Data for: Amplified electron-spin thermal sensitivity in Mn(II) complexes
Data files
Jul 08, 2026 version files 5.17 MB
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Emission_Spectra.zip
9.16 KB
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Heat_Capacity_Data.zip
257.71 KB
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HFEPR.zip
3.89 MB
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MPMS.zip
76.31 KB
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PXRD.zip
616.24 KB
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Qband_EPR.zip
97.83 KB
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README.md
11.66 KB
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Xband_EPR.zip
217.56 KB
Abstract
Understanding the temperature sensitivity of magnetic resonance properties is an essential step toward any application of spin, whether for novel molecular thermometers or quantum sensing platforms. In that light, demonstrations that molecular design is effective at controlling the temperature dependence of zero-field splitting (D), a critical property that governs the electron paramagnetic resonance (EPR) response of open-shell molecules, are vital. Herein we show that ligand design controls the temperature dependence of D. To do so, we prepared and analyzed three different encapsulated Mn(II) complexes. High-field, high-frequency EPR spectroscopy reveal EPR spectra for all complexes that vary in width as a function of temperature, indicating a change in D value. At lower temperatures, these temperature sensitivities change starkly with ligand shell, ranging from 2.2 to 9.8 MHz/K. These results are demonstrate the ability to tune the variable-T nature of D by molecular design, the first such for the Mn(II) metal ion, and exhibit orders of magnitude enhancement over the nitrogen vacancy center of diamond (ca. 74 kHz/K).
https://doi.org/10.5061/dryad.bcc2fqzpj
Description of the data and file structure
All contained data are either the raw data directly from the instruments used to acquire the data, or aggregated collections of the data in a format sufficient for plotting and analysis in external programs. The data that are attached are compressed, zip folders of the raw data and data used to make figures. Unzip these folders to access the raw data.
Files and variables
File: Xband_EPR.zip
Description: This folder contains the raw variable-temperature X-band EPR data for MnL1, MnL2, and MnL3. See manuscript for measurement details (i.e. in solution, concentration, etc). Data sets are labeled with measurement conditions. "MnL1_10K_5mM" corresponds to measurements of complex MnL1 at 10 K with a 5 mM frozen solution.
Raw EPR data is in Bruker DTA/DSC formatting. The DSC (or "description" file) has information about the measurement conditions and instrument settings and can be opened with any text editor. The DTA file has the actual spectral information in it. The DTA file alone cannot be opened with a simple text editor. Instead, it can be opened with the program EasySpin (easyspin.org) in Matlab using the eprload command and processed accordingly. See https://easyspin.org/easyspin/documentation/importexport.html for more details on data import in this manner. Data can also be opened with Bruker's own software, Xepr, and there are also free, python-based packages (e.g. cwepr) that can be used to open the spectra to get information. See the bottom for links to more information on the processing of the DTA/DSC data.
File: HFEPR.zip
Description: EPR data aggregated in origin file format. The program OriginPro (or the free origin viewer) can be used to open the data (see below). Data are organized into worksheets based on the relevant experiment, which also include spreadsheets of any fits of the data. Measurements are labeled by compound name and include all relevant sample data, and variables in this case include intensity (I), magnetic field (B), and temperature. Summary plots.opj contains the aggregated data sets used to make plots for the main paper.
File: PXRD.zip
Description: PXRD data and simulations in origin file format. The program OriginPro (or the free Origin viewer) can be used to open the data. Data are organized into worksheets based on the relevant experiment, which also include spreadsheets of any fits of the data. Files are named according to the complex: MnL1, MnL2, and MnL3. Measurements are labeled by compound name and include all relevant sample data. Relevant variables here are intensity (I) versus diffraction angle (2-theta).
File: Emission_Spectra.zip
Description: This folder contains three sets of data in csv file format. Data can be opened following any spreadsheet program. Measurements are labeled by compound name and include all relevant sample data. The top of each csv has instrumental parameters for the collection (see manuscript for more description of measurement and interpretation). Below that data are two columns of parameters, the left column is wavelength and the right column is emission intensity. Compounds are labeled MnL1, MnL2, and MnL3 for compounds 1, 2, and 3 in the manuscript.
File: Qband_EPR.zip
Description: This folder contains the Q-band EPR data, which constitute a variable-temperature Hahn-echo detected EPR experiment - see manuscript for measurement details; these measurements were only performed on MnL2 as a proof-of-concept measurement for the paper. Files are labeled "MnL2_XK_FS" which indicates the compound name, the temperature of the measurement ("XK") and "FS" indicates the field-swept nature of the measurement. Files labeled "Empty_Resonator" contain the measurement data for the empty resonator under the same conditions to help identify background peaks.
Data are in the form of Bruker DSC/DTA files. Raw EPR data is in Bruker DTA/DSC formatting. The DSC (or "description" file) has information about the measurement conditions and instrument settings and can be opened with any text editor. The DTA file has the actual spectral information in it. The DTA file alone cannot be opened with a simple text editor. Instead, it can be opened with the program EasySpin (easyspin.org) in Matlab using the eprload command and processed accordingly. See https://easyspin.org/easyspin/documentation/importexport.html for more details on data import in this manner. Data can also be opened with Bruker's own software, Xepr, and there are also free, python-based packages (e.g. cwepr) that can be used to open the spectra to get information. See the bottom for links to more information on the processing of the DTA/DSC data.
File: MPMS.zip
Description: data are in standard instrument format (.dat), which can be read and manipulated in any spreadsheet program. Measurements are labeled by compound name. "Mn-iminocryptand-PF6" is compound 1, "Mn-aminocryptand" is compound 2, and "Mn-AssymmetricL-PF6" is compound 3. These files include all relevant sample data. Relevant variables here are temperature (K), magnetic field (T), and moment (emu), though many other parameters are recorded in the raw data. These files are comma-delimited data sets. Briefly, rows listed as "INFO" contain instrumental and sample information, e.g. version of the instrument software, sample mass. Below that are the data and conditions such as temperature, field, etc. Detailed information about the information in these files can be obtained from the manufacturer of the MPMS system, Quantum Design, through their Pharos online library.
File: Heat_Capacity_Data.zip
Description: This file has two subfolders, "Fit summaries" and "PPMS data". We'll describe the PPMS data contents first. This folder contains six excel files labeled by complex: "MnL1", "MnL2", and "MnL3" and in two forms, “PPMS Output File” and “Workup”. Data in the former set of files include temperature, sample heat capacity, molar samples heat capacity, and temperature as output from the program. The workup excel files contain the processed data from the measurements, including data that was directly used to make figures in the main manuscript.
The "Fitting" subfolder has the data output from simulation of these data sets, and we refer the reader to the main manuscript for details. This subfolder includes several pieces of information. First, there are three summary excel files of the fits for each complex, labeled as “MnLx Fitting summary”. These spreadsheets contain several pieces of information. First, the actual data, which is organized in four columns, temperature (T) and then the heat capacities are organized in terms of the field (0, 1, and 2 T, respectively). To the right of the actual data are the results of the best fits of the data. First, there is the simulation from python of only the Debye model contribution to the heat capacity, which is also organized similar to the actual data (temperature then heat capacities to the right). To the right of the fit from python, there is the fit from PHI with a spin-only isotropic g model contribution to the heat capacity, organized like the other two sets, and then to the right of that are the "Total fit" heat capacities that result from summing the two contributions into the total fit. Again, these are all laid out in columns of heat capacities labeled by the magnetic field of collection, organized from left to right. The temperatures for these total fit heat capacities are the same as the temperatures of the actual data. Also in the spreadsheets are the final parameters extracted from these simulations, containing the extracted Debye temperatures, zero-field splittings, and g tensors, all the way on the right.
The fitting subfolder also includes the fits themselves. All files can be opened with a text editor. The individual fits for each MnLx complex are represented with a folder and then an annotated python script “MnLx Debye fits.py”. The python script was used to simulate the heat capacity data using the Debye model. This data was combined with the spin-based (low temperature) component from PHI. The folders "MnLx 2-50K spin only iso" contain the PHI portions of the simulations, which are divided into four different files. All files are labeled with the name of the folder, but different extensions. The "heat.exp" file contains the experimental values of heat capacity that are read into the PHI program and are four columns of temperature, then heat capacity at the three magnetic fields (from left to right 0 , 1, and 2 T). The "heat.res" file is the tabulated output (the "results" or ".res") of the simulation with four columns: temperature, then 0, 1, and 2 T simulated heat capacity values. The ".best" file is the results for the spin hamiltonian parameters that produced the fit (here "g" which is labeled "GF", "CF 1 2 0" is D and then "CF 1 2 2" is E) and then the residual. The ".input" file is the instruction file for PHIs fits, which has the spin Hamiltonian parameters in it, the heat capacity fitting parameters, then other parameters. The PHI instructions (see below) have detailed information about each of these files and what the terms in them mean.
Access information
Other publicly accessible locations of the data: N/A
Data was derived from the following sources:
- Easyspin reference: Stefan Stoll, Arthur Schweiger
EasySpin, a comprehensive software package for spectral simulation and analysis in EPR
J. Magn. Reson. 178(1), 42-55 (2006) DOI: 10.1016/j.jmr.2005.08.013 - Easyspin website, which contains all relevant information on how to open, process, and simulate EPR spectra from Bruker DSC/DTA files: https://easyspin.org/
- cwepr reference: Mirjam Schröder and Till Biskup
cwepr – a Python package for analysing cw-EPR data focussing on reproducibility and simple usage
Journal of Magnetic Resonance 335:107140, 2022. doi:10.1016/j.jmr.2021.107140 - cwepr website: https://www.cwepr.de/index
- PHI reference: N. F. Chilton, R. P. Anderson, L. D. Turner, A. Soncini and K. S. Murray J. Comput. Chem. 34, 1164-1175 (2013).
- PHI website: https://www.nfchilton.com/phi.html
- OriginPro: Origin is a paid software available here: https://www.originlab.com/
- Access to any data recorded in origin files in this submission can be accessed via the free program origin viewer: https://www.originlab.com/viewer/
- Quantum Design has extensive documents (application notes and manuals) available for the instruments that were used to collect the magnetic data (given in MPMS.zip and Heat_Capacity_data.zip). This information is available at their online library (https://qdusa.com/pharosindex/index.html)
Methods and workup are detailed in the methods section of the corresponding manuscript
