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Using the Swift data of GRB 050315, we progress on the uniqueness of ourtheoretically predicted Gamma-Ray Burst (GRB) structure as composed by aproper-GRB (P-GRB), emitted at the transparency of an electron-positron plasmawith suitable baryon loading, and an afterglow comprising the so called "promptemission" as due to external shocks. Thanks to the Swift observations, we cantheoretically fit detailed light curves for selected energy bands on acontinuous time scale ranging over 10^6 seconds. The theoretically predictedinstantaneous spectral distribution over the entire afterglow confirms a clearhard-to-soft behavior encompassing, continuously, the "prompt emission" all theway to the latest phases of the afterglow. Consequences of the instrumentalthreshold on the definition of "short" and "long" GRBs are discussed.

GRB 050315: A step toward the uniqueness of the overall GRB structure and the true nature of long GRBs