scholarly journals Two Dimensional Interferometric Photon Counting Observations with the 6m Telescope

1982 ◽  
Vol 67 ◽  
pp. 223-227
Author(s):  
J. Boulesteix ◽  
Y. Georgelin ◽  
M. Marcelin ◽  
J.A. Fort

This detector has been in use since 1977. Following Labeyrie (1977), it consists of a microchannel plate electrostatically focussed intensifier (TH 9304) coupled by fiber optics to an SIT camera (TH 9655), these parts being manufactured by THOMSON-CSF (FRANCE). The diameter of the S20 photocathode is 25mm but the silicon target is only 18mm wide. The scanning electronics are conventional. The detector is cooled to -5°C, the photocathode being in a dry nitrogen chamber. The system has been described by Boulesteix (1978).

1986 ◽  
Vol 118 ◽  
pp. 71-74
Author(s):  
Sueo Miyaki ◽  
Syuzo Isobe ◽  
Nobuo Shinchara

A system with an electronomulitplier of two-stage microchannel plate and a vidicon TV camera is developed for two dimensional photon-counting imaging and is applied for astronomical observations at the Nasmyth focus of the 75cm alt-az telescope of the Sundai Observatory at Kita-Karuizawa (SOK). Some test results are shown here.


1999 ◽  
Vol 42 (3) ◽  
pp. 237-246 ◽  
Author(s):  
Yu. N. Kul'chin ◽  
O. B. Vitrik ◽  
O. V. Kirichenko

1999 ◽  
Vol 93 (2) ◽  
pp. 163-168 ◽  
Author(s):  
Masaki Kobayashi ◽  
Motohiro Takeda ◽  
Ken-Ichi Ito ◽  
Hiroshi Kato ◽  
Humio Inaba

2011 ◽  
Vol 54 (11) ◽  
pp. 1943-1947 ◽  
Author(s):  
Hao Yang ◽  
BaoSheng Zhao ◽  
QiuRong Yan ◽  
YongAn Liu ◽  
HuiJun Hu

2021 ◽  
Vol 16 (12) ◽  
pp. C12014
Author(s):  
M. Zoladz ◽  
P. Grybos ◽  
R. Szczygiel

Abstract X-ray imaging of moving objects using line detectors remains the most popular method of object content and structure examination with a typical resolution limited to 0.4–1 mm. Higher resolutions are difficult to obtain as, for the detector in the form of a single pixel row, the narrower the detector is, the lower the image Signal to Noise Ratio (SNR). This is because, for smaller pixel sizes, fewer photons hit the pixel in each time unit for a given radiation intensity. To overcome the trade-off between the SNR and spatial resolution, a two-dimensional sensor, namely a pixel matrix can be used. Imaging of moving objects with a pixel matrix requires time-domain integration (TDI). Straightforward TDI implementation is based on the proper accumulation of images acquired during consecutive phases of an object’s movement. Unfortunately, this method is much more demanding regarding data transfer and processing. Data from the whole pixel matrix instead of a single pixel row must be transferred out of the chip and then processed. The alternative approach is on-chip TDI implementation. It takes advantage of photons acquired by multiple rows (a higher SNR), but generates similar data amount as a single pixel row and does not require data processing out of the chip. In this paper, on-chip TDI is described and verified by using a single photon counting two-dimensional (a matrix of 128 × 192 pixels) CdTe hybrid X-ray detector with the 100 µm × 100 µm pixel size with up to four energy thresholds per pixel. Spatial resolution verification is combined with the Material Discrimination X-ray (MDX) imaging method.


1989 ◽  
Vol 131 ◽  
pp. 182-182
Author(s):  
Luciana Bianchi ◽  
Michael Greving ◽  
J. Barnstedt ◽  
Chr. Diesch

We present newly determined expansion velocities for a number of Planetary Nebulae (PNe) which have been observed with the ESO 1.4m CAT and the Coude' Echelle Spectrograph (CES), operated at a r.p. of 105, corresponding to a resolution of about 3km/s at Hα. Two detector systems have been used: the standard ESO Reticon and a two-dimensional photon-counting imaging detector developed at the A.I.T. (AIT-MCP-Camera).


2006 ◽  
Author(s):  
Toru Aoki ◽  
Hisashi Morii ◽  
Gosuke Ohashi ◽  
Yasuhiro Tomita ◽  
Yoshinori Hatanaka

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