to
    Conversi, Luca et al.

    Fecha de publicación:

    9
    2025
    Bibcode
    2025epsc.conf.1329C
    Número de citas
    0