[PDF] Top 20 Diseño y desarrollo de un sistema POV (Persistence Of Vision) mediante PIC
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What is the Real Shape of the Hubble Diagram, z = H0*D or z+1= eH0*t? Analysis of the SN1a Supernovae and Gamma Ray Burst Redshift/Magnitude Data including the High Redshift Range up to z = 8.1
... RS range from z = 0.031–8.1; nevertheless, much more precise data, especially in the high RS range, are required to confirm our ...the range of 0.034 < z ≤ 8.1, which ... See full document
13
Extended Hubble Diagram on the Basis of Gamma Ray Bursts Including the High Redshift Range of z = 0 0331 8 1
... exponential shape of the HD is to use exclusively GRB data to calculate the HD over the whole RS range of z = ...GRB data to calculate the HD [16] [20] [21] [22] [23] with varying ... See full document
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Modelling and Analysis of the Hubble Diagram of 280 Type SNIa Supernovae and Gamma Ray Bursts Redshifts with Analytical and Empirical Redshift/Magnitude Functions
... an analysis of 280 Type SNIa supernovae and gamma-ray bursts redshifts in the range of z = ...the Hubble diagram is shown to follow a strictly exponential slope ... See full document
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Uniqueness of meromorphic solutions sharing values with a meromorphic function to \(w(z + 1)w(z 1) = h(z)w^{m}(z)\)
... where h(z) is a nonzero rational function and m = ±2, ±1, 0. This idea is partly due to the investigation of the uniqueness of meromorphic solutions of some differential equations (see e.g. [1, 9, ... See full document
174
Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey
... Visual morphologies for the galaxies were obtained from the HST morphology catalogue published by Desai et al. (2007). The mor- phological classifications were carried out by five classifiers, and the final morphology ... See full document
17
Investigating a population of infrared bright gamma ray burst host galaxies
... the burst being at very high redshift, and dust obscuration within the ...the burst is at very high redshift, observed optical bands correspond to rest- frame ultraviolet (UV), ... See full document
53
Uniqueness of meromorphic solutions of the difference equation \(R {1}(z)f(z+1)+R {2}(z)f(z)=R {3}(z)\)
... rem D can happen, and the number of shared values cannot be ...Theorem D and considering Remark 1, instead of trying to improve them directly, we are interested in the following natural ... See full document
11
A Model of Dark Matter and Dark Energy Based on Relativizing Newton’s Physics
... Earth. Real galaxies and galaxy structures are in rotation relative to an Earth’s observer, and the stars and planets in each galaxy are also in continuous ...current analysis. We have already em- barked on ... See full document
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High Redshift LAEs and their Cosmic Evolution: Morphologies, SFR and AGN Activity from z~2 to 6
... at z ∼ 6, more light was able to escape from galaxies, producing an increase in the number of LAEs which are observed ...this redshift has been seen to remain approximately constant, with a characteristic ... See full document
7
The Gamma-ray Activity of the high-z Quasar 0836+71
... The parsec-scale jet of the quasar 0836+71 is strongly core dominated at 43 GHz (Figure 7). We have constructed the light curve of the VLBI core, A0, which shows a good correlation with the mm-wave light curves from the ... See full document
8
Constraining the radio jet proper motion of the high redshift quasar J2134 0419 at z = 4 3
... same data from 2015 ...Fig. 1 clearly show the known compact radio structure with two prominent fea- tures, the westernmost ‘core’ and a jet component to its ...Fig. 1. We also attempted to model it ... See full document
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Morphology and the color mass diagram as clues to galaxy evolution at z∼1
... The distribution of galaxies on color-mass diagrams can be used to study how galaxies evolve. The stellar mass of a galaxy tracks its hierarchical growth via merg- ers, as well as its integrated star formation, and the ... See full document
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Barden, Marco (2004): The Evolution of the Tully-Fisher Relation at Redshift z~1. Dissertation, LMU München: Fakultät für Physik
... full range of disc scale lengths, absolute magnitudes and rotation velocities– in such a way that (subjective) biases (when selecting targets for spectroscopy) get minimised, thus presenting a closer picture of ... See full document
13
Multi Wavelength Properties of Submillimeter Selected Galaxies
... of high- z galaxies selected at other wavelengths are related to SMGs or how collectively the different types of galaxies fit into hierarchical ...different high- z populations has proved very ... See full document
6
The redshift evolution of major merger triggering of luminous AGN : a slight enhancement at z∼2
... type 1 AGN from the COSMOS survey. These AGN occupy a large redshift range ...< z < 2.2) and two orders of magnitude in X-ray luminosity ( ∼ 10 43 - 10 45 erg s -1 ... See full document
11
Far infrared observations of an unbiased sample of gamma ray burst host galaxies
... X- ray position of a GRB lies within a large-scale Herschel survey – therefore our sample can be considered completely ...deep data at wavelengths of 100–500 µ m, we tentatively detected 1 out of 20 ... See full document
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A consistent determination of the temperature of the intergalactic medium at redshift z=2 4
... IGM T– relation at z = ...the high-redshift IGM, which is intimately related to hydrogen and helium reionization and to the characteristics of ionizing ...the T– relation advocated by ... See full document
13
An Empirically Calibrated Model for Interpreting the Evolution of Galaxies during the Reionization Era
... at z ¼ 8:1 Y ...s 1 is 30 Y 86 Mpc 3 . The z ’ 8 Y 8:5 LAE luminosity function (assuming fixed model param- eters from z ¼ 5:7) suggests that three to seven sources ... See full document
83
On the Origin of the Gamma Ray Burst Redshift Distribution in the Early Universe
... Observations of some long GRBs reveal a supernova connection. The most widely accepted mechanism in- volves the collapse of the core of an extremely massive, low-metallicity, rapidly rotating star to form a black hole ... See full document
71
The thermal history of the intergalactic medium down to redshift z=1 5: a new curvature measurement
... in redshift bins of z = 0.2. The error bars show the 1 σ uncertainty obtained with a bootstrap tech- nique generated directly from the curvature measurement within each ...the redshift bins, ... See full document
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