The purpose of these pages is to allow
those engaged in determining asteroid lightcurve parameters
to coordinate their efforts so that the best use of observing time can be made.
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| Funding to support the CALL site is provided in part by NASA grants NNG06GI32G and NNX06AB30G and by National Science Foundation grant AST-0607505 | ||||||||||||||||||||||||||
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Check, then ObserveWe're getting another spell of what looks to be unneccessary duplication of effort. PLEASE. Check with the CALL site before you start work on a target, not after you have several sessions. Some times duplication is good because the period cannot be effectively covered by one station or those of similar longitude. However, some times that single station can and does cover those more difficult objects by sticking with it a little longer. In the meantime, there are thousands of asteroids within reach of backyard telescopes that have no lightcurve parameters at all and dozens that are wanting only good coverage at one more apparition for modeling. The CALL site's value as an observing tool is up to the observers. If used effectively, we all benefit as does asteroid research. If poorly used or abused then, like any tool, it eventually breaks and tossed aside. |
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CALL Site Sections
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You are visitor
This page is maintained by
Brian D. Warner
Palmer Divide Observatory (716)
17995 Bakers Farm Rd.
Colorado Springs, CO 80908
under the supervision of Dr. Alan W. Harris and Dr. Petr Pravec. If you have any questions, comments,
or difficulties with the site itself, please contact
Brian Warner. Questions about the contents of the page should be directed to
the appropriate person.
Funding for the CALL site is provided in part through grants from NASA (NNX 09AB48G) and NSF (AST-0607505)