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相关论文: Radio Emission from Exoplanets

200 篇论文

Of the over 200 known extrasolar planets, 14 exhibit transits in front of their parent stars as seen from Earth. Spectroscopic observations of the transiting planets can probe the physical conditions of their atmospheres. One such technique…

天体物理学 · 物理学 2009-10-16 L. Jeremy Richardson , Drake Deming , Karen Horning , Sara Seager , Joseph Harrington

Annihilation of Dark Matter usually produces together with gamma rays comparable amounts of electrons and positrons. The e+e- gyrating in the galactic magnetic field then produce secondary synchrotron radiation which thus provides an…

天体物理学 · 物理学 2009-08-19 Enrico Borriello , Alessandro Cuoco , Gennaro Miele

With the purpose to investigate the radio emission of new ultracool objects, we carried out a targeted search in the recently discovered system VHS J125601.92$-$125723.9 (hereafter VHS 1256$-$1257); this system is composed by an equal-mass…

太阳与恒星天体物理 · 物理学 2018-02-21 J. C. Guirado , R. Azulay , B. Gauza , M. A. Pérez-Torres , R. Rebolo , J. B. Climent , M. R. Zapatero-Osorio

We extend the source sample recently observed by the Breakthrough Listen Initiative by including additional stars (with parallaxes measured by Gaia) that also reside within the FWHM of the GBT and Parkes radio telescope target fields. These…

天体物理仪器与方法 · 物理学 2020-10-14 B. S. Wlodarczyk-Sroka , M. A. Garrett , A. P. V. Siemion

With the improvements in radio interferometry sensitivity, the quest for coherent radio emission from exoplanets and ultra-cool dwarfs, which is indicative of their magnetic fields, has gained significant momentum in recent years. We…

We present maps of the 22MHz radio emission between declinations -28d and +80d, covering ~73% of the sky, derived from observations with the 22MHz radiotelescope at the Dominion Radio Astrophysical Observatory (DRAO). The resolution of the…

天体物理学 · 物理学 2009-10-31 R. S. Roger , C. H. Costain , T. L. Landecker , C. M. Swerdlyk

We present low-frequency, GMRT (Giant Metrewave Radio Telescope) observations at 333 and 617 MHz of the most-distant giant quasar, J1432+158, which is at a redshift of 1.005. The radio source has a total angular extent of 168 arcsec,…

天体物理学 · 物理学 2009-11-10 A. K. Singal , C. Konar , D. J. Saikia

The Exoplanet Tracker is a prototype of a new type of fibre-fed instrument for performing high precision relative Doppler measurements to detect extra-solar planets. A combination of Michelson interferometer and medium resolution…

天体物理学 · 物理学 2009-11-10 J. C. van Eyken , J. Ge , S. Mahadevan , C. DeWitt

We report on a search for engineered signals from a sample of 692 nearby stars using the Robert C. Byrd Green Bank Telescope, undertaken as part of the $Breakthrough~Listen~Initiative$ search for extraterrestrial intelligence. Observations…

In order to study the nature of the far-infrared emission observed in radio-loud active galaxies, we have obtained 1.2 mm observations with the IRAM 30 m telescope for a sample of eight radio-loud active galaxies. In all objects we find…

天体物理学 · 物理学 2009-11-06 Ilse van Bemmel , Frank Bertoldi

Several binary systems consisting of a massive star and a compact object have been detected above 100 GeV in the Galaxy. In most of these sources, gamma-rays show a modulation associated to the orbital motion, which means that the emitter…

高能天体物理现象 · 物理学 2015-05-18 V. Bosch-Ramon

We report the detection of a new transient radio source, GCRT J1742-3001, located ~1 degree from the Galactic center. The source was detected ten times from late 2006 to 2007 May in our 235 MHz transient monitoring program with the Giant…

There are several methods for indirectly detecting exoplanets, such as transit, radial velocity, astrometry, and the conventional gravitational microlensing approach. These methods rely on observing the effects of exoplanets on the emission…

地球与行星天体物理 · 物理学 2024-07-09 Fatemeh Bagheri , Ramon E. Lopez , Amir Shahmoradi

Direct imaging characterization of extrasolar planets is often done at low spectral resolution. We model the spectrograph for the Gemini Planet Imager upgrade (GPI 2.0) and assess the instrument's potential for allowing observers to…

地球与行星天体物理 · 物理学 2022-08-31 Arlene Aleman , Bruce Macintosh , Mary Anne Limbach , Mark Marley , Jeffrey Chilcote , Quinn Konopacky , Dmitry Savransky

We report the discovery of two isolated radio pulsars having the largest inferred surface dipole magnetic fields yet seen in the population: 4.1e10^13 G and 5.5e10^13 G. These pulsars show apparently normal radio emission in a regime of…

天体物理学 · 物理学 2007-05-23 V. M. Kaspi , F. Camilo , A. G. Lyne , R. N. Manchester , J. F. Bell , N. D'Amico , N. P. F. McKay , F. Crawford

The majority of extrasolar planets discovered to date have significantly eccentric orbits, some if not all of which may have been produced through planetary migration. During this process, any planets interior to such an orbit would…

地球与行星天体物理 · 物理学 2009-12-11 Gareth F. Kennedy , Rosemary A. Mardling

The Search for Extra-Terrestrial Intelligence (SETI) has been conducted for over sixty years, yet no technosignatures have been identified. Previous studies have focused on stars in our galaxy, with few searches in the extragalactic…

高能天体物理现象 · 物理学 2023-04-12 Yuri Uno , Tetsuya Hashimoto , Tomotsugu Goto , Simon C. -C. Ho , Tzu-Yin Hsu , Ross Burns

The binary system, LSI+61 303, is unusual both because of the dramatic, periodic, radio outbursts, and because of its possible association with the 100 MeV gamma-ray source, 2CG135+01. We have performed simultaneous radio and Rossi X-ray…

天体物理学 · 物理学 2009-10-31 F. A. Harrison , P. S. Ray , D. A. Leahy , E. B. Waltman , G. G. Pooley

We present a catalog of Faraday rotation measures (RMs) and redshifts for 4003 extragalactic radio sources detected at 1.4 GHz, derived by identifying optical counterparts and spectroscopic redshifts for linearly polarized radio sources…

宇宙学与河外天体物理 · 物理学 2020-04-02 Alison M. Hammond , Timothy Robishaw , B. M. Gaensler

We consider the magnetic interaction of exoplanets orbiting M-dwarfs, calculating the expected Poynting flux carried upstream along Alfv\'{e}n wings to the central star. A region of emission analogous to the Io footprint observed in…

地球与行星天体物理 · 物理学 2018-02-28 S. Turnpenney , J. D. Nichols , G. A. Wynn , M. R. Burleigh