Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/1937Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Asgekar, A | - |
| dc.contributor.author | Deshpande, A. A | - |
| dc.date.accessioned | 2007-10-31T07:17:53Z | - |
| dc.date.available | 2007-10-31T07:17:53Z | - |
| dc.date.issued | 1999 | - |
| dc.identifier.citation | BASI, Vol. 27, No. 1, pp. 209 - 211 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/1937 | - |
| dc.description.abstract | Pulsar observations with improved sensitivity have been initiated at 34.5 MHz and a 1-MHz bandwidth using the Gauribidanur Radio Telescope. We describe our new procedure where the raw (2-bit) signal voltages are recorded and the data are processed optimally off-line. A few preliminary results from these observations are presented. | en |
| dc.format.extent | 209789 bytes | - |
| dc.format.mimetype | application/pdf | - |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/1999BASI...27..209A | en |
| dc.subject | Pulsar | en |
| dc.subject | Telescope | en |
| dc.title | New pulsar observations using the Gauribidanur Radio Telescope | en |
| dc.type | Article | en |
| Appears in Collections: | BASI Publications | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| ashish.pdf | 204.87 kB | Adobe PDF | ![]() View/Open |
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