7-11 July 2014
Africa/Johannesburg timezone
<a href="http://events.saip.org.za/internalPage.py?pageId=16&confId=34"><font color=#0000ff>SAIP2014 Proceedings published on 17 April 2015</font></a>

Modelling Inhomogeneities in the EBL

8 Jul 2014, 17:10
1h 50m
D Ring ground level

D Ring ground level

Board: D1.220
Poster Presentation Track D1 - Astrophysics Poster1

Speaker

Mr Ayman Kudoda (University of the Witwatersrand)

Level for award<br>&nbsp;(Hons, MSc, <br> &nbsp; PhD)?

MSc

Main supervisor (name and email)<br>and his / her institution

Dr. Andreas Faltenbacher,
Andreas.Faltenbacher@wits.ac.za
School of Physics,
University of the Witwatersrand.

Would you like to <br> submit a short paper <br> for the Conference <br> Proceedings (Yes / No)?

yes

Apply to be<br> considered for a student <br> &nbsp; award (Yes / No)?

yes

Abstract content <br> &nbsp; (Max 300 words)<br><a href="http://events.saip.org.za/getFile.py/access?resId=0&materialId=0&confId=34" target="_blank">Formatting &<br>Special chars</a>

Extragalactic Background Light (EBL) is the diffused light accumulated from all the galaxies and stars. EBL is an important tool for studying the cosmic galaxy formation history from the decoupling era until present time. In this work we model the distribution and, in particular, the fluctuations of the EBL. The study is based on the semi analytical galaxy catalogue from the Millennium Simulation data base. As a test of our model we propose to investigate the correlation between steepening of the Gamma ray spectra and the fluctuations of the EBL.

Primary author

Mr Ayman Kudoda (University of the Witwatersrand)

Co-author

Dr Andreas Faltenbacher (University of the Witwatersrand)

Presentation Materials

There are no materials yet.