Sentence examples for which probably originated from inspiring English sources

Miscellaneous records, most of which probably originated with the Secretary of the Faculty and the Office of the Treasurer.

Phylogeographic analyses shed light on the dispersal history of R. cylindraceus, which probably originated on the Isla de la Juventud.

Sugarcane, which probably originated in India, went west, and became the main plantation crop of the West Indies.

These deposits and 14C ages provide the first evidence of Holocene loess in the Great Lakes region, some of which probably originated from the nearby Muskegon River floodplain.

The latter was especially true of early pottery wheels (which probably originated some 5,000 years ago or more), which had to be turned by hand or foot.

Rabbinic Judaism, which probably originated during the Babylonian Exile and became organized after the destruction of the Second Temple of Jerusalem by the Romans in 70 ce, concerned itself primarily with the solution of legal and ethical problems.

The dielectric property for the hybrid compound was further investigated in the temperature range of 20 150 °C and in the frequency region of 1 107 Hz, indicating the existence of the thermally assisted dynamical dipole motion under ac electric field, which probably originates from the ion hopping.

However, there still remains non-negligible displacements, which probably originate in the spatial inhomogeneity of slip on the fault planes and a lack of the contribution of the Idosawa fault.

After 1 mmol of EDTA has been added into the reaction system, the obtained sample exhibits four main diffraction peaks of kesterite CZTS, together with one weak impurity peak located at 31.6°, which probably originates from CuS or Sn2S3.

One may notice that the element O is present in small amounts in the molybdenum nanowall (only 4.80 atom percentage), which probably originates from the amorphous layer on the surface of the individual nanowall (top left in Figure3g and top right in Figure3h).

The infrared spectra of proto-planetary nebulae display broad emission plateaus at 8 and 12 μm, which probably originate from a collection of different in-plane and out-of-plane bending modes of aliphatic groups attached to aromatic rings (Kwok et al., 2001).