cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15156/bio/sh1394518.10fu
title: SH1394518.10FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.15156/bio/sh1394523.10fu
title: SH1394523.10FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.15156/bio/sh1394530.10fu
title: SH1394530.10FU

description: UNITE provides a unified way for delimiting, identifying, communicating, and working with DNA-based Species Hypotheses (SH). All fungal ITS sequences in the international nucleotide sequence databases are clustered to approximately the species level by applying a set of dynamic distance values (<0.5 - 3.0%). All species hypotheses are given a unique, stable name in the form of a DOI, and their taxonomic and ecological annotations are verified through distributed, web-based third-party annotation efforts. SHs are connected to a taxon name and its classification as far as possible (phylum, class, order, etc.) by taking into account identifications for all sequences in the SH. An automatically or manually designated sequence is chosen to represent each such SH. These sequences are released (https://unite.ut.ee/repository.php) for use by the scientific community in, for example, local sequence similarity searches and next-generation sequencing analysis pipelines. The system and the data are updated automatically as the number of public fungal ITS sequences grows.
DOI: 10.48580/dw92.v79
title: Liolaemus jamesi (Boulenger, 1891): restriction of the type locality and holotype characterization (Squamata: Liolaemidae)
DOI: 10.48580/dw97.v82
title: Two more new species of the Cyrtodactylus peguensis group (Squamata: Gekkonidae) from the fringes of the Ayeyarwady Basin, Myanmar
DOI: 10.48580/dw8y.v86
title: Description of a new species of Loxosceles Heineken & Lowe (Araneae, Sicariidae) recluse spiders from Hidalgo, Mexico, under integrative taxonomy: morphological and DNA barcoding data (CO 1 + ITS 2)
DOI: 10.48580/dw94.v80
title: Parochodaeus bituberculatus (Erichson) (Coleoptera: Ochodaeidae) and Faargia gentilii (Martínez) (Coleoptera: Scarabaeidae), two species newly discovered in Chile
DOI: 10.48580/dw8n.v84
title: New species and additional records of Cephalocousya and Drepasiagonusa from China and Russia (Coleoptera: Staphylinidae: Aleocharinae: Oxypodini)
DOI: 10.48580/dw8t.v75
title: On the taxonomy of the genus Sacada Walker, 1862 from India, with descriptions of a new genus and two new species (Pyralinae, Pyralidae, Lepidoptera)
DOI: 10.48580/dw8h.v88
title: New and enigmatic cockroaches (Dictyoptera: Blattodea) of Guyana
DOI: 10.48580/dw8j.v80
title: First record of a non-pollinating fig wasp (Hymenoptera: Sycophaginae) from Dominican amber, with estimation of the size of its host figs
DOI: 10.48577/jpl.lvdlng
title: The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas

description: With four giant planets (m∼5−10 MJup, Teff ∼900−1200 K) orbiting between 15-70 au, HR 879930 provides an unparalleled testbed for studying giant planet formation and probing compositional trends across the protoplanetary disk. We present new JWST/NIRSpec IFU observations (2.85−5.3 µm, R ≈2700) that now include the spectrum of HR 8799 b, and higher S/N spectra for HR 8799 c, d, and e compared to that in J.-B. Ruffio & J. W. Xuan et al. (2025). We detect CO, CH4, H2O, H2S, CO2, and for planet b, NH3. We combine the NIRSpec spectra with 1−5µm photometry to perform atmospheric retrievals that account for disequilibrium chemistry and clouds, and allow C/H, O/H, N/H, and S/H to scale independently. While the four planets are similarly enriched in carbon and oxygen (volatiles), with C/H and O/H between 3−5×stellar, we observe a tentative trend of increasing S/H – a tracer of refractory solids – from 2−5×stellar with increasing orbital distance. From HR 8799 b’s NH3 abundance, we estimate N/H = 21.2+16.2 −8.8 ×stellar, suggesting the outer planet accreted significant amounts of N-rich gas. Overall, the elemental abundance patterns we observe are consistent with a picture where planet b formed between the CO snowline and the more-distant N2 snowline, while the inner planets accreted 3×stellar CO enriched disk gas within the CO snowline. The excess volatile mass from pebble drift and evaporation implies an integrated pebble flux of 750 ±200M⊕. The increase in the planets’ S/H with orbital distance implies more solid accretion further out, which is quantitatively compatible with expectations from both pebble and planetesimal accretion (2× Minimum Mass Solar Nebula) paradigms.
DOI: 10.48580/dw87.v82
title: New Taxonomic and Faunistic Data on the Genus Meteorus H, 1835 (Hymenoptera: Braconidae: Euphorinae) of Gökçeada (Imbros and Bozcaada (Tenedos) from Turkey
DOI: 10.48577/jpl.c8fwpl
title: Large scale mapping of Ci and the Ci-to-CO transition in ρ Ophiuchus molecular cloud

description: Atomic carbon (C i) is a key species in the carbon chemistry of the interstellar medium (ISM). Using the Submillimeter Wave Astronomy Satellite (SWAS), we conducted a [C i] (3P1–3P0) 492 GHz survey covering approximately 4 deg2 of the L1688 and L1689 regions in the ρ Oph molecular cloud, achieving a spatial resolution of 4.25′. The derived Ci column densities, N(C i), range from 4.85 × 1014 cm−2 to 6.29 × 1017 cm−2, corresponding to an abundance ratio N(C i)/N(H2) of 2.24× 10−7 to 2.39×10−4, with a median value of 1.8× 10−5. Combining observations with photodissociation region (PDR) modeling, we find that Ci abundance varies less than CO in regions with UV intensity G0 &gt; 16 and N(H2) &lt; 4.6 × 1021 cm−2, suggesting [C i] is a more reliable tracer of molecular hydrogen in low-density, high-radiation environments where the Ci-to-CO transition occurs. With current observation sensitivity, [C i] emission is detected toward 3.5% pixels of CO-dark gas around the cloud edge. Utilizing [C I] as direct H2 tracer, the CO-dark gas fraction is estimated to be 0.43 , meaning that 43% of the total cloud mass will be missed by conventional calculation based on CO observations but can be calibrated by [C i] emission. The [C i] line widths are systematically broader than those of 13CO, possibly due to contributions from atomic carbon. These findings provide key insights into Galactic [C i] emission and the carbon cycle evolution in the interstellar medium. Future high-sensitivity [C i] (3P1–3P0) surveys with the Chinese Survey Space Telescope (CSST) will significantly advance our understanding of the carbon cycle evolution.
DOI: 10.48580/dw82.v75
title: Hamadiana chapadensis, a new genus and species of diving beetle from Brazil (Coleoptera, Dytiscidae, Laccophilinae, Laccophilini)
DOI: 10.48580/dw83.v77
title: Anthias albofasciatus Fowler and Bean, 1930, a junior synonym of Tosana niwae Smith and Pope, 1906 (Teleostei: Serranidae: Anthiadinae)
DOI: 10.48580/dw84.v78
title: A new subspecies of Dysiatus from the Sangihe and Talaud islands (Coleoptera: Cerambycidae, Prioninae)
DOI: 10.48580/dw85.v82
title: A new species of Caroperla Kohno, 1946 (Plecoptera: Perlidae) from Guangxi of China
DOI: 10.48577/jpl.uxhyrf
title: High Precision Altimetry using Spaceborne Grazing Angle GNSS-Reflectometry over Tonle Sap Lake

description: This study uses spaceborne grazing angle Global Navigation Satellite System-Reflectometry (GNSS-R) signals to measure surface height variations of the Tonl´e Sap Lake (TSL) in Cambodia. The GNSS-R tracks are collected by Spire Global from 2021 to 2024, and GNSS-R altimetry retrievals are compared to co-located Surface Water and Ocean Topography (SWOT), and Ice, Cloud, and Land Elevation Satellite-2 (ICESat- 2) measurements. There is good agreement between all, with surface height correlations &gt; 0.7. Over open water, the average measurement noise level in terms of standard deviation is 3, 2.5, and 1.6 cm for GNSS-R, SWOT, and ICESat-2, respectively. However, GNSS-R altimetry maintains a similar noise level when measuring water height under vegetation, while SWOT and ICESat-2 noise increases significantly to 4.6 and 6.9 cm, respectively. The ability to measure water height under vegetation in all weather and times of day highlights the strength of the GNSS-R altimetry method for inland water studies. Finally, signatures suggestive of the mean lake surface (MLS) of the TSL along tracks in the upper and lower TSL are identified. The TSL was chosen due to its local importance and unique hydrology, but the techniques of this research can be applied to many large lakes.
DOI: 10.48580/dw7r.v79
title: A novelty in Ceratozamia (Zamiaceae, Cycadales) from the Sierra Madre del Sur, Mexico: biogeographic and morphological patterns, DNA barcoding and phenology
DOI: 10.48580/dw7x.v88
title: On the systematic status of the genus Oriocalotes Günther, 1864 (Squamata: Agamidae: Draconinae) with the description of a new species from Mizoram state, Northeast India
DOI: 10.48577/jpl.nsebcy
title: Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Wb from z-0.1 to ~12

description: We explore the evolving relationship between galaxies and their dark matter halos from 𝑧 ∼ 0.1 to 𝑧 ∼ 12 using mass-limited angular clustering measurements in the 0.54 deg2 of the COSMOS-Web survey, the largest contiguous JWST extragalactic survey. This study provides the first mass-limited two-point correlation function at 𝑧 ≥ 10 and a consistent analysis spanning 13.4 Gyr of cosmic history, setting new benchmarks for future simulations and models. Using a halo occupation distribution (HOD) framework, we derive characteristic halo masses and the stellar-to-halo mass relationship (SHMR) across redshifts and stellar mass bins. Our results first indicate that HOD models fit data at 𝑧 ≥ 2.5 best when incorporating a non-linear scale-dependent halo bias, boosting clustering at quasi-linear scales (𝑟 = 10-100 kpc). We find that galaxies at 𝑧 ≥ 10.5 with log(𝑀★/𝑀⊙) ≥ 8.85 are predominantly centrals in halos with 𝑀h ∼ 1010.5 𝑀⊙, achieving a star formation efficiency (SFE) 𝜀SF = 𝑀★/( 𝑓𝑏𝑀h) up to 1 dex higher than at 𝑧 ≤ 1. The high galaxy bias at 𝑧 ≥ 8 suggests that these galaxies reside in massive halos with intrinsic high SFE, challenging stochastic SHMR scenarios. Our SHMR evolves significantly with redshift, starting very high at 𝑧 ≥ 10.5, decreasing until 𝑧 ∼ 2 − 3, then increasing again until the present. Current hydrodynamical simulations fail to reproduce both massive high-𝑧 galaxies and this evolution, while semi-empirical models linking SFE to halo mass, accretion rates, and redshift align with our findings. We propose that early galaxies (𝑧 &gt; 8) experience bursty star formation without significant feedback, altering their growth, driving the rapid growth of massive galaxies observed by JWST. Over time, increasing feedback efficiency and exponential halo growth suppress star formation. At 𝑧 ∼ 2 − 3 and after, halo growth slows down while star formation continues, supported by gas reservoirs in halos.
DOI: 10.48580/dw7h.v82
title: A new species of Tropidion (Neoibidionini), synonymies in Rhinotragini, notes on Pirangoclytus (Clytini) andHemicladus (Calliini), andnew recordsin Cerambycidae (Coleoptera)
DOI: 10.48580/dw7k.v80
title: Brontostoma lilloi Carpintero, 1980, a junior synonym of B. rubrovenosum (Stål, 1860) (Hemiptera: Heteroptera: Reduviidae)
DOI: 10.5281/zenodo.16746722
title: Autoethnographische Reflexion: Zwischen Anspruch und Umsetzung: Reflexionen über Transferprozesse in der Lehrkräftefortbildung

description: Dieser Datensatz einer autoethnographischen Studie enthält:



die Arbeitsanweisung für die autoethnograohischen Reflexionen, sowie

das auf der qualitativen Inhaltsanalyse entstandene Kodebuch.


Die Analysen und Ergebnisse sind im folgenden Beitrag publiziert:



Heck, T.; Schenk, A.; Heijens, M.; Heinemann, T.;  Hiebl, J.; Lauffenburger, M.; Muschaweck, I.; Raschke, N.; Schulze, U. (im Druck). Zwischen Anspruch und Umsetzung: Reflexionen über Transferprozesse in der Lehrkräftefortbildung. Beitrag in derBuchreihe “Kompetenzzentren für digital gestützte Schul- und Unterrichtsentwicklung. Waxmann. 


Die Studie und der Datensatz ist im Rahmen des Teilprojekts (Kennzeichen: 01JA23S06C) von ReTransfer entstanden, gefördert vom Bundesministerium für Bildung, Familie, Senioren, Frauen und Jugend und NextGeneration EU.
DOI: 10.48580/dw74.v84
title: Types of Thyatirinae (Lepidoptera: Drepanidae) in the collection of the Zoological Institute of the Russian Academy of Sciences
DOI: 10.48580/dw75.v80
title: A key to the Mexican genera of Tanymecini (Coleoptera: Curculionidae)
DOI: 10.48580/dw7c.v86
title: A review of Peruvian diving beetles of the genus Hydaticus Leach, 1817, with description of Hydaticus (Prodaticus) panguana sp. nov. and notes on other Neotropical species (Coleoptera: Dytiscidae)
DOI: 10.48580/dw7d.v81
title: A survey of Agroeca Westring, 1861 from China (Araneae: Liocranidae)
DOI: 10.48580/dw6z.v78
title: Ichneumonidae (Hymenoptera) from Anatolia II
DOI: 10.5281/zenodo.16746721
title: Autoethnographische Reflexion: Zwischen Anspruch und Umsetzung: Reflexionen über Transferprozesse in der Lehrkräftefortbildung

description: Dieser Datensatz einer autoethnographischen Studie enthält:



die Arbeitsanweisung für die autoethnograohischen Reflexionen, sowie

das auf der qualitativen Inhaltsanalyse entstandene Kodebuch.


Die Analysen und Ergebnisse sind im folgenden Beitrag publiziert:



Heck, T.; Schenk, A.; Heijens, M.; Heinemann, T.;  Hiebl, J.; Lauffenburger, M.; Muschaweck, I.; Raschke, N.; Schulze, U. (im Druck). Zwischen Anspruch und Umsetzung: Reflexionen über Transferprozesse in der Lehrkräftefortbildung. Beitrag in derBuchreihe “Kompetenzzentren für digital gestützte Schul- und Unterrichtsentwicklung. Waxmann. 


Die Studie und der Datensatz ist im Rahmen des Teilprojekts (Kennzeichen: 01JA23S06C) von ReTransfer entstanden, gefördert vom Bundesministerium für Bildung, Familie, Senioren, Frauen und Jugend und NextGeneration EU.
DOI: 10.48580/dw6w.v80
title: Type specimens of Andrena wollastoni C, 1922 (Hymenoptera, Anthophila): deposition, evaluation and designation of a lectotype
DOI: 10.48577/jpl.nwscgz
title: A candidate high-redshift tidal disruption event at z ≳ 7 in COSMOS-Web: the first photometric search with JWST

description: In this work, we predict TDE rates across upcoming deep surveys with Rubin, Roman, and JWST, first assuming the properties and rates of TDEs at low redshifts determined from the optically-selected sample from the Zwicky Transient Facility (ZTF). Extrapolating the local rate to higher redshifts, we expect thousands of TDEs per year in Rubin, with hundreds at z &gt; 1, tens per year in the Roman High Latitude Time Domain Survey (up to z ∼ 6), and thousands in the Roman Wide Area Survey (up to z ∼ 7), but fewer than one TDE in COSMOS-Web. We suggest, however, that TDE rates at z &gt; 5 may be enhanced by up to two orders of magnitude compared to the local rate because of the higher central stellar mass densities, top-heavy initial mass function, and larger post-merger fractions of galaxies in the early Universe, as revealed by JWST. To test this, we develop a novel methodology for identifying high-redshift TDEs in deep surveys through color and morphology selection criteria and apply it to COSMOS-Web. We discover a high redshift TDE candidate, at redshift 7.2 ⪅ z ⪅ 8.0 which, if validated, confirms the enhancement of the high-redshift TDE rate of at least an order of magnitude. This work is the first demonstration of a method of identifying TDE candidates without time-domain information, and can be applied to find the dozens of z &gt; 4 TDEs present in the Roman Wide Area Survey.
DOI: 10.48577/jpl.z1zwsa
title: SWOT Geostrophic Velocity Validation against in-situ measurements in the California Current

description: The Surface Water and Ocean Topography (SWOT) mission offers unprecedented high-resolution sea surface height (SSH) data, crucial for enhancing our understanding of ocean circulation dynamics. A key objective of SWOT is to convert SSH measurements into ocean velocity estimates. However, deriving reliable velocity estimates from such fine-scale SSH measurements is challenging, and the approach requires rigorous validation. This study evaluates the performance of SWOT in capturing geostrophic velocities within the California Current System (CCS) at 125.044oW, 35.917oN by comparing them to in-situ velocity measurements during the post-launch Calibration and Validation (CalVal) phase, from April 1st to July 4th, 2023. Results indicate that SWOT-derived velocities successfully capture variability at periods greater than 6 days, outperforming conventional satellite altimetry products that capture signals &gt; 25-30 days. The root mean square difference (RMSD) between velocities from SWOT and in-situ measurements is significantly lower, with up to a 58% reduction compared to the in-situ standard deviation. The RMSD for SWOT is 4.2 cm/s, 4.2 cm/s, and 2 cm2/s2 for ug, vg, and EKE, respectively, compared to 4.7 cm/s, 5.8 cm/s, and 2.4 cm2/s2 for conventional altimetry-derived geostrophic velocities. These findings demonstrate SWOT's capability in resolving fine-scale ocean features and validate its potential to advance our understanding of ocean circulation, also highlight the challenges before fully utilizing SWOT's potential in studying ocean circulation in regions with higher internal gravity waves.
DOI: 10.48580/dw6g.v83
title: Patterns of head shape and scutellation in Drymarchon couperi (Squamata: Colubridae) reveal a single species
DOI: 10.48580/dw6s.v76
title: A remarkable new genus and species of Rogadinae (Hymenoptera: Braconidae) of uncertain tribal placement, from Papua New Guinea, resembling Betylobraconini stat. nov.
DOI: 10.48580/dw6m.v76
title: Aphonopelma braunshausenii Tesmoingt, 1996 is a nomen dubium, with review of some historic morphological characters ineffective at species delineation (Araneae: Theraphosidae)
DOI: 10.48577/jpl.ufkr1t
title: Experimental Insights into the Azotosome Hypothesis in Titan’s Lake Fluids

description: Since the discovery of hydrocarbon lakes and seas on Saturn’s moon Titan, there has been much speculation on whether these could serve as suitable environments to host exotic life. A decade ago, molecular dynamics simulations suggested that amphiphilic cyanide species such as acrylonitrile (CH2CHCN) could self-assemble in these cold, non-polar liquid media to form stable closed membranes known as azotosomes, potentially compartmentalizing complex biochemicals reactions. A subsequent thermodynamic study in 2020, however, concluded that azotosomes cannot exist under Titan’s conditions. Motivated by these incongruent computational results, this work undertakes the first experimental test of the azotosome hypothesis where we characterize acrylonitrile/methane and acrylonitrile/ethane mixtures under simulated Titan conditions using a combination of differential scanning calorimetry and Raman microscopy. The results indicate that acrylonitrile forms a stable molecular co-crystal with ethane, while exhibiting little changes in the presence of liquid methane under experimental timescales. These findings suggest that the acrylonitrile-based azotosome structure would be unlikely to form in Titan’s lake fluids.
DOI: 10.48580/dw6c.v83
title: Revision of the species-group of Mischocyttarus (Omega) filiformis (de Saussure 1854), with description of three new species (Hymenoptera, Vespidae)
DOI: 10.48580/dw6d.v82
title: Comments on the taxonomic validity of Camptodontornis yangi (Li, Gong, Zhang Yang, and Hou, 2010) and its relationships to Longipteryx chaoyangensis Zhang Zhou, Hou, and Gu, 2000 and Boluochia zhengi Zhou, 1995
DOI: 10.48580/dw6f.v79
title: One new species of the genus Xizicus Gorochov, 1993 (Orthoptera: Tettigoniidae Meconematinae) from Guangxi, China
DOI: 10.48580/dw6r.v90
title: Five new species of Enchytraeidae (Annelida: Clitellata) from Mediterranean woodlands of Italy and reaffirmed validity of Achaeta etrusca, Fridericia bulbosa and F. miraflores
DOI: 10.25549/garland-ouc11399n1wc
title: Harold Strong Latham, letter, 1921-10-17, to Hamlin Garland

description: Harold Strong Latham (The Macmillan Company), 64-66 5th Avenue, New York, New York, USA, letter, 1921 October 17, to Hamlin Garland, 71 East 92nd Street, New York, New York, USA. "We have once more considered the matter of republishing the following books: Rose of Dutchers Cooly, Main Travelled Roads, Prairie Songs, A Spoil of Office, The Eagle's Heart, Crumbling Idols, The Captain of the Gray Horse Troop." -- first line.
DOI: 10.15468/dl.tdpsp7
title: Occurrence Download

description: A dataset containing 974 species occurrences available in GBIF matching the query:
{
 "and" : [
 "HasGeospatialIssue is false",
 "HasCoordinate is true",
 "OccurrenceStatus is Present",
 {
 "not" : {
 "BasisOfRecord" : [
 "is one of (Fossil, Living Specimen)"
 ]
 }
 },
 "TaxonKey is Sarcosperma"
 ]
}

 The dataset includes 974 records from 33 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0002206-260221153910048/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25549/garland-ouc11399n1wq
title: Harold Strong Latham, letter, 1922-01-20, to Hamlin Garland

description: Harold Strong Latham (The Macmillan Company), 64-66 5th Avenue, New York, New York, USA, letter, 1922 January 30, to Hamlin Garland, 71 East 92nd Street, New York, New York, USA. "I am sorry to have to report that we have no date and can give none for the binding of A Son of the Middle Border in the original style." -- first line.
DOI: 10.25549/garland-ouc11399n1ww
title: Harold Strong Latham, letter, 1922-04-20, to Hamlin Garland

description: Harold Strong Latham (The Macmillan Company), 64-66 5th Avenue, New York, New York, USA, letter, 1922 April 20, to Hamlin Garland, 71 East 92nd Street, New York, New York, USA. "May I just add to my verbal congratulations a little written note." -- first line.