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/

  • THE QUIJOTE EXPERIMENT: COMPONENT SEPARATION ANALYSES WITH MFI DATA AND TFGI COMMISSIONING RESULTS

    This thesis is dedicated to the study of the data from the first two instruments of the Q-U-I JOint Tenerife Experiment (QUIJOTE) experiment: the Multi Frequency Instrument (MFI) and the Thirty-and-Forty Gigahertz Instrument (TFGI). The MFI was installed at the Observatorio del Teide (OT) from 2012 to 2018, observing the sky between 10-20 GHz at

    Mateo Fernández Torreiro

    Advertised on:

    11
    2023
  • Confirmation of TiO absorption and tentative detection of MgH and CrH in the atmosphere of HAT-P-41b

    Understanding the role of optical absorbers is critical for linking the properties of the dayside and terminator atmospheres of hot Jupiters. This study aims to identify the signatures of optical absorbers in the atmosphere of the hot Jupiter HAT-P-41b. We conducted five transit observations of this planet to obtain its optical transmission spectra

    Jiang, C. et al.

    Advertised on:

    2
    2024
    Citations
    0
  • Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley

    Context. TOI-732 is an M dwarf hosting two transiting planets that are located on the two opposite sides of the radius valley. Inferring a reliable demographics for this type of systems is key to understanding their formation and evolution mechanisms. Aims: By doubling the number of available space-based observations and increasing the number of

    Bonfanti, A. et al.

    Advertised on:

    2
    2024
    Citations
    0
  • Constraining the reflective properties of WASP-178 b using CHEOPS photometry

    Context. Multiwavelength photometry of the secondary eclipses of extrasolar planets is able to disentangle the reflected and thermally emitted light radiated from the planetary dayside. Based on this, we can measure the planetary geometric albedo Ag, which is an indicator of the presence of clouds in the atmosphere, and the recirculation efficiency

    Pagano, I. et al.

    Advertised on:

    2
    2024
    Citations
    0
  • EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey

    Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions among stars. Aims: In this paper we present the Extended Westerlund 1 and 2 Open

    Guarcello, M. G. et al.

    Advertised on:

    2
    2024
    Citations
    0
  • Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?

    We present a comprehensive analysis of the Hubble Space Telescope observations of the atmosphere of WASP-121 b, an ultra-hot Jupiter. After reducing the transit, eclipse, and phase-curve observations with a uniform methodology and addressing the biases from instrument systematics, sophisticated atmospheric retrievals are used to extract robust

    Changeat, Q. et al.

    Advertised on:

    2
    2024
    Citations
    0