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On the Nature of the Radio Calibrator and Gamma-Ray Emitting NLS1 Galaxy 3C 286 and Its Multiwavelength Variability
DOI: 10.3390/universe10070289 Bibcode: 2024Univ...10..289K

Komossa, S.; Grupe, D.; Kraus, A. +1 more

The quasar 3C 286, a well-known calibrator source in radio astronomy, was found to exhibit exceptional multiwavelength properties. Its rich and complex optical emission-line spectrum revealed its narrow-line Seyfert 1 (NLS1) nature. Given its strong radio emission, this makes 3C 286 one of the radio-loudest NLS1 galaxies known to date. 3C 286 is a…

2024 Universe
XMM-Newton 1
Scientific Highlights of the AGILE Gamma-ray Mission
DOI: 10.3390/universe10040153 Bibcode: 2024Univ...10..153V

Tavani, Marco; Pittori, Carlotta; Vercellone, Stefano

The γ-ray sky above a few tens of megaelectronvolts (MeV) reveals some of the most powerful and energetic phenomena of our Universe. The Astrorivelatore Gamma ad Immagini LEggero (AGILE) Gamma-ray Mission was launched in 2007 with the aim…

2024 Universe
XMM-Newton 1
X-ray Properties of Two Complementary Samples of Intermediate Seyfert Galaxies
DOI: 10.3390/universe10020069 Bibcode: 2024Univ...10...69D

Berton, Marco; Dalla Barba, Benedetta; Foschini, Luigi +2 more

We present the X-ray spectral analysis of two complementary sets of intermediate Seyfert galaxies (ISs). Analyzing X-ray data, we estimate the hydrogen abundance NH and test its connection with the [O III] luminosity acquired from optical observations. The results confirm the conclusions drawn in a previous study concerning the lack of a direct co…

2024 Universe
XMM-Newton 0
3C 120 Disk/Corona vs. Jet Variability in X-rays
DOI: 10.3390/universe9050212 Bibcode: 2023Univ....9..212F

Fedorova, Elena; Del Popolo, Antonio

The 3C120 (Mrk 1506, UGC 03087, Mrk 9014) is a type 1 Seyfert (Sy1)/broad-line radio galaxy (BLRG) with intriguing variable jet activity featuring "dip" and "outburst" phases. Significant X-ray observational datasets have been collected for 3C120 by INTEGRAL, XMM-Newton, SWIFT, Suzaku, and other X-ray observational facilities. The overall X-ray sp…

2023 Universe
INTEGRAL XMM-Newton 1
Exploring the Fundamental Mechanism in Driving Highest-Velocity Ionized Outflows in Radio AGNs
DOI: 10.3390/universe8110559 Bibcode: 2022Univ....8..559A

Xue, Yongquan; Woo, Jong-Hak; He, Zhicheng +4 more

We investigate the ionized gas kinematics relationship with X-ray, radio and accreting properties using a sample of 348 nearby (z<0.4) SDSS-FIRST-X-ray detected AGNs. X-ray properties of our sample are obtained from XMM-Newton, Swift and Chandra observations. We unveil the ionized gas outflows in our sample manifested by the non-gravitational b…

2022 Universe
XMM-Newton 5
Study of Intra-Day Flux Distributions of Blazars Using XMM-Newton Satellite
DOI: 10.3390/universe8110578 Bibcode: 2022Univ....8..578W

Gaur, Haritma; Wani, Kiran

We present a study of the flux distribution of a sample of 15 Intermediate and Low-energy peaked blazars using XMM-Newton observations in a total of 57 epochs on short-term timescales. We characterise the X-ray variability of all of the light curves using excess fractional variability amplitude and found that only 24 light curves in 7 sources are …

2022 Universe
XMM-Newton 0
Project MOMO: Multiwavelength Observations and Modeling of OJ 287
DOI: 10.3390/universe7080261 Bibcode: 2021Univ....7..261K

Ciprini, S.; Komossa, S.; Gallo, L. C. +9 more

Our project MOMO (Multiwavelength observations and modeling of OJ 287) consists of dedicated, dense, long-term flux and spectroscopic monitoring, and deep follow-up observations of the blazar OJ 287 at >13 frequencies from the radio to the X-ray band since late 2015. In particular, we are using Swift to obtain optical-UV-X-ray spectral energy d…

2021 Universe
XMM-Newton 18
A Long-Term Study of Ultraluminous X-ray Sources in NGC 891
DOI: 10.3390/universe8010018 Bibcode: 2021Univ....8...18E

Earley, Nicholas M.; Dwarkadas, Vikram V.; Cirillo, Victoria

We perform empirical fits to the Chandra and XMM-Newton spectra of three ultraluminous X-ray sources (ULXs) in the edge-on spiral galaxy NGC 891, monitoring the region over a 17-year time window. One of these sources was visible since the early 1990s with ROSAT and was observed multiple times with Chandra and XMM-Newton. Another was visible since …

2021 Universe
XMM-Newton 3
Searching for Gamma-Ray Binaries in Multiwavelength Catalogs
DOI: 10.3390/universe7070214 Bibcode: 2021Univ....7..214M

Luque-Escamilla, Pedro L.; Martí, Josep

The number of gamma-ray binaries currently known is still so small that even a new finding represents a significant expansion of its population. We present a possible hunting strategy based on screening different catalogs to filter potential peculiar stars consistent with gamma-ray sources whose association at lower energies is not yet certain. So…

2021 Universe
XMM-Newton 3