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相关论文: Cosmic Evolution of Mass Accretion Rate and Metali…

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Accretion and star formation (SF) rates in low redshift SDSS type-II active galactic nuclei (AGN) are critically evaluated. Comparison with photoionization models indicates that bolometric luminosity (Lbol) estimates based on L(oiii 5007A)…

星系天体物理 · 物理学 2015-05-13 Hagai Netzer

We present black hole masses and accretion rates for 182 Type 1 AGN in COSMOS. We estimate masses using the scaling relations for the broad Hb, MgII, and CIV emission lines in the redshift ranges 0.16<z<0.88, 1<z<2.4, and 2.7<z<4.9. We…

We present a sample of 930 intermediate-mass black hole (IMBH) active galactic nuclei (AGNs) with black hole masses of $M_\mathrm{BH} \leqslant 2 \times 10^{6}$ M$_{\odot}$, uniformly selected from the Seventeenth Data Release of the Sloan…

星系天体物理 · 物理学 2026-05-12 Wen-Juan Liu , Luis C. Ho , Xiao-Bo Dong , Su Yao , Paulina Lira , Yicheng Guo

We analyze UV spectra for a large sample of 578 Type 1 AGNs and derive Eddington ratios, L/Ledd, from the bolometric luminosities and emission line widths for each object in the sample. The sample spans 5 orders of magnitude in supermassive…

天体物理学 · 物理学 2009-11-10 Craig Warner , Fred Hamann , Matthias Dietrich

It was suggested that the prominent feature of the optical Fe II emission has a connection with the accretion process in active galactic nuclei (AGN). For a large sample of 4037 quasars ($z < 0.8$) with measured $\rm H\beta$ line dispersion…

星系天体物理 · 物理学 2022-10-04 Liu Y. S. , Bian W. H.

We present new H and K bands spectroscopy of 15 high luminosity active galactic nuclei (AGNs) at redshifts 2.3-3.4 obtained on Gemini South. We combined the data with spectra of additional 29 high-luminosity sources to obtain a sample with…

天体物理学 · 物理学 2009-11-13 Hagai Netzer , Paulina Lira , Benny Trakhtenbrot , Ohad Shemmer , Iara Cury

We present a comprehensive spectroscopic and variability-based characterisation of a sample of low-luminosity active galactic nuclei (AGNs) hosting low mass black holes, identified by $H\beta$ full width at half maximum (FWHM) $< 2200$ km…

星系天体物理 · 物理学 2025-12-09 Himanshu Sharma , Vivek Kumar Jha , Hum Chand , Swayamtrupta Panda

We have selected a sample of 292 SDSS Narrow-Emission-Line galaxies known to have formed and evolved in relative isolation to study the nature and origin of the AGN phenomenon. The galaxies in our sample have line fluxes with S/N>3 and were…

宇宙学与河外天体物理 · 物理学 2011-06-09 D. M. Neri-Larios , R. Coziol , J. P. Torres-Papaqui , H. Andernach , J. M. Islas-Islas , I. Plauchu-Frayn , R. A. Ortega-Minakata

The FeII/MgII line flux ratio has been used as an indicator of the Fe/Mg abundance ratio in the broad line region (BLR) of active galactic nuclei (AGNs). On the basis of archival rest-frame UV spectra obtained via the Hubble Space Telescope…

星系天体物理 · 物理学 2021-09-08 Jaejin Shin , Jong-Hak Woo , Tohru Nagao , Minjin Kim , Hyeonguk Bahk

Context: X-ray surveys of Active Galactic Nuclei (AGN) indicate `cosmic downsizing', with the comoving number density of high-luminosity objects peaking at higher redshifts (z about 2) than low-luminosity AGN (z<1). Aims: We test whether…

天体物理学 · 物理学 2009-11-13 A. Babic , L. Miller , M. J. Jarvis , T. J. Turner , D. M. Alexander , S. M. Croom

Narrow-Line Seyfert 1 galaxies (NLS1s) and Narrow-Line quasars (NLQs) seem to amount to ~ 10-30 % of active galactic nuclei (AGNs) in the local universe. Together with their average accretion rate, we argue that the black hole (BH) growth…

天体物理学 · 物理学 2009-11-10 T. Kawaguchi , K. Aoki , K. Ohta , S. Collin

From a parent catalog of 561 changing-look active galactic nuclei (CL-AGNs) identified by Guo et al. (2025), we investigate the evolutionary sequence of broad emission lines using a redshift-selected subset (0.35 < z < 0.45) of 54 CL-AGNs…

We show how accretion rate governs the physical properties of a sample of unobscured broad-line, narrow-line, and lineless active galactic nuclei (AGNs). We avoid the systematic errors plaguing previous studies of AGN accretion rate by…

We present near-infrared spectra of ten luminous, intermediate redshift quasars observed with SofI at the NTT of ESO/La Silla. With these rest-frame optical spectra we probe the Hb -[OIII] emission line region. Using the standard scaling…

宇宙学与河外天体物理 · 物理学 2014-11-18 Matthias Dietrich , Smita Mathur , Dirk Grupe , S. Komossa

It is argued that supermassive black holes in the nuclei of galaxies most likely have grown coevally with their host dark matter halos. A calculation based on Press-Schechter within this framework shows that the mean rate of accretion of…

天体物理学 · 物理学 2007-05-23 L. Miller , W. J. Percival , S. M. Croom

We present a census of the active black hole population at 1<z<2, by constructing the bivariate distribution function of black hole mass and Eddington ratio, employing a maximum likelihood fitting technique. The study of the active black…

We compare all the available observational data on the redshift evolution of the total stellar mass and star formation rate density in the Universe with the mass and accretion rate density evolution of supermassive black holes, estimated…

天体物理学 · 物理学 2015-06-24 A. Merloni , G. Rudnick , T. Di Matteo

We present new near infrared spectroscopic measurements of the H_beta region for a sample of 29 luminous high redshift quasars. We have measured the width of H_beta in those sources, and added archival H_beta width measurements, to create a…

天体物理学 · 物理学 2011-03-10 O. Shemmer , H. Netzer , R. Maiolino , E. Oliva , S. Croom , E. Corbett , L. di Fabrizio

(Abridged) Using an empirical relation between the broad line region size and optical continuum luminosity, we estimated the black hole mass and accretion rate for 135 AGNs with double-peaked broad emission lines in two samples. With black…

天体物理学 · 物理学 2009-11-10 Xue-Bing Wu , F. K. Liu
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