中文

JWST 系外行星系统直接观测早期释放科学计划 IV:NIRISS 孔径掩模干涉测量性能与经验总结

地球与行星天体物理 2024-03-13 v2 天体物理仪器与方法

摘要

我们展示了詹姆斯·韦伯空间望远镜近红外成像仪和无缝光谱仪(JWST/NIRISS)上孔径掩模干涉测量(AMI)模式的性能分析。得益于自校准可观测量,AMI 可触及低至甚至优于经典衍射极限的内工作角。该模式的科学潜力已由早期释放科学(ERS) 1386 计划通过深度搜寻 HIP 65426 系外行星系统中的密近伴星得以证实。作为 ERS 1386 的一部分,我们使用同一数据集探究 NIRISS AMI 可观测量中的随机、静态与校准误差。我们将观测噪声特性和可实现对比度与理论预测进行比较。我们探究了校准误差的可能来源,并表明 HIP 65426 与 point-spread function 校准星的观测间电荷迁移差异可解释所实现的对比度曲线。最后,我们利用自校准测试证明,在充分校准下 NIRISS F380M AMI 可在 λ/D\gtrsim \lambda/D 处达到 910\sim9-10 mag 的对比度水平。这些测试引出了观测规划建议,并强烈推动未来研究以制定考虑这些系统效应的复杂校准策略。这将释放 JWST/NIRISS AMI 前所未有的能力,其对显著更冷、更低质量的系外行星的灵敏度优于低对比度地基 AMI 装置,且处于 JWST 日冕仪无法触及的轨道间距。

关键词

引用

@article{arxiv.2310.11499,
  title  = {The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems IV: NIRISS Aperture Masking Interferometry Performance and Lessons Learned},
  author = {Steph Sallum and Shrishmoy Ray and Jens Kammerer and Anand Sivaramakrishnan and Rachel Cooper and Alexandra Z. Greebaum and Deepashri Thatte and Matthew de Furio and Samuel Factor and Michael Meyer and Jordan M. Stone and Aarynn Carter and Beth Biller and Sasha Hinkley and Andrew Skemer and Genaro Suarez and Jarron M. Leisenring and Marshall D. Perrin and Adam L. Kraus and Olivier Absil and William O. Balmer and Mickael Bonnefoy and Marta L. Bryan and Sarah K. Betti and Anthony Boccaletti and Mariangela Bonavita and Mark Booth and Brendan P. Bowler and Zackery W. Briesemeister and Faustine Cantalloube and Gael Chauvin and Valentin Christiaens and Gabriele Cugno and Thayne Currie and Camilla Danielski and Trent J. Dupuy and Jacqueline K. Faherty and Christine H. Chen and Per Calissendorff and Elodie Choquet and Michael P. Fitzgerald and Jonathan J. Fortney and Kyle Franson and Julien H. Girard and Carol A. Grady and Eileen C. Gonzales and Thomas Henning and Dean C. Hines and Kielan K. W. Hoch and Callie E. Hood and Alex R. Howe and Markus Janson and Paul Kalas and Grant M. Kennedy and Matthew A. Kenworthy and Pierre Kervella and Daniel Kitzmann and Masayuki Kuzuhara and Anne-Marie Lagrange and Pierre-Olivier Lagage and Kellen Lawson and Cecilia Lazzoni and Ben W. P. Lew and Michael C. Liu and Pengyu Liu and Jorge Llop-Sayson and James P. Lloyd and Anna Lueber and Bruce Macintosh and Elena Manjavacas and Sebastian Marino and Mark S. Marley and Christian Marois and Raquel A. Martinez and Brenda C. Matthews and Elisabeth C. Matthews and Dimitri Mawet and Johan Mazoyer and Michael W. McElwain and Stanimir Metchev and Brittany E. Miles and Maxwell A. Millar-Blanchaer and Paul Molliere and Sarah E. Moran and Caroline V. Morley and Sagnick Mukherjee and Paulina Palma-Bifani and Eric Pantin and Polychronis Patapis and Simon Petrus and Laurent Pueyo and Sascha P. Quanz and Andreas Quirrenbach and Isabel Rebollido and Jea Adams Redai and Bin B. Ren and Emily Rickman and Matthias Samland and B. A. Sargent and Joshua E. Schlieder and Glenn Schneider and Karl R. Stapelfeldt and Ben J. Sutlieff and Motohide Tamura and Xianyu Tan and Christopher A. Theissen and Taichi Uyama and Arthur Vigan and Malavika Vasist and Johanna M. Vos and Kevin Wagner and Jason J. Wang and Kimberly Ward-Duong and Niall Whiteford and Schuyler G. Wolff and Kadin Worthen and Mark C. Wyatt and Marie Ygouf and Xi Zhang and Keming Zhang and Zhoujian Zhang and Yifan Zhou and Alice Zurlo},
  journal= {arXiv preprint arXiv:2310.11499},
  year   = {2024}
}

备注

20 pages, 12 figures, accepted to Astrophysical Journal Letters