BLAST-TNG 望远镜平台的飞行性能
天体物理仪器与方法
2021-01-05 v3
摘要
下一代气球载大口径亚毫米波望远镜（BLAST-TNG）是一种用于高角分辨率表征亚毫米波偏振天空的独特仪器。BLAST-TNG 于 2020 年 1 月从南极长期气球设施飞行。尽管飞行时间短，该仪器工作非常好，并提供关于各子系统的重大信息，这对未来的气球任务极具价值。本文中，我们讨论望远镜与吊舱的性能。
引用
@article{arxiv.2012.01039,
title = {In-flight performance of the BLAST-TNG telescope platform},
author = {Gabriele Coppi and Peter A. R. Ade and Peter C. Ashton and Jason E. Austermann and Erin G. Cox and Mark J. Devlin and Bradley J. Dober and Valentina Fanfani and Laura M. Fissel and Nicholas Galitzki and Jiansong Gao and Samuel Gordon and Christopher E. Groppi and Gene C. Hilton and Johannes Hubmayr and Jeffrey Klein and Dale Li and Nathan P. Lourie and Ian Lowe and Hamdi Mani and Philip Mauskopf and Christopher McKenney and Federico Nati and Giles Novak and Giampaolo Pisano and L. Javier Romualdez and Adrian Sinclair and Juan D. Soler and Carole Tucker and Joel Ullom and Michael Vissers and Caleb Wheeler and Paul A. Williams},
journal= {arXiv preprint arXiv:2012.01039},
year = {2021}
}
备注
Submitted to SPIE Astronomical Telescopes + Instrumentation, Ground-based and Airborne Telescopes VIII