cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.48577/jpl.7yi4mr
title: Astrobiology Exploration at Enceladus (AXE): A New Frontiers Mission Concept Study

description: The Saturnian moon Enceladus presents a unique opportunity to sample the contents of a subsurface liquid water ocean in situ via the continuous plume formed over its south polar terrain using a multi-flyby mission architecture. Previous analyses of the plume’s composition by Cassini revealed an energy-rich system laden with salts and organic compounds, representing an environment containing most of the ingredients for life as we know it. Following in the footsteps of the Cassini-Huygens mission, we present Astrobiology eXploration at Enceladus (AXE), a New Frontiers class Enceladus mission concept study carried out during the 2021 NASA Planetary Science Summer School program at the Jet Propulsion Laboratory, California Institute of Technology. We demonstrate that a scientifically compelling geophysical and life detection mission to Enceladus can be carried out within the constraints of a New Frontiers-5 class coast cap using a modest instrument suite, requiring only a narrow angle, high resolution telescopic imager, a mass spectrometer, and a high-gain antenna for radio communications and gravity science measurements. Using a multi-flyby mission architecture, AXE would evaluate the habitability and potential for life at Enceladus through a synergistic combination of in situ chemical analysis measurements aimed at directly detecting the presence of molecular biosignatures, along with geophysical and geomorphological investigations to contextualize chemical biosignatures and further evaluate the habitability of Enceladus over geologic time.
DOI: 10.48577/jpl.optwo2
title: Faint but not forgotten. I. First results from a search for astrospheres around agb stars in the far-ultraviolet

description: Using the GALEX archive, we have discovered extended structures around 10 AGB stars (out of a total 92 searched) emitting in the far-ultraviolet (FUV) band. In all but one, we find the typical morphology expected for a spherical wind moving relative to, and interacting with the ISM to produce an astrosphere. The exception is V\,Hya whose mass-ejection is known to be highly aspherical, where we find evidence of its large parabolic outflows interacting with the ISM, and its collimated, extreme velocity outflows interacting with the circumstellar medium. For 8 objects with relatively large proper motions, we find (as expected) that the termination-shock region lies in a hemisphere that contains the proper motion vector. Radial intensity cuts for each source have been used to locate the termination shock and the astropause's outer edge. In a few objects, the cuts also reveal faint emission just outside the astropause that likely arises in shocked ISM material. We have used these data, together with published mass-loss rates and wind expansion velocities, to determine the total mass lost and duration for each source -- we find that the duration of and total mass in the shocked wind are significantly larger than their corresponding values for the unshocked wind. The combination of FUV and far-IR data on AGB astrospheres, provides a unique database for theoretical studies (numerical simulations) of wind-ISM interactions. We show that a Cyclical Spatial Heterodyne Spectrometer on a small space-based telescope, can provide high-resolution spectra of astrospheres to confirm the emission mechanism.
DOI: 10.48577/jpl.tduldr
title: Dual-band Fourier-transform millimeter wave spectrometry for in-situ gas sensing

description: The exploration of icy body composition in the solar system has often involved spectroscopic measurements of volatiles detected with remote sensing, such measurements portray materials naturally expelled from the surface that enter the exosphere and potentially escape into space. Variations in the ratio of deuterium and hydrogen (DHR) in these measurements have led to inconclusive hypotheses regarding potential cometary origins of Earth's ocean water and/or organics. Observational biases regarding unknown previous processing of the observable ejected materials necessitates studies of more dormant, less-processed bodies. Landed missions on comets have brought focus onto the development of small, sensitive instrumentation capable of similar composition measurements of the nascent surface and near-surface materials. We present an evolution of our compact Fourier Transform millimeter-wave (FTmmw) cavity spectrometer that is tuned for sensitivity at 80.6 and 183 GHz where HDO and H$_2$O exhibit resonance features. We discuss both a low SWaP (size-weight and power) architecture that uses custom micro-chip transceiver elements as well as a modular configuration using traditional GaAs based millimeter wave hardware. New design features for these systems including quartz based coupling elements, system thermal management, and a separable clocking board are discussed in addition to sensitivity studies and applications in potential mission scenarios.
DOI: 10.48577/jpl.ffelrf
title: Narrow loophole for H2-dominated atmospheres on habitable rocky planets around M dwarfs

description: Habitable rocky planets around M dwarfs that have \ce{H2}-dominated atmospheres, if they exist, would permit characterizing habitable exoplanets with detailed spectroscopy using JWST, owing to their extended atmospheres and small stars. However, the \ce{H2}-dominated atmospheres that are consistent with habitable conditions cannot be too massive, and a moderate-size \ce{H2}-dominated atmosphere will lose mass to irradiation-driven atmospheric escape on rocky planets around M dwarfs. We evaluate volcanic outgassing and serpentinization as two potential ways to supply \ce{H2} and form a steady-state \ce{H2}-dominated atmosphere. For rocky planets of $1-7\ M_{\oplus}$ and early, mid, and late M dwarfs, the expected volcanic outgassing rates from a reduced mantle fall short of the escape rates by $&gt;\sim1$ order of magnitude, and a generous upper limit of the serpentinization rate is still less than the escape rate by a factor of a few. Special mechanisms that may sustain the steady-state \ce{H2}-dominated atmosphere include direct interaction between liquid water and mantle, heat-pipe volcanism from a reduced mantle, and hydrodynamic escape slowed down by efficient upper-atmospheric cooling. It is thus unlikely to find moderate-size, \ce{H2}-dominated atmospheres on rocky planets of M dwarfs that would support habitable environments.
DOI: 10.48577/jpl.qss2iy
title: The GeoSTAR Geostationary Microwave Sounder

description: A geostationary microwave sounder, capable of providing continuous all-weather monitoring of temperature, water vapor, clouds, precipitation, and wind, would add tremendously to our ability to observe and predict dynamic atmospheric phenomena, such as hurricanes and severe storms, monsoonal moisture flow, atmospheric rivers, etc. Such a sensor is now feasible, enabled by technology that has been developed at the Jet Propulsion Laboratory (JPL). The Geostationary Synthetic Thinned Aperture Radiometer (GeoSTAR), is essentially an “AMSU in GEO”, providing similar measurements as are now obtained with AMSU (and ATMS) but every 5-15 minutes instead of every 12 hours and covering an entire hemisphere instead of a narrow swath. GEO orbits are almost 50 times higher than the LEO orbits that current microwave sounders operate from, and the corresponding scaling of aperture size required to maintain spatial resolution had stymied the development of such a sensor for many decades. The aperture synthesis approach implemented with GeoSTAR finally overcomes that obstacle, made possible with new technology that has been developed at JPL.
DOI: 10.48577/jpl.inbmjs
title: Powering Mars Exploration

description: No abstract available.
DOI: 10.48577/jpl.wdkpxr
title: Mars Relay Operations Service (MaROS) Capabilities with regard to Lunar Relay

description: No abstract available.
DOI: 10.48577/jpl.g5rjpn
title: F Prime Flight Software Product Line Overview

description: No abstract available.
DOI: 10.48577/jpl.pyotaz
title: An Introduction to NASA’s Jet Propulsion Laboratory, Plume Effects and Contamination Control

description: No abstract available.
DOI: 10.48577/jpl.jamb31
title: Hardy Tree-Mounted Loop Antenna for the Tree of Life Mission

description: No abstract available.
DOI: 10.48577/jpl.xstowl
title: Early Technology Development and Connections with Science

description: No abstract available.
DOI: 10.48577/jpl.64jxzf
title: Merging multiple observational data streams to constrain carbon uptake and water loss in the Amazon basin

description: No abstract available.
DOI: 10.48577/jpl.ahebtg
title: Planetary Interiors, Planetary Habitability, and Magnetic Fields

description: No abstract available.
DOI: 10.48577/jpl.eafyhl
title: Moon Trek Tools that are relevant to Landing Site Selection and Path Planning

description: No abstract available.
DOI: 10.48577/jpl.uqzfiv
title: Making Planetary Science More Inclusive: Accomplishments and Recommendations from the DPS Professional Culture and Climate Subcommittee (PCCS)

description: No abstract available.
DOI: 10.48577/jpl.yyui9b
title: International Mars Ice Mapper Update to MEPAG May 2022

description: No abstract available.
DOI: 10.48577/jpl.jkrrxw
title: Apophis Trajectory, Impact Hazard, and Sensitivity to Spacecraft Contact

description: No abstract available.
DOI: 10.48577/jpl.qr3sgg
title: Distributed Observation Allocation for a Large-Scale Constellation

description: No abstract available.
DOI: 10.48577/jpl.jnddip
title: Delta-X UAVSAR product exploration

description: No abstract available.
DOI: 10.48577/jpl.ycycqs
title: MSL MMRTG Power Modeling for Lifetime Performance Predictions

description: No abstract available.
DOI: 10.5281/zenodo.7884419
title: [IO Islamic 104] مفتاح گلستان

description: <strong>Miftâḥ-i-Gulistân</strong><strong>.</strong> <strong>This manuscript is now IO Islamic 1176 in the India Office collections.</strong> <strong>[metadata:</strong> <strong>Hermann Ethé</strong><strong><em>, </em></strong><strong><em>Catalogue of Persian Manuscripts in the Library of the India Office,</em></strong> <strong>2 vols. (Oxford: India Office, 1903): volume 1,</strong> <strong>number 104 here with notations and hyperlinks].</strong> 1176 Miftâḥ-i-Gulistân (مفتاح گلستان). Short commentary on and glossary to Sa’dî’s Gulistân, composed by Uwais bin ‘Alâ-aldîn, known as Âdam, a pupil of Khwâjah Abû-alfaiḍ Abû-alfaḍl Amîr-aldîn Shâh Ni’mat-allâh Muḥammad bin Muḥammad al-Ḥasanî, and dedicated to the Bahmanî Sulṭân of the Dakhan, Maḥmûdshâh bin Muḥammadshâh (who reigned A.H. 887-924=A.D. 1482-1518, see above , No. 449). According to the last words in No. 3338 (1179 in this Cat.), the work was completed by the author on the day عاشور, i.e. the 10th of Muḥarram, A.H. 900 (A.D.1494, Oct. 11). It is divided into two ḳisms, the <em>first</em> <em>ḳism</em> being a glossary, <em>arranged</em> alphabetically, of the difficult words (قسم اوّل مبوّب از حروف مقطّعات در بيان لغات), the last letter constituting the bâb, the first the faṣl or subdivision; the <em>second</em> <em>ḳism</em> containing an explanation of difficult phrases, verses of the Ḳurân, traditions and sayings of Shaikhs, Arabic baits and invocations of God, etc., which occur in the Gulistân (قسم دوم در تفسير و معانئ آيات و كلام قدسى و احاديث و اقوال و اُدعيّات و اشعار تازى كه در كتاب گلستان مذكور است.) Beginning:فاتحه مر فتّاحى را كه افتتاح كلام خود بفاتحة الكتاب مخصوص گردانيد الخ . <em>First</em> <em>ḳism, </em>on fol. 6<sup>b</sup>; second <em>ḳism, </em>on fol. 57<sup>b</sup>. The copy ends on fol. 69<sup>b</sup>, and is dated the 6th of Sha’bân, A.H. 1052 (A.D. 1642, Oct. 30). On ff. 71<sup>b</sup>-75<sup>a</sup> there are written by another hand some fragments of theological tracts in Arabic, on Muḥammad, the Ḳurân, etc. No. 104, ff. 75, ll. 13; Naskhî; size, 7<sup>1/2</sup> in. by 4<sup>1/4</sup> in.
DOI: 10.5281/zenodo.7884418
title: [IO Islamic 104] مفتاح گلستان

description: <strong>Miftâḥ-i-Gulistân</strong><strong>.</strong> <strong>This manuscript is now IO Islamic 1176 in the India Office collections.</strong> <strong>[metadata:</strong> <strong>Hermann Ethé</strong><strong><em>, </em></strong><strong><em>Catalogue of Persian Manuscripts in the Library of the India Office,</em></strong> <strong>2 vols. (Oxford: India Office, 1903): volume 1,</strong> <strong>number 104 here with notations and hyperlinks].</strong> 1176 Miftâḥ-i-Gulistân (مفتاح گلستان). Short commentary on and glossary to Sa’dî’s Gulistân, composed by Uwais bin ‘Alâ-aldîn, known as Âdam, a pupil of Khwâjah Abû-alfaiḍ Abû-alfaḍl Amîr-aldîn Shâh Ni’mat-allâh Muḥammad bin Muḥammad al-Ḥasanî, and dedicated to the Bahmanî Sulṭân of the Dakhan, Maḥmûdshâh bin Muḥammadshâh (who reigned A.H. 887-924=A.D. 1482-1518, see above , No. 449). According to the last words in No. 3338 (1179 in this Cat.), the work was completed by the author on the day عاشور, i.e. the 10th of Muḥarram, A.H. 900 (A.D.1494, Oct. 11). It is divided into two ḳisms, the <em>first</em> <em>ḳism</em> being a glossary, <em>arranged</em> alphabetically, of the difficult words (قسم اوّل مبوّب از حروف مقطّعات در بيان لغات), the last letter constituting the bâb, the first the faṣl or subdivision; the <em>second</em> <em>ḳism</em> containing an explanation of difficult phrases, verses of the Ḳurân, traditions and sayings of Shaikhs, Arabic baits and invocations of God, etc., which occur in the Gulistân (قسم دوم در تفسير و معانئ آيات و كلام قدسى و احاديث و اقوال و اُدعيّات و اشعار تازى كه در كتاب گلستان مذكور است.) Beginning:فاتحه مر فتّاحى را كه افتتاح كلام خود بفاتحة الكتاب مخصوص گردانيد الخ . <em>First</em> <em>ḳism, </em>on fol. 6<sup>b</sup>; second <em>ḳism, </em>on fol. 57<sup>b</sup>. The copy ends on fol. 69<sup>b</sup>, and is dated the 6th of Sha’bân, A.H. 1052 (A.D. 1642, Oct. 30). On ff. 71<sup>b</sup>-75<sup>a</sup> there are written by another hand some fragments of theological tracts in Arabic, on Muḥammad, the Ḳurân, etc. No. 104, ff. 75, ll. 13; Naskhî; size, 7<sup>1/2</sup> in. by 4<sup>1/4</sup> in.
DOI: 10.5281/zenodo.3902068
title: Dataset test ULM

description: Data set test
DOI: 10.5281/zenodo.3902067
title: Dataset test ULM

description: Data set test
DOI: 10.5281/zenodo.7884356
title: Electron Diffraction (MicroED) Datasets for Aspirin (Glacios TEM with a CETA-D)

description: Electron diffraction datasets collected from aspirin. Microscope: Thermo Fisher Scientific Glacios Transmission Electron Microscope (SDC1G at NanoImaging Services) Camera: Ceta-D camera (bin 2x2, rolling shutter, noise reduction mode) Collection Software: Leginon (Cheng, et. al. 2021)* Collection Parameters: 200keV, -193C, 20um C2, gun lens 7.1, spot size 10, parallel beam, calibrated camera length 1065.7mm (1100 in UI), oscillation per frame 0.89deg, 222ms exposure time, tilt speed 4 deg/s, rotation -60 to +60 (first ~8 degrees not recorded) Grid: Ted Pella 01840 Sample: C<sub>9</sub>H<sub>8</sub>O<sub>4</sub>, 2-acetoxybenzoic acid, 180.16 g/mol Structure: CCDC 2260060 * Data have been converted to SMV format with the addition of an offset value to remove negative pixel values. This offset value can be found in the image headers, along with a suggested pedestal value. A data processing tutorial is available for processing data collected with this setup using DIALS: https://dials.github.io/documentation/tutorials/3DED/Biotin.html
DOI: 10.5281/zenodo.7884355
title: Electron Diffraction (MicroED) Datasets for Aspirin (Glacios TEM with a CETA-D)

description: Electron diffraction datasets collected from aspirin. Microscope: Thermo Fisher Scientific Glacios Transmission Electron Microscope (SDC1G at NanoImaging Services) Camera: Ceta-D camera (bin 2x2, rolling shutter, noise reduction mode) Collection Software: Leginon (Cheng, et. al. 2021)* Collection Parameters: 200keV, -193C, 20um C2, gun lens 7.1, spot size 10, parallel beam, calibrated camera length 1065.7mm (1100 in UI), oscillation per frame 0.89deg, 222ms exposure time, tilt speed 4 deg/s, rotation -60 to +60 (first ~8 degrees not recorded) Grid: Ted Pella 01840 Sample: C<sub>9</sub>H<sub>8</sub>O<sub>4</sub>, 2-acetoxybenzoic acid, 180.16 g/mol Structure: CCDC 2260060 * Data have been converted to SMV format with the addition of an offset value to remove negative pixel values. This offset value can be found in the image headers, along with a suggested pedestal value. A data processing tutorial is available for processing data collected with this setup using DIALS: https://dials.github.io/documentation/tutorials/3DED/Biotin.html
DOI: 10.5281/zenodo.7884454
title: Data files for "Comprehensive Wastewater Sequencing Reveals Community and Variant Dynamics of the Collective Human Virome"

description: Files required to run analyses and generate charts for R notebooks at: https://github.com/cmmr/TX_wastewater_virome
DOI: 10.5281/zenodo.7884453
title: Data files for "Comprehensive Wastewater Sequencing Reveals Community and Variant Dynamics of the Collective Human Virome"

description: Files required to run analyses and generate charts for R notebooks at: https://github.com/cmmr/TX_wastewater_virome
DOI: 10.6084/m9.figshare.22728728
title: Survey responses.xlsx

description: The sheet contains cleaned up data (135 responses) from a survey conducted to explore micro-inequities in the software industry.
DOI: 10.5281/zenodo.7884456
title: CUBirds and CifarFS datasets

description: download links for cubirds and cifarfs datasets pickle files
DOI: 10.5281/zenodo.7884455
title: CUBirds and CifarFS datasets

description: download links for cubirds and cifarfs datasets pickle files
DOI: 10.5281/zenodo.7884434
title: Electron Diffraction (MicroED) Datasets for C20H13O4P (Glacios TEM with a CETA-D)

description: Electron diffraction datasets collected from a chiral pharmaceutical compound. Microscope: Thermo Fisher Scientific Glacios Transmission Electron Microscope (SDC1G at NanoImaging Services) Camera: Ceta-D camera (bin 2x2, rolling shutter, noise reduction mode) Collection Software: Leginon (Cheng, et. al. 2021)* Collection Parameters: 200keV, -193C, 20um C2, gun lens 7.1, spot size 10, parallel beam, calibrated camera length 1065.7mm (1100 in UI), oscillation per frame 0.89deg, 222ms exposure time, tilt speed 4 deg/s, rotation -60 to +60 (first ~8 degrees not recorded) Grid: Ted Pella 01840 Sample: C<sub>20</sub>H<sub>13</sub>O<sub>4</sub>P, (R)-(-)-1,1-Binaphthyl-2,2’-diyl hydrogenphosphate, 348.29 g/mol Structure: CCDC 2260063 * Data have been converted to SMV format with the addition of an offset value to remove negative pixel values. This offset value can be found in the image headers, along with a suggested pedestal value. A data processing tutorial is available for processing data collected with this setup using DIALS: https://dials.github.io/documentation/tutorials/3DED/Biotin.html
DOI: 10.5281/zenodo.7884433
title: Electron Diffraction (MicroED) Datasets for C20H13O4P (Glacios TEM with a CETA-D)

description: Electron diffraction datasets collected from a chiral pharmaceutical compound. Microscope: Thermo Fisher Scientific Glacios Transmission Electron Microscope (SDC1G at NanoImaging Services) Camera: Ceta-D camera (bin 2x2, rolling shutter, noise reduction mode) Collection Software: Leginon (Cheng, et. al. 2021)* Collection Parameters: 200keV, -193C, 20um C2, gun lens 7.1, spot size 10, parallel beam, calibrated camera length 1065.7mm (1100 in UI), oscillation per frame 0.89deg, 222ms exposure time, tilt speed 4 deg/s, rotation -60 to +60 (first ~8 degrees not recorded) Grid: Ted Pella 01840 Sample: C<sub>20</sub>H<sub>13</sub>O<sub>4</sub>P, (R)-(-)-1,1-Binaphthyl-2,2’-diyl hydrogenphosphate, 348.29 g/mol Structure: CCDC 2260063 * Data have been converted to SMV format with the addition of an offset value to remove negative pixel values. This offset value can be found in the image headers, along with a suggested pedestal value. A data processing tutorial is available for processing data collected with this setup using DIALS: https://dials.github.io/documentation/tutorials/3DED/Biotin.html
DOI: 10.6084/m9.figshare.3761562.v2573
title: Online Labour Index: Measuring the Online Gig Economy for Policy and Research

description: Data repository for the data underlying the Online Labour Index. See http://ilabour.oii.ox.ac.uk online-labour-index/ for details.
DOI: 10.5281/zenodo.7884437
title: Spanish 3B words Word2Vec Embeddings [Update for gensim&gt;4]

description: This is the KeyedVectors of the gensim model created by Aitor Almeida and Aritz Bilbao, but compatible with Gensim&gt;4 versions. The training and generation of these vectors are detailed in the GitHub repository and in the official Zenodo. Please, any kind of citation or mention should be made to its original repository since I am not the research scientist who originally generate this model and all the merit is theirs. To load this new version you should use: <em>word_vectors = KeyedVectors.load_word2vec_format("complete.bin",binary=True)</em>
DOI: 10.5281/zenodo.7884436
title: Spanish 3B words Word2Vec Embeddings [Update for gensim&gt;4]

description: This is the KeyedVectors of the gensim model created by Aitor Almeida and Aritz Bilbao, but compatible with Gensim&gt;4 versions. The training and generation of these vectors are detailed in the GitHub repository and in the official Zenodo. Please, any kind of citation or mention should be made to its original repository since I am not the research scientist who originally generate this model and all the merit is theirs. To load this new version you should use: <em>word_vectors = KeyedVectors.load_word2vec_format("complete.bin",binary=True)</em>
DOI: 10.6084/m9.figshare.22714822
title: ExtData_Figure_4_qPCR

description: <em>(E) HEK293T ishXrn1cells were treated with doxycycline for 3-4 days to induce knock down of Xrn1, then transfected with luciferase reporters containing 99 bp insertions from the BCAP31 or TUBA1B, with or without PR8 PA-X. </em> <em>RNA was extracted and luciferase mRNA levels were quantified by qRT-PCR and normalized to 18S. </em> <em>R# --&gt; replicate number; LG### --&gt; experiment number.</em> <br>
DOI: 10.6084/m9.figshare.22714828
title: ExtData_Figure_5_images_for_paper

description: <em>(A) HEK293T ishXrn1cells were treated with doxycycline for 3-4 days to induce knock down of Xrn1, then transfected with luciferase reporters containing insertions of the indicated lengths from the BCAP31 and SLC7A5 genes, with or without PR8 PA-X. RNA was extracted and used to run 5’ RACE. (B) HEK293T ishXrn1cells were treated with doxycycline for 3-4 days to induce knock down of Xrn1, then transfected with luciferase reporters containing 15 bp insertions from the </em>STOML2<em> gene with or without mutations to disrupt/restore the hairpin structure. 24 hours post transfection, cells were infected with WT PR8 or PR8-PA(∆X), or mock infected overnight. RNA was then extracted and used to run 5’ RACE. For all gels, the DNA bands were purified and sequenced to confirm their identities, and images are representative of 3 experiments (B) or 2 experiments (A). </em> <em>Additional replicates can be found in ExtData_Figure_5_replicates dataset.</em> <em>R# --&gt; replicate number; LG### --&gt; experiment number.</em> <em>.sgd files are the original source files acquired with the Syngene Imager. </em>