Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Kilonova Seekers: the GOTO project for real-time citizen science in time-domain astrophysics
    Time-domain astrophysics continues to grow rapidly, with the inception of new surveys drastically increasing data volumes. Democratized, distributed approaches to training sets for machine learning classifiers are crucial to make the most of this torrent of discovery - with citizen science approaches proving effective at meeting these requirements
    Killestein, T. L. et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0
  • OGLE-2015-BLG-0845L: a low-mass M dwarf from the microlensing parallax and xallarap effects
    We present the analysis of the microlensing event OGLE-2015-BLG-0845, which was affected by both the microlensing parallax and xallarap effects. The former was detected via the simultaneous observations from the ground and Spitzer, and the latter was caused by the orbital motion of the source star in a relatively close binary. The combination of
    Hu, Zhecheng et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0
  • The Complex Star Formation History of the Halo of NGC 5128 (Cen A)
    NGC 5128 (Cen A) is the nearest giant elliptical galaxy and one of the brightest extragalactic radio sources in the sky, boasting a prominent dust lane and jets emanating from its nuclear supermassive black hole. In this paper, we construct the star formation history (SFH) of two small fields in the halo of NGC 5128: a northeastern field (Field 1)
    Aghdam, Sima T. et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0
  • The Dark Energy Survey 5-yr photometrically classified type Ia supernovae without host-galaxy redshifts
    Current and future Type Ia Supernova (SN Ia) surveys will need to adopt new approaches to classifying SNe and obtaining their redshifts without spectra if they wish to reach their full potential. We present here a novel approach that uses only photometry to identify SNe Ia in the 5-yr Dark Energy Survey (DES) data set using the SUPERNNOVA
    Möller, A. et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0
  • The dark energy survey supernova program: investigating beyond-ΛCDM
    We report constraints on a variety of non-standard cosmological models using the full 5-yr photometrically classified type Ia supernova sample from the Dark Energy Survey (DES-SN5YR). Both Akaike Information Criterion (AIC) and Suspiciousness calculations find no strong evidence for or against any of the non-standard models we explore. When
    Camilleri, R. et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0
  • The frequency of transiting planetary systems around polluted white dwarfs
    This paper investigates the frequency of transiting planetary systems around metal-polluted white dwarfs using high-cadence photometry from ULTRACAM and ULTRASPEC on the ground and space-based observations with TESS. Within a sample of 313 metal-polluted white dwarfs with available TESS light curves, two systems known to have irregular transits are
    Robert, Akshay et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0