中文

阿塔卡马宇宙学望远镜:跨越三分之一天空的高分辨率成分分离图

宇宙学与河外天体物理 2023-07-06 v1

摘要

毫米波天空的观测包含许多信号的有价值信息,包括黑体宇宙微波背景(CMB)、银河系辐射以及由热苏尼亚耶夫-泽尔多维奇(tSZ)效应引起的康普顿-yy 畸变。提取宇宙学和天体物理学问题的新见解通常需要结合多波长观测以在频谱上分离出某一成分。在这项工作中,我们呈现了一幅新的角分分辨率康普顿-yy 图,它示踪了视线积分的电子压强,以及跨越三分之一天空(约 13,000 平方度)的 CMB 强度和 E 模式偏振图。我们通过联合分析来自阿塔卡马宇宙学望远镜(ACT)数据发布 4 和 6 在约 93、148 和 225 GHz 频率的数据,以及来自 \textit{Planck} 卫星在 30 GHz 至 545 GHz 之间频率的数据来生成这些图。我们详细验证了在 needlet 框架下实现的内部线性组合流水线,它使我们能够高效抑制银河系污染并考虑 ACT 仪器噪声中的空间变化。这些图在噪声水平和分辨率上相比现有的 \textit{Planck} 成分分离图有显著进步,并将支持一系列科学目标,包括星系团和星系天体物理研究、宇宙速度场推断、原初非高斯性搜寻以及 CMB 引力透镜重建。

关键词

引用

@article{arxiv.2307.01258,
  title  = {The Atacama Cosmology Telescope: High-resolution component-separated maps across one-third of the sky},
  author = {William R. Coulton and Mathew S. Madhavacheril and Adriaan J. Duivenvoorden and J. Colin Hill and Irene Abril-Cabezas and Peter A. R. Ade and Simone Aiola and Tommy Alford and Mandana Amiri and Stefania Amodeo and Rui An and Zachary Atkins and Jason E. Austermann and Nicholas Battaglia and Elia Stefano Battistelli and James A. Beall and Rachel Bean and Benjamin Beringue and Tanay Bhandarkar and Emily Biermann and Boris Bolliet and J Richard Bond and Hongbo Cai and Erminia Calabrese and Victoria Calafut and Valentina Capalbo and Felipe Carrero and Grace E. Chesmore and Hsiao-mei Cho and Steve K. Choi and Susan E. Clark and Rodrigo Córdova Rosado and Nicholas F. Cothard and Kevin Coughlin and Kevin T. Crowley and Mark J. Devlin and Simon Dicker and Peter Doze and Cody J. Duell and Shannon M. Duff and Jo Dunkley and Rolando Dünner and Valentina Fanfani and Max Fankhanel and Gerrit Farren and Simone Ferraro and Rodrigo Freundt and Brittany Fuzia and Patricio A. Gallardo and Xavier Garrido and Jahmour Givans and Vera Gluscevic and Joseph E. Golec and Yilun Guan and Mark Halpern and Dongwon Han and Matthew Hasselfield and Erin Healy and Shawn Henderson and Brandon Hensley and Carlos Hervías-Caimapo and Gene C. Hilton and Matt Hilton and Adam D. Hincks and Renée Hložek and Shuay-Pwu Patty Ho and Zachary B. Huber and Johannes Hubmayr and Kevin M. Huffenberger and John P. Hughes and Kent Irwin and Giovanni Isopi and Hidde T. Jense and Ben Keller and Joshua Kim and Kenda Knowles and Brian J. Koopman and Arthur Kosowsky and Darby Kramer and Aleksandra Kusiak and Adrien La Posta and Victoria Lakey and Eunseong Lee and Zack Li and Yaqiong Li and Michele Limon and Martine Lokken and Thibaut Louis and Marius Lungu and Niall MacCrann and Amanda MacInnis and Diego Maldonado and Felipe Maldonado and Maya Mallaby-Kay and Gabriela A. Marques and Joshiwa van Marrewijk and Fiona McCarthy and Jeff McMahon and Yogesh Mehta and Felipe Menanteau and Kavilan Moodley and Thomas W. Morris and Tony Mroczkowski and Sigurd Naess and Toshiya Namikawa and Federico Nati and Laura Newburgh and Andrina Nicola and Michael D. Niemack and Michael R. Nolta and John Orlowski-Scherer and Lyman A. Page and Shivam Pandey and Bruce Partridge and Heather Prince and Roberto Puddu and Frank J. Qu and Federico Radiconi and Naomi Robertson and Felipe Rojas and Tai Sakuma and Maria Salatino and Emmanuel Schaan and Benjamin L. Schmitt and Neelima Sehgal and Shabbir Shaikh and Blake D. Sherwin and Carlos Sierra and Jon Sievers and Cristóbal Sifón and Sara Simon and Rita Sonka and David N. Spergel and Suzanne T. Staggs and Emilie Storer and Eric R. Switzer and Niklas Tampier and Robert Thornton and Hy Trac and Jesse Treu and Carole Tucker and Joel Ullom and Leila R. Vale and Alexander Van Engelen and Jeff Van Lanen and Cristian Vargas and Eve M. Vavagiakis and Kasey Wagoner and Yuhan Wang and Lukas Wenzl and Edward J. Wollack and Zhilei Xu and Fernando Zago and Kaiwen Zheng},
  journal= {arXiv preprint arXiv:2307.01258},
  year   = {2023}
}

备注

The Compton-y map and associated products will be made publicly available upon publication of the paper. The CMB T and E mode maps will be made available when the DR6 maps are made public