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Xmm published presentations and documents on DocSlides.

05760xt2112122b102880xt2112124d108t611602
05760xt2112122b102880xt2112124d108t611602
by hazel
+48t5 5 10�1,440t2 2d1+960x3d1�5...
Magnetic CVs in the XMM-Newton
Magnetic CVs in the XMM-Newton
by test
Era: the . I. ntermediate . P. olars. . D.de. ...
Changing picture brightness using SSE
Changing picture brightness using SSE
by sherrill-nordquist
Another SSE example….. Brightness. Make a simpl...
BASICS OF SPECTROSCOPY Spectroscopy School,
BASICS OF SPECTROSCOPY Spectroscopy School,
by lucy
MSSL, March 17-18, 2009. Frits Paerels. Columbia A...
The deep sky under the X-ray limelight:
The deep sky under the X-ray limelight:
by evans
The. . XMM ultra-deep survey in the CDFS. . Andr...
From High-level Haskell to Efficient Low-level Code
From High-level Haskell to Efficient Low-level Code
by cheryl-pisano
From High-level Haskell to Efficient Low-level Co...
X-ray Diagnostics and Their Relationship to Magnetic Fields
X-ray Diagnostics and Their Relationship to Magnetic Fields
by aaron
David Cohen. Swarthmore College. XMM-Newton. Chan...
IRAC 8 micro
IRAC 8 micro
by liane-varnes
K-band. 0.5-2 keV. X-ray Emission Line Spectrosco...
Type 1 AGN SEDs in the COSMOS
Type 1 AGN SEDs in the COSMOS
by lois-ondreau
A Single Form, Mixing Diagram,. and Outliers . He...
Trimsize:xmmTypearea:xmmBleed:
Trimsize:xmmTypearea:xmmBleed:
by debby-jeon
.BleedallowanceBleedadvertisementsshouldincludeamm...
C luster
C luster
by tatiana-dople
L. ensing . A. nd . S. upernova survey with . H. ...
CURRENT and FUTURE X-RAY SPECTROMETERS
CURRENT and FUTURE X-RAY SPECTROMETERS
by test
Spectroscopy School,. MSSL, March 17-18, 2009. Fr...
XMM-Newton EPIC Cross-Calibration
XMM-Newton EPIC Cross-Calibration
by luanne-stotts
Andy Read. With contributions from . Matteo. . G...