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/

  • Chemodynamics of the Milky Way. I. The first year of APOGEE data
    Context. The Apache Point Observatory Galactic Evolution Experiment (APOGEE) features the first multi-object high-resolution fiber spectrograph in the near-infrared ever built, thus making the survey unique in its capabilities: APOGEE is able to peer through the dust that obscures stars in the Galactic disc and bulge in the optical wavelength range
    Anders, F. et al.

    Advertised on:

    4
    2014
    Citations
    207
  • Characterizing unknown systematics in large scale structure surveys
    Photometric large scale structure (LSS) surveys probe the largest volumes in the Universe, but are inevitably limited by systematic uncertainties. Imperfect photometric calibration leads to biases in our measurements of the density fields of LSS tracers such as galaxies and quasars, and as a result in cosmological parameter estimation. Earlier
    Agarwal, N. et al.

    Advertised on:

    4
    2014
    Citations
    21
  • C/O and N/O ratios in planetary nebulae with [WC] central stars
    Planetary nebulae (PNe) around [WR] central stars (WRPNe) constitute a particular photoionized nebula class, representing about 10-15% of the PNe with known progenitor. We have studied 14 of them, detecting a large number of optical recombination lines (ORLs) from different ions of O and C (O+, O++, C++, C+3). This allows us to determine the C/O
    García-Rojas, J. et al.

    Advertised on:

    4
    2014
    Citations
    0
  • Broad iron emission line and kilohertz quasi-periodic oscillations in the neutron star system 4U 1636-53
    Both the broad iron (Fe) line and the frequency of the kilohertz quasi-periodic oscillations (kHz QPOs) in neutron star low-mass X-ray binaries (LMXBs) can potentially provide independent measures of the inner radius of the accretion disc. We use XMM-Newton and simultaneous Rossi X-ray Timing Explorer observations of the LMXB 4U 1636-53 to test
    Sanna, A. et al.

    Advertised on:

    4
    2014
    Citations
    12
  • 3D Models of Stellar Interactions
    Symbiotic binaries consist of a cool, evolved mass-losing giant and an accreting compact companion. As symbiotic nebulae show similar morphologies to those in planetary nebulae (so much so that it is often difficult to distinguish between the two), they are ideal laboratories for understanding the role a binary companion plays in shaping the
    Mohamed, S. et al.

    Advertised on:

    4
    2014
    Citations
    0
  • X-Shooter Spectral Library (XSL). DR1 (Chen+, 2014)
    We present the first release of XSL, the X-Shooter Spectral Library observed at the European Southern Observatory (ESO). This release contains 237 stars spanning the wavelengths 3000-10200Å observed at a resolving power R~10000. Telluric standard stars used to correct the Earth atmospheric contamination are presented as well. (2 data files).
    Chen, Y.-P. et al.

    Advertised on:

    3
    2014
    Citations
    0