[PDF] Top 20 Radio and optical observations of a complete sample of E and SO galaxies
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Radio and optical observations of a complete sample of E and SO galaxies
... the sample interval was set as shown above, but for the February run it was set by the computer to a value of 2sec 6 seconds so that the sampling interval was constant at ... See full document
365
Near-infrared Hubble Space Telescope polarimetry of a complete sample of narrow-line radio galaxies
... nearby sample of NLRG (Ram´ırez et ...the radio jet (Bailey et ...polarization E-vectors perpendicular to the radio jet axis, in addition to dust lanes orientated perpendicu- lar to the ... See full document
10
Are luminous radio-loud active galactic nuclei triggered by galaxy interactions?
... the optical morphologies of a complete sample of 46 southern 2 Jy radio galaxies at intermediate redshifts ...early-type galaxies: 55 ellipticals at redshifts z ≤ 0.01 from the ... See full document
19
CO observations of high-z radio galaxies MRC 2104-242 and MRC 0943-242: spectral-line performance of the Compact Array Broadband Backend
... the optical, barycentric rest-frame velocity at the redshift of MRC 2104−242 and MRC ...through observations of the Lyα and various metal ...our observations on the redshift of the prominent H ... See full document
10
Starbursts and the triggering of the activity in nearby powerful radio galaxies
... a radio galaxy phase, the radio galaxy phase cannot be coeval with the ULIG phase in all ...between optical/UV starburst activity and far-IR luminosity in radio galaxies (Tadhunter et ... See full document
16
Radio observations confirm young stellar populations in local analogues to z ~5 Lyman break galaxies
... configuration. Observations were taken in the L-band, centred at ...VLA. Radio frequency interference (RFI) reduces the effective frequency bandwidth to ∼ ...and optical, their positions are ...the ... See full document
21
Radio spectra of QSOs and galaxies
... means observations were not available , usually because the source was too weak or had too large a sun distance), degree of linear polarization at 1410 and 2650 MHz, and angular separation of radio and ... See full document
320
Kolwa, Sthabile (2019): The kinematic nature of baryons in the multi-phase circumgalactic media of high-redshift radio galaxies. Dissertation, LMU München: Fakultät für Physik
... is radio-optical ...and optical emission which, as mentioned before, tends to be clumpy or discontinuous rather than homo- ...and optical emission tends to be well aligned with the ... See full document
180
The optical and NIR luminous energy output of the Universe : the creation and utilisation of a 9 waveband consistent sample of galaxies using UKIDSS and SDSS observations with the GAMA and MGC spectroscopic datasets
... their sample to be every source brighter than 13th magnitude; a population of just over 1000 ...of radio astron- ...an optical mapping of all sky North of δ = − 30 deg, with imaging taken using red ... See full document
268
Far infrared observations of an unbiased sample of gamma ray burst host galaxies
... Our sample selection is serendipitous, based only on whether the X- ray position of a GRB lies within a large-scale Herschel survey – therefore our sample can be considered completely ...submillimetre ... See full document
10
Optical emission lines in radio sources of intermediate power
... th e results presented in previous chapters. We reinforce th e notio n th a t th e spectral index of th e radio cores in our sam ple are due to th e in trin sic n a tu re of the ... See full document
418
A Hermeneutical Examination of Creation in Islam at Georgia State University
... particularly radio luminous AGN classified as a broad line radio galaxy (BLRG), a quasar, and a FR ...the radio (VLA’s FIRST survey), infrared (2MASS), optical (SDSS), and X-ray (ROSAT) ... See full document
176
P MaNGA galaxies : emission lines properties – gas ionization and chemical abundances from prototype observations
... strong optical lines (Baldwin, Phillips & Terlevich 1981; Veilleux & Oster- brock ...star-forming galaxies, while the right-wing sequence is associated with other ionisa- tion mechanisms, including ... See full document
36
Optical pulse phased observations of faint pulsars with a phase binning CCD camera
... pixels), so that quantum efficiency and throughput fluctuations are not imprinted differentially on the light ...phases, so that by properly coadding a 10-exposure set, each phase bin will have equal ... See full document
115
Comparison of agreement and efficiency of a swept source-optical coherence tomography device and an optical low-coherence reflectometry device for biometry measurements during cataract evaluation
... All included subjects underwent a complete ophthalmic examination by a cornea specialist (PG). Eyes were excluded from the study if they had evidence of corneal or retinal pathology, prior refractive surgery, or ... See full document
7
Influence of light curing and sample thickness on microhardness of a composite resin
... and three sample thicknesses (0.5 mm, 1 mm, and 2 mm). All samples were polymerized with the light tip 8 mm away from the specimen. Knoop microhardness was then measured on the top and bottom surfaces of each ... See full document
5
Comptonization of the cosmic microwave background by relativistic plasma
... of galaxies or at the accretion shock where the matter is falling onto a ...of galaxies and are called ‘cluster radio relics’ (for reviews, see Jaffe 1992 and Fer- etti & Giovannini ...cluster ... See full document
15
Cosmic downsizing of powerful radio galaxies to low radio luminosities
... powers (P . 10 25 W / Hz) out to z & 2. The R11 power range was thus only able to probe the RLF regimes where the cold-mode sources are in the majority, and therefore we could not draw any conclusions about the ... See full document
7
Optical Scattering and Absorption Characteristics of Silver and Silica/ Silver Core/shell Nanoparticles
... Figure. 6 shows the optical properties for silica\silver core\shell nanoparticles with different sizes. The total nanoparticles radius is kept constant at 50 nm. The spectrum with a peak at 498 nm is the ... See full document
5
Independent of DAZL-T54A variant and AZF microdeletion in a sample of Egyptian patients with idiopathic non-obstructed azoospermia
... Regarding the fact that the p.T54A variant of DAZL gene has not been studied in Egyptian infertile men, yet, we screened A and G alleles for A360G variant of the DAZL gene using PCR-RFLP in 170 alleles of Egyptian ... See full document
7
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