Interpreting the observed 21-cm HI power spectrum

被引:0
|
作者
Minter, A [1 ]
机构
[1] NRAO, Green Bank, WV 24944 USA
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper I investigate what factors - both observational and physical - can change the measured slope of the observed 21-cm H-I power spectrum. The following effects can make the observed turbulence appear two dimensional rather than. three dimensional: 1) if the turbulence is contained in a thin filament or slab; 2) if the medium has a high optical depth; and 3) if any method of observation or analysis is used which effectively limits the emission from the medium under study to a thin slab, for example, by analyzing an individual channel map. Straightforward analysis of data can give misleading or incomplete results if these effects axe not taken into account.
引用
收藏
页码:221 / 224
页数:4
相关论文
共 50 条
  • [1] The 21-cm power spectrum after reionization
    Wyithe, J. Stuart B.
    Loeb, Abraham
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 397 (04) : 1926 - 1934
  • [2] Modelling redshift space distortion in the post-reionization HI 21-cm power spectrum
    Sarkar, Debanjan
    Bharadwaj, Somnath
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 476 (01) : 96 - 108
  • [3] CMBR weak lensing and HI 21-cm cross-correlation angular power spectrum
    Sarkar, Tapomoy Guha
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2010, (02):
  • [4] Charting the parameter space of the 21-cm power spectrum
    Cohen, Aviad
    Fialkov, Anastasia
    Barkana, Rennan
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 478 (02) : 2193 - 2217
  • [5] HI 21-cm absorbers at moderate redshifts
    Lane, W
    SEEING THROUGH THE DUST: THE DETECTION OF HI AND THE EXPLORATION OF THE ISM IN GALAXIES, PROCEEDINGS, 2002, 276 : 469 - 472
  • [6] 21-cm power spectrum in interacting cubic Galileon model
    Bikash R. Dinda
    Md. Wali Hossain
    Anjan A. Sen
    Journal of Astrophysics and Astronomy, 44
  • [7] 21-cm power spectrum in interacting cubic Galileon model
    Dinda, Bikash R.
    Hossain, Md. Wali
    Sen, Anjan A.
    JOURNAL OF ASTROPHYSICS AND ASTRONOMY, 2023, 44 (02)
  • [8] The wedge bias in reionization 21-cm power spectrum measurements
    Jensen, Hannes
    Majumdar, Suman
    Mellema, Garrelt
    Lidz, Adam
    Iliev, Ilian T.
    Dixon, Keri L.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 456 (01) : 66 - 70
  • [9] Predictions for measuring the cross power spectrum of the HI 21-cm signal and the Lyman-α forest using OWFA
    Sarkar, Anjan Kumar
    Bharadwaj, Somnath
    Sarkar, Tapomoy Guha
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2018, (05):
  • [10] Violation of statistical isotropy and homogeneity in the 21-cm power spectrum
    Shiraishi, Maresuke
    Munoz, Julian B.
    Kamionkowski, Marc
    Raccanelli, Alvise
    PHYSICAL REVIEW D, 2016, 93 (10)