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/

  • Spectrophotometric characterization of interstellar comet 2I/Borisov before perihelion passage
    Comets are primitive objects which formed in the outer parts of the proto-planetary disk, beyond the snow line. They can provide key information about the origins of our Solar System and its primordial nebula. The latest interstellar visitor [1], comet 2I/Borisov (initially designated C/2019 Q4), has given us the chance to have a probe from this
    Prodan, George P. et al.

    Advertised on:

    9
    2021
    Citations
    0
  • Spectroscopic study of Ceres' collisional family candidate members: taxonomic classification and comparison to Ceres' surface.
    Despite the observed signs of large impacts on the surface of Ceres, there is no confirmed collisional family associated with this dwarf planet. Carruba et al. (2016) carried out a dynamical study in the `pristine region' of the main asteroid belt and proposed a sample of 156 asteroids as candidates to be members of a Ceres' collisional family. Our
    Tinaut-Ruano, Fernando et al.

    Advertised on:

    9
    2021
    Citations
    0
  • The atmosphere of WASP-76b seen with CARMENES: looking for CaII IRT and HeI
    Currently, one of the most used techniques to study the atmosphere of the exoplanets is transmission spectroscopy by means of high-resolution facilities (R > 105). This methodology has led to the detection of several species in the atmosphere of exoplanets, showing that ultra-hot Jupiters (Teq > 2000 K) are one of the most intriguing exoplanets
    Casasayas-Barris, Núria et al.

    Advertised on:

    9
    2021
    Citations
    0
  • The EU Project NEOROCKS — NEO Rapid Observation, Characterization, and Key Simulations Project
    The knowledge of even some basic physical properties of a NEO such as the composition and the internal structure has strong implications for both science and impact mitigation. Depending on its composition and internal structure a meter-size object can completely burn in the atmosphere or reach the ground excavating an impact crater. To date, only
    Dotto, Elisabetta et al.

    Advertised on:

    9
    2021
    Citations
    2
  • The multi-chord stellar occultation by (19521) Chaos on 2020 November 20
    Physical properties of Trans-Neptunian Objects (TNOs) have been of increasing interest in the last two decades, as these objects are considered to be among the least altered through the Solar System evolution, and thus preserve valuable information about its origin [1]. The study of these objects through the ground-based method of stellar
    Vara-Lubiano, Mónica et al.

    Advertised on:

    9
    2021
    Citations
    0
  • Mapping magnetic activity indicators across the M dwarf domain
    Stellar activity poses one of the main obstacles for the detection and characterisation of exoplanets around cool stars, as it can induce radial velocity (RV) signals that can hide or mimic the presence of companions. Several activity indicators are routinely used to identify activity-related signals in RV measurements, but not all indicators trace
    Lafarga, Marina et al.

    Advertised on:

    10
    2021
    Citations
    0