Academia Sinica Institute of Astronomy & Astrophysics
中央研究院天文及天文物理研究所
回上頁
研究成果藝廊 > 理論及觀測宇宙學

研究成果藝廊

理論及觀測宇宙學

An intensity map of hydrogen 21-cm emission at redshift z ≈ 0.8
圖片來源: Chang et al.
An intensity map of hydrogen 21-cm emission at redshift z ≈ 0.8
A cross-correlation measurement of 21-cm emission measured by the Green Bank Telescope, and the optical galaxies measured by the DEEP2 galaxy survey.
At redshifts around unity, we have recently reported a cross-correlation measurement of 21- cm emission measured by the Green Bank Telescope, and the optical galaxies measured by the DEEP2 galaxy survey. The redshifts of the cross-correlation is at 0.5 < z < 1.1, and at the mean redshift of 0.8, we have reported a HI-optical cross-correlation amplitude that yields constraints on the neutral hydrogen mass content at z=0.8 and its bias factor on 10 h-1 Mpc comoving scales. (Chang et al., 2010, Nature, 466, 463)This is the highest redshift detection of neutral hydrogen, and opens up a promising window for using 21-cm as tracers of the matter distribution, and eventually as a powerful tool for measuring the Baryon Acoustic Oscillation (BAO) features, shedding light on properties of dark energy.
頁首
電話: 886-2-3365-2200 傳真: 886-2-2367-7849
一般事務: asiaa_replace2@_asiaa.sinica.edu.tw 媒體連絡: epo_replace2@_asiaa.sinica.edu.tw
台北市10617羅斯福路四段1號 中央研究院/台灣大學天文數學館11樓