Sentences with phrase «by photometry»

(iii) Far - infrared spectroscopy of dust and ice features will address uncertainties in the mass and composition of dust in galaxies, and the contributions of supernovae to the interstellar dust budget will be quantified by photometry and monitoring of supernova remnants in nearby galaxies.
High - precision radial - velocity measurements confirm a sinusoidal variation with the period and phase predicted by the photometry, and rule out the presence of line - bisector variations that would indicate that the spectroscopic orbit is spurious.
The velocities are indeed noisy, with scatter of 30 m s ^ -1, but exhibit a period and phase consistent with the planet implied by the photometry.

Not exact matches

He was particularly intrigued by a presentation on transit photometry, a theoretical technique that would make it possible to bring those planets into view.
«Thus far, solutions based on incandescent lamps have been used in photometry, i.e. in measuring light detected by the human eye,» explains Tomi Pulli, a doctoral student at Aalto University.
The photometry is obtained from onboard aperture photometry by means of large aperture masks, with a size and shape adapted to the large psf of its exoplanet focal plane, where 50 % of the flux is contained in an elliptical area of about 35 23.
Our longest... ▽ More We present a preliminary analysis of the cool pulsating white dwarf GD 1212, enabled by more than 11.5 days of space - based photometry obtained during an engineering test of the two - reaction - wheel - controlled Kepler spacecraft.
Our latest article, by Eloy Rodríguez, explains how we are using photometry to complement radial velocity data from HARPS.
, by Eloy Rodríguez, explains how we are using photometry to complement radial velocity data from HARPS.
We identify PSO J060.3200 +25.9644 (near - infrared spectral type L1) and PSO J077.1033 +24.3809 (L2) as new members of Taurus based on their VL - G gravity classifications, the consistency of their photometry and proper motions with previously known Taurus objects, and the low probability of contamination by field objects.
No known object reproduces well the properties of planets b and c. Nevertheless, we find that the spectra and WISE photometry of peculiar and / or young early - T dwarfs reddened by submicron grains made of corundum, iron, enstatite, or forsterite successfully reproduce the SED of these two planets.
The characteristics of the host star are well constrained by high - resolution spectroscopy combined with an asteroseismic analysis of the Kepler photometry, leading to an estimated mass and radius of 0.970 + / - 0.060 M... ▽ More A search of the time - series photometry from NASA's Kepler spacecraft reveals a transiting planet candidate orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days.
Considering two different cluster ages (100 and 150 Myr), we selected cluster member candidates on the basis of their location in the (I,I - z) CMD relative to the isochrones, and estimated the contamination by foreground late - type field dwarfs using statistical arguments, infrared photometry and low - resolution optical spectroscopy.
Dedicated spectroscopy earlier this year confirmed the binary nature, the orbit period from photometry, and that the «heartbeat» is caused by the periastron brightening of the system.
The catalog is based on a compilation of literature values for atmospheric properties (temperature, surface gravity, and metallicity) derived from different observational techniques (photometry, spectroscopy, as... ▽ More We present revised properties for 196,468 stars observed by the NASA Kepler Mission and used in the analysis of Quarter 1 - 16 (Q1 - Q16) data to detect and characterize transiting exoplanets.
We manipulate the Tiny Tim PSF FITS files into a format that can be utilized by the effective PSF FORTRAN photometry code.
In order to test if our conclusions are affected by contamination of the Kepler photometry, we have repeated the whole analysis excluding the six binary stars.
Abstract: We present the characterization of the Kepler - 93 exoplanetary system, based on three years of photometry gathered by the Kepler spacecraft.
Communicated by S. K. Pierce, College Park Abstract Six diel TCO2 cycles determined by infrared (IR) photometry from five drift stations occupied between 24 February and 16 March 1979 in the mixed layer of the northwestern Caribbean Sea are examined.
But by comparing the satellite photometry to ground - based observations, it was possible to «calibrate» the satellite photometers, finally yielding very high - quality results (I was part of that effort).
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