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Radio galaxies are uncommon $\gamma$-ray emitters, and only low redshift radio galaxies are detected with Fermi-LAT. However, they offer potential insights into the emission mechanisms of active galaxies, particularly as the alignment of…

高能天体物理现象 · 物理学 2020-06-17 Max Harvey , Cameron B. Rulten , Paula M. Chadwick

The anomalous X-ray pulsars (AXPs) represent a growing class of neutron stars discovered at X-ray energies. While the nature of their multi-wavelength emission mechanism is still under debate, evidence has been recently accumulating in…

天体物理学 · 物理学 2009-11-10 Samar Safi-Harb , Jennifer West

The Fermi Gamma-ray Space Telescope was launched more than 13 years ago and since then it has dramatically changed our knowledge of the gamma-ray sky. With more than three billions photons from the whole sky, collected in the energy range…

高能天体物理现象 · 物理学 2022-09-09 Giacomo Principe

We present precise phase-connected pulse timing solutions for 16 gamma-ray-selected pulsars recently discovered using the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope plus one very faint radio pulsar (PSR J1124-5916)…

The Fermi/LAT collaboration recently reported the detection of starburt galaxies in the high energy gamma-ray domain, as well as radio-loud narrow-line Seyfert 1 objects. Motivated by the presence of sources close to the location of…

宇宙学与河外天体物理 · 物理学 2015-05-19 Jean-Philippe Lenain , Claudio Ricci , Marc Türler , Daniela Dorner , Roland Walter

A large fraction of Fermi-Large Area Telescope (LAT) sources in the fourth Fermi-LAT 14 yr catalog (4FGL) still remain unidentified (unIDed). We continued to improve our machine-learning pipeline and used it to classify 1206 X-ray sources…

高能天体物理现象 · 物理学 2024-08-20 Hui Yang , Jeremy Hare , Oleg Kargaltsev

We present results from a Chandra X-ray Observatory study of the field X-ray source population in the vicinity of the radio galaxy MRC 1138-262. Many serendipitous X-ray sources are detected in an area of 8'x8' around the radio source and…

天体物理学 · 物理学 2009-11-07 L. Pentericci , J. D. Kurk , C. L. Carilli , D. E. Harris , G. K. Miley , H. J. A. Rottgering

We present preliminary results of a study of the low frequency radio continuum emission from the nuclei of Giant Low Surface Brightness (LSB) galaxies. We have mapped the emission and searched for extended features such as radio lobes/jets…

天体物理学 · 物理学 2009-11-13 M. Das , S. S. McGaugh , N. Kantharia , S. N. Vogel

In order to understand the interactions between active galactic nuclei (AGN) and star formation during the evolution of galaxies, we investigate 142 galaxies detected in both X-ray and 70{\mu}m observations in the COSMOS (Cosmic Evolution…

宇宙学与河外天体物理 · 物理学 2016-02-23 Ming-Yi Lin , Yasuhiro Hashimoto , Sebastien Foucaud

The Fermi Gamma-ray Space Telescope has detected the gamma-ray glow emanating from the giant radio lobes of the radio galaxy Centaurus A. The resolved gamma-ray image shows the lobes clearly separated from the central active source. In…

高能天体物理现象 · 物理学 2010-06-22 LAT Collaboration

Context: There is a possibility that the optically unidentified radio source J1218+2953 may act as a gravitational lens, producing an optical arc ~4" away from the radio position. Until now, the nature of the lensing object has been…

宇宙学与河外天体物理 · 物理学 2010-05-05 S. Frey , Z. Paragi , R. M. Campbell , A. Moor

Galaxies which strongly deviate from the radio-far IR correlation are of great importance for studies of galaxy evolution as they may be tracing early, short-lived stages of starbursts and active galactic nuclei (AGNs). The most extreme…

星系天体物理 · 物理学 2016-10-26 F. Costagliola , R. Herrero-Illana , A. Lohfink , M. Pérez-Torres , S. Aalto , S. Muller , A. Alberdi

We present the results of deep, high-resolution, 5 GHz Expanded Very Large Array (EVLA) observations of the nearby, dwarf lenticular galaxy and intermediate mass black hole candidate (M ~4.5 x 10^5 M_sun), NGC 404. For the first time, radio…

星系天体物理 · 物理学 2015-06-04 Kristina Nyland , Josh Marvil , Joan Wrobel , Lisa Young , B. Ashley Zauderer

BL Lac objects are an extreme type of active galactic nuclei (AGNs) that belong to the largest population of $\gamma$-ray sources: blazars. This class of AGNs shows a double-bumped spectral energy distribution that is commonly described in…

高能天体物理现象 · 物理学 2020-04-08 E. J. Marchesini , A. Paggi , F. Massaro , N. Masetti , R. D'Abrusco , I. Andruchow , R. de Menezes

Active galactic nuclei (AGN) have been observed as far as redshift z~7. They are crucial in investigating the early Universe as well as the growth of supermassive black holes at their centres. Radio-loud AGN with their jets seen at a small…

星系天体物理 · 物理学 2023-03-20 K. É. Gabányi , S. Belladitta , S. Frey , G. Orosz , L. I. Gurvits , K. Rozgonyi , T. An , H. Cao , Z. Paragi , K. Perger

Low luminosity active galactic nuclei are more abundant and closer to us than the luminous ones but harder to explore as they are faint. We have selected the four sources NGC 315, NGC 4261, NGC 1275, and NGC 4486, which have been detected…

高能天体物理现象 · 物理学 2021-10-13 Gunjan Tomar , Nayantara Gupta , Raj Prince

Using the 100-m Effelsberg radio telescope operating at 1.36 GHz, we have performed a targeted radio pulsar survey of 289 unassociated gamma-ray sources discovered by the Large Area Telescope (LAT) aboard the Fermi satellite and published…

Evidence of efficient acceleration of cosmic rays in massive young stellar objects has been recently reported. Among these massive protostars, S255 NIRS 3 for which extreme flaring events associated with radio jets have been detected, is…

高能天体物理现象 · 物理学 2023-05-31 Emma de Oña Wilhelmi , Rubén López-Coto , Yang Su

PKS 0521-36 is an Active Galactic Nucleus (AGN) with uncertain classification. We investigate the properties of this source from radio to gamma rays. The broad emission lines in the optical and UV bands and steep radio spectrum indicate a…

On May 15th, 2017, the \emph{FERMI}/LAT gamma-ray telescope observed a transient source not present in any previous high-energy catalogue: J1544-0649. It was visible for two consecutive weeks, with a flux peak on May 21st. Subsequently…