تحلیل توصیفی داده های رصدی ماهواره های Planck و WMAP

[1] P.A.R. Ade, N. Aghanim, M. Arnaud, et al,  Planck Collaboration Planck 2015 results, Astronomy & Astrophysics 594 A13 (2016) 1-63. https://doi.org/10.1051/0004-6361/201525830

[2] K.N. Abazajian, K. Arnold, J. Austermann, et al., Inflation Physics from the Cosmic Microwave Background and Large Scale Structure, Astroparticle Physics 63 (2015) 55-65. https://doi.org/10.1016/j.astropartphys.2014.05.013

[3] C.L. Bennett, D. Larson, J.L. Weiland, et al, Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results. Astrophysical journal supplement series 208 (20) (2013) 1-54. https://doi.org/10.1088/0067-0049/208/2/20

[4] A. Faale Parsa, B. Khaleseh, Big Bang, Astan ghodseh Razavi Publisher, Mashhad, Iran (2006). https://www.adinehbook.com/gp/product/9640201081. ISBN: 978-964-02-0108-4

 [5] P. A. R. Ade et al., Measurement of the Cosmic Microwave Background Polarizatio Lensing Power Spectrum with the POLARBEAR experiment, Physics Review Letters 113 (2014) 021301. https://doi.org/10.1103/PhysRevLett.113.021301

[6] E. Komatsu, K.M. Smith, J. Dunkley, et al, Seven-year Wilkinson Microwave Anisotropy Probe (WMAP)  Observations: Ar  There Cosmic Microwave Background Anomalies?, Astrophysical journal supplement series 192 (17) (2011) 1-47. https://doi.org/10.1088/0067-0049/192/2/18

[7] J.R. Bond, C. Contaldi, D. Pogosyan, Cosmic microwave background snapshots: pre-WMAP and post-WMAP, Royal Society of London Philosophical Transactions Series A 361 2435 (2003) 455-461. https://doi.org/10.1098/rsta.2003.1295

[8] Y. Akrami, et al. Planck 2018 results. I. Overview and the cosmological legacy of Planck, Accepted in Astronomy & Astrophysics (2019) .https://doi.org/10.1051/0004-6361/201833880