| dc.contributor.author | Saha, S. K | |
| dc.contributor.author | Chinnappan, V | |
| dc.date.accessioned | 2008-07-25T07:01:13Z | |
| dc.date.available | 2008-07-25T07:01:13Z | |
| dc.date.issued | 2002-09 | |
| dc.identifier.citation | BASI, Vol. 30, No. 3, pp. 819 - 821 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/2886 | |
| dc.description.abstract | A new generation CCD detector caJ.led low light level OOD (L3CCD) that performs like an intensified CCD without incorporating a micro channel plate (MOP) for light amplification was procured and tested. A series of short exposure images with millisecond integration time has been obtained. The L3CCD is cooled to about -800 0 by Peltier cooling. | en |
| dc.format.extent | 98528 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.subject | Interferometer | en |
| dc.subject | Speckle Imaging | en |
| dc.subject | L3CCD Camera | en |
| dc.title | Performance of the low light level CCD camera for speckle imagmg | en |
| dc.type | Article | en |