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Helium flow cryostat

Manufactured by Oxford Instruments
Sourced in United Kingdom

The Helium flow cryostat is a lab equipment designed to provide a controlled and stable cryogenic environment for various scientific and research applications. The core function of this device is to generate and maintain a flow of liquid helium at low temperatures, enabling researchers to study materials and phenomena at cryogenic conditions.

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8 protocols using helium flow cryostat

1

Spectroscopic Characterization of Paramagnetic Species

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UV-visible absorbance measurements were performed using a Jasco V500 spectrometer, and CD spectra were measured with a Jasco J810 spectropolarimeter. EPR measurements were made with an X-band Bruker EMX EPR spectrometer equipped with a helium flow cryostat (Oxford Instruments). EPR spectra were measured at 10 K at the following instrumental settings: microwave frequency, 9.471 GHz; microwave power, 3.18 mW; modulation frequency, 100 kHz; modulation amplitude, 5 G; time constant, 82 ms; scan rate, 22.6 G s–1; single scan per spectrum. Relative concentrations of the paramagnetic species were measured using the procedure of spectral subtraction with a variable coefficient56 (link) and converted to absolute concentrations by comparing an EPR spectrum second integral to that of a 1 mM Cu(ii) in 10 mM EDTA standard, at non-saturating values of the microwave power.
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2

X-band cw-EPR Spectroscopy Measurements

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X-band cw-EPR measurements were performed on a Bruker E500 ELEXSYS
spectrometer equipped with the Bruker dual-mode cavity (ER4116DM)
and an Oxford Instruments helium flow cryostat (ESR 900). The microwave
bridge was the high-sensitivity bridge Super-X from Bruker (ER-049X)
with integrated microwave frequency counter. The magnetic field controller
(ER032T) was externally calibrated with a Bruker NMR field probe (ER035M).
Spectral analysis and simulations were handled by using the EasySpin
program.34 (link)
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3

EPR and UV-Vis Analysis of Reduced Proteins

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EPR measurements were made using an X-band Bruker EMX EPR spectrometer equipped with a helium flow cryostat (Oxford Instruments). EPR spectra were measured at 10 K at the following instrumental settings: microwave frequency, 9.471 GHz; microwave power, 3.18 mW; modulation frequency, 100 kHz; modulation amplitude, 5 G; time constant, 82 ms; scan rate, 22.6 G s−1; single scan per spectrum. Protein samples for EPR spectroscopy were prepared in an anaerobic glove box. The protein was reduced by the addition of an excess of sodium dithionite, and samples were flash-frozen in liquid nitrogen.
UV-visible spectra were recorded and colorimetric assays performed using a Shimadzu UV-1800 spectrophotometer, quartz cuvettes, and UVprobe software (Shimadzu). A JASCO model J810 circular dichrograph was used to measure CD spectra for the wavelength range 250 to 800 nm. Protein samples were prepared as for EPR spectroscopy but transferred to anaerobic quartz cuvettes for measurement at ambient temperature.
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4

EPR Spectroscopy of Complex I

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EPR measurements were performed using an X/Q-band Bruker Elexsys E580 Spectrometer (Bruker BioSpin GmbH, Germany) equipped with a closed-cycle cryostat (Cryogenic Ltd., UK) and X-band split-ring resonator module (ER 4118X-MD5), or a Bruker EMXMicro spectrometer with a helium flow cryostat (Oxford Instruments, UK). All measurements were performed at X-band (9.7 GHz). The magnetic field was calibrated at room temperature with a Bruker strong pitch standard (g = 2.0028). Baseline spectra of the empty resonator, of samples containing only buffer, as well as of oxidised complex I were found to be identical; all the CW spectra presented have been baseline subtracted. Continuous-wave EPR measurement conditions were 100 kHz modulation frequency, 7 G modulation amplitude; other measurement conditions are given in figure legends.
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5

Absorbance Kinetics and EPR Spectroscopy

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Absorbance kinetic data at A386 nm were recorded via a fibre optic link, as previously described (Crack et al., 2007 (link)). EPR measurements were made with an X-band Bruker EMX EPR spectrometer equipped with a helium flow cryostat (Oxford Instruments). Unless stated otherwise, EPR spectra were measured at 10 K at the following instrumental settings: microwave frequency, 9.471 GHz; microwave power, 3.18 mW; modulation frequency, 100 kHz; modulation amplitude, 5 G; time constant, 82 ms; scan rate, 22.6 G/s; single scan per spectrum. Relative concentrations of the paramagnetic species were measured using the procedure of spectral subtraction with a variable coefficient (Svistunenko et al., 2006 (link)) and converted to absolute concentrations by comparing an EPR spectrum second integral to that of a 1 mM Cu(II) in 10 mM EDTA standard, at non-saturating values of the microwave power. The RirA EPR signal saturation was studied by taking EPR measurements at 13 values of microwave power, ranging from 0.2 µW to 200 mW, at eight temperature values, ranging from 4 K to 50 K. The EPR sample was equilibrated at every new temperature for at least 8 min before the power set of spectra measurements commenced.
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6

X-band EPR of Redox-Poised Samples

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X-band EPR spectra were recorded using a Bruker-Biospin EleXsys E500 spectrometer equipped with a standard rectangular Bruker EPR cavity fitted to an Oxford Instruments helium flow cryostat. Redox poised samples were prepared as previously described9 (link)52 (link). Redox potentials are given in the text with respect to the standard hydrogen electrode.
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7

Continuous-wave EPR Spectroscopy Methodology

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Continuous-wave (cw) X-band EPR measurements
were performed on a Bruker E500 ELEXSYS spectrometer equipped with
the Bruker dual-mode cavity (ER4116DM) or a standard cavity (ER4102ST)
and an Oxford Instruments helium flow cryostat (ESR 900). The microwave
bridge was a high-sensitivity Super-X bridge (Bruker ER-049X) with
integrated microwave frequency counter. The magnetic field controller
(ER032T) was calibrated with a Bruker NMR field probe (ER035M). EPR
simulations have been done with our own routines, esim_gfit and esim_sx.
For spin quantitation, the experimental derivative spectra were numerically
integrated by using the routine eview, and the results were corrected
for their g value dependence for field-swept spectra
by using Aasa and Vänngård approximation,32 (link) i.e. dividing the integrals by the factor,
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8

Cd K-edge XAFS Characterization Protocol

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Samples and standards were measured at the Stanford Synchrotron Radiation Lightsource (SSRL), California at the beamline 7–3, with the SPEAR electron storage ring containing 500 mA at 3.0 GeV, using a Si (220) double crystal monochromator. Samples were maintained at 10 K using a helium flow cryostat (Oxford instruments, Abingdon, UK) with sample cuvettes inclined at 45° to the incident X-ray beam. For each sample, 7 to 11 scans each of about 35 min duration were accumulated. The incident and transmitted X-ray intensities were monitored using nitrogen-filled gas ionization chambers operating at 1.2 atmospheres with a sweeping voltage of 1600 V, while the Cd K-edge X-ray absorption was measured as the X-ray Kα fluorescence excitation spectrum using an array of 30 germanium detectors [24 (link)] with Soller slits and six absorption-length silver metal filters to preferentially eliminate scattered X-rays so as to maintain the detector count rates in the pseudo-linear regime. The energy was calibrated with reference to the lowest energy K-edge inflection of cadmium metal foil which was assumed to be 26714.0 eV. Data were collected using the Web version of the XAS Collect data acquisition software (SSRL, Stanford, CA, USA) [25 (link)].
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