「Redshift」の共起表現一覧(1語右で並び替え)
該当件数 : 82件
| ly large clusters nearly independent of their | redshift, all the way back to the epoch at which clust |
| This | redshift also implies a comoving distance from the ear |
| astronomers observe sources of high | redshift and look for repeating patterns that may indi |
| Doppler | redshift and blueshift. |
| displayed a high | redshift and showed characteristics of a post-starburs |
| ents of the Hubble parameter as a function of | redshift are needed. |
| will differ from the amount of gravitational | redshift as it leaves the region. |
| is also an elliptical galaxy, and displays a | redshift because it is receding from the Milky Way at |
| Using Hubble's law, the | redshift can be used to calculate the distance of an o |
| e performed before the tremendous advances in | redshift cataloging that would be made at the end of t |
| ue colors when compared to similar nearby low | redshift clusters. |
| f 20 km s−1 is placed on the internal Doppler | redshift component of motion in the Coma cluster". |
| of a spiral galaxy, eliminating the intrinsic | redshift component as an effect. |
| ort-hard burst found to that date for which a | redshift could be determined. |
| In order to confirm the | redshift estimated by the color selection, follow-up s |
| ations indicated that Abell 1835 IR1916 has a | redshift factor of z~10.0, |
| dust content and star formation rate in high | redshift galaxies from his comprehensive study of damp |
| eling of quasars- the connection between high | redshift galaxies, active galactic nuclei and their ce |
| e spectroscopy for observing very faint, high | redshift galaxies, and was project scientist for sever |
| At time of the discovery of its | redshift in 1960, this was the remotest object known. |
| "It is especially desirable to determine the | redshift independent of the proper velocities of the o |
| Schmidt noted that | redshift is also associated with the expansion of the |
| Lens | redshift is not the only quantity of interest that can |
| Redshift is a group of educational planetarium and ast | |
| Redshift is planetarium software created by Maris Mult | |
| and then further segregating samples based on | redshift, it is possible to use galaxy-galaxy lensing |
| aham of Trancine in April 2004 indicated that | Redshift make use of a Minimoog and 2 Moog 8*3 sequenc |
| Such a high | redshift means that the burst happened nearly 13 billi |
| tifications across multiple wavelengths, with | redshift measurements for 1.87 million objects, 1.72 b |
| Tired light is a class of hypothetical | redshift mechanisms that was proposed as an alternativ |
| 5 million/14 million light years away, with a | redshift of +243/493 km/s. |
| That burst had a | redshift of 6.7, placing it approximately 190 million |
| This causes the observed mean | redshift of the primary star as a whole to vary from i |
| With a | redshift of 0.545, light from this active galaxy is es |
| the most distant quasar ever observed have a | redshift of 6.96 and 6.43, respectively. |
| sed by the discovery of UDFy-38135539, with a | redshift of 8.6, however it is still the most distant |
| With a | redshift of 5.47, light from this active galaxy is est |
| e universe has been accelerating since around | redshift of z~0.5. |
| Based on a | redshift of 6467 km/s the galaxy is crudely estimated |
| At 12.8 Gly and | redshift of 6.7, the burst was previously the most dis |
| With a | redshift of 0.444, light from this active galaxy is es |
| the universe's creation until a cosmological | redshift of approximately 3400, at which point the exp |
| cally thick to radiation until a cosmological | redshift of approximately 1100, when the universe was |
| Wirtz observed a systematic | redshift of nebulae, which was difficult to interpret |
| lly incorrectly credited with discovering the | redshift of galaxies; these measurements and their sig |
| With a | redshift of 0.464, it is approximately 5 billion light |
| With a | redshift of 0.051, this active galaxy is about 730 mil |
| With an estimated | redshift of 0.021258, the galaxy is about 300 million |
| ingle band is presented, which shows a strong | redshift periodicity of 220 km s−1. |
| young researchers, she organized the Muenster | Redshift Project (MRSP), a method to derive redshifts |
| These findings on | redshift quantization were originally published in 197 |
| laxies in the high-redshift universe (as high | redshift radio galaxies - which also have extended Lym |
| The angular size | redshift relation for a Lambda cosmology, with on the |
| laxies beyond our own local supercluster will | redshift so far that it will become hard to detect the |
| ents are necessary to obtain a high-precision | redshift, spectroscopy is typically much more time-con |
| e relation obtained from observations of high | redshift supernovae. |
| The Center for Astrophysics (CfA) | Redshift Survey was the first attempt to map the large |
| The VIMOS-VLT Deep Survey (VVDS) is a | redshift survey carried out by a collaboration between |
| However, based on | redshift survey data, in 1989 Margaret Geller and John |
| 2003 from the 5-year Two-degree-Field Galaxy | Redshift Survey (2dF) has allowed astronomers to compa |
| The DEEP2 Survey or DEEP2 is a | Redshift survey of the Redshift~1 universe. |
| The first | redshift survey was the CfA Redshift Survey, started i |
| 9 by Margaret Geller and John Huchra based on | redshift survey data from the CfA Redshift Survey. |
| investigator on the ambitious DEEP2 galactic | redshift survey of 50,000 high redshift galaxies. |
| truction of the inner parts of the 2dF Galaxy | Redshift Survey |
| In astronomy, a | redshift survey, or galaxy survey, is a survey of a se |
| matic example of a large-scale structure that | redshift surveys can detect. |
| s of the distribution of matter, e.g., galaxy | redshift surveys. |
| hat was offered was that it was gravitational | redshift that was being measured; this would require a |
| ak galaxies are star-forming galaxies at high | redshift that are selected using the differing appeara |
| Note that beyond a certain | redshift, the angular diameter distance gets smaller w |
| Including the | redshift, this line will be observed at frequencies fr |
| ber 4, 2005: Swift detected GRB 050904 with a | redshift value of 6.29 and a duration of 200 seconds ( |
| Redshift values show that there are approximately 200 | |
| The initial suggestion that local | redshift velocities differ from those seen elsewhere i |
| If the measured | redshift was due to expansion, then the object in ques |
| hat should not be present if the cosmological | redshift was due to a tired light scattering mechanism |
| Schmidt's explanation for the high | redshift was not universally accepted at the time. |
| By combining | redshift with angular position data, a redshift survey |
| , a star large enough to produce the measured | redshift would be well beyond the Hayashi limit. |
| om sources within our own galaxy (even if the | redshift would be so small that it would be hard to me |
| The derived photometric | redshift yielded z approximately equal to 6.5, which i |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると
|
検索履歴を保存できる！
こんにちは ゲスト さん
|
ログイン |
Weblio会員(無料)になると
|
