logo operations portal
    Home
  • Broadcast
  • Downtimes
  • VO Management
  • VO List
  • Dashboard
  • Metrics
  • Sla
  • API
  • SiteMap
  • Contact Us
  • logo argo  ARGO
  • logo vapor
  • VO List
  • User tracking
  • Security
  • Validity
  • Login

VO Id Card : blazarmonitoring.asi.it   Update

  • 1 General Information
  • 2 Aknowledgement statement
  • 3 Resources

General information

Name blazarmonitoring.asi.it
Status Production
Validation date 2019-04-01
Last change 2019-04-24
Discipline
  • Natural Sciences
    • Physical sciences
      • Space science global
Enrollment Url https://voms.recas.ba.infn.it:8443/voms/blazarmonitoring.asi.it/
Homepage Url http://www.openuniverse.asi.it/
Support Procedure Url

Description

The recent progress in the technical capabilities of the ground- and satellite-based observatories have made it possible to investigate the physical processes taking place in the sources by measuring their emission spectra in a large frequency range (multiwavelength astrophysics). Since there is a large number of currently operating telescopes (e.g., Neil Gehrels Swift observatory (Swift), Nuclear Spectroscopic Telescope Array (NuSTAR), Chandra, Fermi Large Area Telescope (Fermi LAT), HESS, MAGIC, etc.) and their data are mostly publicly available, multiwavelength astrophysics has become one of the fastest developing and most progressive fields of astrophysics. A remarkably large number of source classes discovered to date are confirmed to have a nonthermal spectrum ranging from the radio (10^7 Hz) to high and very high energy (~10^25 Hz) gamma-ray bands, among which the most interesting are blazars- an extreme subclass of the active galactic nuclei which have the jet exactly aligned toward the observer. The analyses of multiwavelength data accumulated from the blazar observations will allow to monitor the evolution of blazar variable emission in long time scales and by theoretical modeling of the obtained spectra to understand several fundamental jet features such as its magnetic field, particle energy distribution and density, the processes responsible for the particle acceleration and emission, etc. In this new project, the gamma-ray data accumulated by Fermi LAT during 2008-2018 from the observation of 500 bright blazars will be analyzed. Detailed light curves (emission flux changes in time) and spectra (from 100 MeV to 300 GeV) will be generated. We note that the data analyzed here will be made available to other scientists through a dedicated web page. This will be done within the Open Universe initiative under the auspices of COPUOS/UNOOSA. The project is coordinated by ICRANET, http://www.icranet.org.

Acceptable Use Policy

Text This Acceptable Use Policy applies to all members of blazarmonitoring.asi.it Virtual Organisation,
hereafter referred to as the blazarmonitoring.asi.it, with reference to use of the EGI Infrastructure.
The ICRANET owns and gives authority to this policy.
Goal and description of the blazarmonitoring.asi.it VO
---------------------------------------------------------------------
Members and Managers of the blazarmonitoring.asi.it agree to be bound by the Acceptable Usage Rules, blazarmonitoring.asi.it Security Policy and other relevant EGI Policies, and to use the Infrastructure only in the furtherance of the stated goal of the blazarmonitoring.asi.it.

Acknowledgments Statement

Grant Id
Scientific publications URL
Suggested This work used the EGI infrastructure with the dedicated support of CESGA”.

Resources

Max used physical non-swap i386 memory size 0
Max used physical non-swap x86_64 memory size 0
Max size of scratch space used by jobs 0
Max time of job execution 0
Job wall clock time limit 0
number cores
min number cores :
pref number cores :
max number cores :
number of ram
min number ram :
pref number ram :
max number ram :
scratch space values
min scratch space values :
pref scratch space values :
max scratch space values :

Cloud Resources

CPU Core 24
VM Ram 1
Storage Size 2

For additional details like contacts , please log in
/vo/checkVoName