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/

  • Non-refereed
    Monitoring Black Hole X-Ray Transients in M31 with Chandra and HST
    Our neighbouring galaxy M31 (Andromeda), located 780 kpc away, offers a unique opportunity to study the X-ray population of a galaxy similar to the Milky Way. We have concentrated our monitoring campaign on following the X-ray activity of the stellar-mass black hole candidates, XRNe (X-Ray Novae), in the central region of M31. Observations are made
    Galache, Jose et al.

    Advertised on:

    3
    2008
    Bibcode
    2008HEAD...10.0104G
    Citations
    0
  • Non-refereed
    Massive galaxies in Extended Groth Strip (Trujillo+, 2007)
    We use the Palomar Observatory Wide-field Infrared (POWIR)/DEEP-2 survey (Davis et al., 2003, SPIE, Vol. 4834, p. 161; Bundy et al., 2006ApJ...651..120B ; Conselice et al., 2007ApJ...660L..55C, 2007MNRAS.381..962C) to define a sample of 831 galaxies with masses larger than 1011h70-2M{sun} located over ~710arcmin2 in the Extended Groth Strip (EGS)
    Trujillo, I. et al.

    Advertised on:

    3
    2008
    Bibcode
    2008yCat..73820109T
    Citations
    0
  • Non-refereed
    Massive galaxies in Extended Groth Strip (Trujillo+, 2007)
    We use the Palomar Observatory Wide-field Infrared (POWIR)/DEEP-2 survey (Davis et al., 2003, SPIE, Vol. 4834, p. 161; Bundy et al., 2006ApJ...651..120B ; Conselice et al., 2007ApJ...660L..55C, 2007MNRAS.381..962C) to define a sample of 831 galaxies with masses larger than 1011h70-2M{sun} located over ~710arcmin2 in the Extended Groth Strip (EGS)
    Trujillo, I. et al.

    Advertised on:

    3
    2008
    Bibcode
    2008yCat..83820109T
    Citations
    0
  • Refereed
    MAGIC Observations of the Unidentified γ-Ray Source TeV J2032+4130
    We observed the first known very high energy (VHE) γ-ray-emitting unidentified source, TeV J2032+4130, for 94 hr with the MAGIC telescope. The source was detected with a significance of 5.6 σ. The flux, position, and angular extension are compatible with the previous ones measured by the HEGRA telescope system 5 years ago. The integral flux amounts
    Albert, J. et al.

    Advertised on:

    3
    2008
    Bibcode
    2008ApJ...675L..25A
    Citations
    89