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dc.contributor.authorYERLİ, SİNAN KAAN
dc.contributor.authorAlis, Sinan
dc.contributor.authorYEŞİLYAPRAK, Cahit
dc.date.accessioned2021-03-06T12:42:20Z
dc.date.available2021-03-06T12:42:20Z
dc.identifier.citationAlis S., YEŞİLYAPRAK C., YERLİ S. K. , "DAG Telescope: A New Potential for MOS Observations", Conference on Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields, Santa Cruz de la Palma, İspanya, 2 - 06 Mart 2015, cilt.507, ss.439-442
dc.identifier.othervv_1032021
dc.identifier.otherav_f5241b88-9b8d-4085-a124-2bc262c8cfb8
dc.identifier.urihttp://hdl.handle.net/20.500.12627/160676
dc.description.abstractEast Anatolian Observatory (aka. DAG) is a national project supported by the Turkish Government for building a 4m class telescope which will be working in the optical and near-IR domain. As the tender process has been completed and kick-off to the telescope and the mirror production has been initiated, the project team is looking for possible collaborations for the focal plane instrumentation. This contribution is intended to describe the DAG project and to show its opportunities for a state-of-the-art MOS instrument.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.titleDAG Telescope: A New Potential for MOS Observations
dc.typeBildiri
dc.contributor.departmentAtatürk Üniversitesi , Fen Fakültesi , Astronomi Ve Astrofizik
dc.identifier.volume507
dc.contributor.firstauthorID79461


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