É. Artigau, F. Bouchy, R. Doyon, C. Melo, X. Delfosse, F. Wildi, C. Lovis, P. Figueira, B. C. Martins, J. González-Hernández, S. Thibault, V. Reshetov, F. Pepe, N. Santos, J. D. Medeiros, R. Rebolo, N. Cook, N. Blind, I. Boisse, D. Brousseau, U. Conod, D. Lafreniére, I. Leão, L. Malo, M. Ouellet, Anne-Sophie Poulin-Girard, S. Udry, P. Vallée, A. Cumming, M. Sordet, A. D. M. Martins
{"title":"NIRPS:状态更新和项目概述","authors":"É. Artigau, F. Bouchy, R. Doyon, C. Melo, X. Delfosse, F. Wildi, C. Lovis, P. Figueira, B. C. Martins, J. González-Hernández, S. Thibault, V. Reshetov, F. Pepe, N. Santos, J. D. Medeiros, R. Rebolo, N. Cook, N. Blind, I. Boisse, D. Brousseau, U. Conod, D. Lafreniére, I. Leão, L. Malo, M. Ouellet, Anne-Sophie Poulin-Girard, S. Udry, P. Vallée, A. Cumming, M. Sordet, A. D. M. Martins","doi":"10.1117/12.2561090","DOIUrl":null,"url":null,"abstract":"NIRPS is a near-infrared (YJH bands), fiber-fed, high-resolution precision radial velocity (pRV) spectrograph currently under construction for deployment at the ESO 3.6-m telescope in La Silla, Chile. Through the use of a dichroic, NIRPS will be operated simultaneously with the optical HARPS pRV spectrograph and will be used to conduct ambitious planet-search and characterization surveys through a 720-night of guaranteed time allocation. NIRPS aims at detecting and characterizing Earth-like planets in the habitable zone of low-mass dwarfs and obtain high-accuracy transit spectroscopy of exoplanets. Here we present a summary of the full performances obtained in laboratory tests conducted at Universite Laval (Canada), and the first results of the on-going on-sky commissioning of the front-end. Science operations of NIRPS is expected to start in late-2020, enabling significant synergies with major space and ground instruments such as the JWST, TESS, ALMA, PLATO and the ELT.","PeriodicalId":215000,"journal":{"name":"Ground-based and Airborne Instrumentation for Astronomy VIII","volume":"31 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"NIRPS: status updates and project overview\",\"authors\":\"É. Artigau, F. Bouchy, R. Doyon, C. Melo, X. Delfosse, F. Wildi, C. Lovis, P. Figueira, B. C. Martins, J. González-Hernández, S. Thibault, V. Reshetov, F. Pepe, N. Santos, J. D. Medeiros, R. Rebolo, N. Cook, N. Blind, I. Boisse, D. Brousseau, U. Conod, D. Lafreniére, I. Leão, L. Malo, M. Ouellet, Anne-Sophie Poulin-Girard, S. Udry, P. Vallée, A. Cumming, M. Sordet, A. D. M. Martins\",\"doi\":\"10.1117/12.2561090\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"NIRPS is a near-infrared (YJH bands), fiber-fed, high-resolution precision radial velocity (pRV) spectrograph currently under construction for deployment at the ESO 3.6-m telescope in La Silla, Chile. Through the use of a dichroic, NIRPS will be operated simultaneously with the optical HARPS pRV spectrograph and will be used to conduct ambitious planet-search and characterization surveys through a 720-night of guaranteed time allocation. NIRPS aims at detecting and characterizing Earth-like planets in the habitable zone of low-mass dwarfs and obtain high-accuracy transit spectroscopy of exoplanets. Here we present a summary of the full performances obtained in laboratory tests conducted at Universite Laval (Canada), and the first results of the on-going on-sky commissioning of the front-end. Science operations of NIRPS is expected to start in late-2020, enabling significant synergies with major space and ground instruments such as the JWST, TESS, ALMA, PLATO and the ELT.\",\"PeriodicalId\":215000,\"journal\":{\"name\":\"Ground-based and Airborne Instrumentation for Astronomy VIII\",\"volume\":\"31 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-12-13\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Ground-based and Airborne Instrumentation for Astronomy VIII\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1117/12.2561090\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Ground-based and Airborne Instrumentation for Astronomy VIII","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2561090","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
NIRPS is a near-infrared (YJH bands), fiber-fed, high-resolution precision radial velocity (pRV) spectrograph currently under construction for deployment at the ESO 3.6-m telescope in La Silla, Chile. Through the use of a dichroic, NIRPS will be operated simultaneously with the optical HARPS pRV spectrograph and will be used to conduct ambitious planet-search and characterization surveys through a 720-night of guaranteed time allocation. NIRPS aims at detecting and characterizing Earth-like planets in the habitable zone of low-mass dwarfs and obtain high-accuracy transit spectroscopy of exoplanets. Here we present a summary of the full performances obtained in laboratory tests conducted at Universite Laval (Canada), and the first results of the on-going on-sky commissioning of the front-end. Science operations of NIRPS is expected to start in late-2020, enabling significant synergies with major space and ground instruments such as the JWST, TESS, ALMA, PLATO and the ELT.
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