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/

  • Search for a new scalar resonance decaying to a pair of Z bosons in proton-proton collisions at sqrt{s}=13 TeV
    A search for a new scalar resonance decaying to a pair of Z bosons is performed in the mass range from 130 GeV to 3 TeV, and for various width scenarios. The analysis is based on proton-proton collisions recorded by the CMS experiment at the LHC in 2016, corresponding to an integrated luminosity of 35.9 fb-1 at a center-of-mass energy of 13 TeV
    Sirunyan, A. M. et al.

    Advertised on:

    6
    2018
    Citations
    107
  • Search for a massive resonance decaying to a pair of Higgs bosons in the four b quark final state in proton-proton collisions at √{ s } = 13TeV
    A search for a massive resonance decaying into a pair of standard model Higgs bosons, in a final state consisting of two b quark-antiquark pairs, is performed. A data sample of proton-proton collisions at a centre-of-mass energy of 13 TeV is used, collected by the CMS experiment at the CERN LHC in 2016, and corresponding to an integrated luminosity
    Sirunyan, A. M. et al.

    Advertised on:

    6
    2018
    Citations
    27
  • Resolving the Nuclear Obscuring Disk in the Compton-thick Seyfert Galaxy NGC 5643 with ALMA
    We present ALMA Band 6 12CO(2–1) line and rest-frame 232 GHz continuum observations of the nearby Compton-thick Seyfert galaxy NGC 5643 with angular resolutions 0.″11–0.″26 (9–21 pc). The CO(2–1) integrated line map reveals emission from the nuclear and circumnuclear region with a two-arm nuclear spiral extending ∼10″ on each side. The
    Alonso-Herrero, A. et al.

    Advertised on:

    6
    2018
    Citations
    84
  • Resolving molecular gas to ~500 pc in a unique star forming disk galaxy at z~2
    We have resolved molecular gas in a 'typical' star forming disk galaxy at z>2 down to the scale of ~500 pc. Previous observations of CO and [CI] lines on larger spatial scales have revealed bulk molecular and atomic gas properties indicating that the target is a massive disk galaxy with large gas reserves. Unlike many galaxies studied at high
    Brisbin, Drew et al.

    Advertised on:

    6
    2018
    Citations
    0
  • Report on the Workshop "Dispersing Elements for Astronomy: New Trends and Possibilities"
    Astronomical spectrographs play an important role in addressing some of the biggest challenges in modern astronomy. One of the most critical components of any spectrograph is its dispersing element, since it determines the resolution and dispersion of the spectrograph, and is typically one of the least efficient optical components of the instrument
    Bianco, A. et al.

    Advertised on:

    6
    2018
    Citations
    0
  • Red, redder, reddest: SCUBA-2 imaging of colour-selected Herschel sources
    High-redshift, luminous, dusty star-forming galaxies (DSFGs) constrain the extremity of galaxy formation theories. The most extreme are discovered through follow-up on candidates in large area surveys. Here, we present extensive 850 μm SCUBA-2 follow-up observations of 188 red DSFG candidates from the Herschel Multitiered Extragalactic Survey
    Duivenvoorden, S. et al.

    Advertised on:

    6
    2018
    Citations
    24