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/

  • Principal-component analysis of two-particle azimuthal correlations in PbPb and p Pb collisions at CMS
    For the first time a principle-component analysis is used to separate out different orthogonal modes of the two-particle correlation matrix from heavy ion collisions. The analysis uses data from √{sNN}=2.76 TeV PbPb and √{sNN}=5.02 TeV p Pb collisions collected by the CMS experiment at the CERN Large Hadron Collider. Two-particle azimuthal
    Sirunyan, A. M. et al.

    Advertised on:

    12
    2017
    Citations
    27
  • Precise Masses in the WASP-47 System
    We present precise radial velocity observations of WASP-47, a star known to host a hot Jupiter, a distant Jovian companion, and, uniquely, two additional transiting planets in short-period orbits: a super-Earth in a ≈19 hr orbit, and a Neptune in a ≈9 day orbit. We analyze our observations from the HARPS-N spectrograph along with previously
    Vanderburg, A. et al.

    Advertised on:

    12
    2017
    Citations
    57
  • Photospheric activity of the Sun with VIRGO and GOLF. Comparison with standard activity proxies
    We study the variability of solar activity using new photospheric proxies originally developed for the analysis of stellar magnetism with the CoRoT and Kepler photometric observations. These proxies were obtained by tracking the temporal modulations in the observations associated with the spots and magnetic features as the Sun rotates. We analyzed
    Salabert, D. et al.

    Advertised on:

    12
    2017
    Citations
    38
  • Photoionization instability of the Fe K absorbing plasma in the neutron star transient AX J1745.6-2901
    AX J1745.6-2901 is a low-mass X-ray binary with an accreting neutron star, showing clear evidence for highly ionized absorption. Strong ionized Fe Kα and Kβ absorption lines are always observed during the soft state, whereas they disappear during the hard state. We computed photoionization stability curves for the hard and the soft states, under
    Bianchi, S. et al.

    Advertised on:

    12
    2017
    Citations
    24
  • Optical Spectroscopic Survey of a Sample of Unidentified Fermi Objects
    We present optical spectroscopy secured at the 10 m Gran Telescopio Canarias of the counterparts of 20 extragalactic γ-ray sources detected by the Fermi satellite. The observations allow us to investigate the nature of these sources and to determine their redshift. We find that all optical counterparts have a spectrum that is consistent with a BL
    Paiano, S. et al.

    Advertised on:

    12
    2017
    Citations
    40
  • Observations of the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope
    We observed the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope to provide new constraints on its spectral properties at high frequency. We conducted observations in three frequency bands centred at 1.4, 6.6 and 19 GHz, resulting in beam resolutions of 14, 2.9 and 1 arcmin, respectively. These single-dish data were also combined
    Loi, F. et al.

    Advertised on:

    12
    2017
    Citations
    30