Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • HARMONI at ELT: opto-mechanics of the IFS pre-optics at CDR
    HARMONI is the first light visible and near-IR integral field spectrograph for the Extremely Large Telescope (ELT). It covers a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000 and spatial sampling from 60mas to 4mas. The IFS Pre-Optics (IPO), sub-system under the responsibility of the Institute of Astrophysics of
    Hernández, Elvio et al.

    Advertised on:

    8
    2022
    Citations
    0
  • HARMONI at ELT: mechanisms of the pre-optics at CDR
    HARMONI is the first light visible and near-IR integral field spectrograph for the Extremely Large Telescope (ELT). This instrument covers a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000 and spatial sampling from 60mas to 4mas. The Pre-Optics (sub-system under the responsibility of the IAC) contains five
    Hernández, Elvio et al.

    Advertised on:

    8
    2022
    Citations
    0
  • HARMONI at ELT: designing a laser guide star wavefront sensors for the ELT
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT covering a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000 and spatial sampling from 60mas to 4mas. It can operate in two Adaptive Optics modes - SCAO and LTAO - or with no AO. The project is preparing for Final Design Reviews
    Costille, Anne et al.

    Advertised on:

    8
    2022
    Citations
    0
  • HARMONI - the Extremely Large Telescope first light integral field spectrograph: pre-optics: stray light analysis
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000 and spatial sampling from 60mas to 4mas. The pre-optics take light entering the science cryostat (from the telescope or calibration system), reformatting and
    Garcia, M. A. et al.

    Advertised on:

    8
    2022
    Citations
    0
  • HADES RV Programme with HARPS-N at TNG. XV. Planetary occurrence rates around early-M dwarfs
    Aims: We present the complete Bayesian statistical analysis of the HArps-n red Dwarf Exoplanet Survey (HADES), which monitored the radial velocities of a large sample of M dwarfs with HARPS-N at TNG over the last 6 yr. Methods: The targets were selected in a narrow range of spectral types from M0 to M3, 0.3 M ⊙ < M ★ < 0.71 M ⊙, in order to study
    Pinamonti, M. et al.

    Advertised on:

    8
    2022
    Citations
    43
  • GTC Laser Guide Star Facility thermal design
    The Laser Guide Star Facility (LGSF) of Gran Telescopio Canarias (GTC) will be in charge of generating a Laser Guide Star (LGS) in the high atmosphere for the GTC Adaptive Optics System (GTCAO) to measure and correct the effect of the atmospheric turbulence. This proceeding analyses the thermal response of the LGS launch systems in operation under
    Simoes, R. et al.

    Advertised on:

    8
    2022
    Citations
    0