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Volumn 2011, Issue 6, 2011, Pages

How sensitive is the CMB to a single lens?

Author keywords

CMBR theory; gravitational lensing; non gaussianity

Indexed keywords


EID: 79959952646     PISSN: None     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2011/06/033     Document Type: Article
Times cited : (8)

References (35)
  • 1
    • 17044438084 scopus 로고    scopus 로고
    • Weak lensing of the CMB: A harmonic approach
    • [astro-ph/0001303]
    • W. Hu, 2000 Weak lensing of the CMB: a harmonic approach, Phys. Rev. D 62 043007 [astro-ph/0001303]
    • (2000) Phys. Rev. D , vol.62 , pp. 043007
    • Hu, W.1
  • 2
    • 33645990267 scopus 로고    scopus 로고
    • Weak gravitational lensing of the CMB
    • [astro-ph/0601594]
    • A. Lewis and A. Challinor, 2006 Weak gravitational lensing of the CMB, Phys. Rept. 429 1 [astro-ph/0601594]
    • (2006) Phys. Rept. , vol.429 , pp. 1
    • Lewis, A.1    Challinor, A.2
  • 4
    • 4344575439 scopus 로고    scopus 로고
    • Weak lensing of the CMB by large-scale structure
    • [astro-ph/0403075]
    • A. Amblard, C. Vale and M.J. White, 1, 2004 Weak lensing of the CMB by large-scale structure, New Astron. 9 687 [astro-ph/0403075]
    • (2004) New Astron. , vol.9 , pp. 687
    • Amblard, A.1    Vale, C.2    White, M.J.3
  • 5
    • 33846442054 scopus 로고    scopus 로고
    • The uncorrelated universe: Statistical anisotropy and the vanishing angular correlation function in WMAP years 1-3
    • [astro-ph/0605135]
    • C. Copi, D. Huterer, D. Schwarz and G. Starkman, 2007 The uncorrelated universe: statistical anisotropy and the vanishing angular correlation function in WMAP years 1-3, Phys. Rev. D 75 023507 [astro-ph/0605135]
    • (2007) Phys. Rev. D , vol.75 , pp. 023507
    • Copi, C.1    Huterer, D.2    Schwarz, D.3    Starkman, G.4
  • 8
    • 0142117048 scopus 로고    scopus 로고
    • A high resolution foreground cleaned CMB map from WMAP
    • [astro-ph/0302496]
    • M. Tegmark, A. de Oliveira-Costa and A. Hamilton, 2003 A high resolution foreground cleaned CMB map from WMAP, Phys. Rev. D 68 123523 [astro-ph/0302496]
    • (2003) Phys. Rev. D , vol.68 , pp. 123523
    • Tegmark, M.1    De Oliveira-Costa, A.2    Hamilton, A.3
  • 10
    • 27144446663 scopus 로고    scopus 로고
    • The axis of evil
    • [astro-ph/0502237]
    • K. Land and J. Magueijo, 2005 The axis of evil, Phys. Rev. Lett. 95 071301 [astro-ph/0502237]
    • (2005) Phys. Rev. Lett. , vol.95 , pp. 071301
    • Land, K.1    Magueijo, J.2
  • 11
    • 34249730970 scopus 로고    scopus 로고
    • The axis of evil revisited
    • [astro-ph/0611518]
    • K. Land and J. Magueijo, 2007 The axis of evil revisited, Mon. Not. Roy. Astron. Soc. 378 153 [astro-ph/0611518]
    • (2007) Mon. Not. Roy. Astron. Soc. , vol.378 , pp. 153
    • Land, K.1    Magueijo, J.2
  • 12
    • 58049152279 scopus 로고    scopus 로고
    • Consistently large cosmic flows on scales of 100 Mpc/h: A challenge for the standard LCDM cosmology
    • [0809.4041]
    • R. Watkins, H.A. Feldman and M.J. Hudson, 2009 Consistently large cosmic flows on scales of 100 Mpc/h: a challenge for the standard LCDM cosmology Mon. Not. Roy. Astron. Soc. 392 743 [0809.4041]
    • (2009) Mon. Not. Roy. Astron. Soc. , vol.392 , pp. 743
    • Watkins, R.1    Feldman, H.A.2    Hudson, M.J.3
  • 13
    • 78650129428 scopus 로고    scopus 로고
    • Cosmic flows on 100 Mpc/h scales: Standardized minimum variance bulk flow, shear and octupole moments
    • [0911.5516]
    • H.A. Feldman, R. Watkins and M.J. Hudson, 2010 Cosmic flows on 100 Mpc/h scales: standardized minimum variance bulk flow, shear and octupole moments, Mon. Not. Roy. Astron. Soc. 407 2328 [0911.5516]
    • (2010) Mon. Not. Roy. Astron. Soc. , vol.407 , pp. 2328
    • Feldman, H.A.1    Watkins, R.2    Hudson, M.J.3
  • 14
    • 73949153470 scopus 로고    scopus 로고
    • Cosmic flow from 2MASS redshift survey: The origin of CMB dipole and implications for LCDM cosmology
    • [0810.3658]
    • G. Lavaux, R.B. Tully, R. Mohayaee and S. Colombi, 2010 Cosmic flow from 2MASS redshift survey: the origin of CMB dipole and implications for LCDM cosmology, Astrophys. J. 709 483 [0810.3658]
    • (2010) Astrophys. J. , vol.709 , pp. 483
    • Lavaux, G.1    Tully, R.B.2    Mohayaee, R.3    Colombi, S.4
  • 16
    • 33745263212 scopus 로고    scopus 로고
    • The non-gaussian cold spot in WMAP: Significance, morphology and foreground contribution
    • [astro-ph/0601427]
    • M. Cruz, M. Tucci, E. Martinez-Gonzalez and P. Vielva, 2006 The non-gaussian cold spot in WMAP: significance, morphology and foreground contribution, Mon. Not. Roy. Astron. Soc. 369 57 [astro-ph/0601427]
    • (2006) Mon. Not. Roy. Astron. Soc. , vol.369 , pp. 57
    • Cruz, M.1    Tucci, M.2    Martinez-Gonzalez, E.3    Vielva, P.4
  • 17
  • 18
    • 36849064304 scopus 로고    scopus 로고
    • A cosmic microwave background feature consistent with a cosmic texture
    • [0710.5737]
    • M. Cruz, N. Turok, P. Vielva, E. Martinez-Gonzalez and M. Hobson, 2007 A cosmic microwave background feature consistent with a cosmic texture, Science 318 1612 [0710.5737]
    • (2007) Science , vol.318 , pp. 1612
    • Cruz, M.1    Turok, N.2    Vielva, P.3    Martinez-Gonzalez, E.4    Hobson, M.5
  • 21
    • 79951569148 scopus 로고    scopus 로고
    • Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Are there cosmic microwave background anomalies?
    • [1001.4758]
    • C.L. Bennett et al., 2011 Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: are there cosmic microwave background anomalies?, Astrophys. J. Suppl. 192 17 [1001.4758]
    • (2011) Astrophys. J. Suppl. , vol.192 , pp. 17
    • Bennett, C.L.1
  • 23
    • 0000935126 scopus 로고
    • Global texture and the microwave background
    • N. Turok and D. Spergel, 1990 Global texture and the microwave background, Phys. Rev. Lett. 64 2736
    • (1990) Phys. Rev. Lett. , vol.64 , pp. 2736
    • Turok, N.1    Spergel, D.2
  • 24
    • 33748778756 scopus 로고    scopus 로고
    • Local voids as the origin of large-angle cosmic microwave background anomalies
    • [astro-ph/0602478]
    • K.T. Inoue and J. Silk, 2006 Local voids as the origin of large-angle cosmic microwave background anomalies, Astrophys. J. 648 23 [astro-ph/0602478]
    • (2006) Astrophys. J. , vol.648 , pp. 23
    • Inoue, K.T.1    Silk, J.2
  • 25
    • 58149290037 scopus 로고    scopus 로고
    • The overshoot problem and giant structures
    • [0807.3216]
    • N. Itzhaki, 2008 The overshoot problem and giant structures J. High Energy Phys. JHEP10(2008)061 [0807.3216]
    • (2008) J. High Energy Phys. , vol.2008 , pp. 061
    • Itzhaki, N.1
  • 26
    • 76249099978 scopus 로고    scopus 로고
    • Cosmological imprints of pre-inflationary particles
    • [0911.2100]
    • A. Fialkov, N. Itzhaki and E.D. Kovetz, 2010 Cosmological imprints of pre-inflationary particles J. Cosmol. Astropart. Phys. JCAP02(2010)004 [0911.2100]
    • (2010) J. Cosmol. Astropart. Phys. , vol.2010 , pp. 004
    • Fialkov, A.1    Itzhaki, N.2    Kovetz, E.D.3
  • 27
    • 62349137614 scopus 로고    scopus 로고
    • CMB lensing and the WMAP cold spot
    • [0809.4704]
    • S. Das and D.N. Spergel, 2009 CMB lensing and the WMAP cold spot, Phys. Rev. D 79 043007 [0809.4704]
    • (2009) Phys. Rev. D , vol.79 , pp. 043007
    • Das, S.1    Spergel, D.N.2
  • 28
    • 70350691929 scopus 로고    scopus 로고
    • The cold spot as a large void: Lensing effect on CMB two and three point correlation functions
    • [0905.1073]
    • I. Masina and A. Notari, 2009 The cold spot as a large void: lensing effect on CMB two and three point correlation functions J. Cosmol. Astropart. Phys. JCAP07(2009)035 [0905.1073]
    • (2009) J. Cosmol. Astropart. Phys. , vol.2009 , pp. 035
    • Masina, I.1    Notari, A.2
  • 29
    • 78449269623 scopus 로고    scopus 로고
    • Detecting the cold spot as a void with the non-diagonal two-point function
    • [1007.0204]
    • I. Masina and A. Notari, 2010 Detecting the cold spot as a void with the non-diagonal two-point function J. Cosmol. Astropart. Phys. JCAP09(2010)028 [1007.0204]
    • (2010) J. Cosmol. Astropart. Phys. , vol.2010 , pp. 028
    • Masina, I.1    Notari, A.2
  • 31
    • 67949123393 scopus 로고    scopus 로고
    • Power spectrum estimation I. Basics
    • [astro-ph/0503603]
    • A.J.S. Hamilton, 2008 Power spectrum estimation I. Basics Lect. Notes Phys. 665 415 [astro-ph/0503603]
    • (2008) Lect. Notes Phys. , vol.665 , pp. 415
    • Hamilton, A.J.S.1
  • 32
    • 77950228720 scopus 로고    scopus 로고
    • Statistical methods in cosmology
    • [0911.3105]
    • L. Verde, 2010 Statistical methods in cosmology, Lect. Notes Phys. 800 147 [0911.3105]
    • (2010) Lect. Notes Phys. , vol.800 , pp. 147
    • Verde, L.1
  • 33
    • 85037915310 scopus 로고    scopus 로고
    • Angular trispectrum of the cosmic microwave background
    • [astro-ph/0105117]
    • W. Hu, 2001 Angular trispectrum of the cosmic microwave background, Phys. Rev. D 64 083005 [astro-ph/0105117]
    • (2001) Phys. Rev. D , vol.64 , pp. 083005
    • Hu, W.1
  • 34
    • 79960218689 scopus 로고    scopus 로고
    • A constraint on the integrated mass power spectrum out to z = 1100 from lensing of the cosmic microwave background
    • [1012.1600]
    • J. Smidt et al., 2011 A constraint on the integrated mass power spectrum out to z = 1100 from lensing of the cosmic microwave background, Astrophys. J. 728 L1 [1012.1600]
    • (2011) Astrophys. J. , vol.728 , pp. 1
    • Smidt, J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.