Add to ORKGWe summarize the optical, UV, and X-ray properties of double-peaked emitters -- AGN with double-peaked Balmer emission lines believed to originate in the AGN accretion disk. We focus on the X-ray spectroscopic results obtained from a new sample of the 16 broadest Balmer line AGN observed with Chandra and Swift
We have examined a subset of 18 active galactic nuclei (AGNs) drawn from a sample of 81 galaxies tha...
We demonstrate that the disk-wind model for the broad-line region (BLR) can explain the variability ...
We analyse the integral field spectroscopy data for the ≈10 000 galaxies in final data release of th...
Double-peaked Balmer-line profiles originate in the accretion disks of a few percent of optically se...
We present optical and X-ray spectra of a radio-quiet, X-ray-selected AGN, RX J1042 + 1212 (z = 0.27...
In order to examine the prediction that the broad-line radio galaxies (BLRGs) with double-peaked Bal...
The X-ray source CXOXBJ142607.6+353351 (CXOJ1426+35), which was identified in a 172 ks Chandra image...
We present a model which relates the Broad Emission Line Regions of AGN to the accretion mechanism. ...
We study the FeII properties of double-peaked broad low-ionization emission line AGN (dbp emitters) ...
We present results from spectroscopic observations of AT 2018hyz, a transient discovered by the All-...
The X-ray source CXOXBJ142607.6+353351 (CXOJ1426+35), which was identified in a 172 ks Chandra image...
We present the second catalog and data release of optical spectral line measurements and active gala...
Broad (10,000 km s−1), double-peaked emission-line profiles of Balmer lines emitted by active galact...
We present X-ray spectral analysis of XMM-Newton and Chandra observations in the 31.3 deg2 Stripe-82...
We present results from modeling the broadband X-ray spectrum of the Type 1 active galactic nucleus ...
We have examined a subset of 18 active galactic nuclei (AGNs) drawn from a sample of 81 galaxies tha...
We demonstrate that the disk-wind model for the broad-line region (BLR) can explain the variability ...
We analyse the integral field spectroscopy data for the ≈10 000 galaxies in final data release of th...
Double-peaked Balmer-line profiles originate in the accretion disks of a few percent of optically se...
We present optical and X-ray spectra of a radio-quiet, X-ray-selected AGN, RX J1042 + 1212 (z = 0.27...
In order to examine the prediction that the broad-line radio galaxies (BLRGs) with double-peaked Bal...
The X-ray source CXOXBJ142607.6+353351 (CXOJ1426+35), which was identified in a 172 ks Chandra image...
We present a model which relates the Broad Emission Line Regions of AGN to the accretion mechanism. ...
We study the FeII properties of double-peaked broad low-ionization emission line AGN (dbp emitters) ...
We present results from spectroscopic observations of AT 2018hyz, a transient discovered by the All-...
The X-ray source CXOXBJ142607.6+353351 (CXOJ1426+35), which was identified in a 172 ks Chandra image...
We present the second catalog and data release of optical spectral line measurements and active gala...
Broad (10,000 km s−1), double-peaked emission-line profiles of Balmer lines emitted by active galact...
We present X-ray spectral analysis of XMM-Newton and Chandra observations in the 31.3 deg2 Stripe-82...
We present results from modeling the broadband X-ray spectrum of the Type 1 active galactic nucleus ...
We have examined a subset of 18 active galactic nuclei (AGNs) drawn from a sample of 81 galaxies tha...
We demonstrate that the disk-wind model for the broad-line region (BLR) can explain the variability ...
We analyse the integral field spectroscopy data for the ≈10 000 galaxies in final data release of th...