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QHY-174M-GPS Camera as the Device for Photometry of Artificial Satellites Cover

QHY-174M-GPS Camera as the Device for Photometry of Artificial Satellites

By:  and    
Open Access
|Apr 2022

Figures & Tables

Table 1.

QHY-174M GPS CMOS camera characteristics

ModelQHY174GPS M
SensorSONY IMX174 CMOS
Pixel Size5.86 μm ×5.86 μm
Effective Pixel Area1920 × 1200
Effective Image Area11.25mm×7.03mm
QE78%
AD Sample Depth12/10bit (output as 16bit and 8bit)
Frame Rate138FPS@1936×1216, 260FPS@960×600
Readout Noise5.3e-@Gain0% 2.8e-@Gain60% 1.6e-@Gain100%
Exposure Time Rangefrom 5 μs to 900 sec
Binning1×1,2×2
Anti-Glow ControlYes (Reduces amplifier glow significantly)
Shutter TypeElectric Global Shutter
Computer InterfaceUSB 3.0 Super Speed
Cooling SystemDual Stage TEC cooler (-40C below ambient)
Time-Stamp Precision1 micro-second of the GPS UTC clock
Figure 1.

QHY-174M GPS CMOS camera (left) and view of the camera with GPS antenna (right)

Table 2.

The goodness of star profile fit with different functions

FunctionGaussLorentzMoffat
R20.86230.91660.9477
Figure 2.

Left: star profile with Moffat 2D function fit (red). Right: Residuals.

Table 3.

Selected standard stars from Landolt catalogue

Star NamemVmRV-RSpTypeStar NamemVmRV-RSpType
SA 112 2759.9059.2580.647K2DSA 113 36613.53712.9140.623–
SA 112 59511.35210.4530.899K2:III DSA 113 17713.56013.1040.456–
SA 112 22311.42411.1510.273F5DSA 113 19513.69213.2740.418–
SA 112 70411.45210.6300.822–SA 113 27213.90413.5340.370–
SA 112 82211.54910.9910.558G8:IIIDSA 113 30714.21413.5840.630–
SA 112 80512.08612.0230.063A0DSA 113 18214.37013.9680.402–
SA 112 25012.09511.7780.317F8DSA 114 1769.2398.4390.800K4/5E
SA 113 46610.0049.7230.281F5DSA 114 67011.10110.4560.645K1.5:IIID
SA 113 47510.3069.7360.570G5DSA 114 54811.60110.8630.738K2D
SA 113 34210.87810.3410.537–SA 114 65411.83311.4650.368G0D
SA 113 15611.22410.9210.303–SA 114 75011.91611.8890.027B9D
SA 113 25911.74211.1210.621K0:III DSA 114 44612.06411.6670.397–
SA 113 49311.76711.3370.430G5DSA 114 65612.64412.0970.547K1:IIID
SA 113 44011.79611.4330.363–SA 115 2719.6959.3420.353F8D
SA 113 45912.12511.8180.307–SA 115 51610.4349.8710.563G8IVD
SA 113 49212.17411.8320.342G0ESA 115 42011.16110.8750.286F5D
SA 113 33912.25011.9100.340F8DSA 115 55411.81211.2260.586K1.5:IIIC
SA 113 19112.33711.8660.471–SA 115 41212.20911.8820.327–
SA 113 49512.43711.9250.512G:DSA 115 26812.49412.1280.366–
SA 113 15813.11612.7090.407–
Figure 3.

Example of FITS files to process. Object is in the centre of the frame and its shape is point, the stars have trail shape.

Figure 4.

Logical diagram of the satellite photometry script

Figure 5.

Part of LC of Topex/Poseidon artificial satellite (NORAD 22076) observed at Derenivka station on Aug 06 2020 in R filter. Time of exposition 0.2 sec. Photometry errors are 0.006 ÷ 0.040 mag.

Figure 6.

Top: Observations of satellite COSMOS 2502 (NORAD 40358) from two observational sites - Uzhhoorod in B,V filters with use of photo-multiplier (blue and green lines), Derenivka in R filter with QHY174M-GPS camera (red line).

Observation made on Nov 09 2020. Bottom: Colour indexes B-V, V-R and B-R

DOI: https://doi.org/10.2478/arsa-2022-0003 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859 (formerly 0208-841X)
Language: English
Page range: 47 - 57
Submitted on: Apr 14, 2021
Accepted on: Jan 31, 2022
Published on: Apr 22, 2022
Published by: Polish Academy of Sciences, Space Research Centre
In partnership with: Paradigm Publishing Services

© 2022 Viktor Kudak, Vasyl Perig, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons Attribution 4.0 License.