An interesting 3D map presented with differences for the H0 or the Hubble constant too. EBOSS estimated the Hubble constant, 67.4 and 69.0 km/s/Mpc. Others like Freedman noted this difference. "Freedman also notes that the disagreement over the Hubble constant depends to some extent on what methods are used. She herself has done studies using Cepheid variable stars and red giant stars, which give two different results. “I think we still don't know how this issue will be resolved,” she adds. “It is an interesting time in cosmology.”, ref -
https://skyandtelescope.org/astronomy-news/new-3d-map-universe-growing-cosmological-debate/
Using this cosmology calculator,
http://www.astro.ucla.edu/~wright/CosmoCalc.html, the Hubble time using z = 67.4 is 14.168E+9 years ago for the age of the universe. Using z=69, Hubble time is 13.84E+9 years ago. There is 3.28E+8 years time difference (delta) between these two values for the Hubble time that could change much in the BB cosmology for timelines, e.g. origin of the CMBR and earlier conditions, e.g. inflation. Freedman et al also report other H0 values, some range up to 82 km/s/Mpc. NASA ADS Abstract, 'The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids',
https://ui.adsabs.harvard.edu/abs/2020arXiv200709013A/abstract, July 2020. The arxiv report is attached in this record. The redshift range surveyed is, "eBOSS conducted a 5-year observation program, surveying the large scale structure of the Universe over a redshift range from 0.6 to 3.5." That is some range of redshifts surveyed and SDSS also reported cosmic high-noon for star formation rates too. The early universe according to BB cosmology, created SMBHs, PBHs, star formation rates much faster and higher than anything we see today (e.g. QSO or quasar formations, Population III stars) in astronomy. The universe is running downhill, not uphill and winding down as the universe expands. Processes observed operating today in astronomy are not the same as the early universe in BB cosmology (e.g. inflation, BBN, PBH forming, SMBH forming, quasars forming, Population III stars forming).