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
    TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet
    The Transiting Exoplanet Survey Satellite mission was designed to find transiting planets around bright, nearby stars. Here, we present the detection and mass measurement of a small, short-period (≍4 days) transiting planet around the bright (V = 7.9), solar-type star HD 86226 (TOI-652, TIC 22221375), previously known to host a long-period (∼1600
    Teske, Johanna et al.

    Advertised on:

    8
    2020
    Bibcode
    2020AJ....160...96T
    Citations
    31
  • Refereed
    Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra
    We have modelled the stellar and nebular continua and emission-line intensity ratios of massive stellar populations in the Antennae galaxy using high resolution and self-consistent libraries of model H II regions around central clusters of ageing stars. The model libraries are constructed using the stellar population synthesis code, STARBURST99
    Gunawardhana, M. L. P. et al.

    Advertised on:

    8
    2020
    Bibcode
    2020MNRAS.497.3860G
    Citations
    18
  • Refereed
    Soft X-ray emission lines in the X-ray binary Swift J1858.6-0814 observed with XMM-Newton Reflection Grating Spectrometer: disc atmosphere or wind?
    We find soft X-ray emission lines from the X-ray binary Swift J1858.6-0814 in data from XMM-NewtonReflection Grating Spectrometer (RGS): N VII, O VII, and O VIII, as well as notable residuals short of a detection at Ne IX and other higher ionization transitions. These could be associated with the disc atmosphere, as in accretion disc corona sources
    Buisson, D. J. K. et al.

    Advertised on:

    8
    2020
    Bibcode
    2020MNRAS.498...68B
    Citations
    9
  • Refereed
    SMASHing the low surface brightness SMC
    The periphery of the Small Magellanic Cloud (SMC) can unlock important information regarding galaxy formation and evolution in interacting systems. Here, we present a detailed study of the extended stellar structure of the SMC using deep colour-magnitude diagrams, obtained as part of the Survey of the MAgellanic Stellar History (SMASH). Special
    Massana, Pol et al.

    Advertised on:

    8
    2020
    Bibcode
    2020MNRAS.498.1034M
    Citations
    30
  • Refereed
    Simulations Predicting the Ability of Multi-color Simultaneous Photometry to Distinguish TESS Candidate Exoplanets from False Positives
    The Transiting Exoplanet Survey Satellite (TESS) is currently concluding its 2 yr primary science mission searching 85% of the sky for transiting exoplanets. TESS has already discovered well over one thousand TESS objects of interest (TOIs), but these candidate exoplanets must be distinguished from astrophysical false positives using other
    Louie, Dana R. et al.

    Advertised on:

    8
    2020
    Bibcode
    2020PASP..132h4403L
    Citations
    1
  • Refereed
    Search for the sub-stellar lithium depletion boundary in the open star cluster Coma Berenices
    Aims: We mainly aim to search for the lithium depletion boundary (LDB) among the sub-stellar population of the open star cluster Coma Berenices. Methods: Since the number of brown dwarf candidates in Coma Ber available in the literature is scarce, we carried out a search for additional candidates photometrically using colour-magnitude diagrams
    Martín, E. L. et al.

    Advertised on:

    8
    2020
    Bibcode
    2020A&A...640A...9M
    Citations
    7