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/

  • Refereed
    Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument
    The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg 2 over 5 yr to constrain the cosmic expansion history through precise measurements of baryon acoustic oscillations (BAO). The scientific program for DESI was evaluated during a 5 month survey validation (SV) campaign before beginning full operations
    Adame, A. G. et al.

    Advertised on:

    2
    2024
    Bibcode
    2024AJ....167...62A
    Citations
    0
  • Refereed
    Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument
    The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg 2 over 5 yr to constrain the cosmic expansion history through precise measurements of baryon acoustic oscillations (BAO). The scientific program for DESI was evaluated during a 5 month survey validation (SV) campaign before beginning full operations
    DESI Collaboration et al.

    Advertised on:

    2
    2024
    Bibcode
    2024AJ....167...62D
    Citations
    188
  • Refereed
    TOI-544 b: a potential water-world inside the radius valley in a two-planet system
    We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V = 10.8), which hosts a small transiting planet recently discovered by the Transiting Exoplanet Survey Satellite (TESS). We collected 122 high-resolution High Accuracy Radial velocity Planet Searcher (HARPS) and HARPS-N spectra to spectroscopically confirm

    Advertised on:

    2
    2024
    Bibcode
    2024MNRAS.527.11138
    Citations
    0
  • Refereed
    TOI-544 b: a potential water-world inside the radius valley in a two-planet system
    We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V = 10.8), which hosts a small transiting planet recently discovered by the Transiting Exoplanet Survey Satellite (TESS). We collected 122 high-resolution High Accuracy Radial velocity Planet Searcher (HARPS) and HARPS-N spectra to spectroscopically confirm
    Osborne, H. L. M. et al.

    Advertised on:

    2
    2024
    Bibcode
    2024MNRAS.52711138O
    Citations
    15
  • Refereed
    The three hundred project: mapping the matter distribution in galaxy clusters via deep learning from multiview simulated observations
    A galaxy cluster as the most massive gravitationally bound object in the Universe, is dominated by dark matter, which unfortunately can only be investigated through its interaction with the luminous baryons with some simplified assumptions that introduce an un-preferred bias. In this work, we, for the first time, propose a deep learning method
    de Andres, Daniel et al.

    Advertised on:

    2
    2024
    Bibcode
    2024MNRAS.528.1517D
    Citations
    5
  • Refereed
    The TESS-Keck Survey. XVII. Precise Mass Measurements in a Young, High-multiplicity Transiting Planet System Using Radial Velocities and Transit Timing Variations
    We present a radial velocity (RV) analysis of TOI-1136, a bright Transiting Exoplanet Survey Satellite (TESS) system with six confirmed transiting planets, and a seventh single-transiting planet candidate. All planets in the system are amenable to transmission spectroscopy, making TOI-1136 one of the best targets for intra-system comparison of
    Beard, Corey et al.

    Advertised on:

    2
    2024
    Bibcode
    2024AJ....167...70B
    Citations
    6