adsabs/AstroCLIMB huggingface dataset:
Paper: The FAST Globular Cluster Pulsar Survey (GC FANS)
Authors: Yujie Lian, Zhichen Pan, Haiyan Zhang, Shuo Cao, P. C. C. Freire, Lei Qian, Ralph P. Eatough, Lijing Shao, Scott M. Ransom, Duncan R. Lorimer, Dejiang Yin, Yinfeng Dai, Kuo Liu, Lin Wang, Yujie Wang, Zhongli Zhang, Zhonghua Feng, Baoda Li, Minghui Li, Tong Liu, Yaowei Li, Bo Peng, Yu Pan, Yuxiao Wu, Liyun Zhang, Xingnan Zhang, Peng Jiang
Figure caption: The acceleration model for M92, NGC 6712, and M71. The black solid lines represent the upper and lower limits for the LOS accelerations (aℓGC) caused by the cluster as a function of the total angular offset from the center of the cluster (θ⊥). The triangles pointing down represent independent upper limits for the pulsar accelerations along the LOS, ﹩{a}_{\ell ,{\rm{P}},{\rm{\max }}}﹩. The vertical dashed lines represent the core radii of the different GCs. The cluster models can only account for the acceleration of NGC 6712A and M71D. All the remaining pulsars have values of ﹩{a}_{\ell ,{\rm{P}},{\rm{\max }}}﹩ well above the model’s prediction, indicating that their observed spin-period derivatives are dominated by the intrinsic spin-down of these pulsars.
Paper: The FAST Globular Cluster Pulsar Survey (GC FANS)
Authors: Yujie Lian, Zhichen Pan, Haiyan Zhang, Shuo Cao, P. C. C. Freire, Lei Qian, Ralph P. Eatough, Lijing Shao, Scott M. Ransom, Duncan R. Lorimer, Dejiang Yin, Yinfeng Dai, Kuo Liu, Lin Wang, Yujie Wang, Zhongli Zhang, Zhonghua Feng, Baoda Li, Minghui Li, Tong Liu, Yaowei Li, Bo Peng, Yu Pan, Yuxiao Wu, Liyun Zhang, Xingnan Zhang, Peng Jiang
Figure caption: Gamma-ray SEDs for M92, NGC 6712, and M71, which are typical of SEDs observed for MSPs. The log-parabola fit to the data comes from the 4FGL-DR4 catalog (Fermi-LAT Collaboration et al. 2023). The gray zone shows the 1σ uncertainty range.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: Examples of samples screened based on visual inspection.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: The number and frequency of newly discovered ring galaxies in this study, as well as those from other known catalogs in DR9 that meet the criteria of zspec  =  0.01–0.20 and magr < 17.5. The light blue bars represent the frequency of newly discovered ring galaxies in this study, and the dark blue bars show the frequency of known ring galaxies in DR9. The light orange line denotes the total number of ring galaxies in DR9, and the dark orange line represents the number of newly discovered ring galaxies in this study.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: (a) Swin Transformer architecture. (b) Swin Transformer blocks.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: PR curve for each model. The AUC values are identical across all three models, and the black, purple, and red points in the graph indicate the maximum F1_score achieved by ResNet18, VGG16, and Swin Transformer, respectively. When trained with a positive-to-negative sample ratio of 3:8, the maximum F1_scores were 96.24% (ResNet18), 92.94% (VGG16), and 96.78% (Swin T13-8). Increasing the training ratio to 8:8 resulted in improved maximum F1_scores of 96.62% (ResNet18), 94.90% (VGG16), and 97.35% (Swin T18-8), respectively.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: PR curve for each model. The AUC values are identical across all three models, and the black, purple, and red points in the graph indicate the maximum F1_score achieved by Swin T11-8, Swin T13-8, and Swin T18-8, which are 96.57%, 96.78%, and 97.35%, respectively.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: The distribution of color differences between the newly discovered ring galaxies and other galaxies in DR9 that meet the criteria of zspec​​​​​ = 0.01–0.20 and magr < 17.5. The blue line represents the ring galaxies identified in this study, while the orange line denotes the other galaxies in DR9.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: Thirty-six galaxies from the catalog of 8052 rings.
Paper: Identifying Ring Galaxies in DESI Legacy Imaging Surveys Using Machine Learning Methods
Authors: Aina Zhang, Xiaoming Kong, Bowen Liu, Nan Li, Yude Bu, Zhenping Yi, Meng Liu
Figure caption: The original image and the results of eight samples after applying data augmentation used in this work.
Paper: The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-sky Catalog Based on Gaia DR3
Authors: Yuming Fu, 煜铭 傅, Xue-Bing Wu, R. J. Bouwens, Karina I. Caputi, Yuxuan Pang, Rui Zhu, Da-Ming Yang, Jin Qin, Huimei Wang, Christian Wolf, Yifan Li, Ravi Joshi, Yanxia Zhang, Zhi-Ying Huo, Y. L. Ai
Figure caption: Top row: ensemble photometric redshift (zph) against spectral redshift (zcat) of the validation set with 21,777 quasars (a), zph against RegNet redshift (zxp_nn) (b), and zph of CatSouth vs. that in CatNorth for sources in common (c). Bottom row: comparisons between the spectral redshift (zcat) in the training/validation sample and the Gaia redshift (d), CatSouth zph and Gaia (e), and CatSouth zph and Quaia (f). The plots are color coded with two-dimensional densities (number counts in the pixels) of the samples, the values of which are indicated in the color bars.
Paper: The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-sky Catalog Based on Gaia DR3
Authors: Yuming Fu, 煜铭 傅, Xue-Bing Wu, R. J. Bouwens, Karina I. Caputi, Yuxuan Pang, Rui Zhu, Da-Ming Yang, Jin Qin, Huimei Wang, Christian Wolf, Yifan Li, Ravi Joshi, Yanxia Zhang, Zhi-Ying Huo, Y. L. Ai
Figure caption: HEALPix (K. M. Górski et al. 2005) sky density maps of the CatSouth quasar candidate catalog (a) and the CatGlobe (CatNorth+CatSouth) quasar candidate catalog (b). The maps are plotted in Galactic coordinates, with parameter Nside = 64 and an area of 0.839 deg2 per pixel.
Paper: The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-sky Catalog Based on Gaia DR3
Authors: Yuming Fu, 煜铭 傅, Xue-Bing Wu, R. J. Bouwens, Karina I. Caputi, Yuxuan Pang, Rui Zhu, Da-Ming Yang, Jin Qin, Huimei Wang, Christian Wolf, Yifan Li, Ravi Joshi, Yanxia Zhang, Zhi-Ying Huo, Y. L. Ai
Figure caption: Normalized confusion matrix of the XGBoost classifier computed on the validation set. The matrix is color coded by the number of sources in each cell. Diagonal entries show the fraction of correctly classified objects (i.e., recall or completeness) for each class, while off-diagonal entries indicate the misclassification rates.
Paper: The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-sky Catalog Based on Gaia DR3
Authors: Yuming Fu, 煜铭 傅, Xue-Bing Wu, R. J. Bouwens, Karina I. Caputi, Yuxuan Pang, Rui Zhu, Da-Ming Yang, Jin Qin, Huimei Wang, Christian Wolf, Yifan Li, Ravi Joshi, Yanxia Zhang, Zhi-Ying Huo, Y. L. Ai
Figure caption: Two-dimensional feature representations (color–color and morphology–color diagrams) of sources in the training sample. Quasars are shown as blue contours, galaxies as green contours, and stars as red-shaded density plots. All magnitudes are in the AB system and not dereddened.
Paper: The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-sky Catalog Based on Gaia DR3
Authors: Yuming Fu, 煜铭 傅, Xue-Bing Wu, R. J. Bouwens, Karina I. Caputi, Yuxuan Pang, Rui Zhu, Da-Ming Yang, Jin Qin, Huimei Wang, Christian Wolf, Yifan Li, Ravi Joshi, Yanxia Zhang, Zhi-Ying Huo, Y. L. Ai
Figure caption: Left: joint and marginal density distributions of proper motions of the original GDR3 QSO candidates in R.A. and decl. directions. The two-dimensional joint density plot is color coded with the number of sources. Right: same as the left panel, but for CatGlobe quasar candidates from this work.
Paper: The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-sky Catalog Based on Gaia DR3
Authors: Yuming Fu, 煜铭 傅, Xue-Bing Wu, R. J. Bouwens, Karina I. Caputi, Yuxuan Pang, Rui Zhu, Da-Ming Yang, Jin Qin, Huimei Wang, Christian Wolf, Yifan Li, Ravi Joshi, Yanxia Zhang, Zhi-Ying Huo, Y. L. Ai
Figure caption: Two-dimensional feature representations (color–color and morphology–color diagrams) of sources in the CatSouth quasar candidate catalog (blue contours), quasars from the training/validation sample (gray contours), and stars from the training/validation sample (red-shaded density plots). To avoid clutter in the figures, galaxies are not plotted. All magnitudes are in the AB system and not dereddened.
Paper: The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-sky Catalog Based on Gaia DR3
Authors: Yuming Fu, 煜铭 傅, Xue-Bing Wu, R. J. Bouwens, Karina I. Caputi, Yuxuan Pang, Rui Zhu, Da-Ming Yang, Jin Qin, Huimei Wang, Christian Wolf, Yifan Li, Ravi Joshi, Yanxia Zhang, Zhi-Ying Huo, Y. L. Ai
Figure caption: Apparent G magnitude and photometric redshift distribution of CatGlobe quasar candidates. The G magnitude is not extinction-corrected.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−methanol (13CH4−13CH3OH) ice mixtures before (top) and after (middle) irradiation at 10 K. The 320 K spectra are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 11.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of water−methanol (H2O−13CH3OH) ice mixtures before (top) and after (middle) irradiation at 10 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 7. L indicates libration.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−carbon monoxide (13CH4−13CO) ice mixtures before (top) and after (middle) irradiation at 20 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 9.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−carbon dioxide (13CH4−13CO2) ice mixtures before (top) and after (middle) irradiation at 10 K. The 320 K spectra are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 10. LO indicates longitudinal mode.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−methanol (13CH4−13CH3OH) ice mixtures before (top) and after (middle) irradiation at 20 K. The 320 K spectra are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 11.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−ammonia (13CH4−NH3) ice mixtures before (top) and after (middle) irradiation at 10 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 8.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−ammonia (13CH4−NH3) ice mixtures before (top) and after (middle) irradiation at 20 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 8.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−carbon monoxide (13CH4−13CO) ice mixtures before (top) and after (middle) irradiation at 10 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 9.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of methane−carbon dioxide (13CH4−13CO2) ice mixtures before (top) and after (middle) irradiation at 20 K. The 320 K spectra are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 10. LO indicates longitudinal mode.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Molecules identified on the surface of TNOs. The colors correspond to the following elements: hydrogen (white), carbon (gray), nitrogen (blue), and oxygen (red). Note that ground- and space-based observations also indicate silicates and unassigned refractory carbonaceous materials on TNO surfaces, along with tentative detection of hydrogen sulfide (H2S), which is not presented here.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of water (H2O) before (top) and after (middle) irradiation at 40 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 2. L and d indicate libration and dangling, respectively.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of water (H2O) before (top) and after (middle) irradiation at 10 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. Detailed peak assignments are listed in Table 2. L and d indicate libration and dangling, respectively.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia (NH3) before (top) and after (middle) irradiation at 10 K. Detailed peak assignments are listed in Table 2. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia (NH3) before (top) and after (middle) irradiation at 40 K. Detailed peak assignments are listed in Table 2. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia−carbon dioxide (NH3−13CO2) ice mixtures before (top) and after (middle) irradiation at 40 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 13.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia−carbon dioxide (NH3−13CO2) ice mixtures before (top) and after (middle) irradiation at 10 K. The infrared spectra of the irradiated sample warmed up to 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 13.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia−methanol (NH3−13CH3OH) ice mixtures before (top) and after (middle) irradiation at 40 K. The infrared spectra of processed ices at 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 14.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia−methanol (NH3−13CH3OH) ice mixtures before (top) and after (middle) irradiation at 10 K. The infrared spectra of processed ices at 320 K are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 14.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia−carbon monoxide (NH3−13CO) ice mixtures before (top) and after (middle) irradiation at 20 K. The 320 K spectra are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 12.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of ammonia−carbon monoxide (NH3−13CO) ice mixtures before (top) and after (middle) irradiation at 10 K. The 320 K spectra are shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 12.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of carbon monoxide−methanol (13CO−13CH3OH) ice mixtures before (top) and after (middle) irradiation at 20 K. The infrared spectra of the irradiated sample warmed up to 320 K are also shown at the bottom. The experimental spectra are plotted in black, the deconvoluted peaks are in blue, and the sums are in red. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 16.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of monoxide−carbon dioxide (13CO−13CO2) ice mixtures before (top) and after (middle) irradiation at 20 K. The infrared spectra of the irradiated sample warmed up to 320 K are also shown at the bottom. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 15. L indicates longitudinal.
Paper: Spectroscopic Study of Ice Analogs of Trans-Neptunian Objects Exposed to Ionizing Radiation. II. Infrared Spectra and Functional Groups
Authors: Chaojiang Zhang, Jia Wang, Andrew M. Turner, Leslie A. Young, Ralf I. Kaiser
Figure caption: Infrared spectra of monoxide−carbon dioxide (13CO−13CO2) ice mixtures before (top) and after (middle) irradiation at 10 K. The infrared spectra of the irradiated sample warmed up to 320 K are also shown at the bottom. Only noticeable peaks are labeled for clarity, and detailed peak assignments are listed in Table 15. L indicates longitudinal.