An improved source-subtracted and destriped 408 MHz all-sky map
暂无分享,去创建一个
M. Remazeilles | M.-A. Bigot-Sazy | C. Dickinson | A. J. Banday | A. Banday | C. Dickinson | M. Remazeilles | T. Ghosh | M. Bigot-Sazy | T. Ghosh
[1] A. J. Banday,et al. Connecting Synchrotron, Cosmic Rays, and Magnetic Fields in the Plane of the Galaxy , 2011, 1105.5885.
[2] Portugal,et al. The 2.3 GHz continuum survey of the GEM project , 2007, 0712.3141.
[3] Foreground analysis using cross-correlations of external templates on the 7-year Wilkinson Microwave Anisotropy Probe data , 2011, 1112.0509.
[4] D. Finkbeiner. Microwave Interstellar Medium Emission Observed by the Wilkinson Microwave Anisotropy Probe , 2004 .
[5] A. Stebbins,et al. ALL-SKY INTERFEROMETRY WITH SPHERICAL HARMONIC TRANSIT TELESCOPES , 2013, 1302.0327.
[6] A. Strong,et al. Galactic synchrotron emission with cosmic ray propagation models , 2013, 1309.2947.
[7] P. S. Bunclark,et al. Astronomical Data Analysis Software and Systems , 2008 .
[8] K. Gorski,et al. Monopole and dipole estimation for multi-frequency sky maps by linear regression , 2014, 1411.7616.
[9] C. Dickinson,et al. H i intensity mapping: a single dish approach , 2012, 1209.0343.
[10] A Measurement of the Angular Power Spectrum of the Anisotropy in the Cosmic Microwave Background , 1996, astro-ph/9601197.
[11] C. Dickinson,et al. Towards a free–free template for CMB foregrounds , 2003, astro-ph/0302024.
[12] J. Dunkley,et al. EVIDENCE FOR ANOMALOUS DUST-CORRELATED EMISSION AT 8 GHz , 2011, 1109.5093.
[13] T. Foster,et al. The galactic plane region near $\mathsf{\ell=93^\circ}$ : I. HII region NRAO 655 , 2001 .
[14] R. Franke. Smooth Interpolation of Scattered Data by Local Thin Plate Splines , 1982 .
[15] Edward J. Wollack,et al. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results , 2003, astro-ph/0302207.
[16] M. Zhu,et al. GSH 90-28-17: a possible old supernova remnant , 2013, 1311.4622.
[17] Elena Pierpaoli,et al. Galactic foreground contributions to the 5-year Wilkinson Microwave Anisotropy Probe maps , 2011 .
[18] E. L. Wright,et al. Preliminary separation of galactic and cosmic microwave emission for the COBE Differential Microwave Radiometer , 1992 .
[19] K. Gorski,et al. A determination of the spectra of Galactic components observed by the Wilkinson Microwave Anisotropy Probe , 2006 .
[20] S. Zaroubi,et al. Foregrounds for observations of the cosmological 21 cm line - I. First Westerbork measurements of Galactic emission at 150 MHz in a low latitude field , 2009, 0904.0404.
[21] Edward J. Wollack,et al. NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: FINAL MAPS AND RESULTS , 2012, 1212.5225.
[22] Reappraising foreground contamination in the COBE-DMR data , 2003, astro-ph/0302181.
[23] George D. Nicolson,et al. The Rhodes/HartRAO 2326‐MHz radio continuum survey , 1998 .
[24] David J. Schlegel,et al. Extrapolation of Galactic Dust Emission at 100 Microns to Cosmic Microwave Background Radiation Frequencies Using FIRAS , 1999, astro-ph/9905128.
[25] Michael E. Jones,et al. The C-Band All-Sky Survey (C-BASS): design and implementation of the northern receiver , 2013, 1310.7129.
[26] David F. Moore,et al. A PER-BASELINE, DELAY-SPECTRUM TECHNIQUE FOR ACCESSING THE 21 cm COSMIC REIONIZATION SIGNATURE , 2012, 1204.4749.
[27] Template fitting of WMAP 7‐year data: anomalous dust or flattening synchrotron emission? , 2011, 1112.0432.
[28] X. Gao,et al. Thermal and non-thermal emission in the Cygnus X region , 2013, 1309.6065.
[29] C. Burigana,et al. The impact of Galactic synchrotron emission on CMB anisotropy measurements. I. Angular power spectru , 2008, 0801.0547.
[30] S. Sarkar,et al. Loops and spurs: the angular power spectrum of the Galactic synchrotron background , 2013, 1304.1078.
[31] Max Tegmark,et al. A model of diffuse Galactic radio emission from 10 MHz to 100 GHz , 2008, 0802.1525.
[32] H. Junklewitz,et al. Studying Galactic interstellar turbulence through fluctuations in synchrotron emission , 2013, Astronomy & Astrophysics.
[33] C. Salter,et al. A 408-MHz SURVEY OF THE GALACTIC ANTICENTRE REGION. , 1970 .
[34] P. Reich,et al. A radio continuum survey of the southern sky at 1420 MHz - The atlas of contour maps , 2001 .
[35] J. Aumont,et al. The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths , 2012, 1207.3675.
[36] J. M. Martin,et al. 21 cm observation of large-scale structures at z ~ 1 - Instrument sensitivity and foreground subtraction , 2011, 1108.1474.
[37] C. B. Netterfield,et al. Planck early results. XX. New light on anomalous microwave emission from spinning dust grains , 2011, 1101.2031.
[38] J. May,et al. All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz , 2010, 1011.4298.
[39] I. Sushch,et al. Modeling of the Radio Emission from the Vela Supernova Remnant , 2013, 1312.0777.
[40] R. Davies,et al. Galactic synchrotron emission at high frequencies , 1996 .
[41] D.Maino,et al. A determination of the spectral index of galactic synchrotron emission in the 1-10 GHz range , 1997, astro-ph/9707252.
[42] J. J. Condon. Cosmological evolution of radio sources , 1984 .
[43] H. K. Eriksen,et al. The Joint Large-Scale Foreground-CMB Posteriors of the 3 Year WMAP Data , 2007, 0709.1037.
[44] J. Condon,et al. Confusion and flux-density error distributions , 1974 .
[45] T. Jaffe,et al. The interstellar cosmic-ray electron spectrum from synchrotron radiation and direct measurements. , 2011, 1108.4822.
[46] E. Hivon,et al. Fast estimation of polarization power spectra using correlation functions , 2003, astro-ph/0303414.
[47] S. Zaroubi,et al. Foreground simulations for the LOFAR-epoch of reionization experiment , 2008, 0804.1130.
[48] David F. Moore,et al. THE EFFECTS OF POLARIZED FOREGROUNDS ON 21 cm EPOCH OF REIONIZATION POWER SPECTRUM MEASUREMENTS , 2013, 1302.0876.
[49] K. Gorski,et al. HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , 2004, astro-ph/0409513.
[50] R. Davis,et al. A Circularly Symmetric Antenna Design With High Polarization Purity and Low Spillover , 2011, IEEE Transactions on Antennas and Propagation.
[51] F. B. Abdalla,et al. The effect of foreground subtraction on cosmological measurements from intensity mapping , 2013, 1310.8144.
[52] J. Shakeshaft,et al. A Survey of the Background Radiation at a Frequency of 404 Mc/s , 1962 .
[53] W. Reach,et al. Galactic worms. I - Catalog of worm candidates , 1992 .
[54] M. Bersanelli,et al. Full sky study of diffuse Galactic emission at decimeter wavelenghts , 2003, astro-ph/0303031.
[55] Edward J. Wollack,et al. First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission , 2003, astro-ph/0302208.