Table 1.
BAO constraints from the LoTSS–eBOSS cross-correlation and its combination with the eBOSS auto-correlation.
Measurement | zeff | α | DA(zeff)/rd | χmin2/dof | Δχnw2 |
---|---|---|---|---|---|
Cross (0.6 < z < 0.66) | 0.63 | 1.01 ± 0.11 | 9.997 ± 1.089 | 21.20/25 | 5.02 |
Cross + auto (0.6 < z < 0.66) | 0.63 | ![]() |
![]() |
30.66/50 | 7.27 |
Cross (4 bins combined) | 0.72 | ![]() |
![]() |
99.72/103 | 16.28 |
Notes. The α parameter is converted to angular diameter distance DA using Eq. (11), with a fiducial cosmology from Planck 2018. χmin2/dof denotes the reduced chi-squared of our fits. Also, Δχnw2 compares our results with models lacking BAO features (‘nw’ model; see Eisenstein & Hu 1998).
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