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/

  • WISE Observations of Primitive Asteroid Families
    NASA's Wide-field Survey Explorer (WISE) mapped the sky in four bands at 3.4, 4.6, 12, and 22 μm during its mission. Published on 14 April 2011, the WISE Preliminary Release provides data of more than 150,000 asteroids that were processed with initial calibration and reduction algorithms. Our aim is to carry out an analysis of key physical
    Ziffer, Julie et al.

    Advertised on:

    5
    2011
    Citations
    0
  • UV-to-FIR analysis of sources in the EGS. II. (Barro+, 2011)
    The present work is based on the multi-wavelength catalog of IRAC 3.6+4.5um selected galaxies in the EGS (RA=14h14m, DEC=+53°30') presented in Paper I (Barro et al. 2011, Cat. J/ApJS/193/13). We cross-correlated our IRAC-selected catalog with the X-ray (Chandra) and radio (VLA/20cm) catalogs of Laird et al. (2009, Cat. J/ApJS/180/102) and Ivison et
    Barro, G. et al.

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    5
    2011
    Citations
    0
  • Three MASTER OT's discovery
    The MASTER auto-detection system at Tunka (Baykal Lake) detected a new transient source at the position (R.A., Dec) = 17h 29m 00.07s , +75d 18m 42s.5, (J2000) with a typical uncertainty of 0.5" at 2011-05-12 18:24:47.725 (UT). The OT is seen at 2 images. There is no minor planet and any object brighter 21 mag in DSS at this place. The unfiltered (0
    Balanutsa, P. et al.

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    5
    2011
    Citations
    1
  • The Swift/Fermi GRB 080928 from 1 eV to 150 keV
    We present the results of a comprehensive study of the gamma-ray burst 080928 and of its afterglow. GRB 080928 was a long burst detected by Swift/BAT and Fermi/GBM. It is one of the exceptional cases where optical emission had already been detected when the GRB itself was still radiating in the gamma-ray band. For nearly 100 s simultaneous optical
    Rossi, A. et al.

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    5
    2011
    Citations
    55
  • The supergiant optical counterpart of ULX P13 in NGC 7793
    We have identified the optical counterpart of the ULX source P13 in the nearby spiral galaxy NGC 7793. The object is a V ˜ 20.5 mag star, ten times brighter than any other established counterpart of a ULX in nearby galaxies. Medium resolution optical spectroscopy carried out in 2008 and 2009 with the ESO-VLT reveals the presence of narrow high
    Motch, C. et al.

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    5
    2011
    Citations
    53
  • The Solar Rotation and its Evolution During Cycle 23
    We present the most exhaustive and accurate inferences of the internal solar rotation rate and its evolution during solar cycle 23. A full solar cycle of MDI observations have been analyzed using our state of the art fitting methodology. Time series of various lengths have been fitted, from a single 4608-day long epoch (64 times 72 day or 12.6 yr)
    Korzennik, Sylvain G. et al.

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    5
    2011
    Citations
    0