A high reliability survey of discrete Epoch of Reionization foreground sources in the MWA EoR0 field
暂无分享,去创建一个
Max Tegmark | E. Lenc | D. Kaplan | J. Hewitt | B. Pindor | R. Webster | S. Tingay | M. Morales | C. Trott | A. D. Oliveira-Costa | A. Loeb | D. Oberoi | P. Carroll | A. Rogers | B. Corey | R. Cappallo | A. Whitney | I. Sullivan | R. Wayth | P. Procopio | J. Kasper | A. Offringa | J. Pober | A. Beardsley | G. Bernardi | J. Bowman | J. Dillon | A. Ewall-Wice | B. Hazelton | D. Jacobs | A. Neben | N. Thyagarajan | J. Wyithe | R. Goeke | R. Subrahmanyan | M. Johnston-Hollitt | F. Briggs | B. Gaensler | D. Mitchell | L. Greenhill | S. Ord | C. Lonsdale | S. McWhirter | M. Lynch | M. Waterson | A. Williams | S. Sethi | D. Emrich | N. Hurley-Walker | N. Shankar | K. Srivani | B. McKinley | C. Wu | E. Kratzenberg | T. Prabu | A. Roshi | C. Williams | L. Feng | E. Morgan | J. Riding | J. Line | N. Barry | Hs. Kim | S. Paul
[1] M. Morales,et al. Calibration requirements for detecting the 21 cm epoch of reionization power spectrum and implications for the SKA , 2016, 1603.00607.
[2] S. J. Tingay,et al. Parametrizing Epoch of Reionization foregrounds: a deep survey of low-frequency point-source spectra with the Murchison Widefield Array , 2016, 1602.02247.
[3] A. R. Whitney,et al. THE IMPORTANCE OF WIDE-FIELD FOREGROUND REMOVAL FOR 21 cm COSMOLOGY: A DEMONSTRATION WITH EARLY MWA EPOCH OF REIONIZATION OBSERVATIONS , 2016, 1601.06177.
[4] A. Shulevski,et al. The ASKAP/EMU Source Finding Data Challenge , 2015, Publications of the Astronomical Society of Australia.
[5] M. C. Toribio,et al. The LOFAR Multifrequency Snapshot Sky Survey (MSSS) - I. Survey description and first results , 2015, 1509.01257.
[6] Max Tegmark,et al. CONFIRMATION OF WIDE-FIELD SIGNATURES IN REDSHIFTED 21 cm POWER SPECTRA , 2015, 1506.06150.
[7] E. Lenc,et al. GLEAM: The GaLactic and Extragalactic All-Sky MWA Survey , 2015, Publications of the Astronomical Society of Australia.
[8] Max Tegmark,et al. FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA , 2015, 1502.07596.
[9] R. Ekers,et al. Serendipitous discovery of a dying Giant Radio Galaxy associated with NGC 1534, using the Murchison Widefield Array , 2014, 1412.3856.
[10] Roger Cappallo,et al. The Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14 110 Compact Radio Sources over 6 100 Square Degrees , 2014, Publications of the Astronomical Society of Australia.
[11] S. Velzen,et al. The Very Large Array Low-frequency Sky Survey Redux (VLSSr) , 2014, 1404.0694.
[12] Alan E. E. Rogers,et al. Science with the Murchison Widefield Array , 2012, Publications of the Astronomical Society of Australia.
[13] A. R. Whitney,et al. The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies , 2012, Publications of the Astronomical Society of Australia.
[14] A. A. Deshpande,et al. FAST HOLOGRAPHIC DECONVOLUTION: A NEW TECHNIQUE FOR PRECISION RADIO INTERFEROMETRY , 2012, 1209.1653.
[15] Andrew Hopkins,et al. Compact continuum source finding for next generation radio surveys , 2012, 1202.4500.
[16] Gaël Varoquaux,et al. Scikit-learn: Machine Learning in Python , 2011, J. Mach. Learn. Res..
[17] Michael Biehl,et al. Post‐correlation radio frequency interference classification methods , 2010, 1002.1957.
[18] Christopher L. Williams,et al. The Murchison Widefield Array: Design Overview , 2009, Proceedings of the IEEE.
[19] Trevor Hastie,et al. Multi-class AdaBoost ∗ , 2009 .
[20] Miguel F. Morales,et al. Software holography: interferometric data analysis for the challenges of next generation observatories , 2008, 0810.5107.
[21] J. Usón,et al. Correcting direction-dependent gains in the deconvolution of radio interferometric images , 2008, 0805.0834.
[22] Alexander S. Szalay,et al. TO APPEAR IN THE ASTROPHYSICAL JOURNAL Preprint typeset using LATEX style emulateapj v. 10/09/06 PROBABILISTIC CROSS-IDENTIFICATION OF ASTRONOMICAL SOURCES , 2008 .
[23] Leo Breiman,et al. Random Forests , 2001, Machine Learning.
[24] J. Curran,et al. SUMSS: a wide-field radio imaging survey of the southern sky – II. The source catalogue , 2003, astro-ph/0303188.
[25] J. Bond,et al. 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. Dermer. Variability in blazars , 1999, astro-ph/9901324.
[27] E. Greisen,et al. The NRAO VLA Sky Survey , 1996 .
[28] Michael I. Large,et al. A machine-readable release of the Molonglo Reference Catalogue of Radio Sources , 1991 .
[29] R. Roger,et al. The low-frequency spectra of nonthermal radio sources , 1973 .
[30] A. Eddington,et al. On a Formula for Correcting Statistics for the Effects of a known Probable Error of Observation , 1913 .
[31] 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 .