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Supernova diffractometer

Manufactured by Rigaku
Sourced in Japan

The SuperNova diffractometer is a comprehensive X-ray diffraction system designed for single-crystal analysis. It features a high-intensity micro-focus X-ray source and a fast, low-noise detector to provide efficient and reliable data collection. The SuperNova is capable of performing a range of diffraction experiments on a variety of sample types.

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18 protocols using supernova diffractometer

1

Single-Crystal X-ray Diffraction Protocols

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Single-crystal diffraction data for 1 were collected in an Oxford Diffraction Xcalibur CCD diffractometer using graphite-monochromatic Mo-Kα radiation (λ = 0.71073 Å) at room temperature. Single-crystal diffraction data for 2 and 3 were collected in an Oxford-Diffraction SuperNova diffractometer equipped with a CCD area detector and a graphite monochromator utilising Mo-Kα (for 2) and Cu-Kα radiation (for 3). The structures were solved using SHELXT and [90 (link)] embedded in the OSCAIL software [91 (link)]. The non-H atoms were treated anisotropically, whereas the hydrogen atoms were placed in calculated, ideal positions and refined as riding on their respective carbon atoms. Molecular graphics were produced with DIAMOND [92 ]. We note that crystal twining occurs in 2, which affects the quality of the structure. We carried out many experiments in order to grow single crystals of better quality; however, this has not been achieved. We collected three sets of data using two different diffractometers and used the best set to solve the structure.
Unit cell data and structure refinement details are listed in Table 1. The crystal structures have been deposited with the Cambridge Crystallographic Data Centre (CCDC 2180525-2180527), and they can be accessed, free of charge, by filling out the application form at https://www.ccdc.cam.ac.uk/structures/.
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2

Single Crystal Structure Determination

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Single crystals of complexes 3, 4c, 5a, 6c, 7, 8b, and 9 (CCDC reference numbers 1589484–1589490) suitable for X-ray diffraction were obtained by crystallization from n-hexane/CH2Cl2 (1 : 1). Data collection was performed on an Oxford Diffraction SuperNova diffractometer, processed with CrysalisPro, and processed with Olex2, using ShelXT as the solution program and refined with SheLX-2014/7, or on a Bruker SMART 1000, using graphite-monochromated Mo Kα radiation (ω–2θ scans, λ = 0.71073 Å). The crystal data and summary of X-ray data collection are presented in Tables S1 and S2 in the ESI.
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3

Single Crystal X-ray Diffraction of Large Cation Structure

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A colorless, transparent single crystal was used in the experiment. Single crystal X-ray diffraction data were collected on an Oxford Diffraction Supernova diffractometer equipped with an Atlas CCD detector and MoKα-radiation at Aarhus University. The crystal was cooled to a temperature of 100(1) K using an Oxford Cryosystems Cryostream 700. The maximum achievable resolution was limited (sinθ/λ < 0.93 Å -1 ) due to the thermal motion of the large cations in the crystal structure. Within that resolution range, a complete data set with an average redundancy of 8.6 was collected. The data was integrated using CrysalisPro (version 39.46) and frame scale factors as well as absorption correction were applied using SCALEPACK. The integrated intensities were merged in the Laue group 2/m using SORTAV. [32] [33] A correction for low energy contamination is applied to all (3h3k3l) reflections, which led to a significant improvement of the fit. [34] [35] The structure was solved by direct methods encoded in SHELXT 36 and an independent atom model (IAM) refinement was performed with SHELXL 37 in Olex2 38 to obtain the molecular structure. Relevant crystallographic information is listed in Table 1, and an ORTEP drawing shown in Figure 1.
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4

Single Crystal X-Ray Diffraction Analysis

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Suitable single crystals were coated in inert oil, attached on a fine nylon loop, and mounted on the goniometer of a SuperNova diffractometer (Rigaku, Tokyo, Japan) which was equipped with dual X-ray micro-sources (Mo and Cu), an Eos CCD detector, and a tube operating at 50 kV and 0.8 mA.
Experimental diffraction intensities were collected and corrected for Lorentz, polarization, and absorption effects in the CrysAlis PRO package [15 ]. The crystal structures of GW-1 and GW-4 were solved with the SHELXS solution program [16 (link)] by Direct Methods, while GW-2 and GW-3 were solved with SHELXT [17 (link)] using Intrinsic Phasing. They were refined further via the SHELXL [18 ] refinement package using Least Squares minimization, all being implemented in the Olex2 package [19 (link)].
H atoms on carbons were located, refined, and treated by standard riding procedure, considering the isotropic displacement parameter Uiso(H) = 1.2Ueq(C) for ternary CH groups [C-H = 0.93 Å] and secondary CH2 groups [C-H = 0.97 Å], and 1.5Ueq(C) considered for all methyl CH3 groups [C-H = 0.96 Å].
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5

Crystal Structure Determination Protocol

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For all structures, reflection intensities were measured at 110(2) K using a SuperNova diffractometer (equipped with Atlas detector) Cu Kα radiation (λ = 1.54178 Å) under the program CrysAlisPro (Version 1.171.39.29c, Rigaku OD, 2017). The same program was used to refine the cell dimensions and for data reduction. The structures were solved with the program SHELXS-2014/7 and refined on F2 (link) with SHELXL-2014/7.45 (link) The temperature of the data collection was controlled using the system Cryojet (manufactured by Oxford Instruments). An analytical numeric absorption correction method was used involving a multifaceted crystal model based on expressions derived elsewhere.46
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6

Recrystallization and X-ray Analysis of FBTA

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For crystal structure determination and NMR analysis of the solid, FBTA was recrystallized as a methanol solvate. Commercially sourced FBTA (Fluorochem Ltd) was initially purified by removal of impurities which crystallised first upon cooling of the minimum volume of hot ethanol required to dissolve the sample from hot ethanol followed by precipitation of the FBTA by addition of an equal volume of water. Crystals suitable for X-ray diffraction were then grown by repeatedly crystallising from hot methanol, removing the supernatant liquid and repeating the process 4 times. A suitable crystal was selected and mounted on a Rigaku SuperNova diffractometer with and Atlas detector. The crystal was kept at 100.01(10) K during data collection. The crystallographic data set was solved and refined using the SHELX suite of software.10
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7

Characterization of Novel Organic Compounds

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The optical rotations were determined with a Jasco DIP-3600 digital polarimeter (Jasco, Tokyo, Japan) using a 10 mm cell. The high-resolution mass spectra were recorded using a Micromass-Q-TOF-MS (Waters, Milford, MA, USA). For the DMSO-d6, MeOD, CDCl3, and Acetone-d6, the 1H NMR and 13C NMR spectra were recorded using Bruker DRX (1H NMR, 500 MHz and 13C NMR, 125 MHz) and Bruker Avance 600 (1H NMR, 600 MHz, and 13C NMR, 150 MHz) spectrometers (Bruker, Rheinstetten, Germany), respectively. X-ray crystallography data were collected with a Rigaku Supernova diffractometer using Cu Kα (λ = 1.54184 Å) radiation. Column chromatography (CC) readings were carried out using silica gel (63–200 μm, Merck, Darmstadt, Germany), and Sephadex LH-20. A TLC analysis was performed using percolated aluminum plates backed with silica gel 60 F254 sheets. The TLC plate was visualized under UV light (254 and 365 nm), sprayed with H2SO4 (10%), and then heated.
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8

Cocrystal Formation of cis-A Derivatives

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Cocrystals cis-A‧½(1,2-DCE), cis-A‧½(1,2-DBE), and cis-A‧½C6H14 were obtained via the slow evaporation of the corresponding solutions of cis-A in 1,2-dichloroethane, 1,2-dibromoethane, and a n-hexane/CHCl3 (1:1, v/v) mixture in air at RT. Single crystals of trans-A were grown via the slow evaporation of its 1,2-dichloroethane solution in air at RT. The XRD data for cis-A‧½(1,2-DBE), cis-A‧½C6H14, and trans-A were collected using a Rigaku SuperNova diffractometer and CuKα (λ = 0.154184 nm) radiation, whereas cis-A‧½(1,2-DCE) was studied using a Xcalibur Eos diffractometer and MoKα (λ = 0.71073 nm) radiation. The structure was solved with the ShelXT [59 (link)] structure solution program using Intrinsic Phasing and refined with the ShelXL [60 (link)] refinement program incorporated into the OLEX2 program package [61 (link)] by means of Least Squares minimization. Supplementary crystallographic data for this paper have been deposited at Cambridge Crystallographic Data Centre and can be obtained free of charge via www.ccdc.cam.ac.uk/data_request/cif (accessed on 8 January 2024) (CCDC numbers 2314867 (trans-A), 2314868 (cis-A‧½(1,2-DCE)), 2314869 (cis-A‧½(1,2-DBE)), 2314870 (cis-A‧½C6H14).
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9

X-Ray Crystallography Analysis of Glycine Salicylaldehyde Complexes

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The data for GlySalLi-a and GlySalNa-h were collected using SuperNova diffractometer (Rigaku Oxford Diffraction, Oxford, UK) equipped with Atlas CCD detector and using Cu Kα radiation at 100 K. Unit cell parameters were determined and refined using CrysAlisPro program [18 ]. Additionally, the integration of the collected data was performed with the same program. Both structures were solved using direct methods with SHELXS-2013 program and then refined using SHELXL-2019/2 program [19 (link)]. Nonhydrogen atoms were refined with anisotropic displacement parameters. The hydrogen atoms were fixed at calculated distances and allowed to ride on the parent atoms using suitable constraints in SHELXL [19 (link)].
The crystal structures CIF files for GlySalLi-a and GlySalNa-h have been deposited in a Crystallography Open Database (crystallography.net) under No. 3000421 and 3000422, respectively. The crystal structures have been also deposited at the Cambridge Crystallographic Data Centre. CCDC-2220609 and 2220610 contain the supplementary crystallographic data for this paper. The data can be obtained free of charge via Cambridge Crystallographic Data Centre: www.ccdc.cam.ac.uk/structures (accessed 26 November 2022).
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10

X-ray Analysis of Apremilast Forms

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X-ray analyses of the apremilast multicomponent forms were performed either at 95 K using a SuperNova diffractometer with a micro-focus sealed tube, mirror-collimated Cu Kα radiation (λ = 1.54184 Å) and CCD detector Atlas S2; or at 120 K on an Xcalibur, Gemini ultra diffractometer using Cu Kα radiation (λ = 1.54178 Å) from a fine-focus sealed X-ray tube with a graphite monochromator and CCD detector Atlas S2.
The data reduction and absorption correction were carried out with CrysAlisPro (Rigaku Oxford Diffraction, 2019 ▸ ). The structure was solved by charge flipping methods using the Superflip software (Palatinus & Chapuis, 2007 ▸ ) and refined by full matrix least squares on the F-squared value using the Crystals software (Betteridge et al., 2003 ▸ ). The MCE software (Rohlíček & Hušák, 2007 ▸ ) was used for visualization of residual electron density maps. According to common practice, hydrogen atoms attached to carbon atoms were assigned geometrically with Uiso (H) in the range 1.2–1.5 Ueq of the parent atom (C).
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