Disclosed is an optical time-stamping device, including an optical instrument with a retina having a field of view and being able to produce on the retina images of the field of view, and a high accuracy reference clock signal receive. The time-stamping device also includes: a lighting source at a distance from the retina of an optical instrument, and configured to emit a light signal in the direction of the retina of an optical instrument and in the field of view of an optical instrument, and a control unit connected to the reference clock signal receiver by a first connection and to the lighting source by a second connection, and configured for controlling the lighting source for emitting a light signal in a synchronized way with the reference clock signal. An associated image sensing system and optical time-stamping method are also disclosed.

Disclosed is an optical time-stamping device, including an optical instrument with a retina having a field of view and being able to produce on the retina images of the field of view, and a high accuracy reference clock signal receive. The time-stamping device also includes: a lighting source at a distance from the retina of an optical instrument, and configured to emit a light signal in the direction of the retina of an optical instrument and in the field of view of an optical instrument, and a control unit connected to the reference clock signal receiver by a first connection and to the lighting source by a second connection, and configured for controlling the lighting source for emitting a light signal in a synchronized way with the reference clock signal. An associated image sensing system and optical time-stamping method are also disclosed.

A user device determines a reading speed value for each of a plurality of measurable units of an electronic publication. The user device adds each reading speed value into one of a plurality of data sets or one of a plurality of outlier sets. The user device calculates the average reading speed of the user based on one or more of the plurality of data sets.

A user device determines a reading speed value for each of a plurality of measurable units of an electronic publication. The user device adds each reading speed value into one of a plurality of data sets or one of a plurality of outlier sets. The user device calculates the average reading speed of the user based on one or more of the plurality of data sets.

A system and method for measuring the time of a moving object during at least one training exercise is disclosed. The system includes a mobile device having a camera and a time measurement computer program. After placing the mobile device in a fixed stationary viewing angle position, the camera is arranged to capture digital images and to enter an image calibration mode, an algorithm calibration mode, and a detection mode before executing a time measuring command on the computer program. The system and method utilize histogram calculation for the digital images to trigger the time measuring command and read object movement detection when threshold values are detected.

A system and method for measuring the time of a moving object during at least one training exercise is disclosed. The system includes a mobile device having a camera and a time measurement computer program. After placing the mobile device in a fixed stationary viewing angle position, the camera is arranged to capture digital images and to enter an image calibration mode, an algorithm calibration mode, and a detection mode before executing a time measuring command on the computer program. The system and method utilize histogram calculation for the digital images to trigger the time measuring command and read object movement detection when threshold values are detected.

A method for deriving an independent current time estimate from celestial sources comprising: providing a reference measurement for a variable-intensity celestial source, wherein the reference measurement comprises the celestial source's photometric structure at a known time, at a known stellar period, and at a known periodic phase; creating a phase-folded light curve for the celestial source; measuring an intensity of the celestial source at a subsequent time; comparing the measured intensity of the celestial source to the phase-folded light curve to derive a set of possible phase differences, wherein each possible phase difference corresponds to a potential derived time based on the known time and the known stellar period of the reference measurement; and analyzing the set of possible phase differences to derive the current astrophysical time.

A method for deriving an independent current time estimate from celestial sources comprising: providing a reference measurement for a variable-intensity celestial source, wherein the reference measurement comprises the celestial source's photometric structure at a known time, at a known stellar period, and at a known periodic phase; creating a phase-folded light curve for the celestial source; measuring an intensity of the celestial source at a subsequent time; comparing the measured intensity of the celestial source to the phase-folded light curve to derive a set of possible phase differences, wherein each possible phase difference corresponds to a potential derived time based on the known time and the known stellar period of the reference measurement; and analyzing the set of possible phase differences to derive the current astrophysical time.

A method of determining a location of an optical fibre positioned at least partially inside a scattering medium, the method comprises transmitting pulsed light into the scattering medium, receiving, by a detector, photons of the pulsed light that have passed through the scattering medium, selecting signals corresponding to some of the received photons, wherein the selecting is based on a time of arrival of the received photons; and determining a location of the optical fibre based on the selected signals.