Design of a Skipper CCD Focal Plane for the SOAR Integral Field Spectrograph

被引:8
作者
Villalpando, Edgar Marrufo [1 ,2 ,3 ]
Drlica-Wagner, Alex [2 ,3 ,4 ]
Bonati, Marco [5 ]
Bakshi, Abhishek [3 ]
Macanhan, Vanessa Bawden de Paula [6 ]
Cancino, Braulio [5 ]
Derylo, Gregory E. E. [3 ]
Estrada, Juan [3 ]
Moroni, Guillermo Fernandez [3 ]
Fraga, Luciano [6 ]
Holland, Stephen [7 ]
Jonas, Michelle J. J. [3 ]
Lapi, Agustin [3 ,9 ]
Moore, Peter [5 ]
Malagon, Andres A. Plazas [8 ]
Stefanazzi, Leandro [3 ]
Tiffenberg, Javier [3 ]
机构
[1] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[2] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[3] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[4] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[5] NSFs Natl Opt Infrared Astron Res Lab, Cerro Tololo Interamer Observ, Casilla 603, La Serena, Chile
[6] Lab Nacl Astrofis LNA MCTI, BR-37504364 Itajuba, MG, Brazil
[7] Lawrence Berkeley Natl Lab, One Cyclotron Rd, Berkeley, CA 94720 USA
[8] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[9] Univ Nacl Sur, Dept Ingn Elect & Computadoras, Bahia Blanca, Buenos Aires, Argentina
来源
X-RAY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY X | 2022年 / 12191卷
基金
美国国家科学基金会; 巴西圣保罗研究基金会;
关键词
Skipper CCD; sub-electron noise; photon counting detector; spectroscopy;
D O I
10.1117/12.2629475
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We present the development of a Skipper Charge-Coupled Device (CCD) focal plane prototype for the SOAR Telescope Integral Field Spectrograph (SIFS). This mosaic focal plane consists of four 6k x 1k, 15 mu m pixel Skipper CCDs mounted inside a vacuum dewar. We describe the process of packaging the CCDs so that they can be easily tested, transported, and installed in a mosaic focal plane. We characterize the performance of similar to 650 mu m thick, fully-depleted engineering-grade Skipper CCDs in preparation for performing similar characterization tests on science-grade Skipper CCDs which will be thinned to 250 mu m and backside processed with an antireflective coating. We achieve a single-sample readout noise of 4.5 e(-) rms/pix for the best performing amplifiers and sub-electron resolution (photon counting capabilities) with readout noise sigma similar to 0.16 e(-) rms/pix from 800 measurements of the charge in each pixel. We describe the design and construction of the Skipper CCD focal plane and provide details about the synchronized readout electronics system that will be implemented to simultaneously read 16 amplifiers from the four Skipper CCDs (4-amplifiers per detector). Finally, we outline future plans for laboratory testing, installation, commissioning, and science verification of our Skipper CCD focal plane.
引用
收藏
页数:19
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