Key to source observatory of images.


AAT	Anglo-Australian Telescope 
APO	Apache Point Observatory, New Mexico State University
BBSO	Big Bear Solar Observatory
CAO 	Calar Alto Observatory
CTIO	Cerro Tololo Observatory
ESO	European Southern Observatory
EUVE	Extreme Ultra-Violet Explorer (Satellite)
GAL	Galileo Spacecraft Solid State Imaging Camera
GCO	Grove Creek Observatory
GEA	Grup d'Estudis Astronomics (Non-professional team that follows and cooperates in professional astronomy research
HST	Hubble Space Telescope
IUE	International Ultra-Violet Explorer (Satellite)
IRTF	Infrared Facility Telescope
KAO	Kuiper Airborne Obserservatory
KECK	Keck 10m Telescope
KITT	Kitt Peak National Observatory
LCP	Las Campanas, 2.5m Dupont Telescope
LICK	Lick Observatory
LOW	Lowell Observatory, Flagstaff Arizona
LPM	La Palma (European Sourthen Observatory)
MCD	The University of Texas McDonald Observatory
MSSSO	Mount Stomlo and Siding Spring Observatories
NSFCAM  256 x 256 InSb (1-5 micron_ facility camera at the IRTF	
NSO	National Solar Observatory, Sunspot New Mexico
OAN	Observatorio Astronomico Nacional, MEXICO
ON	Observatorio de la Cote d'Azur 
PAL	Mount Palomar, 200 inch Hale Telescope
PHIL	Air Force Maui Optical Station (Phillips Lab)	
ROS	Rosat High Resolution X-ray Imager
SAAO	South Africa Astronomical Observatory
SPIREX	South Pole Infrared Explorer
TAMU	Texas A&M University
TDE	Teide Observatory
UH	University of Hawaii
VTT	Vaccum Tower Telescope (National Solar Observatory), Sunspot New Mexico
WFS	Wilhelm Foerster Observatory, Berlin Germany
WHAT	Whately Observatory
WIL	Mount Wilson
WIO	Wyoming Infrared Observatory

FILENAMES

An effort has been made to put some sense into image names. From now on, this site will be using a defined system for naming SL9 images.

The first part of the image name will be a keyword coresponding to the source observatory of the image. The keywords list can be found in the file "KEY." There will usually be an underscore (_) separating the first half of the name from the second half of the name. The last part of the image name is the latest Fragment Impact visble, with an index on the end if there more than one...

For example:

MCD_L3.gif breaks down as follows:

MCD -> The University of Texas McDonald Observatory, 
L   -> Fragment L of Comet P/Shoemaker-Levy 9 is the most recent visible 
       fragment 
3   -> It is the third image of this type...

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