R. Doyon, F. Bouchy, É. Artigau, O. Hernandez, F. Wildi, C. Melo, P. Vallée, S. Thibault, X. Delfosse, C. Lovis, F. Pepe, P. Figueira, V. Reshetov, N. Santos, L. Malo, M. Ouellet, D. Brousseau, R. Rebolo-López, N. Blind, Uriel Condo, Stéphane Dry, J. G. Hernández, B. Chazelas, B. C. Martins, J. D. Medeiros
{"title":"The near-infrared planet searcher (NIRPS) (Conference Presentation)","authors":"R. Doyon, F. Bouchy, É. Artigau, O. Hernandez, F. Wildi, C. Melo, P. Vallée, S. Thibault, X. Delfosse, C. Lovis, F. Pepe, P. Figueira, V. Reshetov, N. Santos, L. Malo, M. Ouellet, D. Brousseau, R. Rebolo-López, N. Blind, Uriel Condo, Stéphane Dry, J. G. Hernández, B. Chazelas, B. C. Martins, J. D. Medeiros","doi":"10.1117/12.2313050","DOIUrl":null,"url":null,"abstract":"NIRPS (Near Infra Red Planet Searcher) is a new ultra-stable infrared ( YJH) fiber-fed spectrograph that will be installed on ESO’s 3.6-m telescope in La Silla, Chile. Aiming at achieving a precision of 1 m/s, NIRPS is designed to find rocky planets orbiting M dwarfs, and will operate together with HARPS (High Accuracy Radial velocity Planet Searcher). In this paper we describe NIRPS science cases, present its main technical characteristics and its development status.","PeriodicalId":129032,"journal":{"name":"Ground-based and Airborne Instrumentation for Astronomy VII","volume":"68 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2018-07-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Ground-based and Airborne Instrumentation for Astronomy VII","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2313050","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
NIRPS (Near Infra Red Planet Searcher) is a new ultra-stable infrared ( YJH) fiber-fed spectrograph that will be installed on ESO’s 3.6-m telescope in La Silla, Chile. Aiming at achieving a precision of 1 m/s, NIRPS is designed to find rocky planets orbiting M dwarfs, and will operate together with HARPS (High Accuracy Radial velocity Planet Searcher). In this paper we describe NIRPS science cases, present its main technical characteristics and its development status.
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