A Far-Infrared Spectro-Spatial Space Interferometer by Roser Juanola-Parramon

Author:Roser Juanola-Parramon
Language: eng
Format: epub
Publisher: Springer International Publishing, Cham

From the day of this experiment, the data acquisition process has been modified. Not only a set of dark frames is acquired before the data, also a set of background frames is acquired for a reliable background illumination subtraction. Note that the peak of the measured background illumination is consistent with the position of the source number 12 of the 55 point sources array which presented a drop of visibility of 50 %.

3.2.2.5 An Example: The Pyramid

The 55 point sources array data is a good set for validation and calibration of the WIIT system. However, one of the objectives of WIIT is to observe astronomically representative test scenes, which can be binary sources.

Fig. 3.23Pyramid distribution of sources with CHIP for a source rotation of −90. Numbers assigned to the sources (left) and one of the frames of the data cube (right)

Download

Copyright Disclaimer:
This site does not store any files on its server. We only index and link to content provided by other sites. Please contact the content providers to delete copyright contents if any and email us, we'll remove relevant links or contents immediately.