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
    Submillimetre compactness as a critical dimension to understand the main sequence of star-forming galaxies
    We study the interstellar medium (ISM) properties as a function of the molecular gas size for 77 infrared-selected galaxies at z ~ 1.3, having stellar masses 10 9.4 ≲ M ⋆ ≲ 10 12.0 M ⊙ and star formation rates 12 ≲ SFR FIR ≲ 1000 M ⊙ yr -1. Molecular gas sizes are measured on ALMA images that combine CO(2-1), CO(5-4), and underlying continuum
    Puglisi, Annagrazia et al.

    Advertised on:

    12
    2021
    Bibcode
    2021MNRAS.508.5217P
    Citations
    40
  • Refereed
    Search for Very High-energy Emission from the Millisecond Pulsar PSR J0218+4232
    PSR J0218+4232 is one of the most energetic millisecond pulsars known and has long been considered as one of the best candidates for very high-energy (VHE; >100 GeV) γ-ray emission. Using 11.5 yr of Fermi Large Area Telescope (LAT) data between 100 MeV and 870 GeV, and ~90 hr of Major Atmospheric Gamma Imaging Cherenkov (MAGIC) observations in the
    Acciari, V. A. et al.

    Advertised on:

    12
    2021
    Bibcode
    2021ApJ...922..251A
    Citations
    3
  • Refereed
    Revisiting the Distance to Radio Loops I and IV Using Gaia and Radio/Optical Polarization Data
    Galactic synchrotron emission exhibits large angular scale features known as radio spurs and loops. Determining the physical size of these structures is important for understanding the local interstellar structure and for modeling the Galactic magnetic field. However, the distance to these structures is either under debate or entirely unknown. We
    Panopoulou, G. V. et al.

    Advertised on:

    12
    2021
    Bibcode
    2021ApJ...922..210P
    Citations
    35
  • Refereed
    Rapid contraction of giant planets orbiting the 20-million-year-old star V1298 Tau
    Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years 1,2. These theoretical expectations remain untested so far as the detection and characterization of very young planets is extremely

    Advertised on:

    12
    2021
    Bibcode
    2021NatAs.tmp..252S
  • Refereed
    Rapid contraction of giant planets orbiting the 20-million-year-old star V1298 Tau
    Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years 1,2. These theoretical expectations remain untested so far as the detection and characterization of very young planets is extremely

    Advertised on:

    12
    2021
    Bibcode
    2021NatAs.tmp..234S
  • Refereed
    Probing the atmosphere of WASP-69 b with low- and high-resolution transmission spectroscopy
    Consideration of both low- and high-resolution transmission spectroscopy is key for obtaining a comprehensive picture of exoplanet atmospheres. In studies of transmission spectra, the continuum information is well established with low-resolution spectra, while the shapes of individual lines are best constrained with high-resolution observations. In
    Khalafinejad, S. et al.

    Advertised on:

    12
    2021
    Bibcode
    2021A&A...656A.142K
    Citations
    24