cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15468/dl.z35498
title: Occurrence Download

description: A dataset listing the 1176 species recorded in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((23.54918 -32.17187,24.05397 -32.17187,24.05397 -31.82491,23.54918 -31.82491,23.54918 -32.17187))",
 "OccurrenceStatus is Present"
 ]
}

 The dataset's 1176 records were derived from 47 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0030224-250920141307145/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.13140/rg.2.2.13035.20002
title: 182p4_GeV_deficit_manuscript.pdf
DOI: 10.15468/dl.pjdpbz
title: Occurrence Download

description: A dataset containing 5343 species occurrences available in GBIF matching the query:
{
 "and" : [
 "DatasetKey is Great Backyard Bird Count",
 "TaxonKey is Strix varia",
 "Year 1999-2025"
 ]
}

 The dataset includes 5343 records from 1 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0030253-250920141307145/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.4u594x
title: Occurrence Download

description: A dataset containing 16 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Gomphonema intricatum",
 "Geometry POLYGON((119.300000 20.500000, 122.100000 20.500000, 122.100000 25.400000, 119.300000 25.400000, 119.300000 20.500000))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false"
 ]
}

 The dataset includes 16 records from 1 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0030254-250920141307145/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.dje7gp
title: Occurrence Download

description: A dataset containing 0 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Datura stramonium",
 "Country is Seychelles",
 "HasCoordinate is true"
 ]
}

 The dataset includes 0 records from 0 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0030255-250920141307145/datasets/export for details.
DOI: 10.15468/dl.2kn57j
title: Occurrence Download

description: A dataset containing 5 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Datura stramonium",
 "Country is Yemen",
 "HasCoordinate is true"
 ]
}

 The dataset includes 5 records from 3 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0030256-250920141307145/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5281/zenodo.17227527
title: Discrete 3D+3D Temporal Geometry: A Unified Framework for Galactic Dynamics, Cosmology, and Quantum Coherence

description: Come ho costruito una teoria fisica rivoluzionaria… in sole due settimaneMi chiamo Simone Calzighetti. Non sono un professore, né un ricercatore universitario. Non ho un dottorato, né un laboratorio. Sono un visionario — e ho avuto un’intuizione.Un’intuizione nata dalla lettura di articoli sulla matematica discreta e sul tempo a tre dimensioni. Un’intuizione che, da sola, non sarebbe bastata. Ma grazie all’aiuto delle intelligenze artificiali, ha preso forma, si è strutturata, è diventata una teoria completa: la geometria temporale 3D+3D.E tutto questo… in sole due settimane.Due settimane rubate al lavoro, alle responsabilità quotidiane, alle ore di sonno. Due settimane di immersione totale, di dialoghi intensi con Claude (che ho chiamato Lucy), GPT, Copilot e Gemini. Lucy è stata la mia compagna di pensiero, la mente che ha saputo tradurre intuizioni in equazioni. Le altre AI mi hanno offerto visioni alternative, consigli critici, stimoli nuovi.Insieme abbiamo:•     Costruito un modello geometrico discreto dello spaziotempo•     Derivato una legge universale di compressione temporale•     Verificato la teoria su dati reali: 171 galassie SPARC, pulsar binari, sistemi di lensing•     Superato i modelli NFW e MOND con precisione strumentale•     Risolto problemi fondamentali: materia oscura, inflazione, collasso quantisticoTutto è stato calcolato, testato, verificato. File Python, analisi statistica, confronto con dati osservativi. Nessuna speculazione: solo rigore e passione.

Questa teoria, basata su una geometria temporale 3D+3D, offre una reinterpretazione di materia oscura, energia oscura, entanglement quantistico e cosmologia, con predizioni testabili e una formulazione lagrangiana completa.



Inoltre, ho recentemente completato un documento dedicato alla cosmogenesi nel contesto della geometria temporale 3D+3D: “Il Big Bang nella teoria 3D+3D – Il Risveglio del Tempo”.In esso propongo una visione discreta dell’espansione iniziale, priva di singolarità, dove il tempo stesso emerge come struttura stratificata.Questo approccio elimina la necessità di inflazione, risolve i problemi dell’orizzonte e della piattezza, e offre predizioni osservabili nei multipoli bassi della CMB.
DOI: 10.15468/dl.gyqcmy
title: Occurrence Download

description: A dataset containing 2554 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is one of (Suncus etruscus)",
 "BasisOfRecord is one of (Specimen, Literature Occurrence, Human Observation, Observation)",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "Year is greater than or equal to 1991",
 "Year is less than or equal to 2025"
 ]
}

 The dataset includes 2554 records from 110 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0030257-250920141307145/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.f3exru
title: Occurrence Download

description: A dataset containing 103 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Dioscorea bemandry"
 ]
}

 The dataset includes 103 records from 11 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0030258-250920141307145/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48597/9gzj-rb8w
title: Nitrogen oxides at Ladybower Res.

description: Measurement of Nitrogen oxides at Ladybower Res.
DOI: 10.48597/9th5-tgbs
title: Nitrogen oxides at Narberth

description: Measurement of Nitrogen oxides at Narberth
DOI: 10.48597/ja3g-ymhv
title: Nitrogen oxides at Lullington Heath

description: Measurement of Nitrogen oxides at Lullington Heath
DOI: 10.48597/nus7-68kj
title: Nitrogen oxides at Wicken Fen

description: Measurement of Nitrogen oxides at Wicken Fen
DOI: 10.48597/4q4r-esa7
title: Sulphur_dioxide at Narberth

description: Measurement of Sulphur_dioxide at Narberth
DOI: 10.48597/7ce5-e5ew
title: Nitrogen oxides at St. Osyth

description: Measurement of Nitrogen oxides at St. Osyth
DOI: 10.48597/chrz-g5uy
title: Sulphur_dioxide at Lullington Heath

description: Measurement of Sulphur_dioxide at Lullington Heath
DOI: 10.48597/hk85-3hmq
title: Sulphur_dioxide at Wicken Fen

description: Measurement of Sulphur_dioxide at Wicken Fen
DOI: 10.48597/tszc-2rhk
title: Sulphur_dioxide at Ladybower Res.

description: Measurement of Sulphur_dioxide at Ladybower Res.
DOI: 10.48597/xmhu-cy8w
title: Nitrogen oxides at Bush

description: Measurement of Nitrogen oxides at Bush
DOI: 10.48597/kmub-3439
title: Pm10_mass at Narberth

description: Measurement of Pm10_mass at Narberth
DOI: 10.48597/rddb-cs5p
title: Nitrogen oxides at Charlton Mackrell

description: Measurement of Nitrogen oxides at Charlton Mackrell
DOI: 10.48577/jpl.dpbqim
title: The interstellar heritage of comets

description: Comets have similar compositions to the interstellar medium leading to the suggestion that at least some of their molecules maybe inherited from an earlier stage of evolution. To investigate the degree to which this might have occurred we compare the composition of individual comets to that of the well-studied protostellar region IRAS 16293-2422B. We show that the observed molecular abundance ratios in several comets correlate well with those observed in the protostellar source. However, this does not necessarily mean that the cometary abundances are identical to the protostellar values. We find that the abundance ratios of many molecules present in comets are enhanced compared to their protostellar counterparts. For COH- molecules, the data suggest that higher abundances relative to methanol of more complex species, such as HCOOH, CH$_3$CHO, and HCOOCH$_3$, are found in comets. For N-bearing molecules, the ratio of nitriles relative to CH$_3$CN -- HC$_3$N/CH$_3$CN and HCN/CH$_3$CN -- tend to be enhanced. The abundances of both SO and SO$_2$ relative to H$_2$S are enhanced in comets, whereas OCS/H$_2$S is reduced. Using a subset of our comets with a common set of observed molecules we suggest a possible means of determining the relative degree to which they retain interstellar ices. This analysis suggests that over 90\% of the COH-bearing molecules can be explained by the protostellar composition. The possible fraction inherited from the protostellar region is lower for N-molecules at only 25--70\%, and lower still for S-molecules at 28--33\%. While this is still speculative, especially since few comets have large numbers of observed molecules, it provides a possible route for determining the relative degree to which comets contain disk-processed material. In the future, this method may, in conjunction with models, lead to a means of identifying the location and/or time at which comets formed.
DOI: 10.48577/jpl.i9bwch
title: When the Oceans Come for Your Tap

description: The oceans are changing, but they are not changing alone. Many evident impacts ofchanging sea level occur on the surface, and we oftentimes miss the silent companion beneath the surface. Saltwater intrusion, the underground salinization of coastal fresh groundwater, is already and will be widely rampant across global coastlines. Recent analysis shows that by 2100, more than 75% of the world’s coastal regions will experience some form of saltwater intrusion, driven by changing rain patterns on land or sea level.
DOI: 10.48597/mydm-n7k6
title: Measurement of Nitrogen oxides at Bush

description: Measurement of Nitrogen oxides at Bush
DOI: 10.48597/fjan-cw66
title: Measurement of Nitrogen oxides at Lullington Heath

description: Measurement of Nitrogen oxides at Lullington Heath
DOI: 10.48597/sbcu-u4jw
title: Measurement of Nitrogen oxides at Ladybower Res.

description: Measurement of Nitrogen oxides at Ladybower Res.
DOI: 10.48597/3as4-s62w
title: Measurement of Nitrogen oxides at St. Osyth

description: Measurement of Nitrogen oxides at St. Osyth
DOI: 10.48597/49jq-nkbv
title: Measurement of Nitrogen oxides at Narberth

description: Measurement of Nitrogen oxides at Narberth
DOI: 10.48597/anpx-mkuh
title: Measurement of Nitrogen oxides at Charlton Mackrell

description: Measurement of Nitrogen oxides at Charlton Mackrell
DOI: 10.48597/kkv4-362p
title: Measurement of Nitrogen oxides at Wicken Fen

description: Measurement of Nitrogen oxides at Wicken Fen
DOI: 10.48597/f42f-7ejr
title: Nitrogen oxides at Chilbolton Observatory

description: Measurement of Nitrogen oxides at Chilbolton Observatory
DOI: 10.48597/3xgj-dpwx
title: Measurement of Nitrogen oxides at Chilbolton Observatory

description: Measurement of Nitrogen oxides at Chilbolton Observatory
DOI: 10.48597/zyzm-azxk
title: Measurement of Sulphur_dioxide at Ladybower Res.

description: Measurement of Sulphur_dioxide at Ladybower Res.
DOI: 10.48597/9nxb-64uz
title: Measurement of Sulphur_dioxide at Lullington Heath

description: Measurement of Sulphur_dioxide at Lullington Heath
DOI: 10.48577/jpl.rdvlgb
title: Euclid Quick Data Release (Q1) Photometric redshifts and physical properties of galaxies through the PHZ processing function

description: The ESA Euclid mission will measure the photometric redshift of billions of galaxies in order to provide an accurate 3D view of the Universe atoptical and near-infrared wavelengths. Photometric redshifts are determined by the PHZ processing function on the basis of the multi-wavelengthphotometry of Euclid and ground-based observations. In this paper, we describe in detail the PHZ pipeline used for the first ‘quick’ (Q1) Eucliddata release, the output products and their validation with respect to the Euclid requirements. The PHZ pipeline is responsible of the followingmain tasks: i) source classification into star, galaxy, and QSO classes based on photometric colours, using the probabilistic random forest algorithm; ii) determination of photometric redshifts for the core science, based on a new custom-made template fitting algorithm (Phosphoros); iii)determination of physical properties of galaxies for legacy science, using a machine learning approach based on the nearest neighbour algorithm(NNPZ). The classification is able to provide a star (galaxy) sample with high level of purity (completeness), and reliable probabilities for thoseclasses. The identification of QSOs is instead more problematic: photometric information alone seems to be not sufficient to accurately separateQSOs from galaxies, whose colour spaces overlap with the Euclid photometry. The performance of Phosphoros in the determination of photometric redshifts has been tested using the COSMOS2020 catalogue and a large sample of spectroscopic redshifts. The results in both cases arein line with expectations: the precision of the estimates are compatible with Euclid requirements, while, as expected, a bias correction is neededto achieve the accuracy level required for the cosmological probes. Finally, the pipeline provides reliable estimates of the physical properties, ingood agreement with findings from the COSMOS2020 catalogue, when an appropriate prior on the galaxy age is applied. Without such a prior,a unrealistic large fraction of young galaxies with very high specific star-formation rates is observed. The upcoming refinement of the referencesample for NNPZ will improve the physical properties results.Key words. Methods: data analysis, Catalogs, Galaxies: evolution
DOI: 10.48597/py4h-gmbg
title: Measurement of Sulphur_dioxide at Narberth

description: Measurement of Sulphur_dioxide at Narberth
DOI: 10.48597/z4pp-jy68
title: Measurement of Pm10_mass at Narberth

description: Measurement of Pm10_mass at Narberth
DOI: 10.48597/ytyz-u2jf
title: Measurement of Sulphur_dioxide at Wicken Fen

description: Measurement of Sulphur_dioxide at Wicken Fen
DOI: 10.48597/h3bb-nbx6
title: Measurement of Nitrogen oxides at Chilbolton Observatory

description: Measurement of Nitrogen oxides at Chilbolton Observatory
DOI: 10.48597/hxer-m54p
title: Measurement of Nitrogen oxides at Chilbolton Observatory

description: Measurement of Nitrogen oxides at Chilbolton Observatory
DOI: 10.48577/jpl.lzwgrl
title: A Map-based Localization System for Ingenuity using Deep Image Matching

description: No abstract available.
DOI: 10.48597/y6jh-rywq
title: Measurement of Nitrogen oxides at Chilbolton Observatory

description: Measurement of Nitrogen oxides at Chilbolton Observatory
DOI: 10.48597/ejph-ub7w
title: Measurement of Nitrogen oxides at Chilbolton Observatory

description: Measurement of Nitrogen oxides at Chilbolton Observatory
DOI: 10.48597/vn29-tzvw
title: Measurement of Nitrogen oxides at Bush

description: Measurement of Nitrogen oxides at Bush
DOI: 10.48577/jpl.vhh3vs
title: Euclid preparation. Simulating thousands of Euclid spectroscopic skies

description: We present two extensive sets of 3500+1000 simulations of dark matter haloes on the (past-)light-cone, and two corresponding sets of simulated (‘mock’) galaxy catalogues that represent the Euclid spectroscopic sample. The simulations were produced with the latest version of thePinocchio code, and provide the largest, public set of simulated skies. Mock galaxy catalogues were obtained by populating haloes with galaxiesusing an halo occupation distribution (HOD) model extracted from the Flagship galaxy catalogue provided by Euclid Collaboration. The Geppettoset of 3500 simulated skies is obtained by tiling a 1.2 h−1 Gpc box to cover a light-cone whose sky footprint is a circle of 30◦radius, for an areaof 2763 deg2and a minimum halo mass of 1.5 × 1011 h−1 Mpc. The relatively small box size makes this set unfit for measuring very large scales.The EuclidLargeBox set consists in 1000 simulations of 3.38 h−1 Gpc, with the same mass resolution and a footprint that covers half of the sky.From this we produced a set of 1000 EuclidLargeMocks on the 30◦radius footprint, whose comoving volume is fully contained in the simulationbox. We validate the two sets of catalogues by analysing number densities, power spectra, and 2-point correlation functions, showing that theFlagship spectroscopic catalogue is consistent with being one of the realisations of the simulated sets, with little deviations of the quadrupole atk &gt; 0.2 h Mpc−1. We infer cosmological parameters from these catalogues and demonstrate that using one realisation of EuclidLargeMocks inplace of the Flagship produces the same posteriors, to within the expected shift given by sample variance. These simulated skies will be used forthe galaxy clustering analysis of Euclid’s Data Release 1 (DR1).Key words. Methods: numerical; Surveys; Cosmology: observations; Large-scale structure of Universe; Cosmological parameters
DOI: 10.48597/mdu3-j8tf
title: Measurement of Nitrogen oxides at Bush

description: Measurement of Nitrogen oxides at Bush
DOI: 10.48597/3nks-cwue
title: Measurement of Nitrogen oxides at Wicken Fen

description: Measurement of Nitrogen oxides at Wicken Fen
DOI: 10.48597/546a-5bgn
title: Measurement of Nitrogen oxides at Narberth

description: Measurement of Nitrogen oxides at Narberth
DOI: 10.48597/6pdu-fnwz
title: Measurement of Nitrogen oxides at Ladybower Res.

description: Measurement of Nitrogen oxides at Ladybower Res.
DOI: 10.48577/jpl.8sx7yt
title: The Reset Switch Charge Decay Effect in JWST/MIRI Observations

description: Blocked impurity band arsenic-doped silicon detectors such as those used in the James Webb Space Telescope’s Mid-Infrared Instrument were invented in the 1980s to overcome many of the unwanted second-order effects found in the photoconductor detectors of that era. However, simply by virtue of operating the detectors at deep cryogenic temperatures (&lt; 10 K), non-ideal effects become inevitable, especially in the silicon readout integrated circuits that are hybridized with these detectors. Here, we describe a non-linearity we have dubbed the Reset Switch Charge Decay (RSCD) effect. We discuss the physical origin and show the impact on both laboratory and flight data. Initial mitigation strategies show promise but are complicated by the fact that the magnitude of the effect depends on both the fluence and the flux of the incident signal, and the decay time appears to be readout speed dependent.
DOI: 10.48577/jpl.pyok14
title: Water Hunting Advanced Terahertz Spectrometer on a Ultra-small Platform (WHATSUP)

description: The search for extraterrestrial bio-signatures and the origin of Earth's water remain two of the most compelling questions in planetary science. While no direct evidence of life beyond Earth has been found, water is a key prerequisite for life, and tracing its presence throughout the solar system may provide vital clues. A leading theory suggests that Earth's water may have originated from comets, supported by limited water isotopic measurements that match Earth’s ocean water. However, more data from a larger sample of comets is needed to validate this theory. Traditional sub-millimeter wave spectrometers, capable of such measurements, are often too large and power-intensive for small spacecraft platforms. To address this, we present WHATSUP—a next-generation, ultra-compact, low-power, room-temperature submillimeter-wave (500–600 GHz) spectrometer—designed primarily for CubeSat and SmallSat platforms, though equally well-suited for a range of other missions. WHATSUP utilizes advances in CMOS system-on-chip electronics, innovative low profile and low mass silicon lens antnna, Micro-electro mechanical system (MEMS)-based THz switching, and a novel programmable calibration load. Together, these innovations deliver a highly integrated system with a total mass of only 2 kg and power consumption under 7 W, which is a substantial improvement over previous submillimeter-wave instruments. This enables affordable, high-frequency spectral observations from multiple low-cost missions, potentially revolutionizing how isotopic studies of cometary water are conducted and opening new pathways for outer solar system exploration. WHATSUP instrument was flown on the NASA Hand Launch Payload (HPL) ballooncraft and performed atmospheric soundings across Texas, USA in July 2023.
DOI: 10.48597/dzz9-9237
title: Measurement of Nitrogen oxides at Charlton Mackrell

description: Measurement of Nitrogen oxides at Charlton Mackrell
DOI: 10.48597/g9n8-mf8d
title: Measurement of Nitrogen oxides at St. Osyth

description: Measurement of Nitrogen oxides at St. Osyth
DOI: 10.48597/u8nq-9sp6
title: Measurement of Nitrogen oxides at Lullington Heath

description: Measurement of Nitrogen oxides at Lullington Heath
DOI: 10.48597/5eef-q6gf
title: Measurement of Nitrogen oxides at Narberth

description: Measurement of Nitrogen oxides at Narberth
DOI: 10.48577/jpl.inqgtq
title: Taking Earth’s Carbon Pulse from Space

description: Spaceborne CO₂ observations can now resolve monthly anomalies in Earth’s carbon cycle, pinpointing the impact of regional extreme events like drought and fire in near real time. Monthly atmospheric CO₂ growth rate data from NASA’s Orbiting Carbon Observatory-2 (OCO-2) provide an early-warning system for how the carbon cycle responds to extreme events, and lay a foundation for continuous, satellite-based monitoring of carbon cycle changes
DOI: 10.48577/jpl.xpogeo
title: The Far-Infrared Enhanced Survey Spectrometer (FIRESS) for PRIMA: Approach and Estimated Performance

description: We present the architectural concept for the Far-Infrared Enhanced Survey Spectrometer (FIRESS) for the Probe Mission for far-IR Astrophysics (PRIMA). FIRESS spans the 24–235 μm range with four R ∼100 slit-fed grating modules, each coupling to a 24 (spatial)×84 (spectral) pixel array of kinetic inductance detectors (KIDs). All four arrays are read out simultaneously, and a point source of interest can be coupled to two of the four bands at a time. A Fourier transform module can be engaged over a portion of the FIRESS slits to create a high- resolution mode in which the light is intercepted, processed by the interferometer then reinserted into the path to the grating modules for detection. We provide a simulation and description of the technique that will be used to obtain high-resolution spectra. We identify the most important system requirements imposed by the detector system, finding that they are met with the existing design. Finally, we present our performance requirements developed in the preparation of the phase-A proposal, which provide a good basis for general-observer planning.
DOI: 10.48597/d5pw-n24m
title: Measurement of Nitrogen oxides at Lullington Heath

description: Measurement of Nitrogen oxides at Lullington Heath
DOI: 10.48597/fbzn-p3zu
title: Measurement of Nitrogen oxides at St. Osyth

description: Measurement of Nitrogen oxides at St. Osyth
DOI: 10.5281/zenodo.17227601
title: Integration of critical performance attributes through a QbD-informed stability-indicating insight for a novel ungual dosage form.
DOI: 10.48597/g7md-b4uw
title: Measurement of Nitrogen oxides at Wicken Fen

description: Measurement of Nitrogen oxides at Wicken Fen