Asosiy kontentga oʻtish
AkademIndex

Xizmatlar

J. Agramunt

17 ta ish

University of Valencia

AkademScholarda batafsil koʻrsatkichlar

  1. The WEBT BL Lacertae Campaign 2001 and its extension Optical light curves and colour analysis 1994-2002

    M. Villata, C. M. Raiteri, O. M. Kurtanidze +65

    MaqolaAstrophysics and Cosmic PhenomenaRepository of Digital Objects for Teaching Research and Culture (University of Valencia)200416 iqtibos
    ABI

  2. The awakening of BL Lacertae: observations by Fermi, Swift and the GASP-WEBT★

    C. M. Raiteri, M. Villata, F. D’Ammando +75

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaMonthly Notices of the Royal Astronomical Society201312 iqtibos
    ABI

  3. Another look at the BL Lacertae flux and spectral variability. Observations by GASP-WEBT, XMM-Newton, and Swift in 2008-2009

    C. M. Raiteri, M. Villata, L. Bruschini +68

    Maqola201012 iqtibos
    ABI

  4. Multifrequency monitoring of the blazar 0716+714 during the GASP-WEBT-AGILE campaign of 2007

    M. Villata, C. M. Raiteri, V. M. Larionov +49

    MaqolaOchiq kirish200810 iqtibos
    ABI

  5. The correlated optical and radio variability of BL Lacertae

    M. Villata, C. M. Raiteri, V. M. Larionov +52

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaAstronomy and Astrophysics20099 iqtibos
    ABI

  6. The GASP-WEBT monitoring of 3C 454.3 during the 2008 optical-to-radio and γ-ray outburst

    M. Villata, C. M. Raiteri, Mark Gurwell +57

    MaqolaOchiq kirish20099 iqtibos
    ABI

  7. Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies

    C. M. Raiteri, M. Villata, Paul S. Smith +74

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaAstronomy and Astrophysics20129 iqtibos
    ABI

  8. WEBT multiwavelength monitoring and XMM-Newton observations of 
BL Lacertae in 2007–2008

    C. M. Raiteri, M. Villata, A. Capetti +66

    MaqolaOchiq kirish20099 iqtibos
    ABI

  9. Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006–2007

    V. M. Larionov, S. G. Jorstad, Alan P. Marscher +68

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaAstronomy and Astrophysics20088 iqtibos
    ABI

  10. The long-lasting activity of 3C 454.3

    C. M. Raiteri, M. Villata, M. F. Aller +69

    MaqolaOchiq kirish20118 iqtibos
    ABI

  11. WEBT and XMM-Newton observations of 3C 454.3 during the post-outburst phase. Detection of the little and big blue bumps

    C. M. Raiteri, M. Villata, V. M. Larionov +74

    PreprintOchiq kirishAstrophysics and Cosmic PhenomenaarXiv (Cornell University)20074 iqtibos
    ABI

  12. A new activity phase of the blazar 3C 454.3

    C. M. Raiteri, M. Villata, V. M. Larionov +72

    MaqolaOchiq kirish20083 iqtibos
    ABI

  13. Multi-frequency monitoring of gamma-ray loud blazars: I. Light curves and spectral energy distributions

    U. Bach, C. M. Raiteri, M. Villata +23

    Preprint20063 iqtibos
    ABI

  14. Multi-frequency monitoring of γ-ray loud blazars

    U. Bach, C. M. Raiteri, M. Villata +23

    MaqolaOchiq kirishAstrophysics and Cosmic PhenomenaAstronomy and Astrophysics20063 iqtibos
    ABI

  15. Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006–2007 outburst

    C. M. Raiteri, M. Villata, V. M. Larionov +58

    MaqolaOchiq kirish20082 iqtibos
    ABI

  16. beta-DELAYED gamma-RAY SPECTROSCOPY OF HEAVY NEUTRON RICH NUCLEI "SOUTH" OF LEAD

    A. I. Morales, J. Benlliure, P. H. Regan +45

    MaqolaNuclear Physics and ApplicationsSurrey Research Insight Open Access (The University of Surrey)20090 iqtibos
    ABI

  17. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>−</mml:mo><mml:mn>1</mml:mn><mml:mo>→</mml:mo><mml:mn>0</mml:mn></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>β</mml:mi></mml:math>decays of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Ni</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>54</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">Fe</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>50</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">Cr</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>46</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>, and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Ti</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>42</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>and comparison with mirror<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mo>(</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:math>measurements

    F. Molina, B. Rubio, Y. Fujita +39

    MaqolaOchiq kirishNuclear physics research studiesPhysical Review C20150 iqtibos
    ABI