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Measuring 3-D universe #2

sdpemrofinulighteytt
iiintergalacticnytoi
osnoitautculftthgilo
ntdimensionalaveysss
trnlpsoguarcceegunps
dislvdopwrscxionoerv
ibyivleforestliiedat
surmoyidhlpmovtddrmn
ttomovlteaymeiiniegu
aiseemernesrsnsawsly
noeiadataosogdtponrm
cnctgtirceptfihsdere
edtoeostcejbovexvdpa
seednallowingioetols
rrcitsuocaslxdrdcllu
adlermtpmkraduisownr
snlapawayslxgaewsasi
aucehpvqnaolslscmvgn
uhdpiguugttceasyielg
qfastfneegntielacsas
lyman
apha
forest
allowing
see
clumped
gas
allows
universe
very
far
away
positions
individual
galaxies
sloan
telescope
wide
field
quasars
map
cosmology
measurements
intergalactic
cosmological
distances
early
one
dimensional
fluctuations
density
scale
distribution
matter
dark
energy
uniform
measuring
exspantion
cosmologists
waves
opaque
variations
denser
seeded
acoustic
five
hundred
million
light
years
cosmic
how
fast
exspanding
redshift
light
object
speeding
accelerated
constant
varied
theories

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