Isolated AGNs NGC 5347, ESO 438-009, MCG-02-04-090, and J11366-6002: Swift and NuSTAR joined view
arXiv:2008.05842 · doi:10.1002/asna.202013783
Abstract
We present the spectral analysis with the Nuclear Spectroscopic Telescope Array (NuSTAR) of four isolated galaxies with active galactic nuclei selected from 2MIG catalogue: NGC 5347, ESO 438-009, MCG-02-09-040, and IGR J11366-6002. We also used the Swift/Burst Alert Telescope (BAT) data up to 150 keV for MCG 02-09-040, ESO 438-009, and IGR J11366-6002 as well as the Swift/XRT data in 0.3--10 keV energy band for NGC 5347, ESO 438-009, and IGR J11366-6002. All the sources appear to have the reflected spectrum component with different reflection fractions in addition to the primary power-law continuum. We found that power-law indices for these sources lie between 1.6 to 1.8. The spectra of two sources, NGC 5347 and MCG-02-09-040, show the Fe emission line. For both of these sources, the Fe lines have a large value of EW 1 keV. The X-ray spectrum of NGC 5347 is being best fitted by a pure reflection model with keV and without the presence of any additional primary power-law component. We also found that X-ray spectrum of MCG -02-09-040 shows the presence of heavy neutral obscuration of . However, this provides a non-physical value of reflection in the case with fitting by a simple reflection model. A more appropriate fit is obtained with adopting the physical Monte Carlo based model as BNTorus. It allowed us to determine the absorption value of N and reasonable power-law index of . Results for MCG -02-09-040 are presented for the first time.
11 pages, 3 figures, 3 tables, accepted for publication in Astronomische Nachrichten; any comment welcome
References in corpus (11)
- An XMM-Newton survey of broad iron lines in Seyfert galaxies
- BAT AGN Spectroscopic Survey I: Spectral Measurements, Derived Quantities, and AGN Demographics
- Radiatively Inefficient Accretion in Nearby Galaxies
- Merging and Clustering of the Swift BAT AGN Sample
- Seyfert galaxies in the local Universe (z 0.1): the average X-ray spectrum as seen by
- AGNs and galaxy interactions
- Unveiling the nature of INTEGRAL objects through optical spectroscopy. VI. A multi-observatory identification campaign
- Black hole mass estimation for Active Galactic Nuclei from a new angle
- Catalog of Isolated Galaxies Selected from the 2MASS Survey
- High-order 3D Voronoi tessellation for identifying Isolated galaxies, Pairs and Triplets
- A hard look at NGC 5347: revealing a nearby Compton-thick AGN
Cited by in corpus (4)
- NGC 3521 as the Milky Way near twin: spectral energy distribution from UV to radio decameter ranges
- NGC3521 as the Milky Way analogue: spectral energy distributon from UV to Radio and photometric variability
- Multiwavelength properties of the low-redshift isolated galaxies with active nuclei modelled with CIGALE
- X-ray galaxies selected from HyperLEDA database