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Centaurus A, the cosmic ray accelerator a few Mpc away from us is possibly one of the nearest sources of extremely high energy cosmic rays. We investigate whether the gamma ray data currently available from Centaurus A in the GeV-TeV energy…

天体物理学 · 物理学 2009-06-23 Nayantara Gupta

We report the discovery of high-energy (E>100 MeV) gamma-ray emission from NGC 1275, a giant elliptical galaxy lying at the center of the Perseus cluster of galaxies, based on observations made with the Large Area Telescope (LAT) of the…

Over the last few years, the data obtained using the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope has provided new insights on high-energy processes in globular clusters, particularly those involving compact objects…

高能天体物理现象 · 物理学 2017-02-22 P. H. Thomas Tam , C. Y. Hui , Albert K H. Kong

FERMI-LAT is performing an all-sky gamma-ray survey from 30 MeV to $>$300 GeV with unprecedented sensitivity and angular resolution. FERMI has detected high-energy gamma rays from the Moon and Sun since the first weeks of data taking. This…

太阳与恒星天体物理 · 物理学 2019-08-14 N. Giglietto

We report the ALMA Band 7 observations of 86 Herschel sources that likely contain gravitationally-lensed galaxies. These sources are selected with relatively faint 500 $\mu$m flux densities between 15 to 85 mJy in an effort to characterize…

We searched high resolution spectra of 5600 nearby stars for emission lines that are both inconsistent with a natural origin and unresolved spatially, as would be expected from extraterrestrial optical lasers. The spectra were obtained with…

天体物理仪器与方法 · 物理学 2017-05-24 Nathaniel K. Tellis , Geoffrey W. Marcy

We present evidence for $\gamma$-ray emission from a stacked population of 39 high-latitude globular clusters (GCs) not detected in the Fermi Point Source Catalog, likely attributable to populations of millisecond pulsars within them. In…

高能天体物理现象 · 物理学 2024-10-17 Owen K. Henry , Timothy A. D. Paglione , Yuzhe Song , Joshua Tan , David Zurek , Vanessa Pinto

The {\gamma}-ray data of Fermi-LAT on the giant lobes of Centaurus A are analysed together with the high frequency radio data obtained with the Planck satellite. The large {\gamma}-ray photon statistics, accumulated during seven years of…

高能天体物理现象 · 物理学 2017-08-09 Xiao-na Sun , Rui-zhi Yang , Benjamin Mckinley , Felix Aharonian

Galaxy clusters are the largest gravitationally bound objects in the universe and may be suitable targets for indirect dark matter searches. With 85 months of Fermi-LAT Pass 8 publicly available data, we analyze the gamma-ray emission in…

高能天体物理现象 · 物理学 2016-05-27 Yun-Feng Liang , Zhao-Qiang Shen , Xiang Li , Yi-Zhong Fan , Xiaoyuan Huang , Shi-Jun Lei , Lei Feng , En-Wei Liang , Jin Chang

Centaurus A (Cen A) is a bright radio source associated with the nearby galaxy NGC 5128 where high-resolution radio observations can probe the jet at scales of less than a light-day. The South Pole Telescope (SPT) and the Atacama Pathfinder…

We have searched for nonastrophysical emission lines in the optical spectra of 577 nearby F, G, K, and M main-sequence stars. Emission lines of astrophysical origin would also have been detected, such as from a time--variable chromosphere…

天体物理学 · 物理学 2015-06-24 Amy E. Reines , Geoffrey W. Marcy

Gravitational lensing is a potentially powerful tool for elucidating the origin of gamma-ray emission from distant sources. Cosmic lenses magnify the emission from distance sources and produce time delays between mirage images.…

高能天体物理现象 · 物理学 2015-08-19 Anna Barnacka , Margaret J. Geller , Ian P. Dell'Antonio , Wystan Benbow

The detection of high energy (HE) {\gamma}-ray emission up to about 3 GeV from the giant lobes of the radio galaxy Centaurus A has been recently reported by the Fermi-LAT Collaboration based on ten months of all-sky survey observations. A…

高能天体物理现象 · 物理学 2015-03-19 Rui-zhi Yang , Narek Sahakyan , Emma de Ona Wilhelmi , Felix Aharonian , Frank Rieger

During its first six years of operation, the Fermi Large Area Telescope (LAT) has detected >30 MeV gamma-ray emission from more than 40 solar flares, nearly a factor of 10 more than those detected by EGRET. These include detections of…

高能天体物理现象 · 物理学 2019-08-14 N. Omodei , V. Petrosian , W. Liu , F. Rubio da Costa , Q. Chen , M. Pesce-Rollins , E. Grove , F. Longo

We report simultaneous observations of the nearby flare star Proxima Centauri with VLT/UVES and XMM-Newton over three nights in March 2009. Our optical and X-ray observations cover the star's quiescent state, as well as its flaring activity…

太阳与恒星天体物理 · 物理学 2015-05-30 B. Fuhrmeister , S. Lalitha , K. Poppenhaeger , N. Rudolf , C. Liefke , A. Reiners , J. H. M. M. Schmitt , J. -U. Ness

The Fermi Large Area Telescope (LAT) is the most sensitive instrument ever deployed in space for observing gamma-ray emission >100 MeV. This sensitivity has enabled the LAT to detect gamma-ray emission from the Sun during quiescent periods…

高能天体物理现象 · 物理学 2013-04-04 N. Omodei , V. Petrosian , M. Pesce-Rollins , the Fermi-LAT Collaboration

We report the results of a survey of the Galactic Center region (|l| < 2deg, |b| < 0.5deg) performed with the BeppoSAX satellite. The flux from the center of our Galaxy corresponds to a luminosity of ~3 10^{35} erg/s in the 2-10 keV range.…

天体物理学 · 物理学 2009-10-31 L. Sidoli , S. Mereghetti , G. L. Israel , L. Chiappetti , A. Treves , M. Orlandini

There are $\sim 1$, 0.1 and 0.01 gravitationally lensed X-ray sources per square degree with soft X-ray fluxes exceeding $10^{-15}, 10^{-14}$ and $10^{-13} ergs/s cm^{-2}$ respectively. These sources will be detected serendipitously with…

天体物理学 · 物理学 2009-10-31 J. A. Munoz , C. S. Kochanek , E. E. Falco

With today's millimeter and submillimeter instruments observers use gravitational lensing mostly as a tool to boost the sensitivity when observing distant objects. This is evident through the dominance of gravitationally lensed objects…

天体物理学 · 物理学 2007-05-23 Tommy Wiklind , Danielle Alloin

$\alpha$ Centauri A is the closest solar-type star to the Sun and offers the best opportunity to find and ultimately to characterize an Earth-sized planet located in its Habitable Zone (HZ). Here we describe initial results from an ALMA…

太阳与恒星天体物理 · 物理学 2021-06-23 Rachel Akeson , Charles Beichman , Pierre Kervella , Edward Fomalont , G. Fritz Benedict