Thus, measuring how much gamma rays of different energies are attenuated or weakened from blazars at different distances from Earth indirectly gives a measurement of how many EBL photons of different wavelengths exist
along the line of sight from blazar to Earth over those different distances.
Rusu's contribution was to measure the distribution of mass
along the line of sight from quasar to telescope.
Not exact matches
Follow - up images and analyses, posted June 30 at arXiv.org, showed that light is probably
from a single bright blue star that coincidentally was behind the galaxy cluster, aligned
along Hubble's
line of sight.
Astronomer Dennis Zaritsky
of the University
of Arizona in Tucson notes that the ring could result
from a chance alignment
of dark matter lumps
along Hubble's
line of sight.
To draw that conclusion, the researchers had to rule out other effects, such as polarization that could arise
from dust particles
along the
line of sight.
The spectra revealed each star's velocity
along our
line of sight, because a star moving towards us shows a blue shift in its spectrum, whereas a star moving away
from us shows a red shift.
From these spectra, researchers can identify the molecules present at every point and determine their velocities (speed plus direction)
along the
line -
of -
sight; this information provides the third dimension — the depth
of the coma.
The calculations take into account radiometer noise, intrinsic variability
of the pulses that causes «jitter noise», pulse broadening
from scattering
along the entire
line of sight, and the finite number
of scintles in the timing data.
Based on the extreme, deduced photometric redshift
of GRB 000131 indicating that the gamma rays had travelled an extreme long cosmological distance, astronomers predicted a «break» in the red region
of the spectrum around 670 to 700 nm
from the strong absorption
of light
from intervening intergalactic hydrogen clouds
along the
line of sight between GRB 000131 and the Solar System.
We detect C3 in absorption arising
from the warm envelope surrounding the... ▽ More We present spectrally resolved observations
of triatomic carbon (C3) in several ro - vibrational transitions between the vibrational ground state and the low - energy nu2 bending mode at frequencies between 1654 - 1897 GHz
along the
sight -
lines to the submillimeter continuum sources W31C and W49N, using Herschel's HIFI instrument.
In 1896 Swedish chemist and Nobel laureate Svante Arrhenius used Langley's bolometer to measure the heat
from the Moon at various altitudes above the horizon in order to estimate the dependence
of atmospheric heat trapping on amount
of water vapor and CO2
along the
line of sight to the Moon, a much longer path near the horizon than at 45 degrees.