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/

  • Erratum
    Erratum: Erratum to: Measurements of the Z → 4 ℓ branching fraction, and constraints on anomalous triple gauge couplings at √{s} = 13 TeV
    Reference [6]: "Phys. Lett. B 763, 280" should have been corrected into "Phys. Lett. B 763, 280 (2016)".
    Sirunyan, A. M. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018EPJC...78..515S
    Citations
    9
  • Refereed
    Enhancing SDO/HMI images using deep learning
    Context. The Helioseismic and Magnetic Imager (HMI) provides continuum images and magnetograms with a cadence better than one per minute. It has been continuously observing the Sun 24 h a day for the past 7 yr. The trade-off between full disk observations and spatial resolution means that HMI is not adequate for analyzing the smallest-scale events
    Díaz Baso, C. J. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018A&A...614A...5D
    Citations
    53
  • Refereed
    Enhancing SDO/HMI images using deep learning
    Context. The Helioseismic and Magnetic Imager (HMI) provides continuum images and magnetograms with a cadence better than one per minute. It has been continuously observing the Sun 24 h a day for the past 7 yr. The trade-off between full disk observations and spatial resolution means that HMI is not adequate for analyzing the smallest-scale events
    Díaz Baso, C. J. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018A&A...614A...5B
  • Refereed
    Deep spectroscopy of nearby galaxy clusters - IV. The quench of the star formation in galaxies in the infall region of Abell 85
    Our aim is to understand the role of the environment in the quenching of star formation of galaxies located in the infall cluster region of Abell 85 (A85). This is achieved by studying the post-starburst galaxy population as tracer of recent quenching. By measuring the equivalent width (EW) of the [O II] and Hδ spectral lines, we classify the
    Aguerri, J. A. L. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018MNRAS.477.1921A
    Citations
    6
  • Refereed
    Circumnuclear Star Formation and AGN Activity: Clues from Surface Brightness Radial Profile of PAHs and [{\rm{S}}\,{\rm{IV}}]
    We studied the circumnuclear mid-IR emission in a sample of 19 local active galactic nuclei (AGNs) with high spatial resolution spectra using T-ReCS (Gemini) and CanariCam (GTC), together with Spitzer/IRS observations. We measured the flux and the equivalent width for the 11.3 μm PAH feature and the [S IV] line emission as a function of
    Esparza-Arredondo, D. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018ApJ...859..124E
    Citations
    27
  • Refereed
    Chemical Composition of Two Bright, Extremely Metal-poor Stars from the SDSS MARVELS Pre-survey
    SDSS J082625.70+612515.10 (V = 11.4 [Fe/H] = ‑3.1) and SDSS J134144.60+474128.90 (V = 12.4 [Fe/H] = ‑3.2) were observed with the SDSS 2.5m telescope as part of the SDSS MARVELS spectroscopic pre-survey and identified as extremely metal-poor (EMP; [Fe/H]
    Bandyopadhyay, A. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018ApJ...859..114B
    Citations
    14