adsabs/AstroCLIMB huggingface dataset:
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: False-color renderings of the fiducial simulation, highlighting high densities ρ (blue), β −1 = 1 surfaces (green), and large magnetizations σ (red). For ρ and σ, the color bars indicate the proper distance needed for a ray to achieve a given color; the color bar for β counts how many surfaces the ray crosses. The zoomed-out images use flat spacetime (first panel) and the appropriate Kerr spacetime (second panel) for ray tracing. For the zoomed-in images (third panel, flat; fourth panel, curved), only matter with z < −r hor is considered.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: Top: auxiliary images of affine parameter, unpolarized emission, and unpolarized optical depth in the fiducial simulation. Bottom: averages of electron temperature weighted by the scheme corresponding to the above quantity, as described in the text. Each weighting emphasizes different parts of the simulation.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: Top: true-color images of the fiducial simulation at three different viewing angles, obtained by blueshifting multifrequency data with a Lorentz factor of approximately 1200. Light from the left sides of the middle and right panels is emitted by plasma traveling toward the camera, and the resulting Doppler boost can be seen in the bluer color of the light. Bottom: the corresponding 230 GHz monochromatic images.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: Parallel scaling of Blacklight with number of threads on four different machines, measured by averaging performance across multiple runs to generate each data point. The drop at high thread counts suggests that batch processing of many images should be done with multiple independent processes on a node, each with a small number of cores.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: Unrefined (top) and adaptively refined (bottom) images of the fiducial simulation. The root level consists of 322 pixels in 82 blocks, and refinement is controlled via the absolute pixel-to-pixel intensity gradient. Refinement successfully captures interesting structure in intensity, optical depth, and circular polarization, without increasing resolution in the outer parts of the image.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: False-color, face-on images generated from the innermost regions of the fiducial simulation. Intensity (middle) can be compared with high densities (left) or high electron temperatures (right), with the former better matching the spiral structure easily seen by eye. For ρ and Θe, the color bars indicate the proper distance needed for a ray to achieve a given color.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption:  Blacklight performance as a function of output image resolution on four different machines, measured by averaging the results of multiple runs to generate each data point. Four threads are used in all cases. Solid lines indicate a single image is calculated with each call of the code; the dashed line corresponds to having Blacklight trace 10 images simultaneously.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: The fiducial image resulting from thermal electrons, and three variations made with alternate electron distributions. The power-law and kappa-distribution parameters are chosen to match the total flux of the fiducial image. The “mixed” case assumes one-third of the electrons are in each of the other cases.
Paper: Blacklight: A General-relativistic Ray-tracing and Analysis Tool
Authors: Christopher J. White
Figure caption: Elapsed time and proper length of geodesics in the fiducial simulation. The color scales are the same in geometric units, meaning the slight color differences reflect the fact that ds/dt is not necessarily unity (the speed of light) for null geodesics in a curved spacetime.
Paper: GST Data-processing Workflow: Image Registration and Alignment
Authors: Xu Yang, Wenda Cao, Vasyl Yurchyshyn
Figure caption: Image alignment between GST BFI/TiO, VIS/Hα red wing 0.8 Å, and NIRIS/He 10830 red wing 0.8 Å. Images in panels (a1), (a2), and (a3) present a pore observed on 2019 November 4 in the camera coordinates. Panels (b1) and (b2) are combined images that consist of successful coaligned GST data. The background data are from VIS/Hα and NIRIS/He I, respectively. Data filled in the black rectangle is from part of the BFI/TiO FOV. The combined images are plotted in the heliocentric coordinates system.
Paper: GST Data-processing Workflow: Image Registration and Alignment
Authors: Xu Yang, Wenda Cao, Vasyl Yurchyshyn
Figure caption: Alignment for imaging spectroscopy data with the OF method. Panels (a1) and (a2) display the selected center region (1555 × 1155 pixels) in two VIS/Hα sample wavelengths. The image intensities are normalized with their mean values. Panel (a3) is the OF vector field calculated from (a1) and (a2). The large flow vectors (more than 10 pixels) in the right are caused by the structure difference. Panel (b1) presents the histograms of the OF vector displacement field in (a3). The y-axis labels remark data counts in units of 104. Panels (b2) and (b3) are composite red–green–blue images generated by the Hα spectroscopic data. Panel (b2) consists of Hα ± 0.8 Å data and panel (b3) is combined with the Hα line center and ±0.4, ±0.8 Å data.
Paper: GST Data-processing Workflow: Image Registration and Alignment
Authors: Xu Yang, Wenda Cao, Vasyl Yurchyshyn
Figure caption: Image registration for DST (upper panels) and SST (lower panels) data. Panels (a1)/(b1) are HMI/I  c  images cotemporal to DST/SST observations. Panels (a2)/(b2) are combined by the HMI/I  c  image and DST/SST image, respectively. All panels are plotted in the heliocentric orientation. The SST and DST images are slightly cropped to present better reference-checking points (red and blue arrows).
Paper: GST Data-processing Workflow: Image Registration and Alignment
Authors: Xu Yang, Wenda Cao, Vasyl Yurchyshyn
Figure caption: Background limb-darkening removal for extreme limb observations. Panels (a1) and (a2) are the original GST/BFI TiO image and its SIFT feature map. The solar limb is in the top-right direction. Panels (b1) and (b2) are TiO data with the background removed and its SIFT feature map.
Paper: GST Data-processing Workflow: Image Registration and Alignment
Authors: Xu Yang, Wenda Cao, Vasyl Yurchyshyn
Figure caption: Time-sequence data alignment accuracy for different methods. We plotted residual displacements in the x- and y-directions in two panels. The blue, orange, and green solid lines are for the GFCT, OF, and SIFT methods, respectively.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The calculated absorption coefficient for two CO transitions broadened by air, H2, He, CO2, and H2O at temperatures of 100 (left), 296 (center), and 700 K (right) are shown in the upper panels. For all temperatures, the CO mixing ratio (X CO) is 0.2%, and the calculations are at atmospheric pressure. The residuals with respect to the CO–air calculation are shown in the corresponding lower panels (note the different scales in each plot). At 700 K, the difference between broadening appears to be less pronounced than at lower temperatures; as can be seen, the CO–He (orange) and CO–CO2 (red) peaks are significantly overlapped. In the bottom panels, the magnified differences in absorption coefficients with respect to air broadening are presented.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: A Venn diagram displaying the chemical constituents of the atmospheres of gas giants with H2- and He-dominated atmospheres (blue) and rocky planets or moons with CO2-rich atmospheres (red). The molecules in parentheses refer to the available broadening parameters in HITRAN2020 (Gordon et al. 2022; in addition to air and self broadening). Underlined molecules are not currently available as line lists in the HITRAN database but highlight the need for appropriate broadening parameters. Note, this diagram does not list all known or expected atmospheric constituents for gas giants or rocky planets, and the images represent examples of planets that have H2- and He- (e.g., Jupiter, Saturn, Uranus, Neptune) or CO2- (e.g., Mars and Venus) dominated atmospheres.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The He-broadening coefficients (γ He) for N2O as a function of ∣m∣. The Padé approximant for He broadening of N2O is plotted as the red line on the upper panel using Equation (3), with fitting coefficients given in Table 3. Experimental measurements of He broadening (with error bars) were taken from Nakayama et al. (2007) and Tasinato et al. (2010) for N2O, along with data from Nakamichi et al. (2006) for CO2. All experimental points were included in the fit, and their residuals are shown in the lower panel with a standard deviation of ∼6% for ∣m∣ < 40.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: Temperature exponents (﹩{n}_{{{\rm{H}}}_{2}}﹩) of the H2-broadening parameters for CO using the Voigt profile. The measurements of Sung & Varanasi (2004) are presented for the 1–0 and 2–0 bands. The theoretical calculations by Faure et al. (2013), the measured data by Drascher et al. (1998) and Dick et al. (2009) are also presented. The Padé approximated values using the 2–0 band data in Sung & Varanasi (2004) are displayed by the pink line and can be compared to HITRAN2016 values (also shown). The lower panel shows the standard deviation determined from the residuals of the fit.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: H2-broadening parameters for CO using the Voigt profile. The experimental results by Moal & Severin (1986); Varanasi et al. (1987); Malathy Devi et al. (2004); Sung & Varanasi (2004); Régalia-Jarlot et al. (2005), and Esteki et al. (2017) are displayed. In addition, the theoretically calculated values by Faure et al. (2013) are presented. The new estimated parameters (from a Padé approximant fit of the data in Sung & Varanasi 2004, and Malathy Devi et al. 2004) are also shown (red line), along with the HITRAN2016 values. The lower panel indicates the standard deviation determined from the fitting residuals.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The He-broadening (γ He) for CO2 as a function of ∣m∣. The upper panel displays the fitted Padé approximant for γ He (red line) at 296K using Equation (3), along with the data from Nakamichi et al. (2006; black points with error bars). The Padé approximant coefficients are provided in Table 3. The recent experimental data from Chen et al. (2021; in blue triangles) were not used for the fit, but show very good agreement with the extrapolation applied here. The lower panel indicates the standard deviation of approximately 2% for ∣m∣ < 70, determined from the fitting residuals.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The ﹩{\gamma }_{{{\rm{H}}}_{2}}﹩ values for transitions of CO2, as a function of index, ∣m∣. The air-broadening half-widths for CO2 (in blue) have been scaled by 1.5767 to obtain the ﹩{\gamma }_{{{\rm{H}}}_{2}}﹩ values (black) and are shown on the upper panel. The experimental data (with error bars) were taken from Padmanabhan et al. (2014) and Hanson & Whitty (2014). The lower panel indicates the standard deviation of around 7% for ∣m∣ < 35, determined from the fitting residuals.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The ratio of H2-broadening coefficients to corresponding air-broadening coefficients for H2CO (﹩{\gamma }_{{{\rm{H}}}_{2}/\mathrm{air}}﹩) as a function of index, J + 0.2K  a . Experimental data sets with error bars have been taken from Nerf (1975) and Nadler et al. (1987). The Padé approximant (at 296 K) fitting curve is plotted as a black line and was obtained using Equation (3). The lower panel displays the residuals and corresponding standard deviation. A constraining point was used during the fitting process to constrain the Padé function fit at higher-J values
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: A ratio of the He-broadening and air-broadening coefficients (γ He/γ air) for H2CO is plotted as a function of index, J + 0.2K  a . A fitted Padé approximant (at 296 K) is shown as the red line on the upper panel using Equation (3) and coefficients in Table 3. The data sets with error bars are taken from Nerf (1975), Barry et al. (2003), and Wang & Sharples (2012). The lower panel indicates the standard deviation, determined from the fitting residuals, is around 5% for ∣m∣ ≤ 14.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The He-broadening parameters (γ He) for CO using the Voigt profile. The values determined by Gordon & McGinnis (1971), the measured parameters from BelBruno et al. (1982); Sinclair et al. (1998); Mantz et al. (2005); Predoi-Cross et al. (2016); Luo et al. (2001), and Thibault et al. (1992a) are displayed. Moreover, the rotational transitions measured by Dick et al. (2009) and Beaky et al. (1996) are presented. The HITRAN2016 and the new He-broadening Padé function are also shown. The lower panel presents the standard deviation determined by the function-fit procedure.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The He-broadening coefficients (γ He) for OCS as a function of ∣m∣. The Padé approximant (at 296 K) is plotted as the red line on the upper panel using Equation (3); the data sets with error bars were taken from Hays et al. (2020); Jellali et al. (2019), as well as the previous work from Mäder et al. (1975); Story et al. (1971); Broquier et al. (1986); Bouanich et al. (1989). The lower panel indicates the standard deviation, determined from the residuals (experiment—fit), which is around 4.5% for ∣m∣ < 70.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: Temperature-dependence exponents of the He-broadening parameters (n He) for CO. The measured values from Mantz et al. (2005), Predoi-Cross et al. (2016), and the single value from Dick et al. (2009) are presented. The constant value in HITRAN2016 and the estimated temperature-dependence parameters using the Padé fit are shown (coefficients are given in Table 4). The lower panel indicates the standard deviation determined from the residual of the fit.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: CO2-broadening parameters (﹩{\gamma }_{{\mathrm{CO}}_{2}}﹩) of CO using the Voigt profile. The measurements are shown from the works of Varanasi (1975), Nakazawa & Tanaka (1982), Sung & Varanasi (2005), Dick et al. (2009), and Hashemi et al. (2016) using the Voigt profile. The HITRAN2016 values and the new estimated CO2-broadening parameters from the Padé function are also displayed. The lower panel displays the standard deviation determined from the residuals of the fit.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The temperature-dependence exponents of the CO2-broadened parameters (﹩{n}_{{\mathrm{CO}}_{2}}﹩) of CO using the Voigt profile measured by Nakazawa & Tanaka (1982), Sung & Varanasi (2005), Dick et al. (2009), and Hashemi et al. (2016). The Padé approximant result is shown with the solid line. The lower panel indicates the standard deviation determined from the residuals of the fit.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The H2-broadening coefficients (﹩{\gamma }_{{{\rm{H}}}_{2}}﹩) of OCS as a function of ∣m∣. The Padé approximant (at 296 K) is plotted as the black line on the upper panel using Equation (3). The data and error bars were taken from Broquier et al. (1986). The lower panel indicates the standard deviation determined by the function-fit procedure, which is approximately 5% for ∣m∣ < 65.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: CO2 pressure shift parameters (﹩{\delta }_{{\mathrm{CO}}_{2}}﹩) of different bands of CO applicable for the Voigt profile (at 296 K). The measured shifts by Hashemi et al. (2016) for the 2–0 band and Sung & Varanasi (2005) for the fundamental and the 3–0 bands are displayed. These are compared to the calculated shifts (solid lines) in the present study.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The He-broadening coefficients (γ He) for H2S as a function of index, J + 0.2K  a . The Padé approximant for 296 K is plotted as the red line on the upper panel using Equation (3) and coefficients given in Table 3. The experimental data sets with error bars were taken from Waschull et al. (1994); Kissel et al. (2000) for the ν 2 band, as well as that from the ν 1 and ν 3 band (Sumpf et al. 1997). The lower panel indicates the standard deviation determined from the residuals of the Padé approximant fitting is around 12% for ∣m∣ < 17.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The He-broadening coefficients for HCN, γ He as a function of index, ∣m∣. The Padé approximant (at 296 K) is plotted as the red line on the upper panel. Equation (3) is used to fit the selected experimental data, and a constant value is used for J > 16 in order to avoid the unreliable extrapolation. The total collected experimental data were taken from Charròn et al. (1980), Cohen & Wilson (1973), Mehrotra et al. (1985), D’Eu et al. (2002), Rohart et al. (2007). The selected data (red points) from D’Eu et al. (2002); Rohart et al. (2007) has relatively small uncertainties and was therefore used in the fit. The lower panel indicates the standard deviation determined from the residuals of the fit and is approximately 1% for ∣m∣ ≤ 16. The data provided in the ExoMol database (Tennyson et al. 2016) are shown in magenta for comparison.
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: A screenshot showing an example of how to create a new customized output format at HITRANonline. Available parameters (listed in the panel on the right) can be dragged over to the panel on the left to build a new output format. In this example, the HITRAN transition ID, the standard 160-character output (“.par line”), and the hydrogen-broadening parameters (﹩{\gamma }_{{{\rm{H}}}_{2}}﹩, ﹩{n}_{{{\rm{H}}}_{2}}﹩, ﹩{\delta }_{{{\rm{H}}}_{2}}﹩) have been added to the new output format. The uncertainty and reference codes can also be included with the corresponding radio buttons. The output format is fully customizable and allows multiple options to cater this output for the specific use of each user (e.g., HDF5 output, optional fixed format, choice of field separators, adjustable format specifiers, and inclusion of a header line).
Paper: H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4 
Authors: Yan Tan, Frances M. Skinner, Shanelle Samuels, Robert J. Hargreaves, Robab Hashemi, Iouli E. Gordon
Figure caption: The H2-broadening coefficients for HCN, ﹩{\gamma }_{{{\rm{H}}}_{2}}﹩, as a function of index, ∣m∣. The collected experimental data sets were taken from Charròn et al. (1980), Cohen & Wilson (1973), Mehrotra et al. (1985), D’Eu et al. (2002), Rohart et al. (2007), Landrain et al. (1997); Lemaire et al. (1996). The Padé approximant (Equation (3) and at 296 K) that was based on a fit to the selected experimental data sets is plotted as the red line on the upper panel. The lower panel indicates the standard deviation determined by the function-fit procedure, which is around 3% for ∣m∣ lower than 31. The magenta data provided in the ExoMol database (Tennyson et al. 2016) are shown for comparison.