Uploaded February 2022 | Updated September 2026, 2 weeks ago
Oleg V. Verkhodanov
https://www.sao.ru/Doc-en/Events/2020/Memory/
celestis.com/participants-testimonials/dr-oleg-v-verkhodanov
O. V. Verkhodanov, Series of Anomalies of low multipoles of WMAP and Planck Missions: What are They? Phys. Part. Nuclei, 2015, 46, 237–247.
https://www1.jinr.ru/publish/Pepan/v-46-2/18_verk.pdf
O. V. Verkhodanov, Low Multipoles Anomalies of CMB Maps, in "Radiative Mechanisms of Astrophysical Objects (V. Grining et al., eds.). Yerevan, 2017, 363-370.
P.M. Robitaille, WMAP: A Radiological Analysis, Progr. Phys. 2007, v. 3, no. 1, 3-18. ptep-online.com/2007/PP-08-01.PDF
D. Larson et al.,Comparing PLANCK and WMAP: Maps, spectra, and parameters, Astrophys. J. 2015, 801, 9.
iopscience.iop.org/article/10.1088/0004-637X/801/1/9
G.E. Addison, et al., Quantifying discordance in the 2015 PLANCK CMB spectrum, Astrophys. J. 2016, 818, 132.
iopscience.iop.org/article/10.3847/0004-637X/818/2/132
Hinshaw, et al., Three-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis, Astrophys. J. Suppl. Series, 2003, 170, 288-334.
iopscience.iop.org/article/10.1086/513698/pdf
C. Barnes, et al., First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Side Lobe Pickup, Astrophys. J. Suppl. Series, 2003, 148, 51-62.
iopscience.iop.org/article/10.1086/377227
Y. Akrami, et al., Power Asymmetry in WMAP and Planck Temperature Sky Maps as Measured by Local Variance Estimator, Astrophys. J. Lett. 2014, 784(L42),
iopscience.iop.org/article/10.1088/2041-8205/784/2/L42/pdf
Cold Spot
Discovery paper:
M. Cruz, et al., Detection of a non-Gaussian Spot in WMAP, MNRAS 2005, 356(1), 29–40. https://arXiv:astro-ph/0405341
M. Cruz, et al, The non-Gaussian cold spot in Wilkinson Microwave Anisotropy Probe: significance, morphology and foreground contribution, MNRAS 2006, 369(1), 57–67.
academic.oup.com/mnras/article/369/1/57/1051444
Extragalactic radio sources and the WMAP cold spot L. Rudnick, et al., Extragalactic radio sources and the WMAP cold spot Astrophys. J. 2007
iopscience.iop.org/article/10.1086/522222/pdf
A. Kovács, et al., The DES view of the Eridanus supervoid and the CMB cold spot, MNRAS, 2022, 510(1), 216–229.
doi.org/10.1093/mnras/stab3309
R. Mackenzie, et al, Evidence against a supervoid causing the CMB Cold Spot, MNRAS 2017, 470(2), 2328–2338. academic.oup.com/mnras/article/470/2/2328/3752440?login=false
C.H. Lineweaver, 7: Gold in the Doppler Hills: Cosmological Parameters in the Microwave Background, in “Quantum Fluctuations to Cosmological Structures”, ASP Conference Series 1997, v. 126, 185-205.
https://adsabs.harvard.edu/full/1997ASPC..126..185L
N. Aghanim, et al., Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 2020, A6.
aanda.org/articles/aa/pdf/2020/09/aa33910-18.pdf
N. Aghanin, et al., Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 2020, A5.
aanda.org/articles/aa/pdf/2020/09/aa36386-19.pdf
M. Birkinshaw, The Sunyaev-Zel’dovich Effect, Phys. Reports 1999, v. 310, 97-195. doi.org/10.1016/S0370-1573(98)00080-5
arxiv.org/abs/astro-ph/9808050
J.E. Carlstrom, et al., Ann. Rev. Astron. Astrophys. 2002, v. 40, 643-680.
annualreviews.org/doi/abs/10.1146/annurev.astro.40.060401.093803
ABELL CLUSTER
M. Douspis, Planck SZ Clusters, Société Française d’Astronomie et d’Astrophysique (SF2A) 2011.
http://sf2a.eu/semaine-sf2a/2011/proceedings/2011sf2a.conf..0021D.pdf
https://sci.esa.int/web/planck/-/47697-multi-band-observations-of-the-galaxy-cluster-abell-2319
Abe et al., Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample, Astron. Astrophys. 2011, v. 536, A8.
aanda.org/articles/aa/pdf/2011/12/aa16459-11.pdf
K. S. Cover, Sky maps without anisotropies in the cosmic microwave background are a better fit to WMAP's uncalibrated time-ordered data than the official sky maps. Europhys. Lett., Volume 87, Number 6, 69003.
robots.iopscience.iop.org/article/10.1209/0295-5075/87/69003/pdf
arxiv.org/ftp/arxiv/papers/0905/0905.3971.pdf
All observational images and videos are credited to NASA unless
otherwise specified. Images obtained by the SDO satellite are a courtesy
of NASA/SDO and the AIA, EVE, and HMI science teams. Images obtained by the SOHO satellite are courtesy of SOHO (ESA & NASA).
Link to Professor Robitaille’s papers on Vixra:
vixra.org/author/pierre-marie_robitaille
Outro Music:
Foria: Break Away
soundcloud.com/foria
youtube.com/watch?v=UkUweq5FAcE
Oleg V. Verkhodanov
https://www.sao.ru/Doc-en/Events/2020/Memory/
celestis.com/participants-testimonials/dr-oleg-v-verkhodanov
O. V. Verkhodanov, Series of Anomalies of low multipoles of WMAP and Planck Missions: What are They? Phys. Part. Nuclei, 2015, 46, 237–247.
https://www1.jinr.ru/publish/Pepan/v-46-2/18_verk.pdf
O. V. Verkhodanov, Low Multipoles Anomalies of CMB Maps, in "Radiative Mechanisms of Astrophysical Objects (V. Grining et al., eds.). Yerevan, 2017, 363-370.
P.M. Robitaille, WMAP: A Radiological Analysis, Progr. Phys. 2007, v. 3, no. 1, 3-18. ptep-online.com/2007/PP-08-01.PDF
D. Larson et al.,Comparing PLANCK and WMAP: Maps, spectra, and parameters, Astrophys. J. 2015, 801, 9.
iopscience.iop.org/article/10.1088/0004-637X/801/1/9
G.E. Addison, et al., Quantifying discordance in the 2015 PLANCK CMB spectrum, Astrophys. J. 2016, 818, 132.
iopscience.iop.org/article/10.3847/0004-637X/818/2/132
Hinshaw, et al., Three-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis, Astrophys. J. Suppl. Series, 2003, 170, 288-334.
iopscience.iop.org/article/10.1086/513698/pdf
C. Barnes, et al., First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Side Lobe Pickup, Astrophys. J. Suppl. Series, 2003, 148, 51-62.
iopscience.iop.org/article/10.1086/377227
Y. Akrami, et al., Power Asymmetry in WMAP and Planck Temperature Sky Maps as Measured by Local Variance Estimator, Astrophys. J. Lett. 2014, 784(L42),
iopscience.iop.org/article/10.1088/2041-8205/784/2/L42/pdf
Cold Spot
Discovery paper:
M. Cruz, et al., Detection of a non-Gaussian Spot in WMAP, MNRAS 2005, 356(1), 29–40. https://arXiv:astro-ph/0405341
M. Cruz, et al, The non-Gaussian cold spot in Wilkinson Microwave Anisotropy Probe: significance, morphology and foreground contribution, MNRAS 2006, 369(1), 57–67.
academic.oup.com/mnras/article/369/1/57/1051444
Extragalactic radio sources and the WMAP cold spot L. Rudnick, et al., Extragalactic radio sources and the WMAP cold spot Astrophys. J. 2007
iopscience.iop.org/article/10.1086/522222/pdf
A. Kovács, et al., The DES view of the Eridanus supervoid and the CMB cold spot, MNRAS, 2022, 510(1), 216–229.
doi.org/10.1093/mnras/stab3309
R. Mackenzie, et al, Evidence against a supervoid causing the CMB Cold Spot, MNRAS 2017, 470(2), 2328–2338. academic.oup.com/mnras/article/470/2/2328/3752440?login=false
C.H. Lineweaver, 7: Gold in the Doppler Hills: Cosmological Parameters in the Microwave Background, in “Quantum Fluctuations to Cosmological Structures”, ASP Conference Series 1997, v. 126, 185-205.
https://adsabs.harvard.edu/full/1997ASPC..126..185L
N. Aghanim, et al., Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 2020, A6.
aanda.org/articles/aa/pdf/2020/09/aa33910-18.pdf
N. Aghanin, et al., Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 2020, A5.
aanda.org/articles/aa/pdf/2020/09/aa36386-19.pdf
M. Birkinshaw, The Sunyaev-Zel’dovich Effect, Phys. Reports 1999, v. 310, 97-195. doi.org/10.1016/S0370-1573(98)00080-5
arxiv.org/abs/astro-ph/9808050
J.E. Carlstrom, et al., Ann. Rev. Astron. Astrophys. 2002, v. 40, 643-680.
annualreviews.org/doi/abs/10.1146/annurev.astro.40.060401.093803
ABELL CLUSTER
M. Douspis, Planck SZ Clusters, Société Française d’Astronomie et d’Astrophysique (SF2A) 2011.
http://sf2a.eu/semaine-sf2a/2011/proceedings/2011sf2a.conf..0021D.pdf
https://sci.esa.int/web/planck/-/47697-multi-band-observations-of-the-galaxy-cluster-abell-2319
Abe et al., Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample, Astron. Astrophys. 2011, v. 536, A8.
aanda.org/articles/aa/pdf/2011/12/aa16459-11.pdf
K. S. Cover, Sky maps without anisotropies in the cosmic microwave background are a better fit to WMAP's uncalibrated time-ordered data than the official sky maps. Europhys. Lett., Volume 87, Number 6, 69003.
robots.iopscience.iop.org/article/10.1209/0295-5075/87/69003/pdf
arxiv.org/ftp/arxiv/papers/0905/0905.3971.pdf
All observational images and videos are credited to NASA unless
otherwise specified. Images obtained by the SDO satellite are a courtesy
of NASA/SDO and the AIA, EVE, and HMI science teams. Images obtained by the SOHO satellite are courtesy of SOHO (ESA & NASA).
Link to Professor Robitaille’s papers on Vixra:
vixra.org/author/pierre-marie_robitaille
Outro Music:
Foria: Break Away
soundcloud.com/foria
youtube.com/watch?v=UkUweq5FAcE
