| 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 | |
| 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 |