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
    Search for new physics with the M T2 variable in all-jets final states produced in pp collisions at √{s}=13 TeV
    A search for new physics is performed using events that contain one or more jets, no isolated leptons, and a large transverse momentum imbalance, as measured through the M T2 variable, which is an extension of the transverse mass in events with two invisible particles. The results are based on a sample of proton-proton collisions collected at a
    Khachatryan, V. et al.

    Advertised on:

    10
    2016
    Bibcode
    2016JHEP...10..006K
    Citations
    20
  • Refereed
    Precise radial velocities of giant stars. IX. HD 59686 Ab: a massive circumstellar planet orbiting a giant star in a 13.6 au eccentric binary system
    Context. For over 12 yr, we have carried out a precise radial velocity (RV) survey of a sample of 373 G- and K-giant stars using the Hamilton Échelle Spectrograph at the Lick Observatory. There are, among others, a number of multiple planetary systems in our sample as well as several planetary candidates in stellar binaries. Aims: We aim at
    Ortiz, M. et al.

    Advertised on:

    10
    2016
    Bibcode
    2016A&A...595A..55O
    Citations
    24
  • Refereed
    Phenomenological MSSM interpretation of CMS searches in pp collisions at √{s}=7 and 8 TeV
    Searches for new physics by the CMS collaboration are interpreted in the framework of the phenomenological minimal supersymmetric standard model (pMSSM). The data samples used in this study were collected at √{s}=7 and 8 TeV and have integrated luminosities of 5.0 fb-1 and 19.5 fb-1, respectively. A global Bayesian analysis is performed
    Khachatryan, V. et al.

    Advertised on:

    10
    2016
    Bibcode
    2016JHEP...10..129K
    Citations
    19
  • Non-refereed
    OSIRIS Multi-Object Spectroscopy: Mask Design Process
    The OSIRIS (Optical System for Imaging and Low-Intermediate Resolution Integrated Spectroscopy) instrument at the 10.4 m GTC has offered a multi-object spectroscopic mode since March 2014. In this paper we describe the detailed process of designing a MOS mask for OSIRIS by using the Mask Designer Tool, and give some numbers on the accuracy of the
    Gómez-Velarde, G. et al.

    Advertised on:

    10
    2016
    Bibcode
    2016ASPC..507..191G
    Citations
    4
  • Refereed
    On the estimation of stellar parameters with uncertainty prediction from Generative Artificial Neural Networks: application to Gaia RVS simulated spectra
    Aims: We present an innovative artificial neural network (ANN) architecture, called Generative ANN (GANN), that computes the forward model, that is it learns the function that relates the unknown outputs (stellar atmospheric parameters, in this case) to the given inputs (spectra). Such a model can be integrated in a Bayesian framework to estimate
    Dafonte, C. et al.

    Advertised on:

    10
    2016
    Bibcode
    2016A&A...594A..68D
    Citations
    20
  • Non-refereed
    Non-Vestoid candidates in the inner Main Belt
    Most Howardite-Eucrite-Diogenite (HED) meteorites (analogues to V-type asteroids) are thought to originate from asteroid (4) Vesta. However some HEDs show distinct oxygen isotope ratios and therefore are thought to originate from other asteroids. In this study we try to identify asteroids that may represent parent bodies of those mismatching HEDs
    Moskovitz, Nicholas et al.

    Advertised on:

    10
    2016
    Bibcode
    2016DPS....4832705M
    Citations
    0