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Continuous flow helium cryostat

Manufactured by Oxford Instruments

The Continuous Flow Helium Cryostat is a laboratory instrument designed to provide a controlled and stable cryogenic environment. It utilizes a continuous flow of liquid helium to maintain low temperatures, typically ranging from 1.5 Kelvin to 300 Kelvin. The cryostat is equipped with a sample chamber and various mounting options to accommodate a variety of experimental setups.

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4 protocols using continuous flow helium cryostat

1

CW EPR Spectroscopy of RFQ Samples

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CW X-band EPR spectra of RFQ samples were collected at 10 K at Pennsylvania State University using a Bruker ESP-300 spectrometer (~9.5 GHz) equipped with an ER/4102 ST resonator (Bruker), a continuous flow helium cryostat (Oxford Instruments), and a temperature controller (ITC 502, Oxford Instruments).23 (link) All other CW X-band EPR spectra from 5–30 K (9.62 GHz) were collected at the Ohio Advanced EPR Facility at Miami University using a Bruker EMX instrument equipped with an Oxford Instruments continuous flow helium cryostat and temperature controller (ESR 900). For time-dependent studies of product formation, the temperature was set to 6.67 K to avoid saturation artifacts.17 (link) Spectra were obtained using a microwave power of 20 mW and a modulation frequency and amplitude of 100 kHz and 10 G, respectively. Spin quantitation was carried out using a 250 μM copper(II) azurin standard measured under non-saturating conditions (200 μW).
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2

Formation of Fe-S Center in Ferredoxin

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The formation of the Fe-S center in ferredoxin was also analyzed by Electron paramagnetic resonance EPR. Apo-ferredoxin was prepared as described above. All the reconstitutions were made in the presence of 30 µM apo-ferredoxin, 4 mM DTT, 2 µM IscS, 2 mM L-cysteine and 300 µM E. coli RIC. The spectra of control reactions that contained all components except apo-ferredoxin or RIC were acquired. Two other control reactions in which RIC was replaced by ferrous iron (200 µM) or apo-RIC (300 µM) were also analyzed. In all the assays, the reaction was initiated by the addition of L-cysteine and let proceed for 2 h in an anaerobic chamber, after which, samples were transferred to EPR tubes and frozen in liquid nitrogen. After recording their spectra, samples were thawed (under anaerobic conditions) and reduced by the addition of a few drops of sodium dithionite solution (100 mM), frozen and analyzed again. EPR spectra were obtained on a Bruker EMX spectrometer equipped with an Oxford Instruments continuous flow helium cryostat and were recorded at 9.34 MHz microwave frequency, 2.0 mW microwave power, 1 mT modulation amplitude and at 17 K.
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3

Pulsed EPR Measurements of Protein Structures

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Pulsed EPR measurements were performed at Q band (34 GHz) and −223 °C on an Elexsys 580 spectrometer (Bruker). Therefore, 15 μl of the freshly prepared samples were loaded into EPR quartz tubes with a 1.6 mm outer diameter and shock frozen in liquid nitrogen. During the measurements, the temperature was controlled by the combination of a continuous-flow helium cryostat (Oxford Instruments) and a temperature controller (Oxford Instruments). The four-pulse DEER sequence was applied64 (link) with observer pulses of 32 ns and a pump pulse of 13–18 ns. The frequency separation was set to 70 MHz and the frequency of the pump pulse to the maximum of the nitroxide EPR spectrum. Validation of the distance distributions was performed by means of the validation tool included in DeerAnalysis65 (link) and varying the parameters “Background start” and “Background density” in the suggested range by applying fine grid. A prune level of 1.15 was used to exclude poor fits. Furthermore, interspin distance predictions were carried out by using the rotamer library approach included in the MMM software package19 (link). The calculation of the interspin distance distributions is based on the cryo-EM structures of state 1, state 2 and the crystal structure [5MRW]4 (link) for the comparison with the experimentally determined interspin distance distributions.
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4

UV-Visible and EPR Spectroscopy of Hemoglobins

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UV-visible absorption spectra of haemoglobins (10 µM) were recorded, at room temperature, in a Shimadzu UV-1700 spectrophotometer.
EPR spectra were obtained in a Bruker EMX spectrometer equipped with an Oxford Instruments continuous flow helium cryostat and were recorded at 12 K, 9.4 GHz microwave frequency, 2.0 mW microwave power and 1 mT modulation amplitude.
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