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Jian-Feng Zhou

Publications and source records attributed to Jian-Feng Zhou.

3 recordsLinked to original sources

A Statistical Definition of Image Resolution Based on the Correlation of Pixels

Resolution, usually defined by the Rayleigh criterion or the Full Width at Half Maximum of a Point Spread Function, is a basic property of an image. Here, we present a new statistical definition of image resolution based on the cross-correlation properties of the pixels in an image. It is shown that the new definition of image resolution depends not only on the PSF of an imaging device, but also on the signal-to-noise ratio of the data and on the structures of an object. In an image, the resolution does not have to be uniform. Our new definition is also suitable for the interpretation of the result of a deconvolution. We illustrate this, in this paper, with a Wiener deconvolution. It is found that weak structures can be extracted from low signal-to-noise ratio data, but with low resolution; a high-resolution image was obtained from high signal-to-noise ratio data after a Wiener deconvolution. The new definition can also be used to compare various deconvolution algorithms on their processing effects, such as resolution, sensitivity and sidelobe level, etc.

astro-ph.IM

Reconstructing light curves from HXMT imaging observations

The Hard X-ray Modulation Telescope (HXMT) is a Chinese space telescope mission. It is scheduled for launch in 2015. The telescope will perform an all-sky survey in hard X-ray band (1 - 250 keV), a series of deep imaging observations of small sky regions as well as pointed observations. In this work we present a conceptual method to reconstruct light curves from HXMT imaging observation directly, in order to monitor time-varying objects such as GRB, AXP and SGR in hard X-ray band with HXMT imaging observations.

astro-ph.IM

Accelerated direct demodulation method for image reconstruction with spherical data from Hard X-ray Modulation Telescope

The hard X-ray modulation telescope mission HXMT is mainly devoted to performing an all-sky survey at 1 keV -- 250 keV with both high sensitivity and high spatial resolution. The observed data reduction as well as the image reconstruction for HXMT can be achieved by direct demodulation method (DDM). However the original DDM is computationally too expensive for multi-dimensional data with high resolution to employ for HXMT data. In this article we propose an accelerated direct demodulation method adapted for data from HXMT. Simulations are also presented to demonstrate this method.

astro-ph.IM