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Near-Infrared Images of Comet 9P/Tempel 1 |
Status: Archived
This volume contains raw and reduced near-infrared images of comet 9P/Tempel 1, the target of the Deep Impact mission, as well as a table and plot of the H, J, and K magnitudes of Tempel 1. Images were obtained from UT July 2-9, 2005 by M. Knight, R. Swaters, and N. Samarasinha using the Simultaneous Quad Infrared Imaging Device (SQIID) at the KPNO 2.1-m telescope. Results are published in the paper "Ground-based visible and near-IR observations of Comet 9P/Tempel 1 during the Deep Impact encounter" by Knight et al. (2007).
The entire data set is about 5 GB in size. The data have been divided into two volumes, one for the raw data and one for the reduced data, to facilitate bulk downloading. Individual files can be browsed through the links below.
MD5 checksums for the above files
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In case you're wondering...
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An overview of the volume contents is provided in the aareadme.txt file.
Catalog files contain the overview information and parameters used in loading the PDS central catalog, specifically, or for developing other interfaces to the data outside of PDS. The information they contain, particularly in their descriptive text fields, should be clear, complete, and understandable to a research user who is not necessarily a mission or instrument specialist.
These files are located in the catalog/ subdirectory. The directory contents are described by the catinfo.txt file.
In addition to the small text files located throughout the volume to describe directory contents, some specific documents are provided to assist with understanding the data and processing involved. These files are located in the document/ subdirectory. The directory contents are described by the docinfo.txt file.
Additional explanatory material about the observations has been provided in several separate documents:
In addition, in this directory you will also find ads.txt and its label, which contains information for the ADS Abstract Service databasw.
The data are divided into two subdirectories, which are each further divided by sequential night.
All data files are presented as FITS files with detached PDS labels.
The index directory contains the required PDS index into the files in the data directory, as well as the checksum file.