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Amateur
Achievement Award
Peter Francis Williams
New South Wales, Australia
Each
year since 1979, an Award Committee, appointed by the ASP's Board
of Directors, has selected the recipient of one of its most prestigious
awards, The Amateur Achievement Award. This award is "designed
to recognize significant contributions to astronomy or amateur astronomy
by those not employed in the field of astronomy in a professional
capacity."
This
year's deserving awardee is Peter Francis Williams, a distinguished
amateur astronomer from New South Wales, Australia.
Since
obtaining his first telescope at the age of 14, Peter Williams has
been an active observer. He began variable star observing at 16,
and by age 20 was providing monthly reports to the VSS section of
the Royal Astronomical Society of New Zealand, to whom he has since
also provided numerous alert notices.
Mr.
Williams' contributions have been numerous and varied. He has established
himself as a reliable observer and one whose results are described
by professional astronomers as "of consistently high quality."
His diligence over the past twenty-five years has produced results
that have been made readily available to professional astronomers
(particularly in Australia and New Zealand) who have used them extensively
in their research.
Some
highlights of Williams' research include the early detection
of declines in R Corona Borealis-type stars and the long-term monitoring
of several southern Mira variables and eclipsing binaries. In both
cases, his work has been of direct value to professional astronomers
by alerting them to events in time for follow-up work by satellites
and larger ground-based telescopes.
It
has always been the practice of Peter Williams to scan the night
sky at the start of each night's work in order to detect any
unusual naked eye stellar object. This helped him become the first
person to detect the naked-eye nova, Nova Vel 1999. He specializes
in checking on RCrb stars with a view to promptly advising the worldwide
astronomical community of any decline in such stars. Mr. Williams
contributes untold numbers of hours to variable-star monitoring,
and his contributions have proven invaluable in ongoing efforts
toward the Anglo-Australian Observatory's creation of a major
all-sky survey of stellar radial velocities.
Work
such as that which Mr. Williams has conducted is essential to the
successful symbiosis between amateur and professional communities.
It is evident by the nomination letters submitted that Peter Francis
Williams has provided an essential and very much appreciated link
between the two.
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