• Optics and Precision Engineering
  • Vol. 31, Issue 6, 793 (2023)
Bingli NIU1,2, Zhe KANG1,2,*, Zhenwei LI1,2, You LÜ1, and Chengzhi LIU1,2,*
Author Affiliations
  • 1Changchun Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Changchun307, China
  • 2University of Chinese Academy of Sciences, Beijing100049, China
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    DOI: 10.37188/OPE.20233106.0793 Cite this Article
    Bingli NIU, Zhe KANG, Zhenwei LI, You LÜ, Chengzhi LIU. Simultaneous three-channel photometric system of 1.2 m photoelectric telescope[J]. Optics and Precision Engineering, 2023, 31(6): 793 Copy Citation Text show less
    Simultaneous three-channel photometric system of the 1.2 m photoelectric telescope
    Fig. 1. Simultaneous three-channel photometric system of the 1.2 m photoelectric telescope
    Optical path of the whole and each channel of the simultaneous three-channel photometric system
    Fig. 2. Optical path of the whole and each channel of the simultaneous three-channel photometric system
    Spot diagram of three channels
    Fig. 3. Spot diagram of three channels
    Modulation transfer function of three channels
    Fig. 4. Modulation transfer function of three channels
    Fraction of enclosed energy curves of three channels
    Fig. 5. Fraction of enclosed energy curves of three channels
    Original images of BD+174708 left panel: the original image of the g' channel, with an FOV of 21.5′×21.5′; middle panel: the original image of the r' channel, with an FOV of 21.5′×21.5′; right panel: the original image of the i' channel, with an FOV of 21.3′×21.3′
    Fig. 6. Original images of BD+174708 left panel: the original image of the g' channel, with an FOV of 21.5′×21.5′; middle panel: the original image of the r' channel, with an FOV of 21.5′×21.5′; right panel: the original image of the i' channel, with an FOV of 21.3′×21.3′
    Degradations in optical quality along the off angle direction in the three channels
    Fig. 7. Degradations in optical quality along the off angle direction in the three channels
    Optical elementChannel
    g′r′i′
    Reflector M3Reflectance0.8910.940.92
    Transmittance------
    Transmittance due to material absorption loss------
    Reflector M4Reflectance0.8910.940.92
    Transmittance------
    Transmittance due to material absorption loss------
    Reflector M5Reflectance0.8910.940.92
    Transmittance------
    Transmittance due to material absorption loss------
    Field lensReflectance------
    Transmittance0.940.950.93
    Transmittance due to material absorption loss0.020.020.02
    First beam-splitting lensReflectance0.98----
    Transmittance--0.910.95
    Transmittance due to material absorption loss--0.020.02
    Second beam-splitting lensReflectance--0.90--
    Transmittance----0.95
    Transmittance due to material absorption loss----0.02
    Imaging lens groupReflectance------
    Transmittance0.9270.910.93
    Transmittance due to material absorption loss0.040.040.04
    FiltersReflectance------
    Transmittance0.950.970.95
    Transmittance due to material absorption loss0.020.020.02
    Total optical transmittance0.5290.5150.511
    Table 1. Optical transmittance of optical components in each channel of the photometer
    Star nameR.A.(J2000)Dec.(J2000)V magColor index
    B-VU-BV-RR-I
    SA92-34200:55:10+00:43:1411.6130.436-0.0420.2660.270
    SA92-26300:55:40+00:36:1811.7821.0480.8430.5630.522
    SA93-31701:54:38+00:43:0011.5460.488-0.0550.2930.298
    SA93-33301:55:05+00:45:4412.0110.8320.4360.4690.422
    GCRV 575708:44:05+36:14:4310.8330.739-0.1000.3850.362
    SA100-24108:52:35-00:39:4810.1390.1570.1010.0780.085
    SA101-31509:54:51-00:27:2811.2491.1531.0560.6120.559
    SA101-31609:54:52-00:18:3211.5520.4930.0320.2930.291
    Feige 3410:39:36+43:06:0911.362-0.435-1.277-0.158-0.137
    Ross 10610:50:28+56:26:3112.4460.779-0.0780.4110.386
    SA102-62010:55:06-00:48:1910.0691.0831.0200.6420.524
    Wolf 36511:11:00+06:25:1111.1810.9420.0410.4780.447
    SA113-26021:41:48+00:23:5212.4060.5140.0690.3080.298
    SA113-47521:41:51+00:39:1910.3061.0580.8440.5700.527
    SA115-55423:41:31+01:26:2611.8121.0050.5480.5860.538
    SA115-48623:41:33+01:16:4512.4820.493-0.0490.2980.308
    Table 2. Landolt standard stars used in the research
    Star nameR.A.(J2000)Dec.(J2000)r′magColor index
    u′-g′g′-r′r′-i′i′-z′
    Hilt 3100:28:11.15+64:07:51.810.9960.9990.5870.2940.147
    BD+71003100:43:44.34+72:10:43.110.0910.8960.2600.0790.007
    SA95-19003:53:13.24+00:16:22.812.5931.3000.1260.0020.043
    SA95-19303:53:20.59+00:16:34.713.8442.4891.0970.4070.214
    SA97-28405:58:25.02+00:05:13.510.2992.6411.1550.5210.320
    SA97-28805:58:30.09+00:06:40.710.7181.3310.4010.1060.013
    BD+75032508:10:49.50+74:57:57.89.786-0.508-0.514-0.382-0.323
    BD+54121608:19:22.56+54:05:09.79.5860.8900.3000.1070.010
    BD+9219009:29:15.55+08:38:00.611.0490.9020.2380.0760.009
    Ross88909:40:43.19+01:00:29.510.3800.8750.2200.0680.006
    BD+29209110:47:23.16+28:23:56.010.1230.8640.3660.1320.040
    Feige6612:37:23.52+25:03:59.910.747-0.345-0.476-0.367-0.316
    BD+17470822:11:31.37+18:05:34.19.3500.9200.2900.1000.020
    SA114-53122:40:36.78+00:51:55.611.8801.4190.5400.1870.080
    SA114-65422:41:26.14+01:10:10.711.6721.3980.4490.1370.040
    SA115-42023:42:36.48+01:05:58.811.0631.0910.2900.0800.007
    SA115-51623:44:15.38+01:14:12.510.1072.1670.8070.3170.172
    Table 3. SDSS standard stars used in the research
    EtotalE1.2mEphotometer
    g′30.346.265.6
    r′28.541.768.3
    i′31.950.163.7
    Table 4. Efficiency of three-channel photometric system
    Channelg′r′i′
    2020.1215.4616.8915.93
    2021.0315.3316.5615.71
    2021.0415.0515.8815.36
    2021.1115.1916.2215.51
    Mean value15.2616.3915.63
    Table 5. Limiting magnitude of three-channel photometric system
    Bingli NIU, Zhe KANG, Zhenwei LI, You LÜ, Chengzhi LIU. Simultaneous three-channel photometric system of 1.2 m photoelectric telescope[J]. Optics and Precision Engineering, 2023, 31(6): 793
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