ESAIntegralESA Science
   
Integral in brief
Integral overviewIntegral factsheetA truly international mission
About Integral
The spacecraftThe launcherThe launch site - BaikonurThe journey
Integral's mission
Multimedia
Image galleryPre-launch images, Sept 2002Pre-launch images, October 2002Video gallery3D Flash 'model'Make a model Bookmark and Share
 
 
 
 
Article Images
Understanding our neighbourhood in the universe
 
17 December 2007

Integral’s hard-X-ray map of  bright AGNs
Download:
 HI-RES JPG (Size: 361 kb)
This Integral map (celestial sphere in galactic coordinates) shows the space density of hard X-ray bright Active Galactic Nuclei (AGNs) in different directions of the sky.

As expected, the distribution of nearby AGNs is indeed strongly anisotropic, meaning that AGNs have non-uniform spatial distribution. For comparison, the green contours show a usual tracer of mass concentrations in the local Universe - the surface density of galaxies identified in the 'IRAS point source catalogue red-shift survey' at distances smaller than 70 megaparsecs, or about 230 million light years.

The large-scale feature in the north-east direction is consistent with the projected position of the highest mass concentrations in the local Universe - the Virgo cluster and the Great Attractor. The south-western structure is consistent with the position of the Perseus-Pisces supercluster.

Credits: ESA/Integral/ R.Krivonos et al.

 
 
Auger optical map of highest energy cosmic rays
Download:
 HI-RES JPG (Size: 656 kb)
This celestial sphere in galactic coordinates shows the arrival directions of the 27 highest energy cosmic rays (UHECRs) detected in visible wavelengths by the Auger ground telescopes in Argentina.

The energies are greater than 57 billion of billions of electron-volts, and are shown as circles. The positions of 472 Active Galactic Nuclei (AGNs) within 75 megaparsecs, or about 245 million light years, are shown as red *s. The blue region defines the field of view of the Auger telescope and deeper blue indicates larger exposure.

The solid curve marks the boundary of the field of view. The closest AGN, Centaurus A, is marked as a white *. Two of the 27 cosmic rays have arrival directions within 3 degrees of this galaxy. The dashed curve delineates a region where large numbers of nearby galaxies, including AGNs, are concentrated.

Credits: Auger

 


ESA's gamma-ray astronomy missionArtist's view of Integral
ESApod
Integral anniversary
Related articles
Extension of ESA’s Integral and XMM-Newton missions approvedNew scientific riches from IntegralScience with Integral – five years onGamma-ray lighthouse at the edge of our universeRadioactive iron, a window to the starsIntegral expands our view of the gamma-ray skyIntegral points to the fastest spinning neutron starStar eats companionIntegral sees the Galactic centre playing hide and seekIntegral catches a new erupting black holeESA steps towards a great black hole censusWhere are the supermassive black holes hiding?Integral sees a GRB out of the corner of its eyeIntegral catches stellar 'corpses' by the tailExceptional manoeuvres enable unique Integral scienceIntegral identifies supernova rate for Milky Way
Related ESA publications
Integral results leaflet (pdf)
In depth
Integral in-depth
Related news
Pierre Auger observatory release
 
 
 
   Copyright 2000 - 2010 © European Space Agency. All rights reserved.