| dc.contributor.author | Parmaksizoglu, Murat | |
| dc.contributor.author | Esenoglu, Hasan | |
| dc.contributor.author | HELHEL, SELÇUK | |
| dc.contributor.author | Kirbiyik, Halil | |
| dc.contributor.author | Dindar, Murat | |
| dc.date.accessioned | 2021-03-05T07:44:37Z | |
| dc.date.available | 2021-03-05T07:44:37Z | |
| dc.identifier.citation | Dindar M., Parmaksizoglu M., HELHEL S., Esenoglu H., Kirbiyik H., "A NEW GRB FOLLOW-UP SOFTWARE AT TUG", 4th Workshop on Robotic Autonomous Observatories, Torremolinos, İspanya, 28 Eylül - 02 Ekim 2015, cilt.48, ss.66-69 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_9565ce27-a7b5-49fa-81be-56a1267d56aa | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/100586 | |
| dc.identifier.uri | http://www.astroscu.unam.mx/rmaa/RMxAC..48/PDF/RMxAC..48_part-3.6.pdf | |
| dc.description.abstract | A gamma-ray burst (GRB) optical photometric follow-up system at TUBITAK (Scientic and Technological Research Council of Turkey) National Observatory (TUG) has been planned. It uses the 0.6-m Telescope (T60) and can automatically respond to GRB Coordinates Network (GCN) alerts. The telescopes slew relatively fast, being able to point to a new target field within 30 s upon a request. Whenever available, the 1 m T100 and 2.5 m RTT150 telescopes will be used in the future. As an example in 2015, the GRB software system (will be server side) at T60-telescope responded to GRB alert and started the observation as early as 129 s after the GRB trigger autonomously. | |
| dc.language.iso | eng | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.subject | Fizik | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | A NEW GRB FOLLOW-UP SOFTWARE AT TUG | |
| dc.type | Bildiri | |
| dc.contributor.department | Akdeniz Üniversitesi , , | |
| dc.identifier.volume | 48 | |
| dc.contributor.firstauthorID | 2182116 | |
