Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..442..139a&link_type=abstract
Astronomical Data Analysis Software and Systems XX. ASP Conference Proceedings, Vol. 442, proceedings of a Conference held at Se
Astronomy and Astrophysics
Astronomy
Scientific paper
We investigate how to achieve the best possible ACIS spatial resolution by binning in ACIS sub-pixel and applying an event repositioning algorithm after removing pixel-randomization from the pipeline data. We quantitatively assess the improvement in spatial resolution by (1) measuring point source sizes and (2) detecting faint point sources. The size of a bright (but no pile-up), on-axis point source can be reduced by 20-30%. With the improved resolution, we detect ˜20% more faint sources when embedded in the extended, diffuse emission in a crowded field. We further discuss the false source rate of ˜10% among the newly detected sources, using a few ultra-deep observations.
Allen Glenn E.
Anderson Craig S.
Fabbiano Giuseppina
Glotfelty Kenny J.
Kim Dae Wook
No associations
LandOfFree
ACIS Sub-Pixel Resolution: Improvement in Point Source Detection 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 ACIS Sub-Pixel Resolution: Improvement in Point Source Detection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ACIS Sub-Pixel Resolution: Improvement in Point Source Detection will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-989227