Difference imaging in radio interferometry

Talk presented at the MPIfR/AIfA Lunch Colloquium, 1 October 2008, Bonn

O. Wucknitz [1]

  1. Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany

Abstract

Together with a group of colleagues, the speaker is preparing to use LOFAR to search for new gravitational lens systems. Because the resolution of LOFAR is only barely sufficient to identify lenses by morphological criteria, alternative methods would be very welcome.

A promising approach is to select objects with time-variable extended emission. Since intrinsic variability (but also scintillation) is generally only possible for compact sources, the signature of extended variability provides evidence for several compact components with small separations. In a good fraction of these objects, the multiple images will just be an illusion caused by a gravitational lens.

I discuss the development of a difference imaging algorithm in radio interferometry. Independent deconvolution with subsequent subtraction is not an option, because difference images produced in this way would be dominated by deconvolution errors. A multi-channel adaption of CLEAN is a viable alternative. The availability of powerful deconvolution techniques for variable sources may also be of relevance for other fields of research.

Similar approaches are needed for wide-band imaging, where it is not variability with time but with frequency that has to be taken into account.

A shorter version of this talk was presented at the Hamburg LOFAR meeting. An updated version of selected parts can be found here.




download original presentation
PDF file (1.6 MB, last change 1 Oct 2008)
36 pages, suitable for presentation with acroread. This version also includes some hyperlinks for quick navigation and links to references.

download printable version (small)
PDF file (1.4 MB, last change 1 Oct 2008)
Paper saving version. 5 pages, text in b/w, colour figures. 8 slides per A4 page.



To publications
To my homepage
To the AIfA
To the University of Bonn


Script last modified on 7 Sep 2010
Last change to this data base entry on 8 Oct 2008