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New Developments in Array Technology and Applications - Proceedings of the 167th Symposium of the International Astronomical Union, held in the Hague, the Netherlands, August 23-27, 1994 (Paperback, Softcover reprint of the original 1st ed. 1995)
Loot Price: R4,392
Discovery Miles 43 920
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New Developments in Array Technology and Applications - Proceedings of the 167th Symposium of the International Astronomical Union, held in the Hague, the Netherlands, August 23-27, 1994 (Paperback, Softcover reprint of the original 1st ed. 1995)
Series: International Astronomical Union Symposia, 167
Expected to ship within 10 - 15 working days
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IAU Symposium No. 167 brought together researchers who use CCDs and
arrays, designers and manufacturers of CCDs and Array Mosaics and
those who write the software to control these devices and to reduce
the large amounts of data contained in each frame. At the meeting
such topics as plans for applying the new technology to the new
large telescopes that have been built recently and those planned in
the near future, new developments in infrared arrays, advances and
concerns with the use of CCDs in photometry and spectroscopy and
the creation of large mosaics in photometry and spectroscopy and
the creation of large mosaics of chips which allow larger areas of
the sky to be covered in a single frame were discussed. There were
sessions devoted to the following topics: New Developments in CCD
Technology; New Developments in IR Detector Arrays; Direct Imaging
with CCDs and Other Arrays; Spectroscopy with CCDs and Other
Arrays; and Large Field Imaging with Array Mosaics. Scientific
results of studies made with this technology were covered in the
poster sessions. CCD and Array Detectors have become the detectors
of choice at all the world's optical observatories. Such
instruments on small university and college telescopes have turned
these telescopes into instruments that can now do observations
which in the past were done only on the largest telescopes. CCDs
and Arrays are known as the people's detector' because of their
ability to turn small telescopes into true research instruments. On
large telescopes observations can be made of extremely faint and
crowded objects that were impossible to observe before the advent
of CCD and Array technology. The proceedings of this meeting will
be useful toall those who are interested in the design, manufacture
and use of CCDs and Arrays for astronomical observations.
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