English

Using THELI pipeline in order to reduce Abell 226 multi-band optical images

Instrumentation and Methods for Astrophysics 2013-09-04 v1

Abstract

In this paper we review THELI (Erben & Schrimer, 2005), an image processing pipeline developed to reduce multi-pointing optical images taken by mosaic CCD cameras. This pipeline works on raw images by removing several instrumental contaminations, implementing photometric calibration and astrometric alignment, and constructing a deep co-added mosaic image complemented by a weight map. We demonstrate the procedure of reducing NGC3923 images from raw data to the final results. We also demonstrate the quality of our data reduction strategy using mag-count and mag-error in mag plots. Emphasis is mainly placed on photometric calibration which is of great interest to us due to our scientific case. Based on the cross-association of the extracted catalogue against a reference catalogue of stellar magnitudes, zero-point calibration is performed. Our data reduction strategy and the method employed for cross-correlating large catalogues is also presented.

Keywords

Cite

@article{arxiv.1309.0642,
  title  = {Using THELI pipeline in order to reduce Abell 226 multi-band optical images},
  author = {R. Joveini and S. Sotoudeh and A. Roozrokh and M. Taheri},
  journal= {arXiv preprint arXiv:1309.0642},
  year   = {2013}
}

Comments

5 pages, 2 figures