Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator III: Foreground removal
arXiv:2308.08284 · doi:10.1093/mnras/stad2495
Abstract
Neutral hydrogen (HI) -cm intensity mapping (IM) is a promising probe of the large-scale structures in the Universe. However, a few orders of magnitude brighter foregrounds obscure the IM signal. Here we use the Tapered Gridded Estimator (TGE) to estimate the multi-frequency angular power spectrum (MAPS) from a bandwidth uGMRT Band data at . In foregrounds remain correlated across the entire range, whereas the -cm signal is localized within (typically ). Assuming the range to have minimal -cm signal, we use in this range to model the foregrounds. This foreground model is extrapolated to , and subtracted from the measured . The residual in the range is used to constrain the -cm signal, compensating for the signal loss from foreground subtraction. is found to be noise-dominated without any trace of foregrounds. Using we constrain the -cm brightness temperature fluctuations , and obtain the upper limit at . We further obtain the upper limit where and are the comoving HI density and bias parameters respectively. Although the upper limit is nearly times larger than the expected -cm signal, it is times tighter over previous works using foreground avoidance on the same data.
arXiv commentAccepted for publication in MNRAS. 16 pages (including Appendix), 8 figures (plus 8 in Appendix), 5 Tables. In version 2, the HI symbol is changed in the arxiv abstract; there are no changes in the manuscript
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