Homogeneous search for helium in the atmosphere of 11 gas giant exoplanets with SPIRou

Author:

Allart R.ORCID,Lemée-Joliecoeur P.-B.,Jaziri A. Y.,Lafrenière D.ORCID,Artigau E.ORCID,Cook N.ORCID,Darveau-Bernier A.ORCID,Dang L.ORCID,Cadieux C.ORCID,Boucher A.,Bourrier V.ORCID,Deibert E. K.ORCID,Pelletier S.ORCID,Radica M.ORCID,Benneke B.ORCID,Carmona A.ORCID,Cloutier R.ORCID,Cowan N. B.ORCID,Delfosse X.,Donati J.-F.ORCID,Doyon R.,Figueira P.ORCID,Forveille T.ORCID,Fouqué P.ORCID,Gaidos E.,Gu P.-G.,Hébrard G.,Kiefer F.,Kóspál Á.,Jayawardhana R.,Martioli E.,Dos Santos L. A.ORCID,Shang H.ORCID,Turner J. D.ORCID,Vidotto A. A.ORCID

Abstract

The metastable helium triplet in the near-infrared (10 833 Å) is among the most important probes of exoplanet atmospheres. It can trace their extended outer layers and constrain mass loss. We used the near-infrared high-resolution spectropolarimeter SPIRou on the CFHT to search for the spectrally resolved helium triplet in the atmospheres of eleven exoplanets, ranging from warm mini-Neptunes to hot Jupiters and orbiting G, K, and M dwarfs. Observations were obtained as part of the SPIRou Legacy Survey and complementary open-time programs. We applied a homogeneous data reduction to all datasets and set constraints on the presence of metastable helium, despite the presence of systematics in the data. We confirm published detections for HAT-P-11 b, HD 189733 b, and WASP-69 b and set upper limits for the other planets. We applied the p–winds open source code to set upper limits on the mass-loss rate for the nondetections and to constrain the thermosphere temperature, mass-loss rate, line-of-sight velocity, and the altitude of the thermosphere for the detections. We confirm that the presence of metastable helium correlates with the stellar mass and the extreme-ultraviolet flux received by the planets. We investigated the correlation between the mass-loss rate and the presence of metastable helium, but it remains difficult to draw definitive conclusions. Finally, some of our results are in contradiction with previous results in the literature, and therefore we stress the importance of repeatable, homogeneous, and larger-scale analyses of the helium triplet to obtain robust statistics, study temporal variability, and better understand how the helium triplet can be used to explore the evolution of exoplanets.

Funder

FRQNT

NSERC

ERC

NASA Hubble Fellowship

NASA

ANR

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. ATMOSPHERIX: I- an open source high-resolution transmission spectroscopy pipeline for exoplanets atmospheres with SPIRou;Monthly Notices of the Royal Astronomical Society;2023-09-14

2. DREAM;Astronomy & Astrophysics;2023-08

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3