NAME the Cold Spot , the SIMBAD biblio

NAME the Cold Spot , the SIMBAD biblio (47 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:42:50

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2005MNRAS.356...29C 50 2 302 Detection of a non-Gaussian spot in WMAP. CRUZ M., MARTINEZ-GONZALEZ E., VIELVA P., et al.
2006MNRAS.365..265T 17 1 35 Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe data using the peak-peak correlation function. TOJEIRO R., CASTRO P.G., HEAVENS A.F., et al.
2006MNRAS.369...57C 67 1 135 The non-Gaussian cold spot in WilkinsonMicrowaveAnisotropyProbe: significance, morphology and foreground contribution. CRUZ M., TUCCI M., MARTINEZ-GONZALEZ E., et al.
2006MNRAS.369..598C 10 1 20 No Higher Criticism of the Bianchi-corrected Wilkinson Microwave Anisotropy Probe data. CAYON L., BANDAY A.J., JAFFE T., et al.
2006MNRAS.369.1858M 13 1 27 Non-Gaussianity detections in the Bianchi VIIhcorrected WMAP one-year data made with directional spherical wavelets. McEWEN J.D., HOBSON M.P., LASENBY A.N., et al.
2006MNRAS.373..311A 3 1 6 Statistical analysis of undetected point sources in cosmic microwave background maps. ARGUESO F., SANZ J.L., BARREIRO R.B., et al.
2007MNRAS.377.1473B 345     A     X C       8 1 46 Markov chain Monte Carlo analysis of Bianchi VIIhmodels. BRIDGES M., McEWEN J.D., LASENBY A.N., et al.
2007MNRAS.381..932V 387     A     X   F     9 1 54 Alignment and signed-intensity anomalies in Wilkinson Microwave Anisotropy Probe data. VIELVA P., WIAUX Y., MARTINEZ-GONZALEZ E., et al.
2008MNRAS.385..939W 239           X         6 1 27 Non-Gaussianity analysis on local morphological measures of WMAP data. WIAUX Y., VIELVA P., BARREIRO R.B., et al.
2008MNRAS.390..913C 1588 T   A     X         41 2 86 The CMB
cold spot: texture, cluster or void ? 		CRUZ M., MARTINEZ-GONZALEZ E., VIELVA P., et al.
2008A&A...492L..33G 88           X         2 1 27 Kolmogorov stochasticity parameter measuring the randomness in the cosmic microwave background. GURZADYAN V.G. and KOCHARYAN A.A.
2009A&A...497..343G 91             C       1 1 31 Kolmogorov cosmic microwave background sky. GURZADYAN V.G., ALLAHVERDYAN A.E., GHAHRAMANYAN T., et al.
2009A&A...506L..37G 41           X         1 1 6 The power spectrum of the cosmic microwave background Kolmogorov maps: possible clue to correlation of voids. GURZADYAN V.G., KASHIN A.L., KHACHATRYAN H.G., et al.
2009MNRAS.400..898M 152             C F     2 6 7 Cosmic microwave background anomalies viewed via Gumbel statistics. MIKELSONS G., SILK J. and ZUNTZ J.
2010MNRAS.403....2S 1587           X C F     39 1 46 No evidence for the cold spot in the NVSS radio survey. SMITH K.M. and HUTERER D.
2010MNRAS.403.1739F 124           X   F     2 2 43 The axis of evil - a polarization perspective. FROMMERT M. and ENSSLIN T.A.
2010MNRAS.407..201C 171     A     X         4 1 68 Full-sky map of the ISW and Rees-Sciama effect from Gpc simulations. CAI Y.-C., COLE S., JENKINS A., et al.
2010MNRAS.407..399P 497     A     X C F     11 1 33 Power asymmetries in the cosmic microwave background temperature and polarization patterns. PACI F., GRUPPUSO A., FINELLI F., et al.
2011MNRAS.410...33V 1681 T   A     X C F     41 1 14 Cosmic microwave background polarization as a probe of the anomalous nature of the
cold spot. 		VIELVA P., MARTINEZ-GONZALEZ E., CRUZ M., et al.
2011MNRAS.412.2383C 51           X         1 1 26 Anomalous variance in the WMAP data and galactic foreground residuals. CRUZ M., VIELVA P., MARTINEZ-GONZALEZ E., et al.
2012MNRAS.426...57H 77       S             1 9 14 Faraday rotation as a diagnostic of Galactic foreground contamination of cosmic microwave background maps. HANSEN M., ZHAO W., FREJSEL A.M., et al.
2014A&A...571A..23P 406       S   X         2 1 577 Planck 2013 results. XXIII. Isotropy and statistics of the CMB. PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al.
2015MNRAS.450..288S 1613 T   A     X C F     37 1 81 Detection of a supervoid aligned with the
cold spot of the cosmic microwave background. 		SZAPUDI I., KOVACS A., GRANETT B.R., et al.
2016MNRAS.455.1246F 2595     A S   X C F     61 1 42 Supervoids in the WISE-2MASS catalogue imprinting cold spots in the cosmic microwave background. FINELLI F., GARCIA-BELLIDO J., KOVACS A., et al.
2016MNRAS.459L..71N 3119 T   A S   X C F     74 2 9 Could multiple voids explain the cosmic microwave background
Cold Spot anomaly? 		NAIDOO K., BENOIT-LEVY A. and LAHAV O.
2016MNRAS.460L..15M 2001 T   A     X C       48 1 10 On the void explanation of
the Cold Spot. 		MARCOS-CABALLERO A., FERNANDEZ-COBOS R., MARTINEZ-GONZALEZ E., et al.
2016MNRAS.460L.104L 46           X         1 1 6 Reconstruction of CMB temperature anisotropies with primordial CMB induced polarization in galaxy clusters. LIU G.-C., ICHIKI K., TASHIRO H., et al.
2016MNRAS.461.1363N 44           X         1 1 4 Local analyses of Planck maps with Minkowski functionals. NOVAES C.P., BERNUI A., MARQUES G.A., et al.
2016MNRAS.462.1882K 3051 T   A D S   X C       74 14 18 Cosmic troublemakers:
the Cold Spot, the Eridanus supervoid, and the Great Walls. 		KOVACS A. and GARCIA-BELLIDO J.
2016A&A...594A..16P 1817           X         40 2 425 Planck 2015 results. XVI. Isotropy and statistics of the CMB. PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al.
2016A&A...594A..20P 2346           X         1 1 2306 Planck 2015 results. XX. Constraints on inflation. PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al.
2017MNRAS.465.4166K 90           X         2 2 18 Imprint of DES superstructures on the cosmic microwave background. KOVACS A., SANCHEZ C., GARCIA-BELLIDO J., et al.
2017MNRAS.468.1953P 41           X         1 6 3 Testing isotropy in the Two Micron All-Sky redshift survey with information entropy. PANDEY B.
2017MNRAS.470.2328M 4521 T   A D S   X C F     108 1 13 Evidence against a supervoid causing the
CMB Cold Spot. 		MACKENZIE R., SHANKS T., BREMER M.N., et al.
2017MNRAS.472L..65N 2563 T   A D S   X C F     60 1 4 The cosmic microwave background
Cold Spot anomaly: the impact of sky masking and the expected contribution from the integrated Sachs-Wolfe effect. 		NAIDOO K., BENOIT-LEVY A. and LAHAV O.
2018MNRAS.475.1777K 1140     A S   X C F     25 2 8 The part and the whole: voids, supervoids, and their ISW imprint. KOVACS A.
2018MNRAS.476..359H 768     A     X         19 1 2 Probing supervoids with weak lensing. HIGUCHI Y. and INOUE K.T.
2018ApJ...861....8C 2181 T   A D     X C       52 1 ~ Excessive shift of the CMB acoustic peaks of
the Cold Spot area. 		CHIANG L.-Y.
2019ApJ...880...24T 43           X         1 42 43 Cosmicflows-3: cosmography of the Local Void. TULLY R.B., POMAREDE D., GRAZIANI R., et al.
2019MNRAS.488.4081K 251           X         6 1 ~ An alternative approach to modelling a cosmic void and its effect on the cosmic microwave background. KIM D.Y., LASENBY A.N. and HOBSON M.P.
2019MNRAS.488.5811H 276     A     X         7 1 ~ Environmental effects on halo abundance and weak lensing peak statistics towards large underdense regions. HIGUCHI Y. and INOUE K.T.
2020A&A...641A...1P 222             C       1 8 1103 Planck 2018 results. I. Overview and the cosmological legacy of Planck. PLANCK COLLABORATION, AGHANIM N., AKRAMI Y., et al.
2020A&A...641A...7P 652           X C       12 2 199 Planck 2018 results. VII. Isotropy and statistics of the CMB. PLANCK COLLABORATION, AKRAMI Y., ASHDOWN M., et al.
2020MNRAS.499..320K 834     A S   X C F     17 1 ~ A common explanation of the Hubble tension and anomalous cold spots in the CMB. KOVACS A., BECK R., SZAPUDI I., et al.
2022MNRAS.510..216K 4000 T   A D S   X C F     86 1 13 The DES view of the Eridanus supervoid and the CMB
cold spot. 		KOVACS A., JEFFREY N., GATTI M., et al.
2022MNRAS.513...15K 179             C F     2 1 ~ Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars. KOVACS A., BECK R., SMITH A., et al.
2023A&A...678A.176D 93           X         2 17 ~ Dynamic cosmography of the local Universe: Laniakea and five more watershed superclusters. DUPUY A. and COURTOIS H.M.

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