proper motions
A technique to derive improved proper motions for kepler objects of interest
... yielding proper motions with higher precision than exists in present catalogs for a sample of stars in the Kepler ...increase proper-motion precision, we combine first-moment centroids of Kepler ...
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Beyond the Blur: Construction and Characterization of the First Autonomous AO System and an AO Survev of Magnetar Proper Motions
... the proper motions of five magnetars with a precision of upto ...magnetar proper motions and proved that magnetar kinematics are equivalent to those of radio ...
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Radio Measurements of the Stellar Proper Motions in the Core of the Orion Nebula Cluster
... the proper motion of several objects were measured by Gómez et ...new proper motions to study the overall Galactic motion of the cluster, its internal kinematics, and to identify radio sources with ...
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High Speed Active Release End Effector Motions for Precise Positioning of Adhered Micro Objects
... other motions, whereas three motions (1D motion in the Y-direction and two circular motions) were not significantly different from each ...other motions, this motion is suitable for successful ...
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The origin of pulsar velocities
... The principle aims of this thesis are to determine the proper motions of as many southern hemisphere pulsars as possible using the Parkes-Tidbinbilla radio interferometer, and use this p[r] ...
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The GALAH survey and Gaia DR2: (non-)existence of five sparse high-latitude open clusters
... for various reasons; their uncertainties are mostly Gaussian and in- dependent, which cannot be said for derived parameters [actions, orbital parameters, (U, V, W) velocities, etc.], and when the radial velocity is not ...
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The Gaia sky: version 1.0
... Although the exploitation of the Gaia DR1 data is still in full swing the next data release will arrive soon, in April 2018. Gaia DR2 will be based on 22 months of input data and allow for a Gaia stand-alone astrometric ...
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Parallaxes of 6 7 GHz methanol masers towards the G 305 2 high mass star formation region
... J 1256 − 6449 (green). Left-hand panel: the sky positions with the first and last epochs labelled. We have opted to show the positions with respect to a single quasar for clarity. The expected positions from the fits are ...
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Candidate gravitational microlensing events for future direct lens imaging
... retain modest lens-source separations of 20 mas and thus are unresolvable with present high-resolution systems. For these events, taking an immediate NIR high-resolution image will allow for a single-epoch estimate of ...
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Very low mass stars and brown dwarfs in Upper Scorpius using Gaia DR1 : mass function, disks, and kinematics
... In this paper, we estimate distance, age and spatial depth from higher-mass Upper Scorpius members (Section 2). We establish new samples of VLM members of Upper Scorpius using photometry from the United Kingdom Infrared ...
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The IPHAS POSS I proper motion survey of the Galactic plane
... lower proper motion survey to probe to previously unexplored proper motions in the Galactic ...IPHAS-UVEX proper motion survey (less then 100 mas/yr for objects brighter the r=19) and leaving ...
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Resolving the distance controversy for Sharpless 269. A possible kink in the outer arm
... the massive young star S 269 IRS 2w (Asaki et al. 2014). In the left panel, the molecular cloud appears as a butterfly with two wings separated by a dark fringe where a B0.5 star has been detected in the center (Mo ff at ...
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Resonant motions of the swinging spring
... With cartesian co-ordinates, it is convenient for analysis of small amplitude motions to move the origin to the point of stable equilibrium; the vertical co-ordinate is then z = 2 t We c[r] ...
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Behavior of the interaction between twin transitional round fountains in a homogeneous fluid, Part 1: experimental study
... flapping motions are present at every stage of the start-up and full development of the interaction, as clearly shown in ...flapping motions become almost constant in the later stages of the time series, ...
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The motions of iron particles on graphite
... The discussion in the previous sections suggests that the abrupt changes in mo- tion correspond to changes in the forces driving the particles. Since these forces are primarily due to particle—particle interactions by ...
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FORECASTING AUDIENCE OF MOTION PICTURES CONSIDERING COMPETITIVE ENVIRONMENT
... emotional motions of social robots and humans in order to understand developmental tendencies of social robots and relations between social robots and emotional ...emotional motions of humans based on six ...
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Feasibility Study on Base Mat Uplift of Nuclear Power Plants Using Large Scale Blast Excitations (Part 1: Measurement and Investigation of Ground Motions)
... We investigated the site characteristics and measured the blast-induced ground motions at BTM [3] in order to confirm that the mine site and ground motions are appropria[r] ...
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Bounds on causal parameters of prospective ground motions and their effect on characteristics of selected ground motions
... ground motions for the purpose of ground-motion selection for scenario and probabilistic seismic hazard analysis (PSHA) is ...Ground motions were selected based on the generalized conditional intensity ...
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Channels as Enzymes: Oxymoron and Tautology Topical Review
... and the friction depend on the dynamics of the protein's internalmotions as well as on the static locations of the atoms of the proteins. Or to put the same thing in a more traditional jargon, the interactions of a ...
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A proper test of overconfidence
... the super…cial appearance of being overcon…dent, we do not …nd any evidence that they are in fact overcon…dent. To our knowledge, the only other experiment that conducts a proper test of a better-than-average ...
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