Removing Internal Reflections from Deep Imaging Datasets

Details Removing Internal Reflections from Deep Imaging Datasets Removing Internal Reflections from Deep Imaging Datasets

2009-09-17

arxiv.org/abs/0909.3320v1

Astronomy and Astrophysics

Astrophysics

Instrumentation and Methods for Astrophysics

15 pages, 11 figures. Accepted to PASP

Scientific paper

We present a means of characterizing and removing internal reflections between the CCD and other optical surfaces in an astronomical camera. The stellar reflections appear as out-of-focus images and are not necessarily axisymmetric about the star. Using long exposures of very bright stars as calibration images we are able to measure the position, size, and intensity of reflections as a function of their position on the field. We also measure the extended stellar point-spread function out to one degree. Together this information can be used to create an empirical model of the excess light from bright stars and reduce systematic artifacts in deep surface photometry. We then reduce a set of deep observations of the Virgo cluster with our method to demonstrate its efficacy and to provide a comparison with other strategies for removing scattered light.

Affiliated with

Also associated with

No associations

Rating

Removing Internal Reflections from Deep Imaging Datasets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Removing Internal Reflections from Deep Imaging Datasets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Removing Internal Reflections from Deep Imaging Datasets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-276062