Спутник ФКИ. Suzaku. [Редактировать]

Запущенный 10 июля 2005 года, спутник «Судзаку» был разработан в японском Институте исследования космоса и развития астронавтики (ISAS), который является подразделением Японского агентства по исследованию воздушно-космического пространства (JAXA), в тесном сотрудничестве с НАСА и другими японскими и американскими организациями. По своему целевому предназначению аппарат является рентгеновским и гамма-телескопом, предназначенным для изучения чёрных дыр и сверхновых звёзд. К моменту запуска на орбите уже находилось два рентгеновских телескопа — XMM-Newton и Чандра. Однако новый телескоп принципиально отличается от них: в то время как в последних применяются рентгеновские призмы, в Suzaku используются зеркала. Но главное отличие в том, что электроника фиксирует малейшее изменение температуры датчика, происходящее при поглощении им фотонов рентгеновского и гамма-спектра. Для реализации этого датчик был охлаждён до температуры 0,06 градусов выше абсолютного ноля. Это стало возможным после применения многослойной изоляции: первый слой — жидкий гелий, второй — неоновый лёд. Вся конструкция помещена в специальный термос. Предполагалось, что данная изоляция сможет действовать в течение 2—3 лет. Это должно было обеспечивать работу главного инструмента Astro-EII — XRS (рентгеновский спектрометр). После данного срока XRS должен был завершить работу, но фотокамера (XIS) и детектор высокоэнергетических рентгеновских лучей (HXD) продолжат работу. По расчётам чувствительность и разрешение телескопа в 10 раз превосходят значения этих показателей у предшественников.

Дополнительные наименования

#НаименованияПоиск в новостяхПоиск в документах
1Astro-E2НайтиНайти
228773НайтиНайти

Дополнительная классификация

#Наименования
1Страна оператор(владелец) - Япония
2Страна оператор(владелец) - США
3Тип оператора(владельца) - государственный
4Тип орбиты - НОО
5Страна производитель - Япония

Новостная лента[Найти информацию в новостях] [Найти информацию в документах]

#Новостная лента.
12005-08-08. Отказ X-ray спектрометраТэги: Suzaku

Технические характеристики

#ХарактеристикаЗначение
1Масса, кг1600

Характеристики орбиты

#ХарактеристикаЗначение
1Наклонение, град31.4
2Апогей, км551.7
3Апогей, км551.4
4Перигей, км544.5
5Перигей, км544.4
6Период, минут95.5
7Длинный диаметр эллипса, км6919
8Длинный диаметр эллипса, км6918

Пусковые характеристики

#ХарактеристикаЗначение
1Код NSSDC2005-025A

Информация об удачном запуске

#ХарактеристикаЗначение
1Дата пуска2005-07-10 at 03:30:00 UTC
2Полезная нагрузка 1xSuzaku
3Ракета-носитель 1xM-5

Найдено 510 документов по запросу «Suzaku». [Перейти к поиску]


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0.67/5
...) doi:10.1093/mnras/stu2395 A Suzaku view of IGR J16393–4643... and spectrum analysis from a 44ks Suzaku observation of the source. The... IGR J16393–4643 obtained from a Suzaku observation. We also present results... on December 17, 2014 ABSTRACT Suzaku view of IGR J16393–4643... from the Suzaku Guest Observer Facility.4 3 T I M I N G A N A LY S I S 2 O B S E RVAT I O N S A N D DATA A N A LY S I S Suzaku is... J16393–4643 was observed with Suzaku during 2010 March 12 (ObsId... screening criteria described in the Suzaku ABC guide.1 The XIS light... the orbital phase of the Suzaku observation. The minimum of the... eclipse semi-angle θ E ∼ 17◦ . The Suzaku observations were carried out roughly.../suzaku/analysis/abc/node9.html http://heasarc.gsfc.nasa.gov/docs/suzaku/analysis/pinbgd.html 3 http://heasarc.gsfc.nasa.gov/docs/suzaku....nasa.gov/docs/heasarc/caldb/suzaku MNRAS 446, 4148–4154 (2015... profiles is highlighted in this Suzaku observation. Due to the presence... at epoch MJD 53417.955. Suzaku view of IGR J16393–4643...) (10−11 erg cm−2 s−1 ) χν2 /d.o.f 25+1 −3 3.7+0.8 −0.6 Suzaku view of IGR J16393–4643... IGR J16393–4643 in the Suzaku energy sub-bands. The pulse... the Suzaku observation. Due to the limited statistical quality of this Suzaku... out in this broad-band Suzaku observation. IGR J16393–4643 makes...



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0.16/5
.../suzaku/analysis/abc/ Postscript - ftp://legacy.gsfc.nasa.gov/suzaku/doc/general/suzaku abc guide.ps.gz PDF - ftp://legacy.gsfc.nasa.gov/suzaku/doc/general/suzaku abc guide.pdf For news on the Suzaku.../docs/suzaku/aehp proc.html http://heasarc.gsfc.nasa.gov/docs/suzaku/analysis/watchout.html http://heasarc.gsfc.nasa.gov/docs/suzaku/analysis/suzakumemos.html http://www.astro.isas.jaxa.jp/suzaku/process/caveats/ http://www.astro.isas.jaxa.jp/suzaku/analysis/xis Users are encouraged to contact the Suzaku Guest... 2 2 Software 3 2.1 CALDB . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 2.2 XSELECT . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 2.3 XANADU . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 2.4 Profit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 3 Suzaku Data Specifics and Conventions 3.1 6 Directory... . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9 3.3 Suzaku Coordinates . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9 3.4 Photon Energies and Pulse Heights . . . . . . . . . . . . . . . . . . . . . . . 10 3.5 Timing Information . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11 3.6 Suzaku... analysis and the Suzaku instruments and want to use Suzaku data to extract scientific results. General information on the Suzaku satellite may be obtained from the Suzaku Guest Observer Facility (GOF) page, http://suzaku.gsfc.nasa.gov. Readers who are not familiar with the Suzaku....gsfc.nasa.gov/docs/suzaku/prop tools/suzaku td. This document is... called the “Suzaku FTOOLS”. By using the Suzaku FTOOLS Suzaku users can recalibrate....nasa.gov/docs/suzaku/analysis/suzaku ftools.html. Since Suzaku data files are... the Suzaku GOF will focus support on using HEAsoft to analyze Suzaku... Suzaku data, especially for users not familiar with X-ray spectroscopy. Chapter 3 Suzaku Data Specifics and Conventions This chapter describes the contents of Suzaku... the Suzaku archive at http://heasarc.gsfc.nasa.gov/docs/suzaku/aehp....nasa.gov/docs/suzaku/aehp data analysis.html. 3.3 Suzaku Coordinates The XIS... Information The Suzaku event arrival time is represented by the “Suzaku time... Suzaku data, and has access to the latest versions of the Suzaku....jp/suzaku/log/operation/, http://www.astro.isas.jaxa.jp/suzaku/log/hxd/, and http://www.astro.isas.jaxa.jp/suzaku... of. 4. Via the Suzaku GOF web site. The Suzaku Data Analysis page: http://heasarc.gsfc.nasa.gov/docs/suzaku/aehp.../docs/suzaku/analysis/gso newgain.html. 4.4 Barycentric Correction Aebarycen is a Suzaku specific FTOOL to perform barycentric corrections for Suzaku event and...:SUZAKU-XIS-1-STANDARD > filter region xsel:SUZAKU-XIS-1-STANDARD > extract all xsel:SUZAKU-XIS-1-STANDARD > plot image xsel:SUZAKU-XIS-1-STANDARD > plot curve xsel:SUZAKU-XIS-1-STANDARD > plot spectrum xsel:SUZAKU.../docs/suzaku/analysis/pinbgd.html and ftp://legacy.gsfc.nasa.gov/suzaku.../docs/suzaku/analysis/watchout.html http://www.astro.isas.jaxa.jp/suzaku.../docs/suzaku/aehp proc.html http://www.astro.isas.jaxa.jp/suzaku... the Suzaku memo available at http://www.astro.isas.ac.jp/suzaku... the Suzaku memo available at http://www.astro.isas.ac.jp/suzaku.... See Suzaku memo at http://www.astro.isas.ac.jp/suzaku/doc... Suzaku GOF web pages at http://heasarc.gsfc.nasa.gov/docs/suzaku/analysis/nxb ci6kev.html, in the Suzaku memo available... the Suzaku memos available at http://www.astro.isas.ac.jp/suzaku... official Suzaku CALDB. Now users should use xisnxbgen with the Suzaku CALDB... Model ≥ Suzaku FTOOLS Version 18 – released in 2011 June With Suzaku FTOOLS... the Suzaku GOF web pages. For window mode data only the Suzaku.../suzaku/data/background/gsonxb ver2.5/ and ftp://legacy.gsfc.nasa.gov/suzaku... the Suzaku GOF web pages. For window mode data only the Suzaku... (available since Suzaku FTOOLS version 14, i.e., HEAsoft v.6.8) duplicates the Suzaku processing pipeline... the Suzaku Technical Description at http://heasarc.gsfc.nasa.gov/docs/suzaku/prop tools/suzaku td. 88 ABC Guide... (available since Suzaku FTOOLS version 14, i.e., HEAsoft v.6.8) duplicates the Suzaku processing pipeline....gsfc.nasa.gov/docs/suzaku/prop tools/suzaku td/suzaku td/node6.html....gsfc.nasa.gov/docs/suzaku/prop tools/suzaku td/node11.html). Therefore... the Suzaku CALDB http://heasarc.gsfc.nasa.gov/docs/heasarc/caldb/suzaku.../suzaku/analysis/gso newgain.html http://heasarc.gsfc.nasa.gov/docs/suzaku.../suzaku/data/background/gsonxb ver2.5/ and ftp://legacy.gsfc.nasa.gov/suzaku...-22T abc-guide:SUZAKU-HXD-WELL_PIN > abc-guide:SUZAKU-HXD-WELL_PIN > filter... Primary Suzaku Sites Japan: http://www.astro.isas.jaxa.jp/suzaku/ http://darts.isas.jaxa.jp/ US : http://suzaku.gsfc... available at http://suzaku.gsfc.nasa.gov/docs/suzaku/astroe helpdesk.html...



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0.16/5
... hard band that INTEGRAL and Suzaku observed prior to 2011. If... et al. 2008, 2010). The Suzaku observatory confirmed the presence of... contribution of these components using a Suzaku observation, which we obtained on...). We extracted spectra from the Suzaku XIS0, 1 and 3 detectors from a circular... the XIS0 normalization, following the Suzaku data analysis guide6 . We fixed...://heasarc.gsfc.nasa.gov/docs/suzaku/analysis/abc/node8.html#SECTION00870000000000000000... to that measured for the Suzaku data in 2009 (Hamaguchi et... instrumental normalization difference between the Suzaku XIS0 and NuSTAR/FPMA (Madsen... energies measured by INTEGRAL and Suzaku (see the solid cyan line... right panel of Figure 3). The Suzaku spectra of η Car obtained between... same spectral model for the Suzaku spectral fit in Hamaguchi et... best-fit value of the Suzaku spectrum in a similar orbital phase... and lower than the earlier Suzaku measurement (Hamaguchi et al. 2014b... from fits to INTEGRAL and Suzaku spectra, and the absorption to... consistent with the INTEGRAL and Suzaku spectra (Γ =1.4). We split the NuSTAR... simultaneous fit to the multiple Suzaku spectra (Hamaguchi et al. 2014b... INTEGRAL measurement and 1/3.3 of the Suzaku measurement assuming a Γ = 1.4 power-law spectrum... between 2004 and 2011. Interestingly, a Suzaku observation in 2013 July with...-limit below the INTEGRAL and Suzaku detection before 2011. This indicates... source probably weakened between the Suzaku observation in 2011 and the... NuSTAR NUS140728 Supplement (Deep Minimum): Suzaku SUZ140806 Observation ID Observation Start... it to that of the Suzaku measurement in a similar orbital phase... Shallow 140728 140606 XMM Chandra SUZAKU RXTE/Swift Fig. 1.— RXTE and...-law component measured from the Suzaku observations (Hamaguchi et al. 2014b... minimum spectrum, estimated from the Suzaku observation on August 6th and... 40−70 keV measured with Suzaku, INTEGRAL, and NuSTAR (middle: Leyder...-law component, derived from the Suzaku HXD/PIN spectra below 40... show the timings of the Suzaku observations used for this spectral...



Дата загрузки: 2017-06-14
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0.2/5
... primarily for spectroscopy, of which SUZAKU is still in earth orbit... 2. 3 finished reflectors. Figure 3. Suzaku X-ray telescope. Figure 4. Suzaku two-stage quadrant. fabricate..., a completed quadrant subassembly and a complete Suzaku mirror before a stray light pre... the Suzaku observatory.3 Table 1 shows the relevant parameters for the Suzaku mirrors.... Table 1. Basic parameter comparison between Suzaku and ASTRO-H Focal Length (m) Diameter... (kg) Effective Area (cm2 6 keV) Suzaku 4.75 40 175 1400 18... of the mirrors on the Suzaku observatory is 1.7 arcmin Half Power.... The fact is, however, that Suzaku has been very productive and... obtained in our Lab with Suzaku spare mirror hardware, as well... collaborative instruments with Japan, including Suzaku, has been the low mass... housing ratio of 3 for the Suzaku mirror, the structural integrity of... commercial aluminum alloy sheet. For Suzaku, we used 0.152 mm thick... for this forming process. For Suzaku, we stacked groups of ∼42... the ones we used for Suzaku. A final substrate enhancement involves the... thickness, as we did for Suzaku, was the simplest implementation, albeit... will present a smaller resistance. For Suzaku, we used a ∼25 µm thick buffer... the time we fabricated the Suzaku mirrors, there was marked improvement... loose containment. The ASTRO-E2/Suzaku mirror design followed quickly on... is the case even with Suzaku type reflectors and alignment bars... the case by assembling 60 Suzaku reflector pairs in a quadrant, placing... testing of this scheme with Suzaku spare hardware, we have determined..., in a well adjusted quadrant, even Suzaku reflectors, end up resting on... al.,“The X-Ray Telescope onboard Suzaku”, PASJ, 59, S9, (2007) Serlemitsos...



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0.34/5
... emulateapj v. 11/12/01 THE SUZAKU OBSERVATION OF THE NUCLEUS OF..., Kyoto 606-8502, Japan ABSTRACT A Suzaku observation of the nucleus of... of Cen A made with the Suzaku observatory in August 2005. The.... §2 gives a brief overview of the Suzaku observatory, and describes the observation... of Cen A was observed by Suzaku from 2005 August 19 at... light target for the HXD. Suzaku was launched 2005 July 10... located at the CCD corners. Suzaku also features a non-imaging, collimated... keV. Further details of the Suzaku observatory are given in Mitsuda... al. 2007) provided by the Suzaku team. The screening is based... 256 s of passage through the Suzaku Cen A observation South Atlantic Anomaly... (NEP) to extract a background spectrum. Suzaku observed the NEP on 2005... occurred very early in the Suzaku mission, and the level of... correction. The positional accuracy of Suzaku is ∼1′ at present, as the... gain above Other recently-published Suzaku results have made use of... detected solely with the HXD. Suzaku Cen A observation of 1 denotes solar..., and the PL3 component domi- Suzaku Cen A observation nates at these... the XIS and HXD aboard Suzaku has allowed us to obtain... similar to those for the Suzaku observation, suggesting a lack of strong... the Fe Kα line in the Suzaku observation is consistent with that... obtained using Chandra-HETGS. The Suzaku observation thus shows no evidence... three power-laws observed by Suzaku are consistent with X-ray emission... detect as PL3) in the Suzaku spectrum. Meanwhile, Chandra-HETGS’s low... to the Fe Kα line-emitting Suzaku Cen A observation gas. The width... line intensity compatible with what Suzaku observes. Such a covering fraction suggests... from the thermal plasma The Suzaku XIS has yielded the best... as good a fit to the Suzaku data as collisional ionization models... metallicity value derived from the Suzaku data is consistent with enrichment...” accretion. 5. conclusions Suzaku Cen A observation The combination of Suzaku’s XIS and HXD... X-ray emission lines well. The Suzaku data are consistent with scenarios... last few years. During the Suzaku observation, the hard X-ray flux... and hard work of the Suzaku hardware teams and operations staff... press Fukazawa, Y. et al. 2007, Suzaku Memo 2007-02 Graham, J.A. 1978..., G. & Johnson, W.N. 1998, MNRAS, 299, 449 Suzaku Cen A observation 13 Table 1 Soft... Kα fluorescent emission line intensities, respectively. Suzaku Cen A observation 15 XIS Total... XVII (3s−2p) 2 O VIII O VII Suzaku Cen A observation 1.5 1 0.5 0.5 1 Energy (keV) 1.5 Fig.... 19 0.04 0 0.02 R 0.06 0.08 Suzaku Cen A observation 1.8 1.82 1.84 Γ 1.86... 13.5 NH (/1022 cm−2) 15.5 Suzaku Cen A observation 1.75 1.8 1.85 Γ 1.9 0.09...



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0.51/5
The X-ray Observatory Suzaku Kazuhisa Mitsuda1 , Mark Bautz20 , Hajime ... the key feature of the Suzaku X-ray observatory, launched on 2005... 10, 2005, and was renamed Suzaku. Suzaku is a red bird in asian... bird, Tanaka et al. 1994), Suzaku is a joint Japanese-US mission... many other institutions. After launch, Suzaku first deployed the solar paddles... instruments are working well, and Suzaku retains its excellent X–ray sensitivity... range from 0.2 to 600 keV. Suzaku’s broad bandpass, low background, and... outstanding problems in astrophysics. 2. Spacecraft Suzaku is in many ways similar...%. Fig. 1. Schematic view of the Suzaku satellite in orbit. Both solar... seen. 3 Fig. 2. A side view of Suzaku with the internal structures after...fic Instrumentation The scientific payload of Suzaku (figure 2) initially consisted of three... in telescope 4 Table 1. Overview of Suzaku capabilities S/C XRT Orbit Apogee 568... stray lights. Four XRTs onboard Suzaku (XRT-I0 to XRT-I3... in the energy range of Suzaku , 0.2-12 keV. The effective areas... the X–ray photon. The four Suzaku XISs are designated XIS0, XIS1... extend the bandpass of the Suzaku observatory to the highest feasible... of the Suzaku data processing can be found in the Suzaku web pages1 . 5. Scientific Capabilities Suzaku was designed to.... 2002). The key feature of Suzaku, the high-sensitivity wide-band... had the lowest background, and Suzaku XIS ( BI and FI CCD... estimation. The background rate of Suzaku is the lowest among the...://www.astro.isas.jaxa.jp/suzaku/ 8 Fig. 5. XIS background counting rate... example of the power of Suzaku for obtaining a very wide band... significant advantage of using Suzaku is the good energy response.... The line spread function of Suzaku CCD is very symmetric in... owe the success of the Suzaku observatory to the dedication and..., 9 Fig. 6. Background counting rate of Suzaku HXD as a function of energy... Cen A radio galaxy obtained with Suzaku. The spectrum was obtained with...



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0.15/5
... Suzaku/XIS: Status Report Eric Miller MIT Kavli Institute for the Suzaku...-tuning open issues IACHEC 2011 - Suzaku/XIS Suzaku/XIS - Overview 4 CCDs with... Tsujimoto’s “pocket guide” @"" 3 < 4 3<((4 " " ( " ( 9 ( + ( 0&1 < 4 3<(( = =3( ( 9 ( 9 ( 3 IACHEC 2011 - Suzaku/XIS D7 3 < 4 3<(( = =3( 9 ( "4 ( 4 +( Major XIS Events... August 13, 2005 launch of Suzaku XIS doors open, start of... in XIS1 OBF IACHEC 2011 - Suzaku/XIS 0&1 # 4 $ $ 3 " +3 + %@ 6' 4 "4 + 6 7 + " + 4 "E 3 0&1 4 0&1 %. + ' 7 0&1# %/ +' 7 - ,, " 7 " %? & Fα Fβ , ) ! , ' G " 3 " 4 G 4 ? XIS Status $ , G 7 , D* 4 , 1 9 ) H " " 3 " 6 5 * @ 0&1 % &' 0&1# % &' 0&1 + 3 G %/ +' 806 + 3 ; 6 " 0&1 %*&' 0&1 % &' " 7 / 7 " ! # 6 5 * @ 6 5 * @ I ,, 6 5 * @ %3 ' ; @ + 4 " 4 /&??1 @33... Tsujimoto’s “pocket guide” +5 7 ! J( ( K % &' ) J( ( K %*&' 7 4 7 " E "4 " ?@0& ;0- (@1? ; + " " IACHEC 2011 - Suzaku/XIS " 0&1 + /& - D 7 7 4 7 " + 3 4 + 7 3 4 7 O O Gain and FWHM Tracking... - Suzaku/XIS with charge injection Effective Area Tracking IACHEC 2011 - Suzaku/XIS Background Tracking IACHEC 2011 - Suzaku/XIS Background Tracking... 0.05 0.1 0.2 Energy (keV) IACHEC 2011 - Suzaku/XIS 0.5 Background Tracking NXB ! XIS1... 0.05 0.1 0.2 Energy (keV) IACHEC 2011 - Suzaku/XIS 0.5 Charge Injection Changes • row... 2008 2009 1000 IACHEC 2011 Suzaku/XIS Day from-launch (day...−2010 11:42 IACHEC 2011 - Suzaku/XIS 6 6.5 Energy (keV) 7 7.5 milleric 30...−2010 11:42 IACHEC 2011 - Suzaku/XIS 6 6.5 Energy (keV) 7 7.5 milleric 30...-tuning open issues IACHEC 2011 - Suzaku/XIS Energy Scale Calibration • • at... E0102 (data-model) IACHEC 2011 - Suzaku/XIS Results for Ne He...=20110219 XIS0 XIS1 IACHEC 2011 - Suzaku/XIS Sawada-san Results for...=20110219 XIS0 XIS1 IACHEC 2011 - Suzaku/XIS Sawada-san Results for..., ID=20110219 1.0% @ 0.6 keV (!) IACHEC 2011 - Suzaku/XIS Sawada-san XIS0 XIS1... σ 0.5-1 keV from E0102 IACHEC 2011 - Suzaku/XIS Problems with Response taken... time! extrapolated period IACHEC 2011 - Suzaku/XIS New RMF Params (In... 6 keV XIS1 6 keV IACHEC 2011 - Suzaku/XIS Open Calibration Issues • • • P-Sum... working on it IACHEC 2011 - Suzaku/XIS XIS Status - Summary • • XIS0.../~tsujimot/pg_xis.pdf IACHEC 2011 - Suzaku/XIS



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0.12/5
..., ASCA, RXTE, Chandra, HETE-2, and Suzaku. Such a diverse program involved collaborations..., Exosat, RXTE, Chandra, XMM, Swift, Suzaku, and Fermi. I have also witnessed... underlying fluid quantities. 128.03D – Suzaku Observations of the X-ray Brightest... its virial radius, with the Suzaku X-ray Observatory, in order to...-64 with ASM, MAXI and Suzaku J.B. Coley, R. Corbet, K. Mukai, K. Pottschmidt, UMBC...-sky X-ray Image (MAXI) and Suzaku provide a detailed temporal and spectral... ASM and MAXI. A two day Suzaku observation in Dec. 2010 took... light curve. The two day Suzaku observation reveals large variations in... orbit variability. Flares in the Suzaku light curve can reach nearly.... From a spectral analysis of the Suzaku data, emission lines in the... observatories—Chandra, XMM-Newton, and Suzaku—are operating simultaneously and addressing.... In comparison with those of Suzaku, they represent a factor of 20... is of particular interest, since Suzaku observations have suggested that the... rotation-powered neutron stars do. Suzaku detected hard X-ray radiation and... a decicated XMM legacy program and Suzaku observations providing simultaneous soft X-ray... (~400 ks XMM, ~500 ks Suzaku, ~800 ks NuSTAR) in the... model is correct then, with Suzaku and XMM-Newton, NuSTAR can..., AGNs including simultaneous observations with Suzaku and XMM-Newton, and show... by NuSTAR, XMM-Newton, Chandra, Suzaku, Swift and INTEGRAL taken primarily... keV) results from BeppoSAX and Suzaku where the direct emission from... observations with other missions, notably Suzaku and XMM. In the poster... and L249, recently observed by Suzaku, whose X-ray emission is strongly...-69.9 and 0548-70.4 whose Suzaku spectra can be satisfactorily modeled... correlate O VII fluxes measured with Suzaku with variations in ¼-keV intensity... an additional eighteen from archival Suzaku pointings and correlate these with..., we will discuss our new Suzaku follow-up observations of the...



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0.32/5
... and the Japanese Aerospace Agency’s Suzaku mission. Together, these data will... science and mission operation teams. • Suzaku (Japan), formerly Astro-E2, was... during launch in February 2000. Suzaku includes focusing, grazing-incidence optics... science campaigns between NuSTAR and Suzaku. • NASA’s Fermi Gamma-Ray Space...), JAXA’s successor X-ray mission to Suzaku, also known as the New... working in coordination with Chandra, Suzaku, Swift, and/or XMM-Newton..., 2002 Swift November 20, 2004 Suzaku July 10, 2005 Two Wide...



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0.08/5
... been conducted with Chandra–ACIS, Suzaku–XIS, Swift–XRT, and XMM... the soft-band (2– 8 keV), and Suzaku–HXD-PIN, RXTE–PCA, and... fluxes reported by BeppoSAX and Suzaku are given in Table 7.3. X-ray... Reference Date BeppoSAX–WFC [V+ 07] Suzaku [T+ 08a] 1996 - 4 until 2002 - 4 2006... by BeppoSAX– WFC [V+ 07] and Suzaku [T+ 08a] for the given time... a low state with MAGIC and Suzaku/Swift. In 30th International Cosmic... onboard the Chandra, INTEGRAL, RXTE, Suzaku, Swift, and XMM-Newton observatories...