cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25574/csc2.obs.26150
title: Chandra X-ray Observatory ObsId 26150

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.11684
title: Chandra X-ray Observatory ObsId 11684

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.21461
title: Chandra X-ray Observatory ObsId 21461

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.16050
title: Chandra X-ray Observatory ObsId 16050

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.23394
title: Chandra X-ray Observatory ObsId 23394

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.13487
title: Chandra X-ray Observatory ObsId 13487

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.ve5knc
title: Spherical Bessel Harmonic Gravity Expansions and Their Properties Related to Sir Isaac Newton's Shell Theorem via the Riemann Zeta Function

description: The conventional spherical harmonics used to describe the gravity field surrounding a non-spherical mass only converge exterior to the body’s Brillouin (circumscribing) sphere. The complementary gravity field interior to this sphere is provided by spherical Bessel harmonics. We present an algorithm for calculating the Bessel harmonic coefficients directly from the surface integral of an arbitrary shape with homogenous density. Exploring the special case of a homogenous sphere, we show that the Bessel harmonic expansion is a generalization of Newton's Shell theorem. In this special case, the non-zero Bessel coefficients are shown to be related to the Riemann zeta function.
DOI: 10.25318/1410046901-fra
title: Caractéristiques de l'emploi selon le groupe autochtone vivant hors réserve, données annuelles

description: Estimations de l'emploi selon le groupe autochtone, la géographie, le genre et le groupe d'âge, données annuelles.
DOI: 10.25574/csc2.obs.15577
title: Chandra X-ray Observatory ObsId 15577

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.uxh1gn
title: Developing Contingency Options for INCUS: Differential Drag for Constellation Maintenance

description: No abstract available.
DOI: 10.25574/csc2.obs.22863
title: Chandra X-ray Observatory ObsId 22863

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.07750
title: Chandra X-ray Observatory ObsId 07750

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.11680
title: Chandra X-ray Observatory ObsId 11680

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.18639
title: Chandra X-ray Observatory ObsId 18639

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.04104
title: Chandra X-ray Observatory ObsId 04104

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.6h4ycy
title: Study of Hydrologic Connectivity and Tidal Influence on Water Flow Within Louisiana Coastal Wetlands Using Rapid-Repeat Interferometric Synthetic Aperture Radar

description: The exchange of water, sediment, and nutrients in wetlands occurs through a complex network of channels and overbank flow. Although optical sensors can map channels at high resolution, they fail to identify narrow intermittent channels colonized by vegetation. We applied interferometry techniques to rapid-repeat (~30 min) Synthetic Aperture Radar (SAR) imagery of the southern Atchafalaya basin in Louisiana acquired during rising-to-high and ebbing-to-low tides to identify and differentiate permanent open water channels from intermittent channels in which flow varies with tidal conditions and to identify locations where overbank flow occurs. Open water surfaces appear as low interferometric coherence pixels, and the coherence in 60-minute and 90-minute in-terferograms can efficiently identify channels, some less than 10m wide. The channel networks at rising and ebbing tide show significant differences in the extent of flow, with vegetation-filled small channels more clearly identified at rising-to-high tide. InSAR phase change is used to iden-tify locations on channel banks where overbank flow occurs at rising and ebbing tides, which is a critical component for modelling wetland hydrodynamics. SAR maps the channel network in our study area better than the optical instruments tested, particularly the small channels that are pri-marily active at higher tides and extend deep into the island interiors. The study shows the capa-bility of rapid repeat InSAR to track how water moves through wetlands during a tidal cycle
DOI: 10.25574/csc2.obs.12868
title: Chandra X-ray Observatory ObsId 12868

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25318/3410028901-eng
title: Inventory of core public infrastructure assets by year of completed construction

description: Year of completed construction for core public infrastructure assets by type of owner for all provinces and territories, by urban and rural municipalities, and by size of municipality. Values are presented in numbers, percentages and kilometres.
DOI: 10.25574/csc2.obs.19560
title: Chandra X-ray Observatory ObsId 19560

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.2908/nama_10_fte
title: Average full time adjusted salary per employee
title: Salaire moyen exprimé en équivalents temps plein
title: Durchschnittlicher vollzeitäquivalenter Bruttolohn
DOI: 10.2908/namq_10_lp_ulc
title: Labour productivity and unit labour costs
title: Productivité du travail et coûts salariaux unitaires
title: Arbeitsproduktivität und Lohnstückkosten
DOI: 10.6084/m9.figshare.27633558
title: 2024 - Eichner and Wu et al - Raw Data

description: This dataset are microscopy images of <i>Streptococcus pneumoniae</i> to verify and measure capsule production. A macro for Fiji is also attached including a protocol on how to perform microscopy and macro usage.It further contains raw data of immunoblots of capsular polysaccharides and a detailed protocol on how to perform the blot.
DOI: 10.25574/csc2.obs.04382
title: Chandra X-ray Observatory ObsId 04382

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.16107
title: Chandra X-ray Observatory ObsId 16107

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.05777
title: Chandra X-ray Observatory ObsId 05777

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.26147
title: Chandra X-ray Observatory ObsId 26147

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.sunc0y
title: Glacial Vermicular Ridge Features on Axel Heiberg Island, Nunavut, Canada

description: Vermicular Ridge Features (VRFs) comprise a series of ridges and troughs with a circular, sinuous, and anastomosing morphology composed of clast-rich sandy diamict. VRFs were first reported on the south coast of Devon Island, Nunavut, Canada, in the Dundas Harbour region. Here, we document the presence of VRFs near Mokka Fjord on Axel Heiberg Island, Nunavut, Canada. We utilize field observations, ultra high resolution LiDAR, and ground penetrating radar to characterize and compare the morphometry and sedimentology of VRFs near Mokka Fjord on the eastern coast of Axel Heiberg Island to other periglacial, paraglacial, and glacial landforms. A leading periglacial (i.e., segregation ice features/lithalsas) and glacial (i.e., ring-ridge moraines and kame/kettled terraces) origin are presented. We interpret Mokka Fjord VRFs to be an ice-marginal feature resulting from paraglacial ablation of buried glacial ice producing a hummocky ring-ridge moraine comprised of supra- and englacial debris. This formation mechanism would infer a largely polythermal glacial environment with limited water supply. Likely from occasional warm-based periods at the ice margins which may allow sediment output and ice burial from basal ice debris redistribution or the thinning and subsequent burial of snout ice from glaciofluvial outwash.
DOI: 10.2908/nama_10_nfa_st
title: Capital stocks by industry (NACE Rev.2) and detailed asset type
title: Stocks de capital par branche d’activité (NACE Rév. 2) et type d’actif détaillé
title: Kapitalbestände nach Wirtschaftsbereichen (NACE Rev. 2) und detaillierte Anlagevermögensart
DOI: 10.25574/csc2.obs.20366
title: Chandra X-ray Observatory ObsId 20366

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.04402
title: Chandra X-ray Observatory ObsId 04402

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.22618
title: Chandra X-ray Observatory ObsId 22618

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.03265
title: Chandra X-ray Observatory ObsId 03265

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.18708
title: Chandra X-ray Observatory ObsId 18708

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.19459
title: Chandra X-ray Observatory ObsId 19459

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.1i2ygb
title: Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c

description: Stellar surface heterogeneities, such as spots and faculae, often contaminate exoplanet transit spectra, hindering precise atmospheric characterization. We demonstrate a novel, epoch-based, modelindependent method to mitigate stellar contamination, applicable to multi-planet systems with at least one airless planet. We apply this method using quasi-simultaneous transits of TRAPPIST-1 b and TRAPPIST-1 c observed on July 9, 2024, with JWST/NIRSpec PRISM. These two planets, with nearly identical radii and impact parameters, are likely either bare rocks or possess thin, low-pressure atmospheres, making them ideal candidates for this technique, as variations in their transit spectra would be primarily attributed to stellar activity. Our observations reveal their transit spectra exhibit consistent features, indicating similar levels of stellar contamination. We use TRAPPIST-1 b to correct the transit spectrum of TRAPPIST-1 c, achieving a 2.5× reduction in stellar contamination at shorter wavelengths. At longer wavelengths, lower SNR prevents clear detection of contamination or full assessment of mitigation. Still, out-of-transit analysis reveals variations across the spectrum, suggesting contamination extends into the longer wavelengths. Based on the success of the correction at shorter wavelengths, we argue that contamination is also reduced at longer wavelengths to a similar extent. This shifts the challenge of detecting atmospheric features to a predominantly white noise issue, which can be addressed by stacking observations. This method enables epoch-specific stellar contamination corrections, allowing co-addition of planetary spectra for reliable searches of secondary atmospheres with signals of 60–250 ppm. Additionally, we identify small-scale cold (∼2000 K) and warm (∼2600 K) regions almost uniformly distributed on TRAPPIST-1, with overall covering fractions varying by ∼0.1% per hour.
DOI: 10.25574/csc2.obs.11557
title: Chandra X-ray Observatory ObsId 11557

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.15468/dl.9gjf4s
title: Occurrence Download

description: A dataset containing 132 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Amanoa nanayensis W.J.Hayden"
 ]
}

 The dataset includes 132 records from 22 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010446-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/csc2.obs.11558
title: Chandra X-ray Observatory ObsId 11558

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.qruost
title: WRR paper - Launching into Societal Benefits from the Surface Water and Ocean Topography (SWOT) Mission

description: The 10th Surface Water and Ocean Topography (SWOT) Applications Meeting, held one year after the satellite's launch, highlighted significant milestones in mission progress and showcased the innovative work of SWOT Early Adopters (EA) using mission data products. Over 100 participants from diverse sectors convened to discuss operational applications leveraging SWOT’s unprecedented water surface measurements. The meeting emphasized applied science efforts to enhance hydrology and oceanographic models. This summary highlights the breadth of operational and private-sector uses of SWOT data, emphasizing its potential to drive new innovations and deliver societal benefits, such as improved water resource management, flood prediction, and climate resilience.
DOI: 10.25574/csc2.obs.20367
title: Chandra X-ray Observatory ObsId 20367

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.04383
title: Chandra X-ray Observatory ObsId 04383

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.06106
title: Chandra X-ray Observatory ObsId 06106

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.09194
title: Chandra X-ray Observatory ObsId 09194

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.19627
title: Chandra X-ray Observatory ObsId 19627

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.elwxvx
title: Upcycling titanium-based bulk metallic glass scrap feedstock through compositional steering

description: Bulk metallic glasses (BMGs) are an emerging commercial material with applications in consumer electronics, fasteners, watches, and precision gears, among other uses. Mass-production of hardware using BMGs requires the production of feedstock material using conventional foundry techniques, normally comprising rods, thin sheets, and powder. Due to the unique amorphous nature and highly designed compositions of BMGs, recycling and upcycling waste products are challenging because the properties of BMGs are highly dependent on their chemical composition and impurity content. In this work, an off-composition, scrap titanium-based BMG feedstock material is upcycled into usable material through the novel use of a correction ingot to steer the composition into either a better glass-forming alloy or an alloy that exhibits improved mechanical performance. In one example, the feedstock, initially with exceptionally poor mechanical properties and low glass-forming-ability, can be compositionally steered into a 3.5-mm thick BMG by mixing it with as little as 25% by mass of a designed alloy.
DOI: 10.15468/dl.a9d7j7
title: Occurrence Download

description: A dataset containing 47832 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Populus tremuloides Michx."
 ]
}

 The dataset includes 47832 records from 370 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0010445-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25574/csc2.obs.06905
title: Chandra X-ray Observatory ObsId 06905

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.tkmjah
title: Superconducting nanowire single-photon detector arrays for optical communication, astronomy, and single-photon imaging

description: No abstract available.
DOI: 10.25574/csc2.obs.23740
title: Chandra X-ray Observatory ObsId 23740

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.48577/jpl.aziixq
title: Maneuver Design Techniques for Deploying and Maintaining the SunRISE Constellation

description: The Sun Radio Interferometer Space Experiment (SunRISE) mission will employ a constellation of 6 CubeSats in an orbit 300 km above geostationary to study the transport and acceleration of solar energetic particles associated with coronal mass ejections. While the spacecraft are capable of executing maneuvers anywhere within the orbit, selecting the time of the OTM may minimize the DeltaV, ensure that DeltaV constraints are met, and minimize the chance of close approaches within the constellation during transfers. The present paper focuses on the maneuver design process for deploying and maintaining the constellation in a loose, repeating formation to create the first spaceborne imaging interferometer.
DOI: 10.25574/csc2.obs.05407
title: Chandra X-ray Observatory ObsId 05407

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".
DOI: 10.25574/csc2.obs.14484
title: Chandra X-ray Observatory ObsId 14484

description: CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observations that have been combined in this way is known as a "stack".