Expected characteristics of data from the LYRA mission
The purpose of the LYRA mission is a multi‐color all‐sky survey of objects from 3m to 16m from the International Space Station, to result in a high‐precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.001–0.003m for stars brighter than 12m and 0.01m for...
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| Published in: | Astronomische Nachrichten Vol. 334; no. 8; pp. 828 - 831 |
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| Abstract | The purpose of the LYRA mission is a multi‐color all‐sky survey of objects from 3m to 16m from the International Space Station, to result in a high‐precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.001–0.003m for stars brighter than 12m and 0.01m for the stars down to 16m. The estimated duration of the survey is about 5 years. This paper describes the characteristics of data to be received in the course of the LYRA experiment for future users. (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) |
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| AbstractList | The purpose of the LYRA mission is a multi‐color all‐sky survey of objects from 3
m
to 16
m
from the International Space Station, to result in a high‐precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.001–0.003
m
for stars brighter than 12
m
and 0.01
m
for the stars down to 16
m
. The estimated duration of the survey is about 5 years. This paper describes the characteristics of data to be received in the course of the LYRA experiment for future users. (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) The purpose of the LYRA mission is a multi-color all-sky survey of objects from 3m to 16m from the International Space Station, to result in a high-precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.001-0.003m for stars brighter than 12m and 0.01m for the stars down to 16m. The estimated duration of the survey is about 5 years. This paper describes the characteristics of data to be received in the course of the LYRA experiment for future users. (© 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim) [PUBLICATION ABSTRACT] The purpose of the LYRA mission is a multi‐color all‐sky survey of objects from 3m to 16m from the International Space Station, to result in a high‐precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.001–0.003m for stars brighter than 12m and 0.01m for the stars down to 16m. The estimated duration of the survey is about 5 years. This paper describes the characteristics of data to be received in the course of the LYRA experiment for future users. (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) The purpose of the LYRA mission is a multi-color all-sky survey of objects from 3 super(m) to 16 super(m) from the International Space Station, to result in a high-precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.001-0.003 super(m) for stars brighter than 12 super(m) and 0.01 super(m) for the stars down to 16 super(m). The estimated duration of the survey is about 5 years. This paper describes the characteristics of data to be received in the course of the LYRA experiment for future users. ([copy 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim) |
| Author | Mironov, A.V. Nikolaev, F.N. Tuchin, M.S. Zakharov, A.I. Prokhorov, M.E. Biryukov, A.V. |
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| References | Skrutskie, M.F., Cutri, R.M., Stiening, R., et al. 2006, AJ, 131, 1163 Zakharov, A.I., Mironov, A.V., Prokhorov, M.E., et al. 2013b, Astronomy Reports, 57 195 Kornilov, V.G., Volkov, I.M., Zakharov, A.I., et al. 1991, Trudy Gosud. Astron. Sternberga (Proc. of the Sternberg Astron. Inst.), 63, 1 Johnson, H.L., & Morgan, W.W. 1953, ApJ, 117, 313 Zakharov, A.I., Mironov, A.V., Nikolaev, F.N., Prokhorov, M.E., & Tuchin, M.S. 2013a, Astron. Nachr., 334 823 Monet, D.G., Levine, S.E., Casian, B., et al. 2003, AJ, 125, 984 1953; 117 2006; 131 2005 2013a; 334 2013b; 57 2003; 125 1991; 63 e_1_2_1_7_1 e_1_2_1_8_1 e_1_2_1_5_1 e_1_2_1_6_1 e_1_2_1_4_1 e_1_2_1_2_1 Kornilov V.G. (e_1_2_1_3_1) 1991; 63 |
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| Snippet | The purpose of the LYRA mission is a multi‐color all‐sky survey of objects from 3m to 16m from the International Space Station, to result in a high‐precision... The purpose of the LYRA mission is a multi‐color all‐sky survey of objects from 3 m to 16 m from the International Space Station, to result in a high‐precision... The purpose of the LYRA mission is a multi-color all-sky survey of objects from 3m to 16m from the International Space Station, to result in a high-precision... The purpose of the LYRA mission is a multi-color all-sky survey of objects from 3 super(m) to 16 super(m) from the International Space Station, to result in a... |
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| SubjectTerms | Astronomical bodies Astronomy Errors instrumentation: photometers International Space Station Missions Photometry Reproduction Space stations Stars Stars & galaxies stars: fundamental parameters surveys techniques: photometric telescopes |
| Title | Expected characteristics of data from the LYRA mission |
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