Reference paper cited,
https://iopscience.iop.org/article/10.3847/2041-8213/accd6f
“5. Summary In this work, we provide a brief overview of the JWST ASPIRE program, which will perform a legacy galaxy redshift survey in the fields of 25 reionization-era quasars using NIRCam/WFSS. From the early JWST observation of the field around the quasar J0305–3150, we discovered a filamentary structure traced by the quasar and 10 [O iii] emitters at z = 6.6. This structure has a galaxy overdensity of …making it one of the most overdense structures found in the early universe. By comparing with cosmological simulations, we argue that this filamentary structure traces an early overdensity, which could eventually evolve into a massive galaxy cluster. We also found that the most massive SMBHs in cosmological simulations generally trace galaxy overdensities but with a large variance on the galaxy numbers. This suggests that deep observations of a large sample of quasars (e.g., the ASPIRE program) would be essential for a comprehensive understanding of the cosmic environment of the earliest SMBHs…”
My note, the paper provides values for the BB cosmology used to explain the observations. “Throughout the paper, we adopt a flat ΛCDM cosmology with H0 = 70 km s^−1 Mpc^−1, ΩM = 0.3, and ΩΛ = 0.7.”
Using Ned Wright calculator (
https://lambda.gsfc.nasa.gov/toolbox/calculators.html), z=6.6 and H0 = 70 km/s/Mpc, light time distance from Earth 12.815 Gly. The comoving radial distance = 28.122 Gly where space expands 2.0132352E+00 or 2.013 x c velocity. Any evolution along the comoving radial distance for this object is not observable, so *could eventually evolve into a massive galaxy cluster* is something not observable when using the comoving radial distance from Earth as well as space in that location of the universe today, expanding more than 2x c velocity. The space.com report,
https://www.space.com/james-webb-space-telescope-detects-earliest-cosmic-web-strand, stated this massive galaxy cluster evolution scenario based upon the filament seen.
"The researchers think that eventually, the filament will condense into a cluster of galaxies, similar to the Coma Cluster, which lies approximately 330 million light-years from Earth.”
I like to keep in mind that the quasar, and redshift reported for the filament is some 6.6 or 6.61 redshift while the Coma Cluster redshift 0.0231 reported,
https://en.wikipedia.org/wiki/Coma_Cluster. When reading galaxy evolution reports like this and the cosmic web, I note we do not know if any evolution took place for the *filamentary structure* (or other gases or quasars) along the comoving radial distance from Earth, more than 28 billion light years away now according to the cosmology calculators using FLRW metric for expanding space.