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Related papers: A comprehensive overview of the Cold Spot

200 papers

In a concordant $\Lambda$ Cold Dark Matter ($\Lambda$CDM) model, large-angle Cosmic Microwave Background (CMB) temperature anisotropy due to linear perturbations in the local universe is not negligible. We explore a possible role of an…

Cosmology and Nongalactic Astrophysics · Physics 2012-04-09 Kaiki Taro Inoue

Measurement of the acoustic peaks of the cosmic microwave background (CMB) temperature anisotropies has been instrumental in deciding the geometry and content of the universe. Acoustic peak positions vary in different parts of the sky due…

Cosmology and Nongalactic Astrophysics · Physics 2018-07-11 Lung-Yih Chiang

We investigate the abundance of large-scale hot and cold spots in the WMAP-5 temperature maps and find considerable discrepancies compared to Gaussian simulations based on the LCDM best-fit model. Too few spots are present in the reliably…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-06 Youness Ayaita , Maik Weber , Christof Wetterich

This paper presents a frequentist analysis of the hot and cold spots of the cosmic microwave background data collected by the Wilkinson Microwave Anisotropy Probe (WMAP). We compare the WMAP temperature statistics of extrema (number of…

Astrophysics · Physics 2009-11-10 David L. Larson , Benjamin D. Wandelt

Statistical Isotropy of the Cosmic Microwave Background (CMB) radiation has been studied and debated extensively in recent years. Under this assumption, the hot spots and cold spots of the CMB are expected to be uniformly distributed over a…

Cosmology and Nongalactic Astrophysics · Physics 2022-11-14 Md Ishaque Khan , Rajib Saha

We re-analyse the cosmic microwave background (CMB) Cold Spot (CS) anomaly with particular focus on understanding the bias a mask (contaminated by Galactic and point sources) may introduce. We measure the coldest spot, found by applying the…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-10 Krishna Naidoo , Aurélien Benoit-Lévy , Ofer Lahav

We apply spherical needlets to the Wilkinson Microwave Anisotropy Probe 5-year cosmic microwave background (CMB) dataset, to search for imprints of non-isotropic features in the CMB sky. We use the needlets localization properties to…

We investigate claims of excess ellipticity of hot and cold spots in the WMAP data (Gurzadyan et al. 2005, 2007). Using the cosmic microwave background data from 7 years of observations by the WMAP satellite, we find, contrary to previous…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Eirik Berntsen , Frode K. Hansen

The structure of the cold spot, of a non-Gaussian anomaly in the cosmic microwave background (CMB) sky first detected by Vielva et al. is studied using the data by Planck satellite. The obtained map of the degree of stochasticity (K-map) of…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-24 V. G. Gurzadyan , A. L. Kashin , H. Khachatryan , E. Poghosian , S. Sargsyan , G. Yegorian

Standard inflationary hot big bang cosmology predicts small fluctuations in the Cosmic Microwave Background (CMB) with isotropic Gaussian statistics. All measurements support the standard theory, except for a few anomalies discovered in the…

The non-Gaussian cold spot found in the WMAP data has created controversy about its origin. Here we calculate the Bayesian posterior probability ratios for three different models that could explain the cold spot. A recent work claimed that…

Astrophysics · Physics 2009-11-13 M. Cruz , E. Martinez-Gonzalez , P. Vielva , J. M. Diego , M. Hobson , N. Turok

We estimate the power spectra of CMB temperature anisotropy in localized regions on the sky using the WMAP 7-year data. Here, we report that the north hat and the south hat regions at the high Galactic latitude (|b| >= 30 deg) show anomaly…

Cosmology and Nongalactic Astrophysics · Physics 2017-01-18 Kyeong Yeon Ko , Chan-Gyung Park , Jai-chan Hwang

The Cold Spot is a puzzling large-scale feature in the Cosmic Microwave Background temperature maps and its origin has been subject to active debate. As an important foreground structure at low redshift, the Eridanus supervoid was recently…

Cosmology and Nongalactic Astrophysics · Physics 2022-01-05 A. Kovács , N. Jeffrey , M. Gatti , C. Chang , L. Whiteway , N. Hamaus , O. Lahav , G. Pollina , D. Bacon , T. Kacprzak , B. Mawdsley , S. Nadathur , D. Zeurcher , J. García-Bellido , A. Alarcon , A. Amon , K. Bechtol , G. M. Bernstein , A. Campos , A. Carnero Rosell , M. Carrasco Kind , R. Cawthon , R. Chen , A. Choi , J. Cordero , C. Davis , J. DeRose , C. Doux , A. Drlica-Wagner , K. Eckert , F. Elsner , J. Elvin-Poole , S. Everett , A. Ferté , G. Giannini , D. Gruen , R. A. Gruendl , I. Harrison , W. G. Hartley , K. Herner , E. M. Huff , D. Huterer , N. Kuropatkin , M. Jarvis , P. F. Leget , N. MacCrann , J. McCullough , J. Muir , J. Myles , A. Navarro-Alsina , S. Pandey , J. Prat , M. Raveri , R. P. Rollins , A. J. Ross , E. S. Rykoff , C. Sánchez , L. F. Secco , I. Sevilla-Noarbe , E. Sheldon , T. Shin , M. A. Troxel , I. Tutusaus , T. N. Varga , B. Yanny , B. Yin , Y. Zhang , J. Zuntz , M. Aguena , S. Allam , F. Andrade-Oliveira , J. Annis , E. Bertin , D. Brooks , D. Burke , J. Carretero , M. Costanzi , L. N. da Costa , M. E. S. Pereira , T. Davis , J. De Vicente , S. Desai , H. T. Diehl , I. Ferrero , B. Flaugher , P. Fosalba , J. Frieman , E. Gaztañaga , D. Gerdes , T. Giannantonio , J. Gschwend , G. Gutierrez , S. Hinton , D. L. Hollowood , K. Honscheid , D. James , K. Kuehn , M. Lima , M. A. G. Maia , J. L. Marshall , P. Melchior , F. Menanteau , R. Miquel , R. Morgan , R. Ogando , F. Paz-Chinchon , A. Pieres , A. A. Plazas , M. Rodriguez Monroy , K. Romer , A. Roodman , E. Sanchez , M. Schubnell , S. Serrano , M. Smith , M. Soares-Santos , E. Suchyta , M. E. C. Swanson , G. Tarle , D. Thomas , C. -H. To , J. Weller

The decomposition of a signal on the sphere with the steerable wavelet constructed from the second Gaussian derivative gives access to the orientation, signed-intensity, and elongation of the signal's local features. In the present work,…

Astrophysics · Physics 2009-11-13 Y. Wiaux , P. Vielva , R. B. Barreiro , E. Martinez-Gonzalez , P. Vandergheynst

We introduce the numbers of hot and cold spots, $n_h$ and $n_c$, of excursion sets of the CMB temperature anisotropy maps as statistical observables that can discriminate different non-Gaussian models. We numerically compute them from…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Pravabati Chingangbam , Changbom Park , K. P. Yogendran , Rien van de Weygaert

The recent study of BOOMERanG 150 GHz Cosmic Microwave Background (CMB) radiation maps have detected ellipticity of the temperature anisotropy spots independent on the temperature threshold. The effect has been found for spots up to several…

One of the most striking features found in the cosmic microwave background data is the presence of an anomalous Cold Spot (CS) in the temperature maps made by the Wilkinson Microwave Anisotropy Probe (WMAP). This CS has been interpreted as…

Astrophysics · Physics 2009-06-23 J. A. R. Cembranos , A. de la Cruz-Dombriz , A. Dobado , A. L. Maroto

A new map of the sky representing the degree of randomness in the cosmic microwave background (CMB) temperature has been obtained. The map based on estimation of the Kolmogorov stochasticity parameter clearly distinguishes the contribution…

We report the results of the 2dF-VST ATLAS Cold Spot galaxy redshift survey (2CSz) based on imaging from VST ATLAS and spectroscopy from 2dF AAOmega over the core of the CMB Cold Spot. We sparsely surveyed the inner 5$^{\circ}$ radius of…

Cosmology and Nongalactic Astrophysics · Physics 2017-07-26 Ruari Mackenzie , Tom Shanks , Malcolm N. Bremer , Yan-Chuan Cai , Madusha L. P. Gunawardhana , András Kovács , Peder Norberg , Istvan Szapudi

We study inhomogeneities in the distribution of the excursion sets in the Cosmic Microwave Background (CMB) temperature maps obtained by the three years survey of the Wilkinson Microwave Anisotropy Probe (WMAP). At temperature thresholds…

Astrophysics · Physics 2009-06-23 V. G. Gurzadyan , A. A. Starobinsky , A. L. Kashin , H. Khachatryan , G. Yegorian