cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.7910/dvn/6ah3bg/9tvzte
title: 31- High 4.cdf

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title: 31- High 4.gci

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DOI: 10.7910/dvn/6ah3bg/pdwwwh
title: 30- Heatlhy Control 14.cdf

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DOI: 10.7910/dvn/6ah3bg/dll6vh
title: 34- High 5.cdf

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DOI: 10.7910/dvn/6ah3bg/srzu1x
title: 33-QC6.cdf

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DOI: 10.7910/dvn/6ah3bg/tin64p
title: 33-QC6.gci

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DOI: 10.7910/dvn/6ah3bg/4bxbok
title: 35- Heatlhy Control 15.gci

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DOI: 10.7910/dvn/6ah3bg/bcvuzt
title: 35- Heatlhy Control 15.cdf

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DOI: 10.7910/dvn/6ah3bg/ftbwic
title: 34- High 5.gci

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DOI: 10.7910/dvn/6ah3bg/ug30sf
title: 36- Quiescent 4.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/bp5n10
title: 37- Heatlhy Control 16.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/sshftd
title: 37- Heatlhy Control 16.gci

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DOI: 10.7910/dvn/6ah3bg/wpkko5
title: 36- Quiescent 4.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/8fcchg
title: 39-QC7.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/ibl2lp
title: 38- Heatlhy Control 17.gci

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DOI: 10.7910/dvn/6ah3bg/l2fjhe
title: 38- Heatlhy Control 17.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/9vefhj
title: 39-QC7.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/d1iwwr
title: 40- High 6.cdf

description: :unav
DOI: 10.17199/375c452d-b0cd-43c5-b110-47f7e96264b6
title: Sample data from V20

description: These data were collected at ESS as part of sample data for V20
DOI: 10.5281/zenodo.3362198
title: Systematic screening of DMOF-1 with NH2, NO2, Br and azobenzene functionalities for elucidation of carbon dioxide and nitrogen separation properties

description: <strong>Publication:</strong> M. Xie. N. Prasetya and B. P. Ladewig, Systematic screening of DMOF-1 with NH2, NO2, Br and azobenzene functionalities for elucidation of carbon dioxide and nitrogen separation properties, Inorganic Chemistry Communications (2019). <strong>Preprint:</strong> M. Xie. N. Prasetya and B. P. Ladewig, Systematic screening of DMOF-1 with NH2, NO2, Br and azobenzene functionalities for elucidation of carbon dioxide and nitrogen separation properties, Inorganic Chemistry Communications (2019), https://doi.org/10.26434/chemrxiv.8862239.v1 Dataset supporting publication, including SEM images, optical microscope images, NMR spectra, data used in Figures, and full resolution figures as included in the manuscript. <strong>Abstract:</strong> In this study, dabco MOF-1 (DMOF-1) with four different functional groups (NH<sub>2</sub>, NO<sub>2</sub>, Br and azobenzene) has been successfully synthesized through systematic control of the synthesis condition of their parent framework. The functionalised DMOF-1 is characterized using various analytical techniques including PXRD, TGA and N<sub>2</sub> sorption. The effect of the various functional groups on the performance of the MOFs for post-combustion CO<sub>2</sub> capture is evaluated. DMOF-1s with polar functional groups are found to have better affinity with CO<sub>2</sub> compared with the parent framework as indicated by higher CO<sub>2</sub> heat of adsorption. However, imparting steric hindrance to the framework as in Azo-DMOF-1 enhances CO<sub>2</sub>/N<sub>2</sub> selectivity, potentially as a result of lower N2 affinity for the framework.
DOI: 10.7910/dvn/6ah3bg/1vrgn7
title: 41- Heatlhy Control 18.gci

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DOI: 10.7910/dvn/6ah3bg/ekwdio
title: 41- Heatlhy Control 18.cdf

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DOI: 10.7910/dvn/6ah3bg/gusj7c
title: 42- High 7.cdf

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DOI: 10.7910/dvn/6ah3bg/onnsrl
title: 40- High 6.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/dyn3t9
title: 42- High 7.gci

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DOI: 10.7910/dvn/6ah3bg/g5odb2
title: 43- Heatlhy Control 19.gci

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DOI: 10.7910/dvn/6ah3bg/xj5dtw
title: 43- Heatlhy Control 19.cdf

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DOI: 10.7910/dvn/6ah3bg/g6zeby
title: 44- Heatlhy Control 20.gci

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DOI: 10.7910/dvn/6ah3bg/glm9ej
title: 44- Heatlhy Control 20.cdf

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DOI: 10.7910/dvn/6ah3bg/upatjj
title: 45-QC8-.cdf

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DOI: 10.7910/dvn/6ah3bg/3w36md
title: 47- High 8.cdf

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DOI: 10.7910/dvn/6ah3bg/nfppjc
title: 45-QC8-.gci

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DOI: 10.7910/dvn/6ah3bg/pxfm5k
title: 46- Low 5.cdf

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DOI: 10.7910/dvn/6ah3bg/x8ed57
title: 46- Low 5.gci

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DOI: 10.7910/dvn/6ah3bg/azcpuw
title: 48- Heatlhy Control 21.gci

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DOI: 10.7910/dvn/6ah3bg/jxgotu
title: 47- High 8.gci

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DOI: 10.7910/dvn/6ah3bg/nuibna
title: 48- Heatlhy Control 21.cdf

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DOI: 10.7910/dvn/6ah3bg/1kcic1
title: 49- Low 6..gci

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title: 49- Low 6..cdf

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DOI: 10.7910/dvn/6ah3bg/zqx6kq
title: 50- Heatlhy Control 22.cdf

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title: 51-QC9.cdf

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DOI: 10.7910/dvn/6ah3bg/z6ly9y
title: 50- Heatlhy Control 22.gci

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DOI: 10.7910/dvn/6ah3bg/irdb97
title: 53- Heatlhy Control 23.cdf

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DOI: 10.7910/dvn/6ah3bg/lroh2n
title: 52- High 9.cdf

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title: 52- High 9.gci

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DOI: 10.7910/dvn/6ah3bg/xaijmt
title: 51-QC9.gci

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DOI: 10.7910/dvn/6ah3bg/65i1rh
title: 53- Heatlhy Control 23.gci

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DOI: 10.7910/dvn/6ah3bg/islrhj
title: 54- Heatlhy Control 24.cdf

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DOI: 10.7910/dvn/6ah3bg/lbjjcu
title: 55- Low 7.gci

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DOI: 10.7910/dvn/6ah3bg/uenb2f
title: 54- Heatlhy Control 24.gci

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DOI: 10.7910/dvn/6ah3bg/ygwju6
title: 55- Low 7.cdf

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DOI: 10.7910/dvn/6ah3bg/zqprs5
title: 56- Heatlhy Control 25.cdf

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DOI: 10.7910/dvn/6ah3bg/aql58j
title: 58-QC10.cdf

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DOI: 10.7910/dvn/6ah3bg/cutefr
title: 56- Heatlhy Control 25.gci

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DOI: 10.7910/dvn/6ah3bg/icamqx
title: 58-QC10.gci

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DOI: 10.7910/dvn/6ah3bg/lc0lee
title: 59- Heatlhy Control 26.cdf

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DOI: 10.7910/dvn/6ah3bg/r4vmjk
title: 59- Heatlhy Control 26.gci

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DOI: 10.7910/dvn/6ah3bg/9xafnu
title: 60- Low 8.gci

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DOI: 10.7910/dvn/6ah3bg/dyqhzs
title: 60- Low 8.cdf

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DOI: 10.7910/dvn/6ah3bg/2htbvo
title: 61- High 10.gci

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DOI: 10.7910/dvn/6ah3bg/gyeawh
title: 62- Heatlhy Control 27.cdf

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DOI: 10.7910/dvn/6ah3bg/nznxnt
title: 61- High 10.cdf

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DOI: 10.7910/dvn/6ah3bg/aa9fm4
title: 63- Quiescent 5.cdf

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DOI: 10.7910/dvn/6ah3bg/v32ums
title: 62- Heatlhy Control 27.gci

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DOI: 10.7910/dvn/6ah3bg/a2ncau
title: 64-QC11.cdf

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DOI: 10.7910/dvn/6ah3bg/jxtqmc
title: 64-QC11.gci

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DOI: 10.7910/dvn/6ah3bg/r1fawh
title: 63- Quiescent 5.gci

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DOI: 10.7910/dvn/6ah3bg/0ewoiw
title: 65- Heatlhy Control 28.gci

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DOI: 10.7910/dvn/6ah3bg/qcerq3
title: 65- Heatlhy Control 28.cdf

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DOI: 10.7910/dvn/6ah3bg/0lpsgo
title: 66- Heatlhy Control 29.cdf

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DOI: 10.7910/dvn/6ah3bg/pvsq1i
title: 67- Quiescent 6.cdf

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DOI: 10.7910/dvn/6ah3bg/tzwyln
title: 66- Heatlhy Control 29.gci

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DOI: 10.7910/dvn/6ah3bg/1jgxrt
title: 67- Quiescent 6.gci

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DOI: 10.7910/dvn/6ah3bg/qyju0x
title: 68- Quiescent 7.cdf

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DOI: 10.7910/dvn/6ah3bg/fbx0xx
title: 69- Low 9.gci

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DOI: 10.7910/dvn/6ah3bg/juowdr
title: 68- Quiescent 7.gci

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DOI: 10.7910/dvn/6ah3bg/rgscyi
title: 69- Low 9.cdf

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DOI: 10.7910/dvn/6ah3bg/ppmxpd
title: 70-QC12.cdf

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DOI: 10.7910/dvn/6ah3bg/xelozt
title: 70-QC12.gci

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DOI: 10.7910/dvn/6ah3bg/jyetcf
title: 71- Heatlhy Control 30.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/wmhzmi
title: 71- Heatlhy Control 30.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/42pv6f
title: 73- Low 11.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/qt5wl5
title: 72- Low 10.gci

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DOI: 10.7910/dvn/6ah3bg/z5um91
title: 72- Low 10.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/edvqh1
title: 74- Heatlhy Control 31.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/fegiaw
title: 73- Low 11.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/zxuxbv
title: 74- Heatlhy Control 31.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/cgk7a8
title: 76-QC13.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/fpzcth
title: 75- Quiescent 8.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/lo7tgk
title: 76-QC13.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/wdfnk5
title: 75- Quiescent 8.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/2tyssx
title: 78- High 11.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/8p8gdt
title: 77- Low 12.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/apzo14
title: 77- Low 12.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/5kwyzr
title: 79- Low 13.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/bmfeh8
title: 79- Low 13.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/jfk3kl
title: 78- High 11.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/qenqof
title: 80-- Heatlhy Control 32.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/chgohh
title: 81-QC14.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/eux1bd
title: 80-- Heatlhy Control 32.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/pqynxc
title: 81-QC14.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/kgwwfi
title: 82- Quiescent 9.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/zwt0ss
title: 82- Quiescent 9.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/b4lpsc
title: 84- Low 14.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/ei5cvs
title: 83- High 12.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/vndixp
title: 83- High 12.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/6vwds8
title: 85- Heatlhy Control 33.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/a0gwge
title: 86-QC15.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/d8plcq
title: 85- Heatlhy Control 33.cdf

description: :unav
DOI: 10.7910/dvn/6ah3bg/vlpe5t
title: 84- Low 14.gci

description: :unav
DOI: 10.7910/dvn/6ah3bg/dxqjru
title: 0- Samples Metadata.xls

description: :unav
DOI: 10.7910/dvn/6ah3bg/nex3jb
title: 1-QC1.xls

description: :unav
DOI: 10.35003/67pvdv/h8c7q1
title: Figure7.pptx

description: REE concentrations normalized to CI chondrites (Barrat et al., 2012) for the three impact melt lithologies (IM-1 to IM-3) from Dhofar 1769, in comparison with selected Apollo samples (Haskin et al., 1971, 1973, 1981; Warren & Wasson, 1978). IM-1 has a well-developed positive Eu anomaly related to low abundances of trivalent REE and a high anorthositic contribution, whereas the composition of IM-3 is similar to that of the KREEP basalt Apollo 15386 (Warren & Wasson, 1978). IM-2 has a relatively flat REE pattern. (Color figure can be viewed at wileyonlinelibrary.com) [Colour figure can be viewed at wileyonlinelibrary.com]
DOI: 10.35003/67pvdv/tnuedl
title: Figure6.pptx

description: Ni/Co ratios of metal grains in the complex impact melt lithology of Dhofar 1769: 26 grains from IM-3 (green) and one grain from IM-2 (red). The metal grains in IM-1 were too small for quantitative analysis without contamination by surrounding phases. The black line corresponds to the chondritic trend. Compositional range of Ni/Co for chondritic metal (orange) and iron meteorites (gray) after Day (2020). Except for one grain (arrow), all analyzed metal grains from the impact melt lithologies are different from those typically characterizing a chondritic or iron meteorite origin. (Color figure can be viewed at wileyonlinelibrary.com) [Colour figure can be viewed at wileyonlinelibrary.com]
DOI: 10.35003/67pvdv/vceo6t
title: Figure5.pptx

description: The compositions of olivine within the three impact melt lithologies (IM-1 to IM-3; Komnik, 2021). Olivine within IM-1 is very homogeneous in composition, whereas somewhat variable olivine compositions were found in IM-2 and IM-3. Fa, fayalite. (Color figure can be viewed at wileyonlinelibrary.com) [Colour figure can be viewed at wileyonlinelibrary.com]
DOI: 10.35003/67pvdv/8nj1mp
title: 199 tables.tab

description: :unav
DOI: 10.35003/67pvdv
title: Replication Data for: Anorthositic lunar regolith breccia Dhofar 1769—Clear indications for repeated mixing of impact melt lithologies

description: Abstract The lunar regolith breccia Dhofar 1769, which was found in 2012 as a single 125 g piece in the Zufar desert area of Oman, contains a relatively large, dark-colored impact melt breccia embedded in a fine-grained clastic matrix. The internal texture of the fragment indicates the repeated melt breccia formation on the lunar surface, their repeated brecciation, and mixing in second, third, and fourth generations of brecciated rock types. The chemical and mineralogical data reveal the incorporation of a feldspar-rich subophitic crystalline melt within a feldspar-rich microporphyritic crystalline melt breccia. This lithic paragenesis itself is embedded within a mafic, crystalline melt breccia. The entire breccia with the three different impact melts has been finally incorporated into the whole rock breccia. The three impact melts are mixtures of different source rocks and impact projectiles, based on the obtained minor and trace element compositions (in particular of Ni and the rare earth elements [REE]) of the impact melt lithologies. For all processes of impact melt formation, additional steps of their brecciation and re-lithification require a minimum number of seven impact processes.
DOI: 10.5281/zenodo.10046885
title: Lung250M-4B: A Combined 3D Dataset for CT- and Point Cloud-Based Intra-Patient Lung Registration
title: Lung250M: Pulmonary Vessel Point Clouds for Intra-Patient Lung Registration

description: Point Cloud Data from the Lung250M-4B dataset.
Visit https://github.com/multimodallearning/Lung250M-4B for image data and associated code.
DOI: 10.5281/zenodo.10046884
title: Lung250M-4B: A Combined 3D Dataset for CT- and Point Cloud-Based Intra-Patient Lung Registration
title: Lung250M: Pulmonary Vessel Point Clouds for Intra-Patient Lung Registration

description: Point Cloud Data from the Lung250M-4B dataset.
Visit https://github.com/multimodallearning/Lung250M-4B for image data and associated code.
DOI: 10.5281/zenodo.10046972
title: Drive with Your Brain: Personalized Prediction of Driving Behaviors with DR-EEG Decoding and Situational Embeddings

description: These are the relevant codes for 'Drive with Your Brain: Personalized Prediction of Driving Behaviors with DR-EEG Decoding and Situational Embedding'. It consists of five parts, each containing a 'ReadMe.txt' instruction file. Please read the instructions before using it. It is worth noting to remember to change the file path in the code.
DOI: 10.5281/zenodo.10046971
title: Drive with Your Brain: Personalized Prediction of Driving Behaviors with DR-EEG Decoding and Situational Embeddings

description: These are the relevant codes for 'Drive with Your Brain: Personalized Prediction of Driving Behaviors with DR-EEG Decoding and Situational Embedding'. It consists of five parts, each containing a 'ReadMe.txt' instruction file. Please read the instructions before using it. It is worth noting to remember to change the file path in the code.
DOI: 10.5258/soton/d2794
title: Dataset supporting the University of Southampton Doctoral Thesis "The tumour microenvironment in Oesophageal Adenocarcinoma"

description: Dataset supporting the University of Southampton Doctoral Thesis "The Tumour Microenvironment in Oesophageal Adenocarcinoma". The data includes R markdown file and contains single cell RNA Sequencing data from 23 oesophageal cancer patients tumours and matched normal samples. All samples taken processed and analysed at Southampton General Hospital Licence: Creative Commons Attribution CC-BY Related projects/Funders: Study name: Upper GI Tumour Ecology: IRAS 233065, ERGO 45334. Funded by CRUK, R Walker in receipt of CRUK clinical research training fellowship. Prof T Underwood in recipe of CRUK advanced clinician scientist fellowship.
DOI: 10.6084/m9.figshare.24449197
title: Hand Gestures Dataset

description: Hand Gestures Dataset for Sign Language Recognition (SLR) composed of six hand gesturesbased on American Sign Language (ASL). The dataset is divided into 6 categories which are "Hello", "Bye", "Yes", "No", "Perfect" and "Thank You". Each category is composed of 400 images where each image is preprocessed using the hand tracking module developed by https://www.computervision.zone/projects and saved with the hand skeleton landmarks on each image.
DOI: 10.25824/redu/q9dk1w
title: sdm_channel.py

description: :unav
DOI: 10.25824/redu/3hcdzg
title: capacities_2.npy

description: :unav
DOI: 10.25824/redu/tld381
title: capacities_pdf.pdf

description: :unav
DOI: 10.25824/redu/ehtlgw
title: A Python implementation of the multisection model for simulation of MDG-impaired SDM channels

description: A Python Implementation of the Multisection Model for Simulation of MDG-impaired SDM Channels. This code can be used to simulate de transfer matrix of MDG-impaired SDM Channels and compute important channel parameters, such as channel capacity and modal gains.
DOI: 10.6084/m9.figshare.24115998.v1
title: A trait dataset for freshwater mussels of the United States of America

description: This file contains the raw data with all<i> traitValues</i> and is considered the final dataset.
DOI: 10.34740/kaggle/dsv/6809506
title: Global Genomic Neurofibromatosis Neoplasia
DOI: 10.34740/kaggle/dsv/6809516
title: UNET Lung Segmentation Weights for Chest X Rays
DOI: 10.35003/lzm8au/sk4bh2
title: 194 tables.tab

description: :unav
DOI: 10.35003/lzm8au/xg6cvx
title: Fig 7.jpg

description: Fig. 7. We observed sets of (a) graben (indicated by black arrows), and (b) wrinkle ridges (indicated by white arrows) with LOLA/Kaguya merged DTM data. See reference map in Appendix A1 for panel locations.
DOI: 10.35003/lzm8au/ohhntg
title: Fig 4.jpg

description: Fig. 4. The highland units around the Apollo 14 landing site include: (a) ancient INt unit, (a,b,c) Fra Mauro Formation (Ifm), (a,b) Imbrian plains (Ip), (b) cryptomare (Imc), and (c) Fra Mauro smooth unit (Ifs). The locations of the panels are shown on the reference map in appendix A1.
DOI: 10.35003/lzm8au/vpw4js
title: Fig A3.jpg

description: Fig. A3. Apollo 14 map plate. See also https://zenodo.org/record/8124259
DOI: 10.35003/lzm8au/lohjvj
title: Fig A4.jpg

description: Fig. A4. Shows the area selected for the CSFD measurements on: (a) LRO WAC data, (b) slope map derived from LOLA/Selene DTM, (c) Kaguya image, (d) slope map derived from LOLA/Selene DTM, (e) LRO NAC data, and (e) slope map derived from NAC DTM.
DOI: 10.35003/lzm8au/nubl60
title: Fig A1.jpg

description: Fig. A1. Reference map showing the extent of Fig. 4, Fig. 5, Fig. 6, Fig. 7 with white boxes.
DOI: 10.35003/lzm8au/pimpzc
title: Fig 5.jpg

description: Fig. 5. (a) Imbrian aged dark mantling deposit (Idmm) has low albedo in the Kaguya image (TCO_MAPe04_S06E342S09E345SC), and the pyroclastic vents (Id) are prominent in (b) Kaguya DTM data (DTM_MAPs02_S06E342S09E345SC). The locations of the panels are shown on the reference map in appendix A1.
DOI: 10.35003/lzm8au/zfacmg
title: Fig 1.jpg

description: Fig. 1. The orbital data sets used in this study include: (a) LRO WAC mosaic (100 m/pixel), (b) LOLA/Kaguya merged DTM (60 m/pixel), (c) Kaguya TC mosaic (∼7 m/pixel), (d) Kaguya TC DTM (∼8 m/pixel), (e) LRO NAC image data (∼1 m/pixel), and (f) LRO NAC DTM (2 m/pixel). The black squares in panels (a), (b), (c), and (d) indicate the extent of panels (e) and (f). In panels (e) and (f) the astronaut traverses are marked with a white dotted line, and position of the lunar module (LM) is marked with a plus sign.
DOI: 10.35003/lzm8au/8lcszp
title: Fig A2.jpg

description: Fig. A2. Showing the temporal evolution of the geological units (as mapped in Fig. 3) including (a) ancient highland units, i.e., undivided Imbrian-Nectarian terrains (INt) and Nectarian aged craters (Nc); (b) cyptomare unit (Imc); (c) Imbrian aged: Fra Mauro formation, (d) Imbrian plains (Ip), (e) Fra Mauro smooth plain, and (f) Imbrian mare units and dark mantle deposits.
DOI: 10.35003/lzm8au/6fa8ow
title: Fig 6.jpg

description: Fig. 6. The classes of craters mapped in the study area include: (a) Nectarian craters (Nc) such as Parry crater, (b) Imbrian craters (Ic) such as Gambart crater, (c) Eratosthenian craters (Ec), and (d) Copernican craters (Cc). Panel (b) shows the Imbrian aged Gambart crater surrounded by dark mantle deposits (Idmm), and panel (d) shows the characteristic crater ray material (Ccr) of Copernican craters. See reference map in Appendix A1 for panel locations.
DOI: 10.35003/lzm8au/icivfg
title: Fig 2.jpg

description: Fig. 2. We used (a) M3 spectral data, where lower mafic contents appear in blue hues (plagioclase-dominated) and high mafic contents appear in yellow/green to orange/red hues (olivine-dominated) (140 m/pixel) and (b) Kaguya MI plagioclase abundance, and (c)Kaguya MI FeO abundance around the Apollo 14 landing site, both 60 m/pixel. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.)
DOI: 10.35003/lzm8au/0plnls
title: Fig 8.jpg

description: Fig. 8. (a) Areas selected for CSFD measurements: Neukum (1983, blue, WAC), LRO NAC area (green), Kaguya area (black), and modified WAC area (red, WAC). (b) The CSFDs can be fit with the same N(1) within error bars. The individual fits for the N(1) values for the new measurements are (c) LRO NAC count, (d) Kaguya TC count, and (e) LRO WAC count, which are shown in cumulative and R-plot. Fig. A4 shows individual areas. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.)
DOI: 10.35003/lzm8au/6rgrww
title: Fig 9.jpg

description: Fig. 9. The lunar chronology function (Neukum, 1983; Eq. (1)) with a few of the original Neukum (1983) Apollo-related anchor points shown in grey. Our updated calibration point (red) is compared with points obtained by other studies (Neukum, 1983; Hiesinger et al., 2012; Marchi et al., 2009; Robbins, 2014; Werner et al., 2022). In the inset, our points for the Apollo 14 landing site are highlighted as: red for Ap14_WAC, black for Ap14_Kaguya and light green for Ap14_NAC. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.)
DOI: 10.35003/lzm8au/gho0ek
title: Fig 3.jpg

description: Fig. 3. New geologic map of the Apollo 14 landing site area. The map shows various geologic units in the region, including the Fra Mauro and Cayley Formations, some highland and mare units, wrinkle ridges, rilles, various generations of craters, and ray material. A LOLA/SELENE DEM-derived hill-shade product is used as the base map. (Fig. A2 shows the temporal evolution of highland units around the Apollo 14 landing site. and Fig. A3 in the appendix provides a complete map plate). The map data is archived at https://doi.org/10.5281/zenodo.8124259.
DOI: 10.35003/lzm8au
title: Replication Data for: Geological mapping and chronology of lunar landing sites: Apollo 14

description: • We produced detailed geological map for the Apollo 14 landing site on Fra Mauro formation which is Imbrian basin ejecta. • The N(1) values of the Fra Mauro formation were compared with recently determined radiometric sample ages. • The newly obtained calibration points are consistent with the lunar cratering chronology of Neukum (1983).
DOI: 10.5281/zenodo.10047149
title: A JWST inventory of protoplanetary disk ices. The edge-on protoplanetary disk HH 48 NE, seen with the Ice Age ERS program

description: JWST NIRSpec G395H spectrum for HH 48 NE edge-on disk, as analyzed in Sturm et al. (2023). DOI: 10.1051/0004-6361/202347512