「Photometric」の共起表現一覧(1語右で並び替え)
該当件数 : 57件
| p system, the photosensor detects the total | photometric amount of light, from both daylight and ele |
| Photometric and Arecibo echo spectra observations in 20 | |
| l shape with one bright spot, whilst a 1987 | photometric astrometry study concluded the object was s |
| rding to Lockwood (2002), it has a temporal | photometric behavior very similar to the Sun. |
| by G. Henry: The star was observed to have | photometric brightness variations that have same period |
| ents for 1.87 million objects, 1.72 billion | photometric data points, 8.8 million diameter measureme |
| The team also used | photometric data that had been passively collected by a |
| A preliminary search for transits using | photometric data from Fairborn Observatory was inconclu |
| ithout dark matter using only the available | photometric data (stellar matter and visible gas) and a |
| a on the motions of stars in the bulge, the | photometric data alone cannot adjudge among various opt |
| meda Galaxy; the validation of the Stromvil | photometric filter system; evidence for how the shape a |
| A | photometric investigation was performed in 1962 which s |
| on 8-10m class telescopes and mutual events | photometric lightcurve over several months have served |
| Luminance is a | photometric measure of the luminous intensity per unit |
| s a network of telescopes to rapidly sample | photometric measurements of the magnification of stars |
| planet passing in front of its star before | photometric measurements confirmed that the planet was |
| Photometric measurements of the star over 11 years show | |
| ric contamination can also be important for | photometric measurements. |
| mings of lunar and asteroidal occultations; | photometric measures of variable stars, cluster stars, |
| ay, Highway Patrol, Alcohol Unit, Radar and | Photometric, Metro Rail police and an office to coordin |
| Photometric observations in 2007 revealed a ~3 km satel | |
| In 2007, a team of astronomers made | photometric observations of Fennia, and discovered that |
| ed from the Lick and Keck observatories and | photometric observations at Fairborn Observatory reveal |
| Such | photometric observations also reveal the planet's size. |
| For the | photometric observations of asteroids, the department u |
| Luminosities are obtained from | photometric observations, correcting the observed brigh |
| Because it is so bright, | photometric observers must use equipment with very larg |
| llax guide support to NPOI, and it performs | photometric operations support to astrometric studies ( |
| astronomy, with different meanings are the | Photometric parallax method, Spectroscopic parallax, an |
| The | photometric parallax method is a method of data analysi |
| Unlike the stellar parallax method, | photometric parallax can be used to estimate the distan |
| However, modern | photometric photometry has detected a short "horizontal |
| In the 1960s he studied the | photometric properties of the surface of the moon as pa |
| The derived | photometric redshift yielded z approximately equal to 6 |
| is equipped with a 61 cm astrometrical and | photometric reflector with a CCD camera and a 60 cm pho |
| h as the Biuret, and an analysis is made by | photometric spectrum. |
| lusters, stellar variability and pulsation, | photometric studies of nearby galaxies, Quasars, and tr |
| He performed | photometric studies of globular clusters, and deduced t |
| ina with the star SAO 120774, together with | photometric study made at the Lowell Observatory, was c |
| scovery arose from the first year data of a | photometric survey of the M31/M33 subgrouping of the Lo |
| scovery arose from the first year data of a | photometric survey of the M31/M33 subgroupings of the L |
| One of the authors of the Vilnius | photometric system for the classification of stars. |
| escope, with a standardized and homogeneous | photometric system with identical filters, CCDs, calibr |
| extinction problem associated with the UBV | photometric system became evidient, the UBV Photoelectr |
| ightness catalogue that complies to the UBV | photometric system developed by astronomer Harold Johns |
| s mostly remembered for introducing the UBV | photometric system (also called the Johnson or Johnson- |
| Where J is on the 2MASS | photometric system, I and V represent near infrared and |
| photometer can measure in the 7 band Geneva | photometric system. |
| is one of the two colour indices in the UBV | photometric system. |
| It is named after the Stromvil | photometric system. |
| of 4 Hz, changing between the filtersof the | photometric system. |
| Not to be confused with UBV | photometric system. |
| g Antarctic nights to provide high-accuracy | photometric time series for finding extrasolar planets, |
| ctromechanical oscillograph and a system of | photometric units of measurement. |
| Approximately 20% of nights at MJUO are | photometric, with a larger number available for spectro |
| ope has been used primarily for imaging and | photometric work, in which it regularly outperforms muc |
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