dc.contributor.author |
Deep, A |
|
dc.contributor.author |
Ramaprakash, A. N |
|
dc.contributor.author |
Tandon, S. N |
|
dc.contributor.author |
Gupta, R |
|
dc.contributor.author |
Burse, M. P |
|
dc.contributor.author |
Chordia, P. A |
|
dc.contributor.author |
Das, H. K |
|
dc.contributor.author |
Engineer, S |
|
dc.contributor.author |
Kohok, A. A |
|
dc.contributor.author |
Mestry, V. B |
|
dc.date.accessioned |
2008-07-24T06:23:41Z |
|
dc.date.available |
2008-07-24T06:23:41Z |
|
dc.date.issued |
2002-09 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 3, pp. 791 - 795 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2872 |
|
dc.description.abstract |
In this paper we present the current status of development of the
Near Infrared PICNIC Imager (NIPI), which will be the first near-ffi instrument
on IUCAA telescope. When used at one of the Cassegrain side ports of the
telescope, it gives a plate scale of 0.8 arcsee per pixel at the PICNIC detector
array with a field of view of 2.5 arc minutes. It offers imaging capabilities in J,
H and K filter bands, with the reimager optimized in H-band for which almost
90encircled energy of a. point source is contained in a. pixel. Hardware and
software for infrared readout are being developed at IUCAA. |
en |
dc.format.extent |
157610 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
PICNIC |
en |
dc.subject |
IUCAA Telescope |
en |
dc.subject |
Near Infrared- Imager |
en |
dc.title |
Near Infrared PICNIC Imager (NIPI) for IUCAA Telescope |
en |
dc.type |
Article |
en |