NGC 7027: A comparison of ISOCAM CVF and ground-based mid-infared CVF images

Mathematics – Logic

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Scientific paper

We present a preliminary comparison between ISOCAM CVF and ground-based mid-infrared CVF observation of the planetary nebula NGC 7027. The main focus of this work is directed towards understanding the CAM transients and the CAM CVF calibration. The scientific highlights from this work are presented by Dayal et al. in the 195 meeting of the American Astronomical Society. The current analysis is limited to a morphological comparison between CAM and the Mid InfraRed Array Camera (MIRAC) images. We find that the observed morphology of NGC 7027 in CAM images significantly departs from that seen in MIRAC images after flat-field corrections are applied to CAM images. This is likely due to inaccurate treatment of detector transients. Residual transients are subsequently enhanced by the flat-field correction. Moreover, we find that for CVF data, most transient correction options are ineffective for the NGC 7027 data.

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