The observatory includes three radio telescopes for Very Long Baseline Interferometry (VLBI), which receive radio waves
emitted by quasars.
Not exact matches
It was not until the detection of
quasars, which allow astronomers to see the light
emitted by matter falling into black holes, that we had evidence that they were real objects and not just mathematical curiosities predicted
by Einstein's general theory of relativity.
That was consistent with a
quasar, but dust blocked the definitive
quasar signature of spectral lines
emitted by gas near the black hole.
By gathering the radio signals emitted by any particular quasar at various far - flung points about the globe and measuring the tiny time lag between the signal's arrival at the different locations, people like Ma and Behrend can tell exactly how far apart those locations ar
By gathering the radio signals
emitted by any particular quasar at various far - flung points about the globe and measuring the tiny time lag between the signal's arrival at the different locations, people like Ma and Behrend can tell exactly how far apart those locations ar
by any particular
quasar at various far - flung points about the globe and measuring the tiny time lag between the signal's arrival at the different locations, people like Ma and Behrend can tell exactly how far apart those locations are.
So the astronomers studied light
emitted by 38 faraway
quasars.
The distance to the
quasar is so great (about 10 billion light - years) that the
emitted light is «stretched»
by the expansion of the universe from an invisible ultraviolet wavelength to a visible shade of violet
by the time it reaches the 10 - meter Keck I telescope and the LRIS (Low Resolution Imaging Spectrometer) used for this discovery.
The remote
quasars are so bright that they drown out light
emitted by stars in their proto - galactic clump of stars (more illustrations).
Since these filaments do not
emit any light of their own, the astronomers studied their structure and composition
by analyzing light from distant
quasars as it passed through the cosmic web.
If the
quasar is so distant that the light we observe from it escaped during the «dark ages», its UV light will have been absorbed
by the neutral hydrogen present at the time; if the
quasar is closer and the light we observe was
emitted only after the reionisation, there will have been no neutral hydrogen to impede it (see diagram below).