B. Miller, A. Adamson, J. Blakeslee, A. Stephens, J. Thomas-Osip, Arturo Núñez
{"title":"双子座多信使天文学操作","authors":"B. Miller, A. Adamson, J. Blakeslee, A. Stephens, J. Thomas-Osip, Arturo Núñez","doi":"10.22323/1.357.0050","DOIUrl":null,"url":null,"abstract":"Gemini Observatory will be an important facility for following up time-domain discoveries in the multi-messenger era. Gemini has a variety of time allocation processes in order to accommodate a broad range of project needs and timescales. Time is allocated by regular participant TACs, a common large program TAC, and by proposer peer review for \"fast-turnaround\" proposals. Queue observing allows Gemini to easily execute target-of-opportunity (ToO) observations and this capability will be very important for transient follow-up. Instrumentation includes optical and near-infrared imagers and spectrographs at both sites. New facility instruments and systems are under development including GHOST (high-resolution optical spectrograph), SCORPIO (the broad-wavelength follow-up workhorse), and a new multi-conjugate AO system for Gemini North. Visitor instruments are also highly encouraged. All new facility instruments will be delivered with data reduction pipelines and the data are delivered via a cloud-based science archive. Finally, we summarize planned changes to our operations software to handle the expected increased volume of ToO triggers and to incorporate Gemini into the developing time-domain follow-up infrastructure. These changes will include new interfaces, more programmatic access, a real-time scheduler, and automated data reduction.","PeriodicalId":257968,"journal":{"name":"Proceedings of The New Era of Multi-Messenger Astrophysics — PoS(Asterics2019)","volume":"55 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2019-08-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Gemini Operations for Multi-Messenger Astronomy\",\"authors\":\"B. Miller, A. Adamson, J. Blakeslee, A. Stephens, J. Thomas-Osip, Arturo Núñez\",\"doi\":\"10.22323/1.357.0050\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Gemini Observatory will be an important facility for following up time-domain discoveries in the multi-messenger era. Gemini has a variety of time allocation processes in order to accommodate a broad range of project needs and timescales. Time is allocated by regular participant TACs, a common large program TAC, and by proposer peer review for \\\"fast-turnaround\\\" proposals. Queue observing allows Gemini to easily execute target-of-opportunity (ToO) observations and this capability will be very important for transient follow-up. Instrumentation includes optical and near-infrared imagers and spectrographs at both sites. New facility instruments and systems are under development including GHOST (high-resolution optical spectrograph), SCORPIO (the broad-wavelength follow-up workhorse), and a new multi-conjugate AO system for Gemini North. Visitor instruments are also highly encouraged. All new facility instruments will be delivered with data reduction pipelines and the data are delivered via a cloud-based science archive. Finally, we summarize planned changes to our operations software to handle the expected increased volume of ToO triggers and to incorporate Gemini into the developing time-domain follow-up infrastructure. These changes will include new interfaces, more programmatic access, a real-time scheduler, and automated data reduction.\",\"PeriodicalId\":257968,\"journal\":{\"name\":\"Proceedings of The New Era of Multi-Messenger Astrophysics — PoS(Asterics2019)\",\"volume\":\"55 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2019-08-08\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Proceedings of The New Era of Multi-Messenger Astrophysics — PoS(Asterics2019)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.22323/1.357.0050\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of The New Era of Multi-Messenger Astrophysics — PoS(Asterics2019)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22323/1.357.0050","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Gemini Observatory will be an important facility for following up time-domain discoveries in the multi-messenger era. Gemini has a variety of time allocation processes in order to accommodate a broad range of project needs and timescales. Time is allocated by regular participant TACs, a common large program TAC, and by proposer peer review for "fast-turnaround" proposals. Queue observing allows Gemini to easily execute target-of-opportunity (ToO) observations and this capability will be very important for transient follow-up. Instrumentation includes optical and near-infrared imagers and spectrographs at both sites. New facility instruments and systems are under development including GHOST (high-resolution optical spectrograph), SCORPIO (the broad-wavelength follow-up workhorse), and a new multi-conjugate AO system for Gemini North. Visitor instruments are also highly encouraged. All new facility instruments will be delivered with data reduction pipelines and the data are delivered via a cloud-based science archive. Finally, we summarize planned changes to our operations software to handle the expected increased volume of ToO triggers and to incorporate Gemini into the developing time-domain follow-up infrastructure. These changes will include new interfaces, more programmatic access, a real-time scheduler, and automated data reduction.