Zeitschriftenartikel: „Source X“

1

England, Odette. „Source X Material“. Archives of American Art Journal 63, Nr. 1 (01.03.2024): 65–72. http://dx.doi.org/10.1086/729186.

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2

Jithesh, V., C. Anjana und Ranjeev Misra. „Broadband X-ray spectral study of ultraluminous X-ray source M81 X–6“. Monthly Notices of the Royal Astronomical Society 494, Nr. 3 (13.04.2020): 4026–30. http://dx.doi.org/10.1093/mnras/staa976.

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ABSTRACT Ultraluminous X-ray sources (ULXs) are a class of extragalactic, point-like, off-nuclear X-ray sources with X-ray luminosity from ∼1039 to 1041 erg s−1. We investigated the temporal and broadband X-ray spectral properties of the ULX M81 X–6 using simultaneous Suzaku and NuSTAR observations. To understand the nature of the source, we searched for pulsating signals from the source using the NuSTAR observation. However, we failed to identify any strong pulsating signals from the source. Alternatively, the broadband spectral modelling with accreting magnetic neutron star continuum model provides a statistically acceptable fit, and the inferred spectral parameters, and X-ray colours are consistent with other pulsating ULXs. Thus, our analysis suggests that M81 X–6 is another candidate ULX pulsar.

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3

Broos, Patrick S., Konstantin V. Getman, Matthew S. Povich, Leisa K. Townsley, Eric D. Feigelson und Gordon P. Garmire. „A NAIVE BAYES SOURCE CLASSIFIER FOR X-RAY SOURCES“. Astrophysical Journal Supplement Series 194, Nr. 1 (28.04.2011): 4. http://dx.doi.org/10.1088/0067-0049/194/1/4.

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4

Pile, David. „Plasma X-ray source“. Nature Photonics 9, Nr. 10 (29.09.2015): 631. http://dx.doi.org/10.1038/nphoton.2015.191.

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5

Lin, Dacheng, Natalie A. Webb und Didier Barret. „CLASSIFICATION OF X-RAY SOURCES IN THEXMM-NEWTONSERENDIPITOUS SOURCE CATALOG“. Astrophysical Journal 756, Nr. 1 (10.08.2012): 27. http://dx.doi.org/10.1088/0004-637x/756/1/27.

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6

Iaria, R., G. Augello, N. R. Robba, T. Di Salvo, L. Burderi und L. Lavagetto. „The New X-Ray Pulsar J1802.7-2017 Observed by BeppoSAX“. International Astronomical Union Colloquium 194 (2004): 212. http://dx.doi.org/10.1017/s0252921100152583.

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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+l, during a BeppoSAX observation of the latter source on 2001 September 16-20.The source was outside the FOV of the BeppoSAX/ LECS. We have verified its presence in both the MECS2 and MECS3 images, which probably excludes that this was a ghost image of a source outside the MECS FOV. Moreover, we can be sure that the source was within the PDS FOV. because the source X-ray pulsations were detected also in the PDS data (see below). We searched for known X-ray sources in a circular region of 30' centered at GX 9+1 in the SIMBAD data base. We found no known sources with a position compatible with that of the faint source; we therefore designate this serendipitous source as SAX J1802.7 2017.

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Popkov, N. F., V. I. Kargin, E. A. Ryaslov und A. S. Pikar'. „Plasma X-Ray Radiation Source“. Journal of X-Ray Science and Technology 5, Nr. 3 (1995): 289–94. http://dx.doi.org/10.3233/xst-1995-5305.

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8

Costa, Louelson Afranio Leugirdes de Azevedo Cavalcanti, Montie Alves Vitorino, Mauricio Beltrao de Rossiter Correa, Lucas Vinicius Hartmann und Andre Wild Silva Ramalho. „X-Type Current Source Converters“. IEEE Transactions on Power Electronics 36, Nr. 11 (November 2021): 12843–56. http://dx.doi.org/10.1109/tpel.2021.3082032.

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9

Anan’ev, S. S., Yu L. Bakshaev, P. I. Blinov, V. A. Bryzgunov, V. V. Vikhrev, S. A. Dan’ko, A. A. Zelenin et al. „X-pinch-based neutron source“. Plasma Physics Reports 36, Nr. 7 (Juli 2010): 601–8. http://dx.doi.org/10.1134/s1063780x1007007x.

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10

Ganciu, M., A. M. Pointu und M. Nistor. „Source compacte de rayons X“. Le Journal de Physique IV 11, PR7 (Oktober 2001): Pr7–5—Pr7–6. http://dx.doi.org/10.1051/jp4:2001702.

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11

Goonan, G. W., A. Fouras und S. Dubsky. „Array-source X-ray velocimetry“. Optics Express 26, Nr. 2 (10.01.2018): 935. http://dx.doi.org/10.1364/oe.26.000935.

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12

Telford, Mark. „Static scanning X-ray source“. Materials Today 8, Nr. 7 (Juli 2005): 13. http://dx.doi.org/10.1016/s1369-7021(05)70968-8.

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13

Hird, J. R., C. G. Camara und S. J. Putterman. „A triboelectric x-ray source“. Applied Physics Letters 98, Nr. 13 (28.03.2011): 133501. http://dx.doi.org/10.1063/1.3570688.

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14

Motch, C. „Galactic X-ray source populations“. Astronomische Nachrichten 329, Nr. 2 (Februar 2008): 166–69. http://dx.doi.org/10.1002/asna.200710904.

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15

P, N. „Plasma X-Ray Radiation Source“. Journal of X-Ray Science and Technology 5, Nr. 3 (September 1995): 289–94. http://dx.doi.org/10.1006/jxra.1995.0005.

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16

Hammer, D. A., D. H. Kalantar, K. C. Mittal und N. Qi. „X‐pinch soft x‐ray source for microlithography“. Applied Physics Letters 57, Nr. 20 (12.11.1990): 2083–85. http://dx.doi.org/10.1063/1.103948.

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17

S Yadav, Poonamlata. „Phase-Contrast Imaging using X- Ray & Neutron Source“. International Journal of Science and Research (IJSR) 13, Nr. 5 (05.05.2024): 1085–88. http://dx.doi.org/10.21275/sr24517112544.

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18

Joffre, S., R. Silver, M. Rajagopal, M. Ajello, N. Torres-Albà, A. Pizzetti, S. Marchesi und A. Kaur. „Identifying the 3FHL Catalog. VI. Swift Observations of 3FHL Unassociated Objects with Source Classification via Machine Learning“. Astrophysical Journal 940, Nr. 2 (29.11.2022): 139. http://dx.doi.org/10.3847/1538-4357/ac9797.

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Abstract The Third Catalog of Hard Fermi Large Area Telescope Sources (3FHL) reports the detection of 1556 objects at E > 10 GeV. However, 177 sources remain unassociated and 23 are associated with a ROSAT X-ray detection of unknown origin. Pointed X-ray observations were conducted on 30 of these unassociated and unknown sources with Swift−XRT. A bright X-ray source counterpart was detected in 21 out of 30 fields. In five of these 21 fields, we detected more than one X-ray counterpart, totaling 26 X-ray sources analyzed. Multiwavelength data was compiled for each X-ray source detected. We find that 21 out of the 26 X-ray sources detected display the multiwavelength properties of blazars, while one X-ray source displays the characteristics of a Galactic source. Using trained decision tree, random forest, and support vector machine models, we predict all 21 blazar counterpart candidates to be BL Lacertae objects (BL Lacs). This is in agreement with BL Lacs being the most populous source class in the 3FHL.

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19

Zucchini, F., S. N. Bland, C. Chauvin, P. Combes, D. Sol, A. Loyen, B. Roques und J. Grunenwald. „Characteristics of a molybdenum X-pinch X-ray source as a probe source for X-ray diffraction studies“. Review of Scientific Instruments 86, Nr. 3 (März 2015): 033507. http://dx.doi.org/10.1063/1.4915496.

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20

Wang, Song, Jifeng Liu, Yanli Qiu, Yu Bai, Huiqin Yang, Jincheng Guo und Peng Zhang. „CHANDRA ACIS SURVEY OF X-RAY POINT SOURCES: THE SOURCE CATALOG“. Astrophysical Journal Supplement Series 224, Nr. 2 (17.06.2016): 40. http://dx.doi.org/10.3847/0067-0049/224/2/40.

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21

Kaaret, Philip. „Optical Sources near the Bright X‐Ray Source in NGC 1073“. Astrophysical Journal 629, Nr. 1 (10.08.2005): 233–38. http://dx.doi.org/10.1086/431471.

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22

Girardeau-Montaut, Jean-Pierre, Bélà Kiraly, Claire Girardeau-Montaut und Hubert Leboutet. „Table-top laser-driven ultrashort electron and X-ray source: the CIBER-X source project“. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 452, Nr. 1-2 (September 2000): 361–70. http://dx.doi.org/10.1016/s0168-9002(00)00419-8.

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23

Simon, Arleyn W., Destiny L. Crider, Tatsuya Murakami und Barry Wilkens. „Arizona Salado turquoise: source studies with proton-induced X-ray emission and X-ray diffraction“. Open Journal of Archaeometry 1, Nr. 1 (31.12.2013): 10. http://dx.doi.org/10.4081/arc.2013.e10.

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We compare the composition of turquoise source materials from Arizona to prehistoric blue-green stone artifacts recovered from Salado platform mounds (ca. AD 1275-1450) in the Tonto Basin of Central Arizona. Turquoise samples from known source areas in Arizona including Kingman, Castle Dome, in the Globe- Miami area are compare with others that may have been potential sources of turquoise artifacts recovered from the Salado platform mounds. The complementary techniques of proton-induced X-ray emission (PIXE) for chemical analysis and X-ray diffraction (XRD) for mineralogical signatures are used for nondestructive characterisation of both source area samples and archaeological artifacts. The results of the source area sample characterisations are compared quantitatively with the results of archaeological samples, which are evaluated in terms of their likelihood of being from each of the regional sources. The combination of mineralogical and chemical data to identify source materials provides a more thorough identification of the complex variations within turquoise related materials that may not be distinguished by visual inspection. The PIXE and XRD analysis are compared using a set of multivariate statistics including principal components analysis and discriminant analysis. Additionally, a set of Munsell colour charts specifically for the blue-green range of colours is used to objectively qualify colour in comparison to chemical and mineralogical signatures, as colour alone is not a reliable indicator of composition. The results provide objective data to assess directionality of procurement of turquoise and regional social and economic ties to better understand Salado regional connections during this dynamic period in the American Southwest.

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24

Eggl, Elena, Martin Dierolf, Klaus Achterhold, Christoph Jud, Benedikt Günther, Eva Braig, Bernhard Gleich und Franz Pfeiffer. „The Munich Compact Light Source: initial performance measures“. Journal of Synchrotron Radiation 23, Nr. 5 (22.07.2016): 1137–42. http://dx.doi.org/10.1107/s160057751600967x.

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While large-scale synchrotron sources provide a highly brilliant monochromatic X-ray beam, these X-ray sources are expensive in terms of installation and maintenance, and require large amounts of space due to the size of storage rings for GeV electrons. On the other hand, laboratory X-ray tube sources can easily be implemented in laboratories or hospitals with comparatively little cost, but their performance features a lower brilliance and a polychromatic spectrum creates problems with beam hardening artifacts for imaging experiments. Over the last decade, compact synchrotron sources based on inverse Compton scattering have evolved as one of the most promising types of laboratory-scale X-ray sources: they provide a performance and brilliance that lie in between those of large-scale synchrotron sources and X-ray tube sources, with significantly reduced financial and spatial requirements. These sources produce X-rays through the collision of relativistic electrons with infrared laser photons. In this study, an analysis of the performance, such as X-ray flux, source size and spectra, of the first commercially sold compact light source, the Munich Compact Light Source, is presented.

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25

TOMIE, Toshihisa. „Laser-Plasma X-Ray Source and X-Ray Microscopy.“ Review of Laser Engineering 19, Nr. 11 (1991): 1048–56. http://dx.doi.org/10.2184/lsj.19.11_1048.

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26

Okada, I. „A plasma x-ray source for x-ray lithography“. Journal of Vacuum Science & Technology B: Microelectronics and Nanometer Structures 4, Nr. 1 (Januar 1986): 243. http://dx.doi.org/10.1116/1.583449.

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27

Sinars, D. B., S. A. Pikuz, T. A. Shelkovenko, K. M. Chandler und D. A. Hammer. „Temporal parameters of the X-pinch x-ray source“. Review of Scientific Instruments 72, Nr. 7 (Juli 2001): 2948–56. http://dx.doi.org/10.1063/1.1379961.

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28

Arkadiev, V., H. Bräuninger, W. Burkert, A. Bzhaumikhov, H. E. Gorny, N. Langhoff, A. Oppitz und J. Rabe. „Monochromatic X-ray source for calibrating X-ray telescopes“. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 455, Nr. 3 (Dezember 2000): 589–95. http://dx.doi.org/10.1016/s0168-9002(00)00536-2.

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29

Grisé, F., M. W. Pakull, R. Soria, C. Motch, I. A. Smith, S. D. Ryder und M. Böttcher. „The ultraluminous X-ray source NGC 1313 X-2“. Astronomy & Astrophysics 486, Nr. 1 (27.05.2008): 151–63. http://dx.doi.org/10.1051/0004-6361:200809557.

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30

Evans, Ian N., Janet D. Evans, J. Rafael Martínez-Galarza, Joseph B. Miller, Francis A. Primini, Mojegan Azadi, Douglas J. Burke et al. „The Chandra Source Catalog Release 2 Series“. Astrophysical Journal Supplement Series 274, Nr. 2 (16.09.2024): 22. http://dx.doi.org/10.3847/1538-4365/ad6319.

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Abstract The Chandra Source Catalog (CSC) is a virtual X-ray astrophysics facility that enables both detailed individual source studies and statistical studies of large samples of X-ray sources detected in Advanced CCD Imaging Spectrometer and High Resolution Camera-I imaging observations obtained by the Chandra X-ray Observatory. The catalog provides carefully curated, high-quality, and uniformly calibrated and analyzed tabulated positional, spatial, photometric, spectral, and temporal source properties, as well as science-ready X-ray data products. The latter includes multiple types of source- and field-based FITS format products that can be used as a basis for further research, significantly simplifying follow-up analysis of scientifically meaningful source samples. We discuss in detail the algorithms used for the CSC Release 2 Series, including CSC 2.0, which includes 317,167 unique X-ray sources on the sky identified in observations released publicly through the end of 2014, and CSC 2.1, which adds Chandra data released through the end of 2021 and expands the catalog to 407,806 sources. Besides adding more recent observations, the CSC Release 2 Series includes multiple algorithmic enhancements that provide significant improvements over earlier releases. The compact source sensitivity limit for most observations is ∼5 photons over most of the field of view, which is ∼2× fainter than Release 1, achieved by coadding observations and using an optimized source detection approach. A Bayesian X-ray aperture photometry code produces robust fluxes even in crowded fields and for low-count sources. The current release, CSC 2.1, is tied to the Gaia-CRF3 astrometric reference frame for the best sky positions for catalog sources.

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31

Rawat, B., C. Sharma und Sunil Ghildiyal. „Nature of variability in cone and seed characteristics and germination behaviour of different seed sources of silver fir (Abies pindrow Spach.)“. Indian Journal of Forestry 31, Nr. 4 (01.12.2008): 651–58. http://dx.doi.org/10.54207/bsmps1000-2008-uo763j.

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Five seed sources of A. pindrow, collected from Garhwal Himalaya were studied for cone and seed characteristics and germination behaviour. Three different sizes of cones (large, medium and small) were observed in all the seed sources. The dimensions of large (14.25 x 4.76-16.04 x 4.56 cm), medium (11.45 x 4.17-12.28 x 4.43 cm) and small (9.01 x 4.05-9.68 x 4.08 cm) sized cones in 5 different seed sources of A. pindrow oscillated greatly. The maximum cone moisture content also varied significantly (45.22-55.37%) in the cones. The largest seed observed was 1.17 cm long x 0.87 cm wide and the smallest was 0.56 cm long x 0.19 cm wide. The seed mass was heaviest with wings (7,35 gm/100 seeds) and without wings (6.84 gm/100 seeds) in Tapovan seed source on fresh weight basis. The highest (56.0%) germination was observed in Dudhatoli seed source at 10oC and the lowest (10.0%) at 25oC in Tapovan seed source. Dudhatoli seed source was recorded to be the best seed source, which may give highest productivity if tried on other sites. This seed source may be used to establish Seedling Seed Orchards due to additive genetic gain and higher germination percentage of seeds.

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32

Soltan, Andrzej. „The X-Ray Background“. Highlights of Astronomy 9 (1992): 299–308. http://dx.doi.org/10.1017/s1539299600009102.

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AbstractVarious models of the X-ray background are discussed. It is postulated that the only explanation consistent with all the existing data is discrete sources. Present observational material suggests that known classes of active galactic nuclei also dominate the source counts below the lowest detectable flux levels.

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33

Haakonsen, Christian Bernt, und Robert E. Rutledge. „XID II: STATISTICAL CROSS-ASSOCIATION OF ROSAT BRIGHT SOURCE CATALOG X-RAY SOURCES WITH 2MASS POINT SOURCE CATALOG NEAR-INFRARED SOURCES“. Astrophysical Journal Supplement Series 184, Nr. 1 (25.08.2009): 138–51. http://dx.doi.org/10.1088/0067-0049/184/1/138.

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34

An, Mou, und Yaoqin Xie. „A Novel CT Imaging System with Adjacent Double X-Ray Sources“. Computational and Mathematical Methods in Medicine 2013 (2013): 1–6. http://dx.doi.org/10.1155/2013/391212.

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Current computed tomography (CT) scanners rotate fast to reduce motion artifact. X-ray tube must work in a high power to make the image clear under short exposure time. However, the life span of such a tube may be shortened. In this paper, we propose a novel double sources CT imaging system, which puts two of the same X-ray sources closely with each other. The system is different from current dual source CT with orthogonal X-ray sources. In our system, each projection is taken twice by these two sources to enhance the exposure value and then recovered to a single source projection for image reconstruction. The proposed system can work like normal single source CT system, while halving down the working power for each tube.

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35

Wolter, Anna, Ginevra Trinchieri und Monica Colpi. „Variability of ultraluminous X-ray sources in the Cartwheel Ring“. Proceedings of the International Astronomical Union 2, S238 (August 2006): 255–58. http://dx.doi.org/10.1017/s174392130700508x.

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AbstractThe Cartwheel is one of the most outstanding examples of a dynamically perturbed galaxy where star formation is occurring inside the ring–like structure. In previous studies with Chandra, we detected 16 Ultra Luminous X-ray sources lying along the southern portion of the ring. Their Luminosity Function is consistent with them being in the high luminosity tail of the High Mass X-ray Binaries distribution, but with one exception: source N.10. This source, detected with Chandra at LX = 1 × 1041 erg s−1, is among the brightest non–nuclear sources ever seen in external galaxies. Recently, we have observed the Cartwheel with XMM-Newton in two epochs, six months apart. After having been at its brightest for at least 4 years, the source has dimmed by at least a factor of two between the two observations. This fact implies that the source is compact in nature. Given its extreme isotropic luminosity, there is the possibility that the source hosts an accreting intermediate–mass black hole. Other sources in the ring vary in flux between the different datasets. We discuss our findings in the context of ULX models.

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Nazri, Nurnabilah, und Adlyka Annuar. „X-ray source population in the polar ring galaxy NGC 660 as observed by Chandra“. Research in Astronomy and Astrophysics 21, Nr. 11 (01.12.2021): 289. http://dx.doi.org/10.1088/1674-4527/21/11/289.

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Abstract We present Chandra observations of the nearby polar ring galaxy NGC 660 to study its X-ray source population. Based on our analysis, we detected a total of 23 X-ray sources in the 0.5−8 keV band, with luminosities ranging from ∼1037 to ∼1039 erg s−1. Twenty-two of these sources are located off-nuclear and have luminosities below the ultraluminous X-ray source (ULX) threshold value of L 0.5−8 keV < 1039 erg s−1, suggesting that they are likely to be X-ray binary (XRB) candidates. The remaining source is located at the center of the galaxy, suggesting it is an active galactic nucleus (AGN). However, we estimated that four of the detected sources could be associated with background objects. Based on the source count rates in each of the Chandra observations, we found evidence for variability in nine of the 23 sources, including the AGN. However, further investigation with spectral analysis suggested no significant differences in the AGN luminosities between the observations. The X-ray luminosity distribution of the galaxy was found to be generally lower than that expected from previous studies on star forming and collisional ring galaxies. No ULX was also detected in the galaxy, in contrast with what was expected from the galaxyʼs SFR and metallicity (i.e., SFR = 14.43 ± 0.19 M ⊙ yr−1 and Z = 0.94 ± 0.01 Z ⊙, respectively). These results suggest a deficit in the X-ray sources detected. Based on source hardness ratio distribution, we found evidence that the fainter sources have a harder source spectrum, indicating higher absorption. This further suggests that there could be more X-ray sources that were not detected in the galaxy due to significant obscuration.

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37

MOCHIZUKI, Takayasu. „Incoherent laser plasma X-ray source.“ Review of Laser Engineering 18, Nr. 11 (1990): 856–60. http://dx.doi.org/10.2184/lsj.18.11_856.

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38

HIROSE, Masaoki. „Light Source for X-ray Lithography.“ Review of Laser Engineering 29, Nr. 10 (2001): 653–58. http://dx.doi.org/10.2184/lsj.29.653.

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39

Cerjan, Charles. „X-ray plasma source design simulations“. Applied Optics 32, Nr. 34 (01.12.1993): 6911. http://dx.doi.org/10.1364/ao.32.006911.

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40

Liu Xin, Yi Ming-Hao und Guo Jin-Chuan. „Line focal X-ray source imaging“. Acta Physica Sinica 65, Nr. 21 (2016): 219501. http://dx.doi.org/10.7498/aps.65.219501.

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41

Monakhov, A. A. „A hydrodynamic X-ray radiation source“. Doklady Physics 58, Nr. 6 (Juni 2013): 258–60. http://dx.doi.org/10.1134/s1028335813060116.

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42

Fabbiano, G. „X-ray Source Populations in Galaxies“. Chinese Journal of Astronomy and Astrophysics 3, S1 (31.12.2003): 193–201. http://dx.doi.org/10.1088/1009-9271/3/s1/193.

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43

Bharkhada, Deepak, Hengyong Yu, Hong Liu, Robert Plemmons und Ge Wang. „Line-Source Based X-Ray Tomography“. International Journal of Biomedical Imaging 2009 (2009): 1–8. http://dx.doi.org/10.1155/2009/534516.

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Current computed tomography (CT) scanners, including micro-CT scanners, utilize a point x-ray source. As we target higher and higher spatial resolutions, the reduced x-ray focal spot size limits the temporal and contrast resolutions achievable. To overcome this limitation, in this paper we propose to use a line-shaped x-ray source so that many more photons can be generated, given a data acquisition interval. In reference to the simultaneous algebraic reconstruction technique (SART) algorithm for image reconstruction from projection data generated by an x-ray point source, here we develop a generalized SART algorithm for image reconstruction from projection data generated by an x-ray line source. Our numerical simulation results demonstrate the feasibility of our novel line-source based x-ray CT approach and the proposed generalized SART algorithm.

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44

Hayama, K., S. D. Mohanty, S. Desai, M. Rakhmanov, T. Summerscales und S. Yoshida. „Source tracking for Sco X-1“. Classical and Quantum Gravity 25, Nr. 18 (02.09.2008): 184021. http://dx.doi.org/10.1088/0264-9381/25/18/184021.

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45

Bacal, M., C. Gaudin, A. Bourdier, J. Bruneteau, J. M. Buzzi, K. S. Golovanivsky, L. Hay, C. Rouillé und L. Schwartz. „A compact radiological X-ray source“. Nature 384, Nr. 6608 (Dezember 1996): 421. http://dx.doi.org/10.1038/384421a0.

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46

Michette, A. G., R. Fedosejevs, S. J. Pfauntsch und R. Bobkowski. „A scanned source X-ray microscope“. Measurement Science and Technology 5, Nr. 5 (01.05.1994): 555–59. http://dx.doi.org/10.1088/0957-0233/5/5/014.

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Zakharov, O. P. „An extra-bright X-ray source“. Instruments and Experimental Techniques 53, Nr. 6 (November 2010): 866–72. http://dx.doi.org/10.1134/s0020441210060187.

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Seres, J., E. Seres, A. J. Verhoef, G. Tempea, C. Streli, P. Wobrauschek, V. Yakovlev, A. Scrinzi, C. Spielmann und F. Krausz. „Source of coherent kiloelectronvolt X-rays“. Nature 433, Nr. 7026 (Februar 2005): 596. http://dx.doi.org/10.1038/433596a.

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Wu, Jianyi, Wenli Zhang und Xiangyue Miao. „New X-ray source system design“. Procedia Engineering 7 (2010): 190–94. http://dx.doi.org/10.1016/j.proeng.2010.11.029.

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Tang, Chuanxiang, Wenhui Huang, Renkai Li, Yingchao Du, Lixin Yan, Jiaru Shi, Qiang Du et al. „Tsinghua Thomson scattering X-ray source“. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 608, Nr. 1 (September 2009): S70—S74. http://dx.doi.org/10.1016/j.nima.2009.05.088.

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