2020
DOI: 10.1007/s00340-020-07425-4
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On the performance of wavelength meters: Part 1—consequences for medium-to-high-resolution laser spectroscopy

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Cited by 29 publications
(17 citation statements)
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“…The amplitude of this relative deviation can be regarded as the lowest uncertainty limit for the precision in case of laser scans. The WS7 behaved similar to the WS7-IR which are also examined in more detail in [14]. The temporal stability of the investigated wavelength meters in a temperature-stabilized room is given for a settling time of 1 h, of 2 days and with automatic calibration.…”
Section: Resultsmentioning
confidence: 93%
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“…The amplitude of this relative deviation can be regarded as the lowest uncertainty limit for the precision in case of laser scans. The WS7 behaved similar to the WS7-IR which are also examined in more detail in [14]. The temporal stability of the investigated wavelength meters in a temperature-stabilized room is given for a settling time of 1 h, of 2 days and with automatic calibration.…”
Section: Resultsmentioning
confidence: 93%
“…During every period, the deviation from the real frequency changes quite rapidly: a laser scan by a few 100 MHz can easily lead to nonlinearities in the frequency axis of the order of several MHz. This contradicts the hope for a high relative precision of the wavelength meters in short-ranged scans and is of utmost importance if, e.g., hyperfine structure parameters or isotope shifts are to be extracted from the spectrum as is discussed in a second paper on this topic [14]. In Table 1 the amplitudes of the fluctuations are listed for the investigated wavelength meters in the third row.…”
Section: Coarse Scanmentioning
confidence: 99%
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“…Both lasers have an external reference cavity to ensure short-term stability. To ensure long-term wavelength stability, these reference cavities can in turn be locked to a HighFinesse WSU-10 wavemeter using a builtin software plug-in or to a frequency-stabilized HeNe laser using a transfer cavity [7]. The (frequency-doubled) laser light required for the atomic transitions studied in this work is [8] focused into a 1 mm spot in front of the PMT using a telescope system.…”
Section: Methodsmentioning
confidence: 99%
“…In our previous experiments, frequency locking of the emitted NesCOPO radiation has been achieved with variations in the low MHz range over serval minutes [40]. However, these results were obtained by locking the signal frequency with a commercial wavemeter, which is prone to bias and can display frequency drifts if not calibrated regularly [55].…”
Section: Nescopo Frequency Locking By Wavemetermentioning
confidence: 99%