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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: Viktor Kudak and  Vasyl Perig  
Open Access
|Apr 2022

Figures & Tables

Figure 1.

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

Figure 2.

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

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.
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
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.
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
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

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

The goodness of star profile fit with different functions

FunctionGaussLorentzMoffat
R20.86230.91660.9477

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 70411.45210.6300.822SA 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 34210.87810.3410.537SA 114 65411.83311.4650.368G0D
SA 113 15611.22410.9210.303SA 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 44011.79611.4330.363SA 115 2719.6959.3420.353F8D
SA 113 45912.12511.8180.307SA 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 19112.33711.8660.471SA 115 41212.20911.8820.327
SA 113 49512.43711.9250.512G:DSA 115 26812.49412.1280.366
SA 113 15813.11612.7090.407
DOI: https://doi.org/10.2478/arsa-2022-0003 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859
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
Publication frequency: 4 issues per year

© 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.