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/

  • CaII triplet in Sextans dSph galaxy (Battaglia+, 2011)
    The spectroscopic observations were carried out at VLT/FLAMES between 2003 and 2004, with the exception of one pointing which was re-observed in 2008 May, during the commissioning of the upgraded Grating Instrument for Radiation Analysis with a Fiber-FedEchelle (GIRAFFE) spectrograph CCD. (1 data file).
    Battaglia, G. et al.

    Advertised on:

    10
    2011
    Citations
    0
  • CALIFA reveals prolate rotation in massive early-type galaxies: A polar galaxy merger origin?
    We present new evidence for eight early-type galaxies (ETGs) from the CALIFA Survey that show clear rotation around their major photometric axis ("prolate rotation"). These are LSBCF560-04, NGC 0647, NGC 0810, NGC 2484, NGC 4874, NGC 5216, NGC 6173, and NGC 6338. Including NGC 5485, a known case of an ETG with stellar prolate rotation, as well as
    Tsatsi, A. et al.

    Advertised on:

    10
    2017
    Citations
    31
  • CALIFA, the Calar Alto Legacy Integral Field Area survey. IV. Third public data release
    This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public, including the 200 galaxies of the second public data release (DR2). Data were obtained with the integral-field spectrograph PMAS/PPak mounted on the 3.5 m telescope at
    Sánchez, S. F. et al.

    Advertised on:

    10
    2016
    Citations
    217
  • Candidate Planetary Nebulae in M81 (Magrini+, 2001)
    File table1.dat contains the identification number, the coordinates (2000), the [OIII]5007 and the Hα+[NII] flux of the candidate PNe detected in Messier 81, using the Isaac Newton Telescope (INT) (La Palma, Spain) in 2000, December and 2001, January. The accuracy on position is approximately 0.5 arcsec. (1 data file).
    Magrini, L. et al.

    Advertised on:

    10
    2001
    Citations
    0
  • CAOS: a numerical simulation tool for astronomical adaptive optics (and beyond)
    We present recent developments of the CAOS "system", an IDL-based Problem Solving Environment (PSE) whose original aim was to define and simulate as realistically as possible the behavior of a generic adaptive optics (AO) system, from the atmospheric propagation of light, to the sensing of the wave-front aberratoins and the correction through a
    Carbillet, Marcel et al.

    Advertised on:

    10
    2004
    Citations
    22