Results 1 to 10 of about 3,454,371 (195)
The first public 0.9–4.4 μ m NIRCam images of the North Ecliptic Pole Time Domain Field uncovered galaxies displaying point-source features in their cores as seen in the longer-wavelength filters. We visually identified a sample of 66 galaxies (∼1 galaxy
Rafael Ortiz III +38 more
doaj +1 more source
Mid-infrared Variability in Nearby Galaxies from the MaNGA Sample
We use mid-infrared variability in galaxies to search for active galactic nuclei (AGN) in the local universe. We use a sample of 10,220 galaxies from the Mapping Nearby Galaxies at Apache Point Observatory survey, part of the Sloan Digital Sky Survey ...
Aashay Pai +2 more
doaj +1 more source
A Catalog of Broad Hα and Hβ Active Galactic Nuclei in MaNGA
Broad H α and H β emission lines (FWHM > 1000 km s ^−1 ) are incredibly efficient tracers of the high-velocity clouds encircling active galactic nuclei (AGNs).
James Negus +2 more
doaj +1 more source
We report the discovery of ultrafast outflows (UFOs) in the super-Eddington active galactic nucleus (AGN) IRAS F12397+3333, detected in both the hard- and soft-X-ray bands, and present an investigation of the coronal geometry and accretion flow ...
Deblina Lahiri +2 more
doaj +1 more source
A Comprehensive Analysis of WISE Mid-infrared Colors for Obscured AGN Selection
In this paper, we investigate the robustness of Wide-field Infrared Survey Explorer mid-IR color selection (W1 − W2) for identifying obscured (type 2) active galactic nuclei (AGNs) at low redshift ( z 0.5 selection emerges as optimal in terms of purity
Anika Goel +6 more
doaj +1 more source
The QPO in RE J1034+396 Originates in the Hot Corona
RE J1034+396 is one of the few active galactic nuclei (AGNs) with a significant quasiperiodic oscillation (QPO). The QPO has been observed in over 1 Ms of XMM-Newton observations spanning over a decade. We investigate the power spectral density function (
Chloe S. Taylor +2 more
doaj +1 more source
PACHA: Probing AGN Coronae with High-redshift AGN
The X-ray emission of active galactic nuclei (AGN) is generally attributed to the inverse Compton scattering in a compact corona. In local AGN, directly constraining coronal properties is challenging because the key spectral signature, the high-energy ...
Xiurui Zhao +20 more
doaj +1 more source
We present Stokes I continuum analysis for a volume-limited sample (
Andrew J. Sargent +7 more
doaj +1 more source
VLA FRAMEx. II. Radio Spectra of Nearby Active Galactic Nuclei at Subarcsecond Resolution
We present 4–12 GHz in-band spectral energy distributions with accompanying 6 GHz and 10 GHz imaging results for a volume-complete sample ( 0) spectral indices.
Andrew J. Sargent +7 more
doaj +1 more source

