The GMRT Epoch of Reionization experiment: a new upper limit on the neutral hydrogen power spectrum at z≈ 8.6
Abstract
We present a new upper limit to the 21-cm power spectrum during the Epoch of Reionization (EoR) which constrains reionization models with an unheated IGM. The GMRT-EoR experiment is an ongoing effort to make a statistical detection of the power spectrum of 21-cm neutral hydrogen emission at redshift z∼ 9. Data from this redshift constrain models of the EoR, the end of the Dark Ages arising from the formation of the first bright UV sources, probably stars or mini-quasars. We present results from approximately 50 h of observations with the Giant Metrewave Radio Telescope in India from 2007 December. We describe radio-frequency interference (RFI) localization schemes which allow bright sources on the ground to be identified and physically removed in addition to automated flagging. Singular-value decomposition is used to remove the remaining broad-band RFI by identifying ground sources with large eigenvalues. Foregrounds are modelled using a piecewise linear filter and the power spectrum is measured using cross-correlations of foreground-subtracted images.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- May 2011
- DOI:
- arXiv:
- arXiv:1006.1351
- Bibcode:
- 2011MNRAS.413.1174P
- Keywords:
-
- intergalactic medium;
- cosmology: observations;
- dark ages;
- reionization;
- first stars;
- diffuse radiation;
- radio lines: general;
- Astrophysics - Cosmology and Nongalactic Astrophysics
- E-Print:
- 11 pages, 11 figures, accepted for publication in MNRAS