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/

  • ESPRESSO observations of HE 0107−5240 and other CEMP-no stars with [Fe/H] ≤ -4.5
    Context. HE 0107−5240 is a hyper metal-poor star with [Fe/H] = −5.39, one of the lowest-metallicity stars known. Its stellar atmosphere is enhanced in carbon, with [C/Fe] = +4.0, without a detectable presence of neutron-capture elements. Therefore, it belongs to the carbon-enhanced metal-poor (CEMP−no) group, along with the majority of the most
    Aguado, D. S. et al.

    Advertised on:

    12
    2022
    Citations
    13
  • Fastcc: Fast Color Corrections for Broadband Radio Telescope Data
    Broadband receiver data need color corrections applying to correct for the different source spectra across their wide bandwidths. The full integration over a receiver bandpass may be computationally expensive and redundant when repeated many times. Color corrections can be applied, however, using a simple quadratic fit based on the full integration
    Peel, Mike W. et al.

    Advertised on:

    12
    2022
    Citations
    7
  • Fossil group origins. XII. The large-scale environment around fossil systems
    Aims: We analyse the large-scale structure out to 100 Mpc around a sample of 16 confirmed fossil systems using spectroscopic information from the Sloan Digital Sky Survey Data Release 16. Methods: We computed the distance between our fossil groups (FGs) and the centres of filaments and nodes from the literature. We also studied the density of
    Zarattini, S. et al.

    Advertised on:

    12
    2022
    Citations
    2
  • Gamma-ray observations of MAXI J1820+070 during the 2018 outburst
    MAXI J1820+070 is a low-mass X-ray binary with a black hole (BH) as a compact object. This binary underwent an exceptionally bright X-ray outburst from 2018 March to October, showing evidence of a non-thermal particle population through its radio emission during this whole period. The combined results of 59.5 h of observations of the MAXI J1820+070
    Abe, H. et al.

    Advertised on:

    12
    2022
    Citations
    4
  • Hubble tensions: a historical statistical analysis
    Statistical analyses of measurements of the Hubble-Lemaître constant H 0 (163 measurements between 1976 and 2019) show that the statistical error bars associated with the observed parameter measurements have been underestimated - or the systematic errors were not properly taken into account - in at least 15-20 per cent of the measurements. The fact
    López-Corredoira, Martín

    Advertised on:

    12
    2022
    Citations
    7
  • J-PLUS: Uncovering a large population of extreme [OIII] emitters in the local Universe
    Context. Over the past decades, several studies have discovered a population of galaxies that undergo very strong star formation events. They are called extreme emission line galaxies (EELGs). Aims: We exploit the capabilities of the Javalambre Photometric Local Universe Survey (J-PLUS), a wide-field multifilter survey, with which 2000 square
    Lumbreras-Calle, A. et al.

    Advertised on:

    12
    2022
    Citations
    13