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PIXIS 成像型與光譜型相機

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PIXIS是市場上*的一款提供全金屬真空封存,深度制冷的科研級CCD相機。真空質(zhì)量終生質(zhì)保。高量子效率,高度集成化,低噪聲設(shè)計的科學(xué)成像/光譜相機,可應(yīng)用于紫外到近紅外各類實驗。

詳細(xì)信息 在線詢價

 

普林斯頓儀器(PI)的成像產(chǎn)品,包括:CCD相機,高速增強型ICCD,電子增益型EMCCD,高速增益emICCD,X射線相機,銦鎵砷相機。我們致力于為您提供創(chuàng)新的方案,解決你棘手挑戰(zhàn)性的問題。

我們堅持技術(shù)創(chuàng)新來為科研工作者提供高性能的成像技術(shù),包括SOPHIA,ProEM,PI-MAX4,NIRvana等突破性的產(chǎn)品。

 

PIXIS 成像型與光譜型相機

行業(yè)標(biāo)準(zhǔn),高性能CCD相機

PIXIS系列相機是集成度高,低噪聲設(shè)計的科學(xué)成像/光譜相機,響應(yīng)范圍從紫外到近紅外。結(jié)合PI*的XP制冷技術(shù),PIXIS是市場上*的一款提供全金屬真空封存,深度制冷的科研級CCD相機。真空質(zhì)量終生質(zhì)保。

高量子效率,超低噪聲電子電路,使得PIXIS成為高要求的低光實驗中理想的選擇,例如拉曼光譜,波什-愛因斯坦凝聚態(tài)(BEC),太陽能器件檢測,熒光實驗等等

PIXIS相機可以選擇eXcelon鍍膜技術(shù),增加其敏感度同時抑制近紅外波段的干涉現(xiàn)象。

image of PIXIS <br> 成像型與光譜型相機

 

PIXIS相機具有以下特點:

 支持不同芯片尺寸

 頻譜響應(yīng)從~ 180nm至~1100nm (紫外到近紅外)波段,更有eXcelon抗干涉技術(shù)eXcelon technology

 的全金屬真空封存技術(shù)

 靈活的讀出設(shè)置

 高速USB2.0接口

 功能強大的 64位 LightField 操作平臺

 

 

產(chǎn)品綜述

PIXIS系列相機是高度集成化,低噪聲設(shè)計的科學(xué)成像/光譜相機,可應(yīng)用于紫外到近紅外各類實驗。

PIXIS系列有前照型CCD,后照型CCD,后照深耗盡型CCD,適合成像或成譜的芯片格式。每一款PyLoN相機都提供了同類相機中的敏感度,的噪聲以及的動態(tài)范圍。   

BEC vortices

Images courtesy of Prof. Wolfgang Ketterle, MIT.

 

 

產(chǎn)品特點

探測范圍180nm 至 1100nm:

可滿足各類實驗需求

可選高于95%的量子效率

紫外波段的量子效率,可選擇紫外增強型CCD 或者 Unichrome/Lumogen phosphor鍍膜

結(jié)合eXcelon技術(shù),提升相機的敏感度

img3

普林斯頓儀器的真空封存技術(shù):

終生真空質(zhì)保

風(fēng)冷或者水冷均可達(dá)-90

長時間曝光下的超低暗噪聲

單層透射窗口增加芯片的敏感度

無需額外的維護

img4

的eXcelon技術(shù),用于背照型CCD:

增強的靈敏度,帶來更好的量子效率

減少背照式CCD的近紅外干涉現(xiàn)象

查看更多 eXcelon 的信息

img5

 

雙讀出放大器:

增強的系統(tǒng)靈活性

高敏讀出放大器具有極低的讀出噪聲

大動態(tài)讀出放大器增加了數(shù)據(jù)深度

img6

高速USB2.0數(shù)據(jù)接口:

任何電腦直接連接,無需額外硬件

即插即用

真正的16位數(shù)據(jù)傳輸能力,可達(dá)2MHz讀出速度

USB2

LightField的64-位操作平臺:

直觀易上手的用戶界面設(shè)計.

內(nèi)置數(shù)學(xué)引擎,實時獲得圖像與光譜的數(shù)據(jù)分析.

PICAM(64)位通用程序語言,方便的程序修改與編譯.

與LabVIEW,MATLAB,EPICS等第三方軟件無縫對接.

IntelliCal 精準(zhǔn)的波長校準(zhǔn)和強度校準(zhǔn),一鍵完成。

img8

 

 

 

型號規(guī)格

用于成像和光譜學(xué)的PIXIS CCD相機型號比較和數(shù)據(jù)表

Imaging Models

Sensor Type

Pixel Size

Readout Amplifiers

Peak QE

512 x 512 datasheet pdf

BX, B

24 x 24 µm

single

view QE data

1024 x 1024 datasheet pdf

BRX, BR, BX, B, BUV, F

13 x 13 µm

single

view QE data

1340 x 1300 datasheet pdf

BX, B, BUV, F

20 x 20 µm

dual

view QE data

2048 x 2048 datasheet pdf

BRX, BR, BX, B, BUV, F

13.5 x 13.5 µm

dual mode

view QE data

 

Spectroscopy Models

Sensor Type

Pixel Size

Readout Amplifiers

Peak QE

1340 x 100 datasheet pdf

BRX, BR, BX, B, F

20 x 20 µm

dual

view QE data

1340 x 400 datasheet pdf

BRX, BR, BX, B, F

20 x 20 µm

dual

view QE data

2048 x 512 datasheet pdf

BX, B, BUV

13.5 x 13.5 µm

dual mode

view QE data

1024 x 252 datasheet pdf

BR, E

26 x 26 µm

single

view QE data

 

 

Imaging cameras (anchor link to table) | Spectroscopy cameras (anchor link to table)

 

Sensor Types:

 

Princeton Instruments' proprietary eXcelon process increases detector sensitivity in the blue and NIR while suppressing etalon interference fringes.

B/I DD (Back-illuminated deep depletion) sensors have up to 95% QE in the NIR with minimal etaloning.

B/I (Back-illuminated) sensors have up to 95% QE in the visible but are subject to etaloning in the NIR.

BUV (Enhanced UV) sensors offer the highest UV sensitivity with moderate visible sensitivity.

F/I (Front-illuminated) CCD sensors offer economical performance from ~400-1000 nm with up to ~50% QE and negligible etaloning. Open Electrode architecture improves QE by reducing the area of the electrodes.

 

Pixel Size:

 

All PIXIS cameras offer 99% fill factors

Larger pixels offer higher well capacity

Smaller pixels offer higher spatial resolution in some cases; for more information, see hyperlink to IsoPlane page

 

Peak QE:

 

Maximum values of quantum efficiency (QE) are n at 25° C.

 

產(chǎn)品應(yīng)用

Tip-Enhanced Raman Spectroscopy

TERS - Tip-Enhanced Raman spectroscopy

 

Fluorescence, Phosphorescence, and Photoluminescence Spectroscopy

Fluorescence, phosphorescence and photoluminescence occur when a sample is excited by absorbing photons and then emits them with a decay time that is characteristic of the sample environment.

 

Astronomical Imaging

Astronomical imaging can be broadly divided into two categories: (1) steady-state imaging, in which long exposures are required to capture ultra-low-light-level objects, and (2) time-resolved photometry, in which integration times range from milliseconds to a few seconds.

 

General Raman

The most common application of Raman spectroscopy involves the vibrational energy levels of a molecule. Incident laser light in the UV, visible or NIR, is scattered from molecular vibrational modes.

 

Surface-Enhanced Raman Spectroscopy

SERS - Surface-enhanced Raman spectroscopy

 

Bose-Einstein Condensate

Bose-Einstein condensate (BEC) can be regarded as matter made from matter waves. It is formed when a gas composed of a certain kind of particles, referred to as “bosonic” particles, is cooled very close to absolute zero.

 

Coherent Anti-Stokes Raman Spectroscopy

Coherent Anti-Stokes Raman spectroscopy (CARS) a type of non-linear Raman spectroscopy. Instead of the traditional single laser, two very strong collinear lasers irradiate a sample.

 

Stimulated Raman Scattering

Stimulated Raman scattering takes place when an excess of Stokes photons that were previously generated by normal Raman scattering are present or are deliberately added to the excitation beam.

 

Micro-Computed Tomography

Micro Computer Tomography is a unique technique for the noninvasive, nondestructive 3D characterization of materials down to a micrometer scale.

 


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