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相关论文: The discovery of X-rays from Venus with Chandra

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On January 10 and 13, 2001, Venus was observed for the first time with an X-ray astronomy satellite. The observation, performed with the ACIS-I and LETG/ACIS-S instruments on Chandra, yielded data of high spatial, spectral, and temporal…

天体物理学 · 物理学 2009-11-07 K. Dennerl , V. Burwitz , J. Englhauser , C. Lisse , S. Wolk

On 4 July 2001, X-rays from Mars were detected for the first time. The observation was performed with the ACIS-I detector onboard Chandra and yielded data of high spatial and temporal resolution, together with spectral information. Mars is…

天体物理学 · 物理学 2009-11-07 Konrad Dennerl

We report the first unambiguous detection of X-ray emission originating from Saturn with a Chandra observation, duration 65.5 ksec with ACIS-S3. Beyond the pure detection we analyze the spatial distribution of X-rays on the planetary…

天体物理学 · 物理学 2009-11-10 J. -U. Ness , J. H. M. M. Schmitt , S. J. Wolk , K. Dennerl , V. Burwitz

Northern auroral regions of Earth were imaged with energetic photons in the 0.1-10 keV range using the High-Resolution Camera (HRC-I) aboard the Chandra X-ray Observatory at 10 epochs (each ~20 min duration) between mid-December 2003 and…

Using the Advanced CCD Imaging Spectrometer (ACIS), the Chandra X-ray Observatory (CXO) observed the Saturnian system for one rotation of the planet (~37 ks) on 20 January, 2004, and again on 26-27 January, 2004. In this letter we report…

Saturn was observed by Chandra ACIS-S on 20 and 26-27 January 2004 for one full Saturn rotation (10.7 hr) at each epoch. We report here the first observation of an X-ray flare from Saturn's non-auroral (low-latitude) disk, which is seen in…

Far-ultraviolet spectra of Venus and Mars in the range 820-1840 A at 4 A resolution were obtained on 13 and 12 March 1995, respectively, by the Hopkins Ultraviolet Telescope (HUT), which was part of the Astro-2 observatory on the Space…

天体物理学 · 物理学 2009-10-31 Paul D. Feldman , Eric B. Burgh , Samuel T. Durrance , Arthur F. Davidsen

The atmosphere of a transiting planet shields the stellar radiation providing us with a powerful method to estimate its size and density. In particular, because of their high ionization energy, atoms with high atomic number (Z) absorb…

地球与行星天体物理 · 物理学 2015-07-02 Fabio Reale , Angelo F. Gambino , Giuseppina Micela , Antonio Maggio , Thomas Widemann , Giuseppe Piccioni

We report the detection at X-rays of the radio/optical jet of 3C 371, from a short (10 ks) Chandra exposure in March 2000. We also present a new MERLIN observation at 1.4 GHz together with a renalysis of the archival HST WFPC2 F555W image.…

天体物理学 · 物理学 2009-11-06 Joseph E. Pesce , Rita M. Sambruna , F. Tavecchio , L. Maraschi , C. C. Cheung , C. Megan Urry , R. Scarpa

We report Venus image observations around the two maximum elongations of the planet at June and October 2015. From these images we describe the global atmospheric dynamics and cloud morphology in the planet before the arrival of JAXA…

The core-dominated radio-loud quasar PKS 0637-752 (z = 0.654) was the first celestial object observed with the Chandra X-ray Observatory, offering the early surprise of the detection of a remarkable X-ray jet. Several observations with a…

The transit of Venus in 2004 offered the rare possibility to remotely sense a well-known planetary atmosphere using ground-based observations for absorption spectroscopy. Transmission spectra of Venus' atmosphere were obtained in the near…

地球与行星天体物理 · 物理学 2015-05-28 P. Hedelt , R. Alonso , T. Brown , M. Collados Vera , H. Rauer , H. Schleicher , W. Schmidt , F. Schreier , R. Titz

Many observers in the past gave detailed descriptions of the telescopic aspect of Venus during its extremely rare transits across the Solar disk. In particular, at the ingress and egress, the portion of the planet's disk outside the Solar…

地球与行星天体物理 · 物理学 2015-06-03 P. Tanga , Th. Widemann , B. Sicardy , J. M. Pasachoff , J. Arnaud , L. Comolli , A. Rondi , S. Rondi , P. Suetterlin

We present a first analysis of a high resolution X-ray spectrum of the ionized stellar wind of Vela X-1 during eclipse. The data were obtained with the High Energy Transmission Grating Spectrometer onboard the Chandra X-ray Observatory. The…

天体物理学 · 物理学 2009-11-07 Norbert S. Schulz , Claude R. Canizares , Julia C. Lee , Masao Sako

We present the observations of the gravitationally lensed system QSO 2237+0305 performed with the Chandra X-ray Observatory on 2000 Sept. 6, and on 2001 Dec. 8 for 30.3 ks and 9.5 ks, respectively. Imaging analysis resolves the four X-ray…

天体物理学 · 物理学 2009-11-07 X. Dai , G. Chartas , E. Agol , M. W. Bautz , G. P. Garmire

We present Chandra and XMM-Newton observations of the composite star-forming/Seyfert galaxy IRAS20051-1117. The X-ray imaging and spectral properties reveal the presence of an active nucleus. The Chandra image shows a strong nuclear point…

天体物理学 · 物理学 2009-11-10 I. Georgantopoulos , I. Papadakis , A. Zezas , M. J. Ward

We report new high-precision observations of the polarization of light scattered from the atmosphere of Venus, made 100 years after the pioneering studies by Bernard Lyot. The new observations include disk-integrated observations in a range…

地球与行星天体物理 · 物理学 2026-03-10 Jeremy Bailey , Daniel V. Cotton , Kimberly Bott , Ievgeniia Boiko

We present the first high-resolution X-ray spectrum of the Seyfert 1.5 galaxy NGC 4151. Observations with the Chandra High Energy Transmission Grating Spectrometer reveal a spectrum dominated by narrow emission lines from a spatially…

天体物理学 · 物理学 2009-10-31 P. M. Ogle , H. L. Marshall , J. C. Lee , C. R. Canizares

We have analyzed data from two sets of calibration observations of the Moon made by the Chandra X-ray Observatory. In addition to obtaining a spectrum of the bright side that shows several distinct fluorescence lines, we also clearly detect…

天体物理学 · 物理学 2009-11-10 B. J. Wargelin , M. Markevitch , M. Juda , V. Kharchenko , R. Edgar , A. Dalgarno

During the last few years our knowledge about the X-ray emission from bodies within the solar system has significantly improved. Several new solar system objects are now known to shine in X-rays at energies below 2 keV. Apart from the Sun,…

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