dc.contributor.author |
Chandrasekhar, T |
|
dc.contributor.author |
Shah, R |
|
dc.contributor.author |
Mondal, S |
|
dc.date.accessioned |
2008-06-27T11:05:15Z |
|
dc.date.available |
2008-06-27T11:05:15Z |
|
dc.date.issued |
2003 |
|
dc.identifier.citation |
BASI, Vol. 31, No. 3&4, pp. 471 - 474 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2534 |
|
dc.description.abstract |
Recently we have successfully observed the lunar occulation of a carbon star IRC+20120 and a M5 star IRC+10241 with the NICMOS sub array at the 1.2m Gurushikhar telescope. The integration times were respectively 5 millisec and 3 millisec per sample in the broad K band. The interval between two integrations was ~ 16 millisec. FOV of the sub array was 10 arcsec x 10 arcsec. Details of the experiment and results are discussed. |
en |
dc.format.extent |
115163 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2003BASI...31..471C |
en |
dc.subject |
Infrared arrays |
en |
dc.subject |
Lunar occultaion |
en |
dc.subject |
High angular resolution |
en |
dc.title |
Lunar Occulations with Infrared Arrays |
en |
dc.type |
Article |
en |