The FHD/εppsilon Epoch of Reionisation power spectrum pipeline
暂无分享,去创建一个
J. C. Pober | A. P. Beardsley | R. Byrne | N. Barry | B. Hazelton | M. F. Morales | I. Sullivan | M. Morales | I. Sullivan | J. Pober | A. Beardsley | B. Hazelton | N. Barry | R. Byrne
[1] Ruby Byrne,et al. Fundamental Limitations on the Calibration of Redundant 21 cm Cosmology Instruments and Implications for HERA and the SKA , 2018, The Astrophysical Journal.
[2] N. Udaya Shankar,et al. IMAGING THE EPOCH OF REIONIZATION: LIMITATIONS FROM FOREGROUND CONFUSION AND IMAGING ALGORITHMS , 2011, 1106.1297.
[3] Bryna Hazelton,et al. FOUR FUNDAMENTAL FOREGROUND POWER SPECTRUM SHAPES FOR 21 cm COSMOLOGY OBSERVATIONS , 2012, 1202.3830.
[4] Jason Manley,et al. OPENING THE 21 cm EPOCH OF REIONIZATION WINDOW: MEASUREMENTS OF FOREGROUND ISOLATION WITH PAPER , 2013, 1301.7099.
[5] M. Morales,et al. THE FUNDAMENTAL MULTI-BASELINE MODE-MIXING FOREGROUND IN 21 cm EPOCH OF REIONIZATION OBSERVATIONS , 2013, 1301.3126.
[6] Hannes Jensen,et al. Reionization and the Cosmic Dawn with the Square Kilometre Array , 2012, 1210.0197.
[7] J. V. Vleck,et al. The spectrum of clipped noise , 1966 .
[8] Suhaila E. Al-jawder,et al. Managing acute respiratory decompensation in the morbidly obese , 2012, Respirology.
[9] Foregrounds for 21-cm observations of neutral gas at high redshift , 2003, astro-ph/0302099.
[10] A. Ghosh,et al. Visibility-based angular power spectrum estimation in low-frequency radio interferometric observations , 2014, 1409.7789.
[11] E. Lenc,et al. Understanding instrumental Stokes leakage in Murchison Widefield Array polarimetry , 2014, 1412.4466.
[12] Lourdes Verdes-Montenegro,et al. Advancing Astrophysics with the Square Kilometre Array , 2015 .
[13] M. Morales,et al. Calibration requirements for detecting the 21 cm epoch of reionization power spectrum and implications for the SKA , 2016, 1603.00607.
[14] J. Hewitt,et al. Assessment of Ionospheric Activity Tolerances for Epoch of Reionization Science with the Murchison Widefield Array , 2018, The Astrophysical Journal.
[15] L. Koopmans,et al. The impact of interference excision on 21-cm epoch of reionization power spectrum analyses , 2019, Monthly Notices of the Royal Astronomical Society.
[16] Abhirup Datta,et al. BRIGHT SOURCE SUBTRACTION REQUIREMENTS FOR REDSHIFTED 21 cm MEASUREMENTS , 2010 .
[17] Tapering the sky response for angular power spectrum estimation from low-frequency radio-interferometric data. , 2016, Monthly notices of the Royal Astronomical Society.
[18] Miguel F. Morales,et al. Toward Epoch of Reionization Measurements with Wide-Field Radio Observations , 2003 .
[19] Tim J. Cornwell,et al. The Noncoplanar Baselines Effect in Radio Interferometry: The W-Projection Algorithm , 2008, IEEE Journal of Selected Topics in Signal Processing.
[20] Stefan J. Wijnholds,et al. Fast gain calibration in radio astronomy using alternating direction implicit methods: Analysis and applications , 2014, 1410.2101.
[21] IoA,et al. Radio Foregrounds for the 21 Centimeter Tomography of the Neutral Intergalactic Medium at High Redshifts , 2001, astro-ph/0109241.
[22] Cathryn M. Trott,et al. THE IMPACT OF POINT-SOURCE SUBTRACTION RESIDUALS ON 21 cm EPOCH OF REIONIZATION ESTIMATION , 2012, 1208.0646.
[23] David R. DeBoer,et al. WHAT NEXT-GENERATION 21 cm POWER SPECTRUM MEASUREMENTS CAN TEACH US ABOUT THE EPOCH OF REIONIZATION , 2013, 1310.7031.
[24] Ue-Li Pen,et al. Coaxing cosmic 21 cm fluctuations from the polarized sky using m -mode analysis , 2014, 1401.2095.
[25] A Fast Gridded Method for the Estimation of the Power Spectrum of the Cosmic Microwave Background from Interferometer Data with Application to the Cosmic Background Imager , 2002, astro-ph/0205385.
[26] C. Contaldi,et al. A Fast Gridded Method for the Estimation of the Power Spectrum of the CMB from Interferometer Data with Application to the Cosmic Background Imager , 2022 .
[27] R. Sault,et al. Understanding radio polarimetry. I. Mathematical foundations , 1996 .
[28] P. Murdin. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY , 2005 .
[29] N. Lomb. Least-squares frequency analysis of unequally spaced data , 1976 .
[30] U. Pen,et al. The GMRT Epoch of Reionization experiment: a new upper limit on the neutral hydrogen power spectrum at z≈ 8.6 , 2010, 1006.1351.
[31] M. Morales,et al. Understanding the diversity of 21 cm cosmology analyses , 2018, Monthly Notices of the Royal Astronomical Society.
[32] Is long QT syndrome a disease of abnormal mechanical contraction? , 2010, Circulation.
[33] Cathryn M. Trott,et al. Epoch of reionization window. I. Mathematical formalism , 2014, 1404.2596.
[34] W. Beyer. CRC Standard Probability And Statistics Tables and Formulae , 1990 .
[35] B. Pindor,et al. Characterization of the ionosphere above the Murchison Radio Observatory using the Murchison Widefield Array , 2017, 1707.04978.
[36] David R. DeBoer,et al. Improved 21 cm Epoch of Reionization Power Spectrum Measurements with a Hybrid Foreground Subtraction and Avoidance Technique , 2018, The Astrophysical Journal.
[37] J. Scargle. Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data , 1982 .
[38] J. Usón,et al. Correcting direction-dependent gains in the deconvolution of radio interferometric images , 2008, 0805.0834.
[39] A. Stebbins,et al. ALL-SKY INTERFEROMETRY WITH SPHERICAL HARMONIC TRANSIT TELESCOPES , 2013, 1302.0327.
[40] Roger J. Cappallo,et al. Real-Time Calibration of the Murchison Widefield Array , 2008, IEEE Journal of Selected Topics in Signal Processing.
[41] David F. Moore,et al. A PER-BASELINE, DELAY-SPECTRUM TECHNIQUE FOR ACCESSING THE 21 cm COSMIC REIONIZATION SIGNATURE , 2012, 1204.4749.
[42] K. Gorski,et al. HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , 2004, astro-ph/0409513.
[43] Miguel F. Morales,et al. Software holography: interferometric data analysis for the challenges of next generation observatories , 2008, 0810.5107.
[44] David W. Hogg,et al. Distance measures in cosmology , 1999, astro-ph/9905116.