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The detection of gravitationally redshifted optical emission lines has been reported just for a few active galaxies. In this paper we give a short overview of studies that analyzed or exploited the detection of the gravitational redshift in…

Astrophysics of Galaxies · Physics 2016-02-12 Nataša Bon , Edi Bon , Paola Marziani , Predrag Jovanović

Aims. We quantify the effect of gravitational redshift on emission lines to explore the transition region from the Newtonian to the Einsteinian regime. With the emitting region closer to the Kerr black hole, lines are successively subjected…

Astrophysics · Physics 2007-05-23 Andreas Mueller , Margrethe Wold

We study and quantify gravitational redshift by means of relativistic ray tracing simulations of emission lines. The emitter model is based on thin, Keplerian rotating rings in the equatorial plane of a rotating black hole. Emission lines…

Astrophysics · Physics 2007-05-23 Andreas Mueller

The emission line luminosity function of active galactic nuclei (AGN) is measured from about 3000 AGN included in the main galaxy sample of the Sloan Digital Sky Survey within a redshift range of $0<z<0.15$. The $\Ha$ and [OIII]$\lambda…

Wojtak {\it et al} have stacked 7,800 clusters from the SDSS survey in redshift space. They find a small net blue-shift for the cluster galaxies relative to the brightest cluster galaxies, which agrees quite well with the gravitational…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Nick Kaiser

Gravitational waves from inspiraling compact binaries are known to be an excellent absolute distance indicator, yet it is unclear whether electromagnetic counterparts of these events are securely identified for measuring their redshifts,…

Cosmology and Nongalactic Astrophysics · Physics 2016-04-20 Masamune Oguri

Aims. We investigate the gravitational redshift in clusters of galaxies in the symmetron and Hu-Sawicky $f(R)$ models. The characteristic feature of both models is the screening mechanism that hides the fifth force in dense environments…

Cosmology and Nongalactic Astrophysics · Physics 2014-09-05 Max B. Gronke , Claudio Llinares , David F. Mota

A key observational prediction of Einstein's Equivalence Principle is that light undergoes redshift when it escapes from a gravitational field. Although astrophysics provides a wide variety of physical conditions in which this redshift…

Astrophysics of Galaxies · Physics 2022-04-20 Carlos M. Gutiérrez , Nataliya Ramos-Chernenko

We provide a novel, unifying physical interpretation on the origin, the average shape, the scatter, and the cosmic evolution for the main sequences of starforming galaxies and active galactic nuclei at high redshift z $\gtrsim$ 1. We…

Astrophysics of Galaxies · Physics 2018-06-20 Claudia Mancuso , A. Lapi , J. Shi , J. Gonzàlez-Nuevo , M. Bèthermin , L. Danese

Gravitational redshift as a relativistic effect in cosmological objects is investigated. Possible signatures of the gravitational redshift in measurements of satellite galaxies in clusters of galaxies, intracluster gas, as well as galaxies…

Cosmology and Nongalactic Astrophysics · Physics 2018-03-21 Daiki Sakuma , Ayumu Terukina , Kazuhiro Yamamoto , Chiaki Hikage

The gravitational redshift effect allows one to directly probe the gravitational potential in clusters of galaxies. Following up on Wojtak et al. [Nature (London) 477, 567 (2011)], we present a new measurement. We take advantage of new data…

Cosmology and Nongalactic Astrophysics · Physics 2015-02-23 Iftach Sadeh , Low Lerh Feng , Ofer Lahav

To establish the connection between galaxies and UV-detected absorption systems in the local universe, a deep ($g\leq20$) and wide ($\sim20^{\prime}$ radius) galaxy redshift survey is presented around 47 sight lines to UV-bright AGN…

We propose and apply a new test of Einstein's Equivalence Principle (EEP) based on the gravitational redshift induced by the central super massive black hole of quasars in the surrounding accretion disk. Specifically, we compare the…

Cosmology and Nongalactic Astrophysics · Physics 2021-06-30 E. Mediavilla , J. JimÉnez-Vicente

The recent measurement of the gravitational redshifts of galaxies in galaxy clusters by Wojtak et al. has opened a new observational window on dark matter and modified gravity. By stacking clusters this determination effectively used the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Rupert A. C. Croft

I explore a possibility to measure the gravitational redshift (GR) effect in the gravitational field of massive central nuclei residing in active galaxies (AGN). The activity of central nuclei is associated with the bipolar jet ejection of…

Astrophysics · Physics 2007-05-23 T. G. Arshakian

The large-scale Universal structure comprises strands of dark matter and galaxies with large under-dense volumes known as voids. We measure the fraction of the line of sight that intersects voids for active galactic nuclei (AGN) detected by…

High Energy Astrophysical Phenomena · Physics 2025-01-24 Amy Furniss , Josepf N. Amador , Olivier Hervet , Ollie Jackson , David A. Williams

Averaged spectral energy distributions (SEDs) of active and starburst galaxies from the 12 micron sample in the Local Universe and Quasars, from an optically selected sample at a mean redshift <z>=0.7, are built from optical/near-IR/far-IR…

Astrophysics · Physics 2009-11-10 Paola Andreani , Luigi Spinoglio , Matthew A. Malkan

Based on the gravitational redshift, one prediction of Einstein's general relativity theory, of broad optical emission lines in active galactic nuclei (AGNs), a new method is proposed to estimate the virial factors $f$ in measuring black…

Astrophysics of Galaxies · Physics 2017-02-06 H. T. Liu , H. C. Feng , J. M. Bai

Aims: The knowledge of the redshift of a lensing galaxy that produces multiple images of a background quasar is essential to any subsequent modeling, whether related to the determination of the Hubble constant H_0 or to the mass profile of…

Astrophysics · Physics 2009-11-11 A. Eigenbrod , F. Courbin , G. Meylan

Gravitational redshifts in solar-type main-sequence stars are expected to be some 500 ms$^{-1}$ greater than those in giants. Such a signature is searched for between groups of open-cluster stars which share the same average space motion…

Solar and Stellar Astrophysics · Physics 2015-05-20 L. Pasquini , C. Melo , C. Chavero , D. Dravins , H. -G. Ludwig , P. Bonifacio , R. De La Reza
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