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Galactic black hole candidate Swift~J1753.5-0127 was discovered on 2005 June30 by the Swift Burst Alert Telescope. We study the accretion flow propertiesduring its very first outburst through careful analysis of the evolution of thespectral and the temporal properties using the two-component advective flow(TCAF) paradigm. RXTE proportional counter array spectra in $2.5-25$ keV arefitted with the current version of the TCAF model fits file to estimatephysical flow parameters, such as two component (Keplerian disk andsub-Keplerian halo) accretion rates, properties of the Compton cloud, probablemass of the source, etc. The source is found to be in harder (hard andhard-intermediate) spectral states during the entire phase of the outburst withvery significant jet activity. Since in TCAF solution, the model normalizationis constant for any particular source, any requirement of significantlydifferent normalization to have a better fit on certain days would point toX-ray contribution from components not taken into account in the current TCAFmodel fits file. By subtracting the contribution using actual normalization, wederive the contribution of X-rays from the jets and outflows. We study itsproperties, such as its magnitude and spectra. We find that on some days, up toabout 32\% X-ray flux is emitted from the base of the jet itself.

Properties of X-ray Flux of Jets During 2005 Outburst of Swift J1753.5-0127 Using TCAF Solution