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/

  • Detections of solar-like oscillations in dwarfs and subgiants with Kepler DR25 short-cadence data
    During the survey phase of the Kepler mission, several thousand stars were observed in short cadence, allowing for the detection of solar-like oscillations in more than 500 main-sequence and subgiant stars. These detections showed the power of asteroseismology in determining fundamental stellar parameters. However, the Kepler Science Office
    Mathur, S. et al.

    Advertised on:

    1
    2022
    Citations
    25
  • Detection of the tidal deformation of WASP-103b at 3 σ with CHEOPS
    Context. Ultra-short period planets undergo strong tidal interactions with their host star which lead to planet deformation and orbital tidal decay. Aims: WASP-103b is the exoplanet with the highest expected deformation signature in its transit light curve and one of the shortest expected spiral-in times. Measuring the tidal deformation of the
    Barros, S. C. C. et al.

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    1
    2022
    Citations
    43
  • Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog
    We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the selection and photometric biases of the Dark Energy Survey (DES) Year 3 (Y3) data set. We systematically inject onto the single-epoch images of a random 20% subset of the DES footprint an ensemble of nearly 30 million realistic galaxy models derived
    Everett, S. et al.

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    1
    2022
    Citations
    70
  • Dark Energy Survey Year 3 results: galaxy-halo connection from galaxy-galaxy lensing
    Galaxy-galaxy lensing is a powerful probe of the connection between galaxies and their host dark matter haloes, which is important both for galaxy evolution and cosmology. We extend the measurement and modelling of the galaxy-galaxy lensing signal in the recent Dark Energy Survey Year 3 cosmology analysis to the highly non-linear scales (~100 kpc)
    Zacharegkas, G. et al.

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    1
    2022
    Citations
    36
  • Dark Energy Survey Year 3 results: galaxy sample for BAO measurement
    In this paper, we present and validate the galaxy sample used for the analysis of the baryon acoustic oscillation (BAO) signal in the Dark Energy Survey (DES) Y3 data. The definition is based on a colour and redshift-dependent magnitude cut optimized to select galaxies at redshifts higher than 0.5, while ensuring a high-quality determination. The
    Carnero Rosell, A. et al.

    Advertised on:

    1
    2022
    Citations
    19
  • Dark Energy Survey Year 3 results: galaxy sample for BAO measurement
    In this paper, we present and validate the galaxy sample used for the analysis of the baryon acoustic oscillation (BAO) signal in the Dark Energy Survey (DES) Y3 data. The definition is based on a colour and redshift-dependent magnitude cut optimized to select galaxies at redshifts higher than 0.5, while ensuring a high-quality determination. The
    Carnero Rosell, A. et al.

    Advertised on:

    1
    2022