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Hb175 facial solarium

Manufactured by Philips

The HB175 Facial Solarium is a piece of lab equipment designed for controlled exposure to UV light. It provides a regulated source of ultraviolet radiation, primarily intended for research and testing applications. The device's core function is to generate and deliver UV light, allowing for controlled experiments and evaluations.

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2 protocols using hb175 facial solarium

1

Photochemical Thiol-ene Synthesis of DNGSH

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All reagents were purchased from
Sigma-Aldrich or Alfa Aesar and were used without further purification.
The UV light was provided by a Philips HB175 Facial Solarium (UVA,
365 nm, P = 4 × 15 W). Reverse phase column
chromatography was conducted on a Fluka Ltd. silica gel 100 C18 reversed
phase column. Analytical TLC analysis was performed using Merck 60
RP-18 F254S aluminum-supported thin layer chromatography
sheets and visualized using an ethanolic solution of ninhydrin. 1H and 13C nuclear magnetic resonance (NMR) spectra
were recorded on a Bruker Avance 400 (400 and 100 MHz) or Bruker Avance
III (500 and 125 MHz) spectrometer. Optical rotations were recorded
at 20 °C at the sodium D line (589 nm).
DNGSH was synthesized
from GSH and N-allyl-5-(dimethylamino)naphthalene-1-sulfonamide
via the photochemical thiol-ene. Glutathione-S-conjugates were synthesized
from GSH and a range of electrophiles in H2O or a H2O/methanol mixture and sodium hydroxide, via 1,4-addition.
Further details of synthesis and compound characterization are provided
in the Supporting Information.
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2

Synthesis and Characterization of Molecular Compounds

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All reagents were purchased from Sigma Aldrich or Alfa Aesar and were used without further purification. The UV light source was provided by a Philips HB175 Facial Solarium (UVA, 365 nm, P = 4 × 15 W). Reverse phase column chromatography was carried out on Fluka Ltd silica gel 100 C18-reversed phase, under a positive pressure of compressed air. Analytical TLC analysis was performed using Merck 60 RP-18 F254S aluminium-supported thin layer chromatography sheets and visualised using ninhydrin. 1H and 13C NMR spectra were recorded on a Bruker Avance 400 (400 MHz, 100 MHz, respectively) or Bruker Avance III (500 MHz, 125 MHz, respectively). 1H and 13C spectra were assigned using 2D NMR experiments including COSY, HSQC and HMBC. Melting points were performed on a Kofler Hotstage microscope and are uncorrected; the crystallisation solvent is shown in parentheses. IR spectra were recorded using a Bruker Tensor 27 spectrometer. Elemental analyses were submitted to the Elemental Analysis Service, London Metropolitan University. Optical rotations were recorded at 20 °C at the sodium D line (589 nm). ESG was prepared as previously reported.3 (link) Selected examples of synthetic procedures are included below. Further details are available in the ESI.
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