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With the recent observational evidence in extra galactic astronomy, the interpretation of the nature of quasar redshift continues to be a research interest. Very high redshifts are being detected for extragalactic objects that are…

星系天体物理 · 物理学 2024-08-15 Arindam Mal , Sarbani Palit , Christopher C. Fulton , Sisir Roy

We test the periodicity of quasar redshifts in the 2dF and SDSS surveys. In the overall surveys redshift peaks are already apparent in the brighter quasars. But by analyzing sample areas in detail it is shown that the redshifts fit very…

天体物理学 · 物理学 2007-05-23 H. Arp , C. Fulton , D. Roscoe

The quantification of the redshifts of the lines observed in the spectra of the quasars and the galaxies (the redshifts of their lines have some of the values given by the formula z=a+0.062m where a depends on the object, and m is an…

天体物理学 · 物理学 2007-05-23 Jacques Moret-Bailly

A fundamental prediction of relativistic cosmologies is that, due to the expansion of space, observations of the distant cosmos should be time dilated and appear to run slower than events in the local universe. Whilst observations of…

宇宙学与河外天体物理 · 物理学 2023-06-08 Geraint F. Lewis , Brendon J. Brewer

Quasars have long been known to be variable sources at all wavelengths. Their optical variability is stochastic, can be due to a variety of physical mechanisms, and is well-described statistically in terms of a damped random walk model. The…

In this article we present a historical review of study of the redshift periodicity of galaxies, starting from the first works performed in the seventies of the twentieth century until the present day. We discuss the observational data and…

天体物理学 · 物理学 2009-04-15 K. Bajan , P. Flin , W. Godlowski , V. P. Pervushin

Quasars of high redshift may be ejected from a nearby active galaxy of low redshift. This physical association then leads to the suggestion that the redshifts of quasars are not really an indication of their distances. In this…

综合物理 · 物理学 2007-05-23 Ching-Chuan Su

Recent theoretical work determines the correct coupling constant of a scalar field to the Ricci curvature of spacetime in general relativity. The periodicity in the redshift distribution of galaxies observed by Broadhurst {\em et al.}, if…

广义相对论与量子宇宙学 · 物理学 2010-11-30 Valerio Faraoni

In this letter, the old issue of whether redshifts of quasars are of cosmological origin is investigated. We make a plot of absorption redshifts versus emission redshifts for quasars with large amounts of data. Our study shows that, almost…

天体物理学 · 物理学 2007-05-23 Yi-Ping Qin , Guang-Zhong Xie , Xue-Tang Zheng , En-Wei Liang

The large observed redshift of quasars has suggested large cosmological distances and a corresponding enormous energy output to explain the brightness or luminosity as seen at earth. Alternative or complementary sources of redshift have not…

综合物理 · 物理学 2016-09-07 Peter M. Hansen

We have obtained complete redshift information for a sample of 442 radio-loud quasars with flux densities S(11cm) >= 0.25Jy. These come from a completely-identified sample of 878 flat-spectrum radio sources, so there is no optical magnitude…

天体物理学 · 物理学 2007-05-23 P. A. Shaver , I. M. Hook , C. A. Jackson , J. V. Wall , K. I. Kellermann

The introduction of low-frequency radio arrays is expected to revolutionize the study of the reionization epoch. Observation of the contrast in redshifted 21cm emission between a large HII region and the surrounding neutral inter-galactic…

天体物理学 · 物理学 2009-11-13 Stuart Wyithe

Discrete Fourier analysis on the quasar number count, as a function of redshift, $z$, calculated from the Sloan Digital Sky Survey DR6 release appears to indicate that quasars have preferred periodic redshifts with redshift intervals of…

天体物理学 · 物理学 2010-04-14 John G. Hartnett

Measurements of the cosmic redshift drift - the change in redshift of a source over time - will enable independent detection of cosmological expansion thanks to the immense precision soon reached by new facilities such as the Square…

宇宙学与河外天体物理 · 物理学 2025-10-16 Sofie Marie Koksbang , Asta Heinesen , Hayley J. Macpherson

Redshift drift provides a direct kinematic measurement of cosmic acceleration but it occurs with a characteristic time scale of a Hubble time. Thus redshift observations with a challenging precision of $10^{-9}$ require a 10 year time span…

宇宙学与河外天体物理 · 物理学 2015-05-01 Alex G. Kim , Eric V. Linder , Jerry Edelstein , David Erskine

This study investigates the anomalies associated with redshifts from emission lines in certain quasar candidates and the viability of a blueshift interpretation instead. The sample was taken from the Million Quasars Catalog (MILLIQUAS),…

星系天体物理 · 物理学 2024-04-16 Justin Singh , Shirin Haque

The cosmological redshifts z in the frequencies of spectral lines from distant galaxies as compared with their values observed in terrestrial laboratories, which are due to the scale factor a(t), frequently are interpret as a…

综合物理 · 物理学 2011-12-07 Branislav Vlahovic

Two new samples of QSOs have been constructed from recent surveys to test the hypothesis that the redshift distribution of bright QSOs is periodic in $\log(1+z)$. The first of these comprises 57 different redshifts among all known close…

天体物理学 · 物理学 2009-10-31 G. Burbidge , W. M. Napier

Light rays from a multiply imaged quasar usually sample different path lengths across the deflector. Extinction in the lensing galaxy may thus lead to a differential obscuration and reddening between the observed macro-lensed QSO images.…

天体物理学 · 物理学 2007-05-23 C. Jean , J. Surdej

Since the discovery of quasars in papers often appeared and appear the assertions that the redshift quasar distribution includes a periodic component with the period $\Delta z = 0.063$ or 0.11. A statement of such kind, if it is correct,…

宇宙学与河外天体物理 · 物理学 2015-05-20 Serge V. Repin , Boris V. Komberg , Vladimir N. Lukash
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