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
    The Magnetic Sensitivity of the Stokes I Profile of the 15260 Å Line of Mn I
    The near-IR line of Mn I at 15262.7 Å has recently been proposed as a new tool for diagnosing the magnetic field strength and magnetic energy density associated with unresolved magnetic structures, due to the enhanced sensitivity of the Stokes I profile. In this paper, the behavior of the line, focusing on the properties of the Stokes I profile, is
    Asensio Ramos, A.

    Advertised on:

    1
    2009
    Bibcode
    2009ApJ...690..416A
    Citations
    3
  • Non-refereed
    The Lowest Metallicity Stars from SDSS/SEGUE
    The first extension of the Sloan Digital Sky Survey (SDSS-II), which included the program SEGUE: Sloan Extension for Galactic Understanding and Exploration, ended in July, 2008. This effort has already produced the largest sample of medium-resolution stellar spectra yet obtained. These data are revolutionizing our understanding of the nature of the
    Beers, Timothy C. et al.

    Advertised on:

    1
    2009
    Bibcode
    2009AAS...21341612B
    Citations
    2
  • Refereed
    The June 2008 Flare of Markarian 421 from Optical to TeV Energies
    We present optical, X-ray, high-energy (lap30 GeV) and very high energy (gap100 GeV; VHE) observations of the high-frequency peaked blazar Mrk 421 taken between 2008 May 24 and June 23. A high-energy γ-ray signal was detected by AGILE with √{TS}=4.5 between June 9 and 15, with F(E>100 MeV) = 42+14 -12 × 10-8 photons cm-2 s-1. This flaring state is
    Donnarumma, I. et al.

    Advertised on:

    1
    2009
    Bibcode
    2009ApJ...691L..13D
    Citations
    113
  • Non-refereed
    The Hobby-Eberly Telescope Chemical Abundances of Stars in the Halo (CASH) Project
    The chemical evolution of the Galaxy and the early Universe is a key topic in modern astrophysics. The most metal-poor Galactic halo stars are now frequently used in an attempt to reconstruct the onset of the chemical and dynamical formation processes of the Galaxy. These stars are an easily-accessible local equivalent of the high-redshift Universe
    Shetrone, Matthew D. et al.

    Advertised on:

    1
    2009
    Bibcode
    2009AAS...21340811S
    Citations
    0