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Related papers: First Results from BeppoSAX

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Vela X-1 has been observed by the Italian/Dutch X-ray satellite BeppoSAX during its Science Verification Phase. During the ~ 50 ksec observation (orbital phases 0.27-0.34) two different intensity state are present, situation very common in…

Astrophysics · Physics 2007-05-23 M. Orlandini , D. Dal Fiume , L. Nicastro , E. Palazzi , F. Frontera

The high energy experiment PDS is one of the Narrow Field Instruments aboard the X-ray astronomy satellite BeppoSAX. It covers the energy band from 15 to 300 keV. Here we report results on its in-flight performance and observations of…

We present preliminary results on our campaign of observations of the X-ray binary pulsar GX301-2. BeppoSAX observed this source six times in January/February 1998: at the periastron and apoastron, and at other four, intermediate, orbital…

When the first CubeSats were launched nearly two decades ago, few people believed that the miniature satellites would likely prove to be a useful scientific tool. Skeptics abounded. However, the last decade has seen the highly successful…

The broad band sensitivity and flexibility of the BeppoSAX satellite have allowed unprecedented studies of the X-ray emission from blazars. Here we focus on recent results on the SEDs of a group of blazars with emission lines, allowing to…

Astrophysics · Physics 2007-05-23 L. Maraschi , F. Tavecchio

During the operational life of the Italian/Dutch X-ray satellite (1996-2002), BeppoSAX, its two Wide Field Cameras performed observations that covered the full sky at different epochs. Although the majority of analysis performed on BeppoSAX…

High Energy Astrophysical Phenomena · Physics 2015-05-28 F. Capitanio , A. J. Bird , M. Fiocchi , S. Scaringi , P. Ubertini

The European Space Agency's Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009. Its performance is well in line with expectations, and it will continue to gather…

Instrumentation and Methods for Astrophysics · Physics 2016-11-26 Planck Collaboration , P. A. R. Ade , N. Aghanim , M. Arnaud , M. Ashdown , J. Aumont , C. Baccigalupi , M. Baker , A. Balbi , A. J. Banday , R. B. Barreiro , J. G. Bartlett , E. Battaner , K. Benabed , K. Bennett , A. Benoît , J. -P. Bernard , M. Bersanelli , R. Bhatia , J. J. Bock , A. Bonaldi , J. R. Bond , J. Borrill , F. R. Bouchet , T. Bradshaw , M. Bremer , M. Bucher , C. Burigana , R. C. Butler , P. Cabella , C. M. Cantalupo , B. Cappellini , J. -F. Cardoso , R. Carr , M. Casale , A. Catalano , L. Cayón , A. Challinor , A. Chamballu , J. Charra , R. -R. Chary , L. -Y Chiang , C. Chiang , P. R. Christensen , D. L. Clements , S. Colombi , F. Couchot , A. Coulais , B. P. Crill , G. Crone , M. Crook , F. Cuttaia , L. Danese , O. D'Arcangelo , R. D. Davies , R. J. Davis , P. de Bernardis , J. de Bruin , G. de Gasperis , A. de Rosa , G. de Zotti , J. Delabrouille , J. -M. Delouis , F. -X. Dèsert , J. Dick , C. Dickinson , K. Dolag , H. Dole , S. Donzelli , O. Dorè , U. Dörl , M. Douspis , X. Dupac , G. Efstathiou , T. A. Enfllin , H. K. Eriksen , F. Finelli , S. Foley , O. Forni , P. Fosalba , M. Frailis , E. Franceschi , M. Freschi , T. C. Gaier , S. Galeotta , J. Gallegos , B. Gandolfo , K. Ganga , M. Giard , G. Giardino , G. Gienger , Y. Giraud-Hèraud , J. González , J. González-Nuevo , K. M. Górski , S. Gratton , A. Gregorio , A. Gruppuso , G. Guyot , J. Haissinski , F. K. Hansen , D. Harrison , G. Helou , S. Henrot-Versillè , C. Hernández-Monteagudo , D. Herranz , S. R. Hildebrandt , E. Hivon , M. Hobson , W. A. Holmes , A. Hornstrup , W. Hovest , R. J. Hoyland , K. M. Huffenberger , A. H. Jaffe , T. Jagemann , W. C. Jones , J. J. Juillet , M. Juvela , P. Kangaslahti , E. Keihänen , R. Keskitalo , T. S. Kisner , R. Kneissl , L. Knox , M. Krassenburg , H. Kurki-Suonio , G. Lagache , A. Lähteenmäki , J. -M. Lamarre , A. E. Lange , A. Lasenby , R. J. Laureijs , C. R. Lawrence , S. Leach , J. P. Leahy , R. Leonardi , C. Leroy , P. B. Lilje , M. Linden-Vørnle , M. López-Caniego , S. Lowe , P. M. Lubin , J. F. Macìas-Pèrez , T. Maciaszek , C. J. MacTavish , B. Maffei , D. Maino , N. Mandolesi , R. Mann , M. Maris , E. Martìnez-González , S. Masi , M. Massardi , S. Matarrese , F. Matthai , P. Mazzotta , A. McDonald , P. McGehee , P. R. Meinhold , A. Melchiorri , J. -B. Melin , L. Mendes , A. Mennella , C. Mevi , R. Miniscalco , S. Mitra , M. -A. Miville-Deschínes , A. Moneti , L. Montier , G. Morgante , N. Morisset , D. Mortlock , D. Munshi , A. Murphy , P. Naselsky , P. Natoli , C. B. Netterfield , H. U. Nørgaard-Nielsen , F. Noviello , D. Novikov , I. Novikov , I. J. O'Dwyer , I. Ortiz , S. Osborne , P. Osuna , C. A. Oxborrow , F. Pajot , R. Paladini , B. Partridge , F. Pasian , T. Passvogel , G. Patanchon , D. Pearson , T. J. Pearson , O. Perdereau , L. Perotto , F. Perrotta , F. Piacentini , M. Piat , E. Pierpaoli , S. Plaszczynski , P. Platania , E. Pointecouteau , G. Polenta , N. Ponthieu , L. Popa , T. Poutanen , G. Prèzeau , S. Prunet , J. -L. Puget , J. P. Rachen , W. T. Reach , R. Rebolo , M. Reinecke , J. -M. Reix , C. Renault , S. Ricciardi , T. Riller , I. Ristorcelli , G. Rocha , C. Rosset , M. Rowan-Robinson , J. A. Rubiñ-Martìn , B. Rusholme , E. Salerno , M. Sandri , D. Santos , G. Savini , B. M. Schaefer , D. Scott , M. D. Seiffert , P. Shellard , A. Simonetto , G. F. Smoot , C. Sozzi , J. -L. Starck , J. Sternberg , F. Stivoli , V. Stolyarov , R. Stompor , L. Stringhetti , R. Sudiwala , R. Sunyaev , J. -F. Sygnet , D. Tapiador , J. A. Tauber , D. Tavagnacco , D. Taylor , L. Terenzi , D. Texier , L. Toffolatti , M. Tomasi , J. -P. Torre , M. Tristram , J. Tuovinen , M. Türler , M. Tuttlebee , G. Umana , L. Valenziano , J. Valiviita , J. Varis , L. Vibert , P. Vielva , F. Villa , N. Vittorio , L. A. Wade , B. D. Wandelt , C. Watson , S. D. M. White , M. White , A. Wilkinson , D. Yvon , A. Zacchei , A. Zonca

In this contribution we discuss briefly a few calibration items relevant to the data analysis and present some preliminary scientific results. The discussion on instrumental topics focuses on the response matrix and Point Spread Function…

The second Miniature X-ray Solar Spectrometer (MinXSS-2) CubeSat, which begins its flight in late 2018, builds on the success of MinXSS-1, which flew from 2016-05-16 to 2017-05-06. The science instrument is more advanced -- now capable of…

The high spatial resolution of the MECS experiment on board Beppo-SAX has encouraged a few scientists, including the author, to perform observations of galaxy clusters. Results from the analysis of the first few observed objects are…

Astrophysics · Physics 2009-10-30 S. Molendi

BeppoSAX observed several galactic binary X-ray pulsars during the Science Verification Phase and in the first year of the regular program. The complex emission spectra of these sources are an ideal target for the BeppoSAX instrumentation,…

PKS 2155-304 was observed with BeppoSAX in November 1997 for 64 ksec (total elapsed time 33.5 hours) and, for the first time, simultaneously in gamma-rays with EGRET on board the Compton Gamma Ray Observatory and with the ground based TeV…

The Chandra X-Ray Observatory (CXO), the x-ray component of NASA's Great Observatories, was launched on 1999, July 23 by the Space Shuttle Columbia. After satellite systems activation, the first x-rays focussed by the telescope were…

Astrophysics · Physics 2008-11-26 M. C. Weisskopf , B. Brinkman , C. Canizares , G. Garmire , S. Murray , L. P. Van Speybroeck

Planck was successfully launched on May 14th, 2009, from the Kourou space port, in French Guyana. After recalling the objectives that we set out - back in 1996 - to fulfill with this project, I recall some of the technological breakthroughs…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-17 F. R. Bouchet

During its life, BeppoSAX observed several isolated pulsars, giving important contributions to the knowledge of the phenomenology and properties of the X-ray emission from this class of sources. In this paper I review the spectral and…

Astrophysics · Physics 2009-11-10 G. Cusumano

With its large effective area at hard X-rays, high time resolution and having co-aligned other instruments, AstroSat/LAXPC was designed to usher in a new era in rapid variability studies and wide spectral band measurements of the X-ray…

High Energy Astrophysical Phenomena · Physics 2021-06-23 J. S. Yadav , P. C. Agrawal , Ranjeev Misra , Jayashree Roy , Mayukh Pahari , R. K. Manchanda

On the 19th of December 2013, the Gaia spacecraft was successfully launched by a Soyuz rocket from French Guiana and started its amazing journey to map and characterise one billion celestial objects with its one billion pixel camera. In…

We report on the serendipitous discovery of a new X-ray source, SAX J1802.7-2017, ~22' away from the bright X-ray source GX 9+1, during a BeppoSAX observation of the latter source on 2001 September 16-20. SAX J1802.7-2017 remained…

Astrophysics · Physics 2009-11-10 G. Augello , R. Iaria , N. R. Robba , T. Di Salvo , L. Burderi , G. Lavagetto , L. Stella

The in-orbit results and lessons learned of the first Finnish satellite Aalto-1 are briefly presented in this paper. Aalto-1, a three-unit CubeSat which was launched in June 2017, performed AaSI (Aalto Spectral Imager), Radiation Monitor…

Shemar et al. (2016) presented results based on the output of a feasibility study for the European Space Agency (ESA) on the use of X-ray pulsars for deep space navigation, a concept often referred to as 'XNAV'. Here we describe some of the…

Instrumentation and Methods for Astrophysics · Physics 2018-05-16 Setnam Shemar , George Fraser , Lucy Heil , David Hindley , Adrian Martindale , Philippa Molyneux , John Pye , Robert Warwick
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