2007MNRAS.378..182R

We present the results of the analysis of Rossi X-ray Timing Explorer (RXTE) observations of the new X-ray transient, SWIFT J1753.5-0127, during its outburst in 2005 July. The source was caught at the peak of the burst with a flux of 7.19e-09 erg/s/cm2 in the 3-25 keV energy range and observed until it decreased by about a factor of 10. The photon index of the power-law component, which is dominant during the entire outburst, decreases from ∼1.76 to 1.6. However, towards the end of the observations the photon index is found to increase, indicating a softening of the spectra. The presence of an ultrasoft thermal component, during the bright phases of the burst, is clear from the fits to the data. The temperature associated with this thermal component is 0.4 keV. We believe that this thermal component could be due to the presence of an accretion disc. Assuming a distance of 8.5 kpc, L_X/L_Edd≃ 0.05 at the peak of the burst, for a black hole of mass 10M_☉. The source is found to be locked in the low/hard state during the entire outburst and likely falls in the category of the X-ray transients that are observed in the low/hard state throughout the outburst. We discuss the physical scenario of the low/hard state outburst for this source.