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/

  • The PSU/TCfA Search for Planets Around Evolved Stars: V sin i Measurements for Slow Rotating F-K Giants
    We present results of our projected rotational velocities (V sin i) measurements of F, G and K giants obtained from the cross-correlation function (CCF) constructed from high signal to noise spectra. We also present the calibration of the HET/HRS cross-correlation function to determine accurate projected rotational velocities V sin i for slowly
    Nowak, G. et al.

    Advertised on:

    2008
    Citations
    1
  • The PSU/TCfA Search for Planets Around Evolved Stars: Bisector Analysis of Activity of a Sample of Red Giants.
    Searches for planets around evolved G-K subgiant and giant stars are essential for developing general understanding of planet formation and evolution of the planetary systems. Precise radial velocity (RV) measurements of giants have lead to the discovery of ten planets around such star. However, the long period radial velocity variations of red
    Nowak, G. et al.

    Advertised on:

    2008
    Citations
    1
  • The Magellanic Clouds as a Template for the Study of Stellar Populations and Galaxy Interactions
    The Magellanic System represents one of the best places to study the formation and evolution of galaxies. Photometric surveys of various depths, areas and wavelengths have had a significant impact on our understanding of the system; however, a complete picture is still lacking. VMC (the VISTA near-infrared YJKs survey of the Magellanic System) will
    Cioni, M.-R. L. et al.

    Advertised on:

    2008
    Citations
    14
  • Gemini 3D-Spectroscopy of IRAS 17002+5153 and IRAS 07598+6508: Evidence of Two New Exploding BAL + IR + Fe ii QSOs.
    New results of a program to study BAL + IR + FeII QSOs, using Gemini/GMOS-IFU spectroscopy and HST data, are presented for IRAS 17002+5153 and IRAS 07598+6508. In particular, the Gemini GMOS-IFU data show that: (i) IRAS 17002+5153: the 3D spectra in the region of the shells (at radius of 1.3") show multiple emission line components (with Δ V~280-
    Lípari, S. et al.

    Advertised on:

    2008
    Citations
    1