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相关论文: High-redshift quasars and their host galaxies I: k…

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(abriged)In this paper we study different properties of quasars and their host galaxies at high redshifts up to z~3.4. We compare our results to those of other authors and discuss the correlation between galaxy evolution and quasar…

天体物理学 · 物理学 2009-11-13 C. Villforth , J. Heidt , K. Nilsson

I review the current understanding of some key properties of the earliest growing supermassive black holes (SMBHs), as determined from the most up-to-date observations of z>=5 quasars. This includes their accretion rates and growth history,…

星系天体物理 · 物理学 2021-02-02 Benny Trakhtenbrot

We conduct a study of the gas kinematics of two quasar host galaxies at $z\gtrsim6$ traced by the [CII] emission line using ALMA. By combining deep observations at both low and high resolution, we recover the diffuse emission, resolve its…

Recently, the relation between the masses of the black hole ($M_{BH}$) and the host galaxy ($M_{host}$) in quasars has been probed down to the parameter space of $M_{BH}\sim10^8 M_\odot$ and $M_{host}\sim10^{11} M_\odot$ at z $<$ 0.5. In…

星系天体物理 · 物理学 2014-10-14 Jimit Sanghvi , Jari Kotilainen , Renato Falomo , Roberto Decarli , Kalle Karhunen , Michela Uslenghi

ALMA [CII] line and continuum observations of five redshift z>6 quasars are presented. This sample was selected to probe lower black hole mass quasars than most previous studies. We find a wide dispersion in properties with CFHQS…

星系天体物理 · 物理学 2017-12-06 Chris J. Willott , Jacqueline Bergeron , Alain Omont

We measure the evolution of the $M_{\rm BH}-M_*$ relation using 584 uniformly-selected SDSS quasars at $0.2<z<0.8$. The black-hole masses ($M_{\rm BH}$) are derived from the single-epoch virial mass estimator using the H$\beta$ emission…

The growth of the supermassive black holes (BHs) that reside at the centres of most galaxies is intertwined with the physical processes that drive the formation of the galaxies themselves. The evolution of the relations between the mass of…

宇宙学与河外天体物理 · 物理学 2015-05-18 C. M. Booth , Joop Schaye

We apply the empirical method built for z=0 in the previous work of Wang et al. to a higher redshift, to link galaxy stellar mass directly with its hosting dark matter halo mass at z~0.8. The relation of the galaxy stellar mass and the host…

宇宙学与河外天体物理 · 物理学 2015-05-14 Lan Wang , Y. P. Jing

Recent observations from the EIGER JWST program have measured for the first time the quasar-galaxy cross-correlation function at $z\approx6$. The auto-correlation function of faint $z\approx6$ quasars was also recently estimated. These…

We compare observed clustering of quasars and galaxies as a function of redshift, mass, luminosity, & color/morphology, to constrain models of quasar fueling and spheroid-BH co-evolution. High redshift quasars are shown to be drawn from…

We investigate the formation and properties of galaxies hosting z~6 quasars, in the gigaparsec scale cosmological hydrodynamical simulation: MassiveBlack, which includes a self-consistent model for star formation, black hole accretion and…

宇宙学与河外天体物理 · 物理学 2015-06-03 Nishikanta Khandai , Yu Feng , Colin DeGraf , Tiziana Di Matteo , Rupert A. C. Croft

JWST has detected many overmassive galactic systems at $z > 4$, where the mass of the black hole, $M_\bullet$, is $10-100$ times larger than expected from local relations, given the host's stellar mass, $M_\star$. This Letter presents a…

星系天体物理 · 物理学 2024-03-29 Fabio Pacucci , Abraham Loeb

In the local universe, the masses of Super-Massive Black-Holes (SMBH) appear to correlate with the physical properties of their hosts, including the mass of the dark-matter halo. Using these clues as a starting point many studies have…

天体物理学 · 物理学 2015-06-24 Stuart Wyithe , T. Padmanabhan

We study the dependence of the number density and properties of quasars on the background galaxy density using the currently largest spectroscopic datasets of quasars and galaxies. We construct a galaxy number density field smoothed over…

宇宙学与河外天体物理 · 物理学 2016-08-17 Hyunmi Song , Changbom Park , Heidi Lietzen , Maret Einasto

The presence of massive galaxies at high $z$ as recently observed by JWST appears to contradict the current $\Lambda$CDM cosmology. Here we aim to alleviate this tension by incorporating uncertainties from three sources in counting…

星系天体物理 · 物理学 2025-04-08 Yangyao Chen , H. J. Mo , Kai Wang

The tight correlations found between masses of supermassive black holes (SMBHs) and the luminosities, total stellar masses, and velocity dispersions of their host galaxies are often interpreted as a sign of their co-evolution. Studying…

High-redshift quasars ($z\gtrsim6$), powered by black holes (BHs) with large inferred masses, imply rapid BH growth in the early Universe. The most extreme examples have inferred masses of $\sim \! 10^9\,$M$_\odot$ at $z = 7.5$ and $\sim \!…

星系天体物理 · 物理学 2023-11-09 Jake S. Bennett , Debora Sijacki , Tiago Costa , Nicolas Laporte , Callum Witten

The impact of quasars on their galaxy neighbours is an important factor in the understanding of galaxy evolution models. The aim of this work is to characterize the intermediate-scale environments of quasars at low redshift (z $<$ 0.2) with…

宇宙学与河外天体物理 · 物理学 2012-05-11 Beatriz Villarroel

We investigate the evolutionary properties of a sample of quasars at 5<z<6.4 using the semi-analytical hierarchical model GAMETE/QSOdust. We find that the observed properties of these quasars are well reproduced by a common formation…

星系天体物理 · 物理学 2015-06-22 Rosa Valiante , Raffaella Schneider , Stefania Salvadori , Simona Gallerani