This low - mass companion was discovered using radial
velocity measurements in 1996, possibly confirming Louis Berman's discovery of a spectroscopic companion to Star B in 1931.
The paper is titled «Demonstration of a near - IR line - referenced electro - optical laser frequency comb for precision radial
velocity measurements in astronomy.»
Demonstration of a Near - IR Laser Comb for Precision Radial
Velocity Measurements in Astronomy
Not exact matches
Measurement of Hydrodynamic Growth near Peak
Velocity in an Inertial Confinement Fusion Capsule Implosion using a Self - Radiography Technique
Measurements of collective fuel
velocities in deuterium - tritium exploding pusher and cryogenically layered deuterium - tritium implosions on the NIF
At one point Fizeau's
measurement of the
velocity of light
in water seemed a conclusive refutation of the corpuscular theory of light; but the latter returned,
in a new form,
in Einstein's theory of photons.
If nothing is found wrong with this neutrino -
velocity measurement, then of course the modern understanding of physics is thrown entirely «up
in the air.»
As detailed
in this video, Laniakea's discovery emerged from
measurements of galactic positions and
velocities that reveal how galaxies are moving
in relation to concentrations of nearby matter and the universe's overall expansion.
Semantic Scholar tries to reveal what's «hot»
in the field by measuring the «
velocity» and «acceleration» of bodies of work,
measurements of how rapidly others are citing certain work, and whether that is trending.
«If you really want to have a precise mass
measurement of the black hole
in a specific galaxy, you'd better use the slightly more cumbersome
velocity dispersion method,» Ferrarese says.
In 1929 Edwin Hubble used these
velocities and his own
measurements of these galaxies» distances from Earth to deduce that the Universe is expanding.
These two figures show the internal waves at Dongsha Island on April 23, 2010, as seen by the radar on TerraSAR - X
in its conventional mode of operation (left) and
in the experimental new mode that permits direct
velocity measurements (right), with the measured surface
velocities shown
in color.
Vogt and Butler's team found the new planet by combining 119 star
velocity measurements from HARPS with 122
measurements taken with a similar instrument called HIRES, which is mounted on the 10 - metre Keck 1 telescope
in Hawaii.
Estimates of data like temperature and wind
velocity also had to be used
in some border areas, which were under control of FARC (the Revolutionary Armed Forces of Colombia) and were not easily accessible for
measurements, he adds.
The research team, led by professor Kazuyo Tsuzuki, had the subjects sleep
in two bedrooms set to the same temperature using ACs set at different airflow
velocities, then made a comparison of the depth of sleep and body temperature control using electroencephalogram (EEG)
measurements as well as subjective reporting by the subjects.
The researchers took
measurements of small - scale temperature and
velocity fluctuations, to measure the diapycnal movements
in the Antarctic Circumpolar Current (ACC) across the Drake Passage region of the Southern Ocean.
«When the electron comes out, we measure its energy and
velocity, and what we found is that electrons coming out of the cadmium arsenide had
measurements that were similar to what is seen
in particles that are massless,» Neupane said.
These seismic
measurements enabled scientists to visualize these ultralow
velocity zones
in some regions along the core - mantle boundary, by observing the slowing down of seismic waves passing through them.
These
velocity measurements led the Dutch astronomer Jan Oort
in 1928 to propose that the Milky Way rotates.
In July 2008, astronomers (Michael Endl and Martin Kürster) analyzed used seven years of differential radial
velocity measurements for Proxima Centauri to submit a paper indicating that large planets are unlikely to be orbiting Sol's closest stellar neighbor within its habitable zone — around 0.022 to 0.054 AU with a corresponding orbital period of 3.6 to 13.8 days.
The Keck / DEIMOS combination is the only one
in the world capable of making these
velocity measurements for large numbers of Andromeda stars.»
Abstract: We report precise radial
velocity (RV)
measurements of WASP - 47, a G star that hosts three transiting planets
in close proximity (a hot Jupiter, a super-Earth and a Neptune - sized planet) and a non-transiting planet at 1.4 AU.
For the super-Earth WA... ▽ More We report precise radial
velocity (RV)
measurements of WASP - 47, a G star that hosts three transiting planets
in close proximity (a hot Jupiter, a super-Earth and a Neptune - sized planet) and a non-transiting planet at 1.4 AU.
The initial transit signal was identified
in KELT - North survey data, and the planetary nature of the occulter was established using a combination of follow - up photometry, high - resolution imaging, high - resolution spectroscopy, and precise radial
velocity measurements.
We measure eclipse timing variations (ETVs), which are then combined with the single - lined radial
velocity measurements to yield masses
in a manner equivalent to double - lined spectroscopic binaries.
As a subgiant star subject to pulsations which affect careful
measurements of variations
in radial
velocity caused by the gravitational pull of substellar companions, astronomers would find it very difficult to detect any Earth - type planet around Beta Hydri using present methods.
We identified the initial transit signal
in the KELT - North survey data and established the planetary nature of the companion through precise follow - up photometry, high - resolution spectroscopy, precise radial
velocity measurements, and high - resolution adaptive optics imaging.
In to - tal, 148 high - quality radial -
velocity measurements were obtained over two observing seasons.
We present new mass
measurements of three of the planets
in the Kepler - 20 system facilitated by 104 radial
velocity measurements from the HARPS - N spectrograph and 30 archival Keck / HIRES observations, as well as an updated photometric analysis of the Kepler data and an asteroseismic analysis of the host star (MStar = 0.948 + -0.051 Msun and Rstar = 0.964 + -0.018 Rsun).
«Geodetic
measurements of vertical crustal
velocity in West Antarctica and the implications for ice mass balance.»
Preliminary Determination of Ice Flow
Velocity in West Antarctica Using High Precision GPS
Measurements, ION - 96 Proceedings, Kansas City, Missouri, September 17 - 20, 1996, 1853 - 1861.
Furthermore, by knowing the mass of a planet from radial
velocity measurements and the radius of a planet based on how much starlight it blocked, it is a simple calculation to determine a planet's density, which can tell astronomers whether that planet is rocky or gaseous
in nature, or whether it has a small core and a thick atmosphere, or whether it has a large core covered
in deep oceans.
In the EDEN / RV component we are utilizing stellar reflex motion (radial
velocity measurements) to search for extrasolar planets around nearby stars.
Putting the
measurements together, the team determined the star is moving at about 1,200 kilometers per second — much higher than the
velocities of previously known stars
in the Milky Way galaxy.
We detected the transit light - curve signature
in the course of the TrES multi-site transiting planet survey, and confirmed the planetary nature of the companion via multicolor photometry and precise radial
velocity measurements.
Recently developed,
in - situ techniques for direct volume determination, acoustic wave
velocity measurements, and x-ray diffraction at HPCAT, along with molecular dynamics simulations, were employed to explore the nature of the unusual and pressure - tunable, compression and elastic properties.
The researchers took high - resolution mean and fluctuating
velocity and density field
measurements in an RM flow, which was shocked and reshocked, to understand production and dissipation
in a two - fluid, developing turbulent flow field.
These involved calculating weights for the
velocity time series from the
measurement uncertainties and adjusting them
in order to minimize the noise level of the combined data.
Optical fiber modal noise
in the 0.8 to 1.5 micron region and implications for near infrared precision radial
velocity measurements
We find that the asteroseismic parameters allow us to test cluster - membership of the stars, and even with the limited seismic data
in hand, we can already identify four possible non-members despite their having a better than 80 % membership probability from radial
velocity measurements.
By contrast, Hubble's
measurements are based on the
velocities of stars whirling around
in the dense cores of globular clusters, which yield a direct
measurement of the black hole masses.
In addition, Tau Ceti does not appear to have a close stellar or substellar companion based on astrometric
measurements (Lippincott and Worth, 1980), radial
velocity variations (Campbell et al, 1988; and near - infrared interferometry (Di Folco et al, 2007).
Misalignments
in a broader class of systems had been predicted as a consequence of torques from wide - orbiting companions, and indeed radial -
velocity measurements revealed a third companion
in a wide orbit
in the Kepler - 56 system.
Kepler 10b was detected using the transit method from more than eight months of data collected by the spacecraft between May 2009 and early January 2010 and confirmed by radial
velocity measurements, and there evidence for another planet (KOI 72.02)
in an outer orbit with a period around 45.3 days (Kepler news release; images, animations, and discovery page; and Batalha et al, 2011).
No hints for the presence of an additional planetary companion
in the two systems were found either from the photometric or radial
velocity measurements.
This gave them 25 small planets
in 12 star systems from radial
velocity measurements.
It was discovered by J.B. Irwin
in 1956, its membership was confirmed by radial
velocity measurements conducted by M.W. Feast of Radcliffs Observatory (the common RV of the cluster members is +4 km / sec).
It can be simply measured using dynamometry by taking multiple
measurements in the same dynamometer of the same joint angle movement, at different angular
velocities.
When different studies use the same angular
velocity for
measurement, these can be compared to one another, so long as differences between the populations tested are acknowledged, and so long as the dynamometer used is the same
in both cases, as differences have been observed between brands (Francis & Hoobler, 1987; Thompson et al. 1989; Gross et al. 1991).
I can determine the standard uncertainty for all the measured variables from statistics It is falsifiable — i can move a body at a certain
velocity for a certain time and measure the traveled distance If the traveled distance does not fit with calculated distance within the uncertainty calculated by using the international standard Guide to the expression of Uncertainty
in Measurement the model might be wrong.