語系:
繁體中文
English
說明(常見問題)
回圖書館首頁
手機版館藏查詢
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Assembly, characterization, and oper...
~
Pappas, Christine Goodwin.
FindBook
Google Book
Amazon
博客來
Assembly, characterization, and operation of large-scale TES detector arrays for ACTPol.
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Assembly, characterization, and operation of large-scale TES detector arrays for ACTPol./
作者:
Pappas, Christine Goodwin.
面頁冊數:
166 p.
附註:
Source: Dissertation Abstracts International, Volume: 77-07(E), Section: B.
Contained By:
Dissertation Abstracts International77-07B(E).
標題:
Astronomy. -
電子資源:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10010812
ISBN:
9781339468235
Assembly, characterization, and operation of large-scale TES detector arrays for ACTPol.
Pappas, Christine Goodwin.
Assembly, characterization, and operation of large-scale TES detector arrays for ACTPol.
- 166 p.
Source: Dissertation Abstracts International, Volume: 77-07(E), Section: B.
Thesis (Ph.D.)--Princeton University, 2016.
The Polarization-sensitive Receiver for the Atacama Cosmology Telescope (ACTPol) is designed to measure the Cosmic Microwave Background (CMB) temperature and polarization anisotropies on small angular scales. Measurements of the CMB temperature and polarization anisotropies have produced arguably the most important cosmological data to date, establishing the LambdaCDM model and providing the best constraints on most of its parameters. To detect the very small fluctuations in the CMB signal across the sky, ACTPol uses feedhorn-coupled Transition-Edge Sensor (TES) detectors. A TES is a superconducting thin film operated in the transition region between the superconducting and normal states, where it functions as a highly sensitive resistive thermometer. In this thesis, aspects of the assembly, characterization, and in-field operation of the ACTPol TES detector arrays are discussed. First, a novel microfabrication process for producing high-density superconducting aluminum/polyimide flexible circuitry (flex) designed to connect large-scale detector arrays to the first stage of readout is presented. The flex is used in parts of the third ACTPol array and is currently being produced for use in the AdvACT detector arrays, which will begin to replace the ACTPol arrays in 2016. Next, we describe methods and results for the in-lab and on-telescope characterization of the detectors in the third ACTPol array. Finally, we describe the ACTPol TES R(T,I) transition shapes and how they affect the detector calibration and operation. Methods for measuring the exact detector calibration and re-biasing functions, taking into account the R(T,I) transition shape, are presented.
ISBN: 9781339468235Subjects--Topical Terms:
517668
Astronomy.
Assembly, characterization, and operation of large-scale TES detector arrays for ACTPol.
LDR
:02569nmm a2200277 4500
001
2077105
005
20161114130223.5
008
170521s2016 ||||||||||||||||| ||eng d
020
$a
9781339468235
035
$a
(MiAaPQ)AAI10010812
035
$a
AAI10010812
040
$a
MiAaPQ
$c
MiAaPQ
100
1
$a
Pappas, Christine Goodwin.
$3
3192596
245
1 0
$a
Assembly, characterization, and operation of large-scale TES detector arrays for ACTPol.
300
$a
166 p.
500
$a
Source: Dissertation Abstracts International, Volume: 77-07(E), Section: B.
500
$a
Adviser: Suzanne Staggs.
502
$a
Thesis (Ph.D.)--Princeton University, 2016.
520
$a
The Polarization-sensitive Receiver for the Atacama Cosmology Telescope (ACTPol) is designed to measure the Cosmic Microwave Background (CMB) temperature and polarization anisotropies on small angular scales. Measurements of the CMB temperature and polarization anisotropies have produced arguably the most important cosmological data to date, establishing the LambdaCDM model and providing the best constraints on most of its parameters. To detect the very small fluctuations in the CMB signal across the sky, ACTPol uses feedhorn-coupled Transition-Edge Sensor (TES) detectors. A TES is a superconducting thin film operated in the transition region between the superconducting and normal states, where it functions as a highly sensitive resistive thermometer. In this thesis, aspects of the assembly, characterization, and in-field operation of the ACTPol TES detector arrays are discussed. First, a novel microfabrication process for producing high-density superconducting aluminum/polyimide flexible circuitry (flex) designed to connect large-scale detector arrays to the first stage of readout is presented. The flex is used in parts of the third ACTPol array and is currently being produced for use in the AdvACT detector arrays, which will begin to replace the ACTPol arrays in 2016. Next, we describe methods and results for the in-lab and on-telescope characterization of the detectors in the third ACTPol array. Finally, we describe the ACTPol TES R(T,I) transition shapes and how they affect the detector calibration and operation. Methods for measuring the exact detector calibration and re-biasing functions, taking into account the R(T,I) transition shape, are presented.
590
$a
School code: 0181.
650
4
$a
Astronomy.
$3
517668
650
4
$a
Electrical engineering.
$3
649834
690
$a
0606
690
$a
0544
710
2
$a
Princeton University.
$b
Physics.
$3
2101570
773
0
$t
Dissertation Abstracts International
$g
77-07B(E).
790
$a
0181
791
$a
Ph.D.
792
$a
2016
793
$a
English
856
4 0
$u
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=10010812
筆 0 讀者評論
館藏地:
全部
電子資源
出版年:
卷號:
館藏
1 筆 • 頁數 1 •
1
條碼號
典藏地名稱
館藏流通類別
資料類型
索書號
使用類型
借閱狀態
預約狀態
備註欄
附件
W9309973
電子資源
11.線上閱覽_V
電子書
EB
一般使用(Normal)
在架
0
1 筆 • 頁數 1 •
1
多媒體
評論
新增評論
分享你的心得
Export
取書館
處理中
...
變更密碼
登入