'Velocities' web sites
About the institute. institute of astronomy
www.ast.cam.ac.uk 2013-02-28 ⚑r&d
velocities of stars is conducted using the 36.inch telescope in Cambridge. Instrumentation development is also an important area of activity, involving charge coupled devices and detector arrays for rapid recording of very faint light and the design and construction of novel spectrographs. The Institute comprises about 88 postdoctoral staff, 63 graduate students and 26 support staff. There are close links with the Cavendish
www.ast.cam.ac.uk 2013-02-28 ⚑r&d
velocities of stars is conducted using the 36.inch telescope in Cambridge. Instrumentation development is also an important area of activity, involving charge coupled devices and detector arrays for rapid recording of very faint light and the design and construction of novel spectrographs. The Institute comprises about 88 postdoctoral staff, 63 graduate students and 26 support staff. There are close links with the Cavendish
Summer research programme 2013. university of oxford department of physics [..]
www2.physics.ox.ac.uk 2013-03-20 ⚑r&d ⚑blog ⚑enterprise
velocities Supervisor Ed Macaulay, Ryan Houghton Measuring the distribution of the masses of galaxy clusters is one of the ways we can test the CDM cosmological model. The mass is usually inferred from a correlation with the observed x.ray luminosity. In this project, we will try to directly infer the gravitational potential of clusters, by looking at the dispersion of velocities of the galaxies in the cluster. Local galaxy
www2.physics.ox.ac.uk 2013-03-20 ⚑r&d ⚑blog ⚑enterprise
velocities Supervisor Ed Macaulay, Ryan Houghton Measuring the distribution of the masses of galaxy clusters is one of the ways we can test the CDM cosmological model. The mass is usually inferred from a correlation with the observed x.ray luminosity. In this project, we will try to directly infer the gravitational potential of clusters, by looking at the dispersion of velocities of the galaxies in the cluster. Local galaxy
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Oxford supercomputing centre. providing on.demand high performance computing [..]
velocities in specific internal quantum states has proved difficult. The OSC supported this work through the implementation of Hibridon, software for Molecular Inelastic Scattering and Photodissociation on its systems. Search this site Why use high performance computing. HPC is a proven transforming and game.changing technology across all disciplines. Our case studies illustrate some of the ground breaking research enabled by the
Usgs water resources of montana
mt.water.usgs.gov 2013-08-27 ⚑r&d
velocities , and Dispersion Rates in the Missouri River Upstream from Canyon Ferry Lake, Montana In 2010, the U.S. Geological Survey, in cooperation with the Montana Department of Environmental Quality, initiated a dye.tracer study to determine travel times, streamflow velocities , and longitudinal dispersion rates for the Missouri River upstream from Canyon Ferry Lake. For this study, rhodamine WT RWT dye was injected at two
mt.water.usgs.gov 2013-08-27 ⚑r&d
velocities , and Dispersion Rates in the Missouri River Upstream from Canyon Ferry Lake, Montana In 2010, the U.S. Geological Survey, in cooperation with the Montana Department of Environmental Quality, initiated a dye.tracer study to determine travel times, streamflow velocities , and longitudinal dispersion rates for the Missouri River upstream from Canyon Ferry Lake. For this study, rhodamine WT RWT dye was injected at two
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Http://hvo.wr.usgs.gov/volcanowatch/1998/98_08_20.html
velocities can be easily detected. Through seismic refraction studies, USGS seismologists discovered that the Moho was bowed downward by as much as 8 km 4.8 mi beneath Mauna Loa. This flexure of the crust beneath the volcano is due to the weight of the mountain. On top of the downwarped crust is a layer of oceanic sediments. This layer is the plane where most large earthquakes on the island take place. Friday, August 21, was the
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Usgs idaho water science center
velocities , and increased water temperatures as much as 10 F, stressing fish and the macroinvertebrates they feed on. Cold.water adapted macroinvertebrates, such as this stonefly, are good indicators for the health of an ecosystem. Our assessment will track the macroinvertebrate community throughout the Kilpatrick Pond restoration project. On Kilpatrick Pond, we ve installed artificial substrate top inset that aquatic insects can
Systemic console tutorial 3
oklo.org 2014-11-14 ⚑blog
velocities , 16 taken at Lick Observatory during the 1990s, and 155 obtained at Keck observatory over the past eight years The Gl 876 observations come from two different telescopes Lick and Keck. Because the two telescopes have different iodine cells and spectrographs, they have independent radial velocity zero points. this means that both data sets can be adjusted by adding or subtracting a constant baseline velocity from each.
oklo.org 2014-11-14 ⚑blog
velocities , 16 taken at Lick Observatory during the 1990s, and 155 obtained at Keck observatory over the past eight years The Gl 876 observations come from two different telescopes Lick and Keck. Because the two telescopes have different iodine cells and spectrographs, they have independent radial velocity zero points. this means that both data sets can be adjusted by adding or subtracting a constant baseline velocity from each.
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Systemic console tutorial 2
velocities relative to the sinusoidal pattern produced by a single 4.617.day circular orbit suggests that more than one planet may be contributing to the overall radial velocity signal. There are trends in the distribution of points which clearly unfold over periods of hundreds of days and more. Ignore these longer.term trends for the moment, and focus on pinning down the orbit of the 4.617 day planet. Click on the 8220;Mean
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Systemic about
velocities resonance Rossiter.McLaughlin Saturn Spitzer sub.Neptunes super Earths Systemic Console TESS transits Transitsearch TrES.2 TTVs Upsilon Andromedae Valuations WASP.12 WASP.17 WASP.18 Wordpress Categories detection non.technical systemic faq worlds Blogroll ADS query page astro.ph.EP Centauri Dreams Exoplanet Encyclopedia Exoplanet Transit Database Molybdenum The Five Ages Archives April 2014 January 2014 November 2013
Known problems. sdss dr7
www.sdss.org 2012-11-27 ⚑music
velocities Check redshift status zStatus for reliability of redshifts Zero equivalent width emission lines Main survey spectra without tsTargets files or target targetInfo entries in CAS Treatment of galactic extinction correction in spectra Plates with not.quite.perfect spectrophotometry Mismatches between spectra and photometric data Reliability of galaxy velocity dispersion measurements Bonus plates with coverage extending
www.sdss.org 2012-11-27 ⚑music
velocities Check redshift status zStatus for reliability of redshifts Zero equivalent width emission lines Main survey spectra without tsTargets files or target targetInfo entries in CAS Treatment of galactic extinction correction in spectra Plates with not.quite.perfect spectrophotometry Mismatches between spectra and photometric data Reliability of galaxy velocity dispersion measurements Bonus plates with coverage extending
Superdarn
geoscan.jhuapl.edu 2013-02-16 ⚑tech ⚑news
velocities Global Convection Parameters Derived Electric Field Velocity Potential Cross Polar Cap Potential Fit Statistics Spherical Harmonic Coefficients SOFTWARE General Purpose Analysis Software Altitude Adjusted Corrected Geomagnetic Coordinate AACGM System International Geophysical Reference Field Radar Software Toolkit SuperDARN Data Analysis Software Radar Operating System Old SuperDARN Software SuperDARN Data Analysis
geoscan.jhuapl.edu 2013-02-16 ⚑tech ⚑news
velocities Global Convection Parameters Derived Electric Field Velocity Potential Cross Polar Cap Potential Fit Statistics Spherical Harmonic Coefficients SOFTWARE General Purpose Analysis Software Altitude Adjusted Corrected Geomagnetic Coordinate AACGM System International Geophysical Reference Field Radar Software Toolkit SuperDARN Data Analysis Software Radar Operating System Old SuperDARN Software SuperDARN Data Analysis
Cmp. open public shooting
www.thecmp.org 2013-03-10 ⚑tech
velocities of 600 fps or less. Sporter class air rifles Daisy M853 are available as loaners at the range at no cost. We also have the new National Match Air Rifles available to rent for 5.00. Shooters should supply their own pellets or may purchase them at the range for 7.50 pack of 500 pellets. CMP Marksmanship Center North, Camp Perry, OH Open Tuesday and Thursday evenings 5 30PM. 8 00PM, September. December. Please direct any
www.thecmp.org 2013-03-10 ⚑tech
velocities of 600 fps or less. Sporter class air rifles Daisy M853 are available as loaners at the range at no cost. We also have the new National Match Air Rifles available to rent for 5.00. Shooters should supply their own pellets or may purchase them at the range for 7.50 pack of 500 pellets. CMP Marksmanship Center North, Camp Perry, OH Open Tuesday and Thursday evenings 5 30PM. 8 00PM, September. December. Please direct any
Wiggle room calculator. positive incline
positiveincline.com 2016-01-06
velocities optional Historical velocities hv velocities achieved in recent iterations, comma.separated Inputs Planned iterations ni planned iterations Velocity v estimation units achieved on average per iteration Velocity variation vv standard deviation of velocity as percentage of velocity Creep rc estimation units added to backlog per iteration Calculated Effective velocity ev v 8211; rc Iteration length variation lv 1 1 8211;
positiveincline.com 2016-01-06
velocities optional Historical velocities hv velocities achieved in recent iterations, comma.separated Inputs Planned iterations ni planned iterations Velocity v estimation units achieved on average per iteration Velocity variation vv standard deviation of velocity as percentage of velocity Creep rc estimation units added to backlog per iteration Calculated Effective velocity ev v 8211; rc Iteration length variation lv 1 1 8211;
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Release calculator. positive incline
velocities optional Historical velocities hv velocities achieved in recent iterations, comma.separated Inputs Planned release backlog pb estimation units Velocity v estimation units achieved on average per iteration Velocity variation vv standard deviation of velocity as percentage of velocity Creep rc estimation units added to backlog per iteration Calculated Effective velocity ev v 8211; rc Expected iterations 50 confidence ni
Fire on the web
www.fire.nist.gov 2013-03-01 ⚑r&d ⚑tech
velocities cm s are included for two diffusion flame systems. Residential Fire Sprinklers. Two tests are presented that demonstrate how a fire is affected by a sprinkler. Residential Smoke Alarms. In cooperation with the United States Fire Administration, U.S. Consumer Product Safety Commission, and other sponsors,, NIST has evaluated current and emerging smoke alarm technology responses to common residential fire scenarios and
www.fire.nist.gov 2013-03-01 ⚑r&d ⚑tech
velocities cm s are included for two diffusion flame systems. Residential Fire Sprinklers. Two tests are presented that demonstrate how a fire is affected by a sprinkler. Residential Smoke Alarms. In cooperation with the United States Fire Administration, U.S. Consumer Product Safety Commission, and other sponsors,, NIST has evaluated current and emerging smoke alarm technology responses to common residential fire scenarios and
Gro file format
manual.gromacs.org 2012-11-16
velocities in stead of 8 with 3 with 4 for velocities . Upon reading, the precision will be inferred from the distance between the decimal points which will be n 5. Columns contain the following information from left to right residue number 5 positions, integer residue name 5 characters atom name 5 characters atom number 5 positions, integer position in nm, x y z in 3 columns, each 8 positions with 3 decimal places velocity in nm
manual.gromacs.org 2012-11-16
velocities in stead of 8 with 3 with 4 for velocities . Upon reading, the precision will be inferred from the distance between the decimal points which will be n 5. Columns contain the following information from left to right residue number 5 positions, integer residue name 5 characters atom name 5 characters atom number 5 positions, integer position in nm, x y z in 3 columns, each 8 positions with 3 decimal places velocity in nm
Summer research programme 2013. university of oxford department of physics [..]
www2.physics.ox.ac.uk 2013-03-20 ⚑r&d ⚑blog ⚑enterprise
velocities Supervisor Ed Macaulay, Ryan Houghton Measuring the distribution of the masses of galaxy clusters is one of the ways we can test the CDM cosmological model. The mass is usually inferred from a correlation with the observed x.ray luminosity. In this project, we will try to directly infer the gravitational potential of clusters, by looking at the dispersion of velocities of the galaxies in the cluster. Local galaxy
www2.physics.ox.ac.uk 2013-03-20 ⚑r&d ⚑blog ⚑enterprise
velocities Supervisor Ed Macaulay, Ryan Houghton Measuring the distribution of the masses of galaxy clusters is one of the ways we can test the CDM cosmological model. The mass is usually inferred from a correlation with the observed x.ray luminosity. In this project, we will try to directly infer the gravitational potential of clusters, by looking at the dispersion of velocities of the galaxies in the cluster. Local galaxy
Systemic console tutorial 3
oklo.org 2014-11-14 ⚑blog
velocities , 16 taken at Lick Observatory during the 1990s, and 155 obtained at Keck observatory over the past eight years The Gl 876 observations come from two different telescopes Lick and Keck. Because the two telescopes have different iodine cells and spectrographs, they have independent radial velocity zero points. this means that both data sets can be adjusted by adding or subtracting a constant baseline velocity from each.
oklo.org 2014-11-14 ⚑blog
velocities , 16 taken at Lick Observatory during the 1990s, and 155 obtained at Keck observatory over the past eight years The Gl 876 observations come from two different telescopes Lick and Keck. Because the two telescopes have different iodine cells and spectrographs, they have independent radial velocity zero points. this means that both data sets can be adjusted by adding or subtracting a constant baseline velocity from each.
MORE
ⓘ
Systemic console tutorial 2
velocities relative to the sinusoidal pattern produced by a single 4.617.day circular orbit suggests that more than one planet may be contributing to the overall radial velocity signal. There are trends in the distribution of points which clearly unfold over periods of hundreds of days and more. Ignore these longer.term trends for the moment, and focus on pinning down the orbit of the 4.617 day planet. Click on the 8220;Mean
Summer research programme 2013. university of oxford department of physics [..]
www2.physics.ox.ac.uk 2013-03-20 ⚑r&d ⚑blog ⚑enterprise
velocities Supervisor Ed Macaulay, Ryan Houghton Measuring the distribution of the masses of galaxy clusters is one of the ways we can test the CDM cosmological model. The mass is usually inferred from a correlation with the observed x.ray luminosity. In this project, we will try to directly infer the gravitational potential of clusters, by looking at the dispersion of velocities of the galaxies in the cluster. Local galaxy
www2.physics.ox.ac.uk 2013-03-20 ⚑r&d ⚑blog ⚑enterprise
velocities Supervisor Ed Macaulay, Ryan Houghton Measuring the distribution of the masses of galaxy clusters is one of the ways we can test the CDM cosmological model. The mass is usually inferred from a correlation with the observed x.ray luminosity. In this project, we will try to directly infer the gravitational potential of clusters, by looking at the dispersion of velocities of the galaxies in the cluster. Local galaxy
Known problems. sdss dr7
www.sdss.org 2012-11-27 ⚑music
velocities Check redshift status zStatus for reliability of redshifts Zero equivalent width emission lines Main survey spectra without tsTargets files or target targetInfo entries in CAS Treatment of galactic extinction correction in spectra Plates with not.quite.perfect spectrophotometry Mismatches between spectra and photometric data Reliability of galaxy velocity dispersion measurements Bonus plates with coverage extending
www.sdss.org 2012-11-27 ⚑music
velocities Check redshift status zStatus for reliability of redshifts Zero equivalent width emission lines Main survey spectra without tsTargets files or target targetInfo entries in CAS Treatment of galactic extinction correction in spectra Plates with not.quite.perfect spectrophotometry Mismatches between spectra and photometric data Reliability of galaxy velocity dispersion measurements Bonus plates with coverage extending
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