CATCH: chasing all transients constellation hunters space mission

Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunt...
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Autor*in:	Li, Panping [verfasserIn] Yin, Qian-Qing Li, Zhengwei Tao, Lian Wen, Xiangyang Zhang, Shuang-Nan Qi, Liqiang Zhang, Juan Zhao, Donghua Li, Dalin Yu, Xizheng Bu, Qingcui Chen, Wen Chen, Yupeng Huang, Yiming Huang, Yue Jin, Ge Li, Gang Liu, Hongbang Liu, Xiaojing Ma, Ruican Peng, Wenxi Tang, Ruijing Wang, Yusa Xiao, Jingyu Xiong, Shaolin Yang, Sheng Yang, Yanji Zhang, Chen Zhang, Tianchong Zhang, Liang Zhang, Xuan Zhao, Haisheng Zhao, Kang Zhao, Qingchang Zhao, Shujie Zhou, Xing

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Astronomy X-ray constellation Follow-up observations Time-domain astronomy

Anmerkung:	© The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.

Übergeordnetes Werk:	Enthalten in: Experimental astronomy - Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989, 55(2023), 2 vom: 06. Jan., Seite 447-486
Übergeordnetes Werk:	volume:55 ; year:2023 ; number:2 ; day:06 ; month:01 ; pages:447-486

Links:	Volltext

DOI / URN:	10.1007/s10686-022-09879-0

Katalog-ID:	SPR050002546

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700	1		\|a Zhao, Haisheng \|4 aut
700	1		\|a Zhao, Kang \|4 aut
700	1		\|a Zhao, Qingchang \|4 aut
700	1		\|a Zhao, Shujie \|4 aut
700	1		\|a Zhou, Xing \|4 aut
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allfields	10.1007/s10686-022-09879-0 doi (DE-627)SPR050002546 (SPR)s10686-022-09879-0-e DE-627 ger DE-627 rakwb eng Li, Panping verfasserin aut CATCH: chasing all transients constellation hunters space mission 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. Astronomy X-ray constellation (dpeaa)DE-He213 Follow-up observations (dpeaa)DE-He213 Time-domain astronomy (dpeaa)DE-He213 Yin, Qian-Qing aut Li, Zhengwei aut Tao, Lian aut Wen, Xiangyang aut Zhang, Shuang-Nan aut Qi, Liqiang aut Zhang, Juan aut Zhao, Donghua aut Li, Dalin aut Yu, Xizheng aut Bu, Qingcui aut Chen, Wen aut Chen, Yupeng aut Huang, Yiming aut Huang, Yue aut Jin, Ge aut Li, Gang aut Liu, Hongbang aut Liu, Xiaojing aut Ma, Ruican aut Peng, Wenxi aut Tang, Ruijing aut Wang, Yusa aut Xiao, Jingyu aut Xiong, Shaolin aut Yang, Sheng aut Yang, Yanji aut Zhang, Chen aut Zhang, Tianchong aut Zhang, Liang aut Zhang, Xuan aut Zhao, Haisheng aut Zhao, Kang aut Zhao, Qingchang aut Zhao, Shujie aut Zhou, Xing aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 55(2023), 2 vom: 06. Jan., Seite 447-486 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:55 year:2023 number:2 day:06 month:01 pages:447-486 https://dx.doi.org/10.1007/s10686-022-09879-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 55 2023 2 06 01 447-486
spelling	10.1007/s10686-022-09879-0 doi (DE-627)SPR050002546 (SPR)s10686-022-09879-0-e DE-627 ger DE-627 rakwb eng Li, Panping verfasserin aut CATCH: chasing all transients constellation hunters space mission 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. Astronomy X-ray constellation (dpeaa)DE-He213 Follow-up observations (dpeaa)DE-He213 Time-domain astronomy (dpeaa)DE-He213 Yin, Qian-Qing aut Li, Zhengwei aut Tao, Lian aut Wen, Xiangyang aut Zhang, Shuang-Nan aut Qi, Liqiang aut Zhang, Juan aut Zhao, Donghua aut Li, Dalin aut Yu, Xizheng aut Bu, Qingcui aut Chen, Wen aut Chen, Yupeng aut Huang, Yiming aut Huang, Yue aut Jin, Ge aut Li, Gang aut Liu, Hongbang aut Liu, Xiaojing aut Ma, Ruican aut Peng, Wenxi aut Tang, Ruijing aut Wang, Yusa aut Xiao, Jingyu aut Xiong, Shaolin aut Yang, Sheng aut Yang, Yanji aut Zhang, Chen aut Zhang, Tianchong aut Zhang, Liang aut Zhang, Xuan aut Zhao, Haisheng aut Zhao, Kang aut Zhao, Qingchang aut Zhao, Shujie aut Zhou, Xing aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 55(2023), 2 vom: 06. Jan., Seite 447-486 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:55 year:2023 number:2 day:06 month:01 pages:447-486 https://dx.doi.org/10.1007/s10686-022-09879-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 55 2023 2 06 01 447-486
allfields_unstemmed	10.1007/s10686-022-09879-0 doi (DE-627)SPR050002546 (SPR)s10686-022-09879-0-e DE-627 ger DE-627 rakwb eng Li, Panping verfasserin aut CATCH: chasing all transients constellation hunters space mission 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. Astronomy X-ray constellation (dpeaa)DE-He213 Follow-up observations (dpeaa)DE-He213 Time-domain astronomy (dpeaa)DE-He213 Yin, Qian-Qing aut Li, Zhengwei aut Tao, Lian aut Wen, Xiangyang aut Zhang, Shuang-Nan aut Qi, Liqiang aut Zhang, Juan aut Zhao, Donghua aut Li, Dalin aut Yu, Xizheng aut Bu, Qingcui aut Chen, Wen aut Chen, Yupeng aut Huang, Yiming aut Huang, Yue aut Jin, Ge aut Li, Gang aut Liu, Hongbang aut Liu, Xiaojing aut Ma, Ruican aut Peng, Wenxi aut Tang, Ruijing aut Wang, Yusa aut Xiao, Jingyu aut Xiong, Shaolin aut Yang, Sheng aut Yang, Yanji aut Zhang, Chen aut Zhang, Tianchong aut Zhang, Liang aut Zhang, Xuan aut Zhao, Haisheng aut Zhao, Kang aut Zhao, Qingchang aut Zhao, Shujie aut Zhou, Xing aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 55(2023), 2 vom: 06. Jan., Seite 447-486 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:55 year:2023 number:2 day:06 month:01 pages:447-486 https://dx.doi.org/10.1007/s10686-022-09879-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 55 2023 2 06 01 447-486
allfieldsGer	10.1007/s10686-022-09879-0 doi (DE-627)SPR050002546 (SPR)s10686-022-09879-0-e DE-627 ger DE-627 rakwb eng Li, Panping verfasserin aut CATCH: chasing all transients constellation hunters space mission 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. Astronomy X-ray constellation (dpeaa)DE-He213 Follow-up observations (dpeaa)DE-He213 Time-domain astronomy (dpeaa)DE-He213 Yin, Qian-Qing aut Li, Zhengwei aut Tao, Lian aut Wen, Xiangyang aut Zhang, Shuang-Nan aut Qi, Liqiang aut Zhang, Juan aut Zhao, Donghua aut Li, Dalin aut Yu, Xizheng aut Bu, Qingcui aut Chen, Wen aut Chen, Yupeng aut Huang, Yiming aut Huang, Yue aut Jin, Ge aut Li, Gang aut Liu, Hongbang aut Liu, Xiaojing aut Ma, Ruican aut Peng, Wenxi aut Tang, Ruijing aut Wang, Yusa aut Xiao, Jingyu aut Xiong, Shaolin aut Yang, Sheng aut Yang, Yanji aut Zhang, Chen aut Zhang, Tianchong aut Zhang, Liang aut Zhang, Xuan aut Zhao, Haisheng aut Zhao, Kang aut Zhao, Qingchang aut Zhao, Shujie aut Zhou, Xing aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 55(2023), 2 vom: 06. Jan., Seite 447-486 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:55 year:2023 number:2 day:06 month:01 pages:447-486 https://dx.doi.org/10.1007/s10686-022-09879-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 55 2023 2 06 01 447-486
allfieldsSound	10.1007/s10686-022-09879-0 doi (DE-627)SPR050002546 (SPR)s10686-022-09879-0-e DE-627 ger DE-627 rakwb eng Li, Panping verfasserin aut CATCH: chasing all transients constellation hunters space mission 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. Astronomy X-ray constellation (dpeaa)DE-He213 Follow-up observations (dpeaa)DE-He213 Time-domain astronomy (dpeaa)DE-He213 Yin, Qian-Qing aut Li, Zhengwei aut Tao, Lian aut Wen, Xiangyang aut Zhang, Shuang-Nan aut Qi, Liqiang aut Zhang, Juan aut Zhao, Donghua aut Li, Dalin aut Yu, Xizheng aut Bu, Qingcui aut Chen, Wen aut Chen, Yupeng aut Huang, Yiming aut Huang, Yue aut Jin, Ge aut Li, Gang aut Liu, Hongbang aut Liu, Xiaojing aut Ma, Ruican aut Peng, Wenxi aut Tang, Ruijing aut Wang, Yusa aut Xiao, Jingyu aut Xiong, Shaolin aut Yang, Sheng aut Yang, Yanji aut Zhang, Chen aut Zhang, Tianchong aut Zhang, Liang aut Zhang, Xuan aut Zhao, Haisheng aut Zhao, Kang aut Zhao, Qingchang aut Zhao, Shujie aut Zhou, Xing aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 55(2023), 2 vom: 06. Jan., Seite 447-486 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:55 year:2023 number:2 day:06 month:01 pages:447-486 https://dx.doi.org/10.1007/s10686-022-09879-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 55 2023 2 06 01 447-486
language	English
source	Enthalten in Experimental astronomy 55(2023), 2 vom: 06. Jan., Seite 447-486 volume:55 year:2023 number:2 day:06 month:01 pages:447-486
sourceStr	Enthalten in Experimental astronomy 55(2023), 2 vom: 06. Jan., Seite 447-486 volume:55 year:2023 number:2 day:06 month:01 pages:447-486
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Astronomy X-ray constellation Follow-up observations Time-domain astronomy
isfreeaccess_bool	false
container_title	Experimental astronomy
authorswithroles_txt_mv	Li, Panping @@aut@@ Yin, Qian-Qing @@aut@@ Li, Zhengwei @@aut@@ Tao, Lian @@aut@@ Wen, Xiangyang @@aut@@ Zhang, Shuang-Nan @@aut@@ Qi, Liqiang @@aut@@ Zhang, Juan @@aut@@ Zhao, Donghua @@aut@@ Li, Dalin @@aut@@ Yu, Xizheng @@aut@@ Bu, Qingcui @@aut@@ Chen, Wen @@aut@@ Chen, Yupeng @@aut@@ Huang, Yiming @@aut@@ Huang, Yue @@aut@@ Jin, Ge @@aut@@ Li, Gang @@aut@@ Liu, Hongbang @@aut@@ Liu, Xiaojing @@aut@@ Ma, Ruican @@aut@@ Peng, Wenxi @@aut@@ Tang, Ruijing @@aut@@ Wang, Yusa @@aut@@ Xiao, Jingyu @@aut@@ Xiong, Shaolin @@aut@@ Yang, Sheng @@aut@@ Yang, Yanji @@aut@@ Zhang, Chen @@aut@@ Zhang, Tianchong @@aut@@ Zhang, Liang @@aut@@ Zhang, Xuan @@aut@@ Zhao, Haisheng @@aut@@ Zhao, Kang @@aut@@ Zhao, Qingchang @@aut@@ Zhao, Shujie @@aut@@ Zhou, Xing @@aut@@
publishDateDaySort_date	2023-01-06T00:00:00Z
hierarchy_top_id	312841116
id	SPR050002546
language_de	englisch
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author	Li, Panping
spellingShingle	Li, Panping misc Astronomy X-ray constellation misc Follow-up observations misc Time-domain astronomy CATCH: chasing all transients constellation hunters space mission
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topic_title	CATCH: chasing all transients constellation hunters space mission Astronomy X-ray constellation (dpeaa)DE-He213 Follow-up observations (dpeaa)DE-He213 Time-domain astronomy (dpeaa)DE-He213
topic	misc Astronomy X-ray constellation misc Follow-up observations misc Time-domain astronomy
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title	CATCH: chasing all transients constellation hunters space mission
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title_full	CATCH: chasing all transients constellation hunters space mission
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author_browse	Li, Panping Yin, Qian-Qing Li, Zhengwei Tao, Lian Wen, Xiangyang Zhang, Shuang-Nan Qi, Liqiang Zhang, Juan Zhao, Donghua Li, Dalin Yu, Xizheng Bu, Qingcui Chen, Wen Chen, Yupeng Huang, Yiming Huang, Yue Jin, Ge Li, Gang Liu, Hongbang Liu, Xiaojing Ma, Ruican Peng, Wenxi Tang, Ruijing Wang, Yusa Xiao, Jingyu Xiong, Shaolin Yang, Sheng Yang, Yanji Zhang, Chen Zhang, Tianchong Zhang, Liang Zhang, Xuan Zhao, Haisheng Zhao, Kang Zhao, Qingchang Zhao, Shujie Zhou, Xing
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doi_str_mv	10.1007/s10686-022-09879-0
title_sort	catch: chasing all transients constellation hunters space mission
title_auth	CATCH: chasing all transients constellation hunters space mission
abstract	Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
abstractGer	Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
abstract_unstemmed	Abstract In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabilities. We have thus proposed an intelligent X-ray constellation, the Chasing All Transients Constellation Hunters (CATCH) space mission. Consisting of 126 micro-satellites in three types, CATCH will have the capability to perform follow-up observations for a large number of different types of transients simultaneously. Each satellite in the constellation will carry lightweight X-ray optics and use a deployable mast to increase the focal length. The combination of different optics and detector systems enables different types of satellites to have multiform observation capabilities, including timing, spectroscopy, imaging, and polarization. Controlled by the intelligent system, different satellites can cooperate to perform uninterrupted monitoring, all-sky follow-up observations, and scanning observations with a flexible field of view (FOV) and multi-dimensional observations. Therefore, CATCH will be a powerful mission to study the dynamic universe. Here, we present the current design of the spacecraft, optics, detector system, constellation configuration and observing modes, as well as the development plan. © The Author(s), under exclusive licence to Springer Nature B.V. 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
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title_short	CATCH: chasing all transients constellation hunters space mission
url	https://dx.doi.org/10.1007/s10686-022-09879-0
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author2	Yin, Qian-Qing Li, Zhengwei Tao, Lian Wen, Xiangyang Zhang, Shuang-Nan Qi, Liqiang Zhang, Juan Zhao, Donghua Li, Dalin Yu, Xizheng Bu, Qingcui Chen, Wen Chen, Yupeng Huang, Yiming Huang, Yue Jin, Ge Li, Gang Liu, Hongbang Liu, Xiaojing Ma, Ruican Peng, Wenxi Tang, Ruijing Wang, Yusa Xiao, Jingyu Xiong, Shaolin Yang, Sheng Yang, Yanji Zhang, Chen Zhang, Tianchong Zhang, Liang Zhang, Xuan Zhao, Haisheng Zhao, Kang Zhao, Qingchang Zhao, Shujie Zhou, Xing
author2Str	Yin, Qian-Qing Li, Zhengwei Tao, Lian Wen, Xiangyang Zhang, Shuang-Nan Qi, Liqiang Zhang, Juan Zhao, Donghua Li, Dalin Yu, Xizheng Bu, Qingcui Chen, Wen Chen, Yupeng Huang, Yiming Huang, Yue Jin, Ge Li, Gang Liu, Hongbang Liu, Xiaojing Ma, Ruican Peng, Wenxi Tang, Ruijing Wang, Yusa Xiao, Jingyu Xiong, Shaolin Yang, Sheng Yang, Yanji Zhang, Chen Zhang, Tianchong Zhang, Liang Zhang, Xuan Zhao, Haisheng Zhao, Kang Zhao, Qingchang Zhao, Shujie Zhou, Xing
ppnlink	312841116
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doi_str	10.1007/s10686-022-09879-0
up_date	2024-07-04T03:05:01.200Z
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