A microwave kinetic inductance detector for the DAG telescope
Yükleniyor...
Dosyalar
Tarih
2016
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
SPIE
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
We present the details of a proposed microwave kinetic inductance detector (MKID) for the DAG (Eastern Anatolia Observatory in Turkish) telescope, DAG-MKID. The observatory will have a modern 4m size telescope that is currently under construction. Current plan to obtain the first light with the telescope is late 2019. The proposed MKID based instrument will enable astronomers to simultaneously detect photons in the relatively wide wavelength range of 4000-13500 Å with a timing accuracy of ?s and spectral resolution R = /? =10-25. With a planned field of view of approximately an arcminute, DAG-MKID will mostly be used for follow-up observations of transient or variable objects as well as a robust tool to measure photometric redshifts of a large number of galaxies or other extra-galactic objects.
Açıklama
Anahtar Kelimeler
Inductance, Infrared detectors, Observatories, Eastern Anatolia, Extra-galactic, Field of views, Follow up, Kinetic inductance detectors, Red shift, Turkishs, Wavelength ranges, Telescopes, Photometric redshifts, Galaxy Cluster, Arcons, Focal plane instrumentation, Microwave kinetic inductance
Kaynak
Proceedings of SPIE - The International Society for Optical Engineering
WoS Q Değeri
N/A
Scopus Q Değeri
N/A
Cilt
9915
Sayı
Künye
Güver, T., Mazin, B. A., O'Brien, K., Kay, B., Aliş, S., Yelkenci, F. K., Yeşilyaprak, C., Erol, A., Yerli, S. K. & Keskin, O. (2016). A microwave kinetic inductance detector for the DAG telescope. Paper presented at the Proceedings of SPIE - The International Society for Optical Engineering, 9915, 1-8. doi:10.1117/12.2234281
