Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=9cm,clip]{0404680101_2_fc.eps} \end{figure}$ Figure 1: Finding chart based on the DSS2 red image of the region around XMMU J004814.1-731003. The optical counterpart is marked with a vertical arrow. The error circle of the X-ray position is smaller than the size of the star on the image. The H ${\alpha }$ emission line star [MA93] 215 is also labelled.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=9cm,clip]{lc_macho_ogle.ps} \end{figure}$ Figure 2: MACHO B- and R - and OGLE I-band light curves of the optical counterpart of XMMU J004814.1-731003. For the MACHO data only data points with errors less than 0.05 mag are plotted.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{fig3.eps} \end{figure}$ Figure 3: Power spectrum of the MACHO R-band data of the opticalcounterpart (star 212.15849.52).
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{aa09540f4.eps}\end{figure}$ Figure 4: Power spectrum of XMMU J004814.1-731003 produced from the 1.0-10.0 keV combined EPIC data.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{P0404680101PNS003PIEVLI0000_sc2-bg2_efold25.5_5bands.ps}\end{figure}$ Figure 5: Folded EPIC-PN light curves of XMMU J004814.1-731003 in the standard EPIC energy bands (the lower energy bands 0.2-0.5 keV and 0.5-1.0 keV were combined and rebinned by a factor of two due to the low count rate). The panels show the pulse profiles for the different energies specified in keV. The intensity profiles are background subtracted and normalised to the average count rate (in cts s^-1: 0.00082, 0.0073, 0.0135, 0.0093, 0.0310 from top to bottom).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=9cm,clip]{spectrum_2_pow.ps}\end{figure}$ Figure 6: EPIC spectra of XMMU J004814.1-731003. EPIC-PN is shown in black and EPIC-MOS in red (M1) and green (M2) (both grey in black and white representation). The histograms show the best-fit absorbed power-law model.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0404680101_2_fc.eps} \end{figure}$	Figure 1: Finding chart based on the DSS2 red image of the region around XMMU J004814.1-731003. The optical counterpart is marked with a vertical arrow. The error circle of the X-ray position is smaller than the size of the star on the image. The H ${\alpha }$ emission line star [MA93] 215 is also labelled.
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$\begin{figure} \par\includegraphics[angle=-90,width=9cm,clip]{lc_macho_ogle.ps} \end{figure}$	Figure 2: MACHO B- and R - and OGLE I-band light curves of the optical counterpart of XMMU J004814.1-731003. For the MACHO data only data points with errors less than 0.05 mag are plotted.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{fig3.eps} \end{figure}$	Figure 3: Power spectrum of the MACHO R-band data of the opticalcounterpart (star 212.15849.52).
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$\begin{figure} \par\includegraphics[width=9cm,clip]{aa09540f4.eps}\end{figure}$	Figure 4: Power spectrum of XMMU J004814.1-731003 produced from the 1.0-10.0 keV combined EPIC data.
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$\begin{figure} \par\includegraphics[angle=-90,width=9cm,clip]{spectrum_2_pow.ps}\end{figure}$	Figure 6: EPIC spectra of XMMU J004814.1-731003. EPIC-PN is shown in black and EPIC-MOS in red (M1) and green (M2) (both grey in black and white representation). The histograms show the best-fit absorbed power-law model.
Open with DEXTER