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/

  • Measurements of the charm jet cross section and nuclear modification factor in pPb collisions at √{sNN} = 5.02 TeV
    The CMS Collaboration presents the first measurement of the differential cross section of jets from charm quarks produced in proton-lead (pPb) collisions at a nucleon-nucleon center-of-mass energy of √{sNN} = 5.02TeV, as well as results from charm quark jets in proton-proton (pp) collisions at √{ s} = 2.76 and 5.02TeV. By comparing the yields of
    Sirunyan, A. M. et al.

    Advertised on:

    9
    2017
    Citations
    22
  • Measurement of the t\overline{t} production cross section using events with one lepton and at least one jet in pp collisions at √{s}=13 TeV
    A measurement of the t\overline{t} production cross section at √{s}=13 TeV is presented using proton-proton collisions, corresponding to an integrated luminosity of 2.2 fb-1, collected with the CMS detector at the LHC. Final states with one isolated charged lepton (electron or muon) and at least one jet are selected and categorized according to the
    Sirunyan, A. M. et al.

    Advertised on:

    9
    2017
    Citations
    21
  • MASSIVE OBSCURE CLUSTERS IN THE MILKY WAY
    KLAUS SIMON RUBKE ZUÑIGA

    Advertised on:

    9
    2017
  • MAGIC gamma-ray telescopes hunting for neutrinos and their sources
    The discovery of an astrophysical flux of high-energy neutrinos by the IceCube Collaboration marks a major breakthrough in the ongoing search for the origin of cosmic rays. Presumably, the neutrinos, together with gamma rays, result from pion decay, following hadronic interactions of protons accelerated in astrophysical objects to ultra
    Góra, D. et al.

    Advertised on:

    9
    2017
    Citations
    1
  • LOCAL HELIOSYSMOLOGY IN THE TACHOCLINE AND THE DEEP PART OF THE CONVENTION. HELIOSISMOLOGÍA LOCAL EN LA TACOCLINA Y LA PARTE PROFUNDA DE LA ZONA DE CONVECCIÓN.
    La tacoclina solar situada en la base de la zona de convección es la capa de cizalladura que conecta la rotación diferencial en la envoltura convectiva y la rotación rígida en el interior radiativo. Generalmente se cree que alberga la localización de la dinamo solar y desempeña un importante papel en la generación y almacenamiento de los campos
    Manuel Díaz Alfaro

    Advertised on:

    9
    2017
  • Integral field spectroscopy of nearby quasi-stellar objects - II. Molecular gas content and conditions for star formation
    We present single-dish 12CO(1-0) and 12CO(2-1) observations for 14 low-redshift quasi-stellar objects (QSOs). In combination with optical integral field spectroscopy, we study how the cold gas content relates to the star formation rate (SFR) and black hole accretion rate. 12CO(1-0) is detected in 8 of 14 targets and 12CO(2-1) is detected in 7 out
    Urrutia, T. et al.

    Advertised on:

    9
    2017
    Citations
    45