cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.3535/311-055-n9z
title: Philoscia muscorum muscorum (Scopoli, 1763)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/tdy-yhx-8rs
title: Philoscia muscorum muscorum (Scopoli, 1763)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/f9a-r4j-y2k
title: Philoscia muscorum muscorum (Scopoli, 1763)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/b43-p7a-erk
title: Pseudocalanus elongatus (Brady, 1865)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wt7-dmh-rh4
title: Rocinela danmoniensis Leach, 1818

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/997-lk6-vkb
title: Tanaissus lilljeborgi (Stebbing, 1891)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/hw7-5ee-kjx
title: Ratania atlantica Farran, 1926

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/2cd-pj1-gn7
title: Lernaeenicus sprattae (Sowerby, 1806)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/3qw-6w3-b6q
title: Temora longicornis (Müller O.F., 1785)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/9sp-fax-zpa
title: Eudiaptomus gracilis gracilis (Sars G.O., 1863)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/aqw-krh-gvy
title: Aspidomolgus stoichactinus Humes, 1969

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/33t-qcj-lpg
title: Notodelphys agilis Thorell, 1859

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/ls0-as4-4fy
title: Drepanopus pectinatus Brady, 1883

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.fokw9x
title: A New Approach to Compiling Exoatmospheric Target Lists And Quantifying the Ground-Based Resources Needed to Vet Them

description: Transiting exoplanet atmospheric characterization is currently in a golden age as dozens of transit- ing exoplanet atmospheres are being studied by NASA’s Hubble and James Webb Space Telescopes. This trend is likely to continue for the foreseeable future with the 2025 launch of NASA’s Pandora smallsat, the 2029 launch of ESA’s Ariel mission, which includes a contribution from NASA’s CASE project, and eventually the Habitable Worlds Observatory, expected to launch in the early 2040s, all of which are centered around studying the atmospheres of exoplanets. Here we explore a new approach to constructing large scale exoatmospheric survey lists, which combines the use of traditional trans- mission/emission spectroscopy figures of merit with a focus on more-evenly sampling planets across a range of radii and equilibrium temperatures. After assembling a sample target list comprised of 750 transmission spectroscopy targets and 75 emission spectroscopy targets, we quantify the potential time lost to stale transit and eclipse ephemerides finding that hundreds of hours of space-based observing could be wasted given current uncertainties in orbital periods, transit epochs, and orbital eccentric- ity. We further estimate the amount of ground-based telescope time necessary to obtain sufficiently precise exoplanet masses and find that it exceeds 100 nights of 10m telescope time. Based upon these findings, we provide a list of recommendations that would make community efforts for preparation and interpretation of atmospheric characterization endeavors more effective and efficient. The strategies we recommend here, including the target lists we develop, can be used to support both current (e.g., HST and JWST) and future atmospheric spectroscopy missions (e.g., Pandora, Ariel, and the Habitable Worlds Observatory).
DOI: 10.3535/40z-zdh-q1r
title: Porcellionides pruinosus pruinosus (Brandt, 1833)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/whq-0w9-2jf
title: Lernaeocera Blainville, 1822

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.xzzzta
title: The InSight Mars lander’s meteor search

description: Meteor surveys on other planets, such as Mars, can be used to constrain the variation in the meteoroid flux away from Earth. Images from the Spirit rover have previously been used for one such survey. We report on the sampling and results of a new survey conducted with InSight lander images. The InSight survey used cameras with wider fields of view and faster optics than the Spirit survey and comprised 9.7 h of cumulative exposure time, compared to 2.7 h for Spirit. No meteors were identified. We determined that while the InSight survey was more sensitive to bright meteors, it was less sensitive to faint meteors due to compression-related issues. Further, we determined that the Spirit survey was substantially less sensitive than previously reported, and neither survey had sufficient sensitivity to test theoretical expectations given expected detections ≪1. We conclude with recommendations for the design of any future surveys.
DOI: 10.3535/a69-y31-mqq
title: Ligia pallasii Brandt, 1833

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/6rj-6pd-30v
title: Euchaeta acuta Giesbrecht, 1893

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/mq2-0qe-t22
title: Philoscia muscorum muscorum (Scopoli, 1763)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/6c8-5gg-2sc
title: Philoscia muscorum muscorum (Scopoli, 1763)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/xqg-ym2-wmc
title: Paraeuchaeta barbata barbata (Brady, 1883)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.aw6hk8
title: The Discovery of 25 μm Interstellar Methanol

description: We present the first astrophysical detection of methanol (CH3OH) in the torsional band near 25 μm. Using high resolution mid-infrared (MIR) spectroscopy, we identified over seventy gas-phase CH3OH absorption lines between 20 and 28 μm towards the massive protostar NGC 7538 IRS 1 with SOFIA/EXES. We derive a temperature of 180 K and a total column density of 2 × 1017 cm−2, comparable to sub-mm surveys. These MIR absorption lines likely probe the CH3OH in the disk close to the central star, as confirmed by complementary analysis of C2H2. Furthermore, we report the detection of the same 25 μm CH3OH absorption feature in JWST/MIRI archival data towards a massive protostar, five Class 0 and Class I low mass protostars, and eleven protoplanetary disks. The detection of this CH3OH feature through three stages of protostellar evolution suggests that this molecule has been directly inherited from the icy, natal cloud phase. The access to this CH3OH band will enable further exploration of how complex organic molecules could be inherited from the earliest protostellar disks and survive to the central regions of planet forming disks, where future planets will reside. Indeed, this work has nearly tripled the total number of protoplanetary disks with CH3OH detections. We provide an updated line list for the torsional band of CH3OH, which was generated from lab work and computation.
DOI: 10.3535/6zr-rdb-x47
title: Ligia oceanica (Linnaeus, 1767)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/pzf-47k-6b7
title: Notodelphys agilis Thorell, 1859

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.3jdn1i
title: Full Polarimetric GNSS-R Sensitivity Assessment of Ocean Roughness

description: The sensitivity of Global Navigation Satellite System Reflectometry (GNSS-R) to ocean surface roughness is well-established within the scientific and technological communities. Missions like the CYclone GNSS (CYGNSS) have been specifically designed to detect and monitor hurricanes and other oceanic storms. Additionally, data from the Soil Moisture Active Passive (SMAP) mission's radar, operating in receive mode, known as SMAP-Reflectometer or SMAP-R, provide opportunities to evaluate the polarimetric sensitivities of GNSS-R measurements to ocean surface roughness. This enables exploration of potential applications that can be achieved or enhanced through the use of polarimetric techniques. This study provides a sensitivity analysis of wind-driven changes in surface roughness using a comprehensive view of full polarization GNSS-R signals over the ocean. The results show an improvement of ~0.6% on ocean wind speed retrievals for dual polarization GNSS-R missions respect to single polarization GNSS-R missions. The results show an improvement of ~4.5% on ocean wind speed retrievals for full polarization GNSS-R missions respect to single polarization GNSS-R missions.
DOI: 10.3535/pnm-kkq-9vk
title: Lernaeocera branchialis (Linnaeus, 1767)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/z5r-vsy-abq
title: Temora discaudata Giesbrecht, 1889

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/xvj-wh8-b2j
title: Astacilla longicornis (Sowerby, 1806)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/9nm-s8c-92q
title: Apseudes spinosus (M. Sars, 1858)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/k2d-548-lsc
title: Aphiloscia vilis (Budde-Lund, 1885)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/8y3-052-1th
title: Lernaeocera branchialis (Linnaeus, 1767)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/kl5-yw2-80j
title: Temora discaudata Giesbrecht, 1889

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/4bb-yt5-119
title: Telotha henselii (von Martens, 1869)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/lsy-axt-yck
title: Chirundina indica Sewell, 1929

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.o16sw2
title: Predictions of satellite retrieval failures of air quality using machine learning

description: The growing fleet of Earth Observation (EO) satellites is capturing unprecedented quantities of information about the concentration and distribution of trace gases in the Earth’s atmosphere. Depending on the instrument and algorithm, the yield of good remote soundings can be a few percent owing to interferences such as clouds, non-linearities in the retrieval algorithm, and systematic errors in radiative transfer algorithm leading to inefficient use of computational resources. In this study, we investigate Machine Learning (ML) techniques to predict failures in the trace gas retrieval process based upon the input satellite radiances alone allowing for efficient production of good-quality data. We apply this technique to ozone and other retrievals using measurements from two sets of measurements: Suomi National Polar-Orbiting Partnership Cross-Track Infrared Sounder (Suomi NPP CrIS), and joint retrievals from Atmospheric Infrared Sounder (AIRS) - Ozone Monitoring Instrument (OMI). Retrievals are performed using the MUlti-SpEctra, MUlti-SpEcies, Multi-SEnsors (MUSES) algorithm. With this tool, we can identify 80% of ozone retrieval failures using the MUSES algorithm, at a cost of 20% false positives from CrIS. For AIRS-OMI, 98% of ozone retrieval failures are identified, at a cost of 2% false positives. The ML tool is simple to generate and takes &lt;0.1 s to assess each measured spectrum. The results suggest this tool can be applied to many EO satellites, and reduce the processing load for current and future instruments.
DOI: 10.3535/qng-dw2-6jr
title: Trichoniscoides modestus modestus (Racovitza, 1908)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/0q6-exl-c9z
title: Ligia oceanica (Linnaeus, 1767)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/4n6-t6z-vlx
title: Valdiviella insignis Farran, 1908

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/10r-y59-xn4
title: Asellus (Asellus) aquaticus aquaticus Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/2kc-r6y-hhe
title: Ligia oceanica (Linnaeus, 1767)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/v2b-lyk-tkm
title: Lamippula pallida (Zulueta, 1908)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.plm2tj
title: The Science of Entry, Descent, and Landing in the Venus, Jupiter, and Saturn Systems

description: The design of the entry, descent, and landing (EDL) process is meant to bring a hypersonic spacecraft through a planet’s atmosphere and safely onto its surface. When a spacecraft probe visits a planet, such as a gas giant, without a defined surface, the ‘entry’ and ‘descent’ elements of the process that remain are no less critical for mission success. Irrespective of the destination, however, the steps of the EDL process follow the same basic approach. Following an initial period of frictional deceleration during the entry phase, which slows the spacecraft from hypersonic to supersonic speeds, a period of further deceleration on parachute—the descent phase—begins. During the descent phase, the spacecraft is slowed even further, to speeds as low as 10s m/s, at which point the final—landing—phase of EDL may begin. Depending on destination, either active or passive landing measures are employed to bring the spacecraft to a safe touchdown on the surface. With time and experience, EDL has become a reliable process, though it is still not without its challenges. A number of failures in the early years of planetary exploration of Venus by the Soviet Union led to stepwise improvements in spacecraft design, and a corresponding growth in the number of planetary targets for in situ exploration. In many instances, such as for Venus, these early probes were used as test vehicles to characterize a planet’s atmosphere for the very first time—failure was almost assured for these early missions. Slowly, though, acquisition of data from the descent probes allowed for the reconstruction of atmospheric temperature and density profiles, along with wind, composition, and cloud structure. In the outer solar system, new ground was also broken by delivery of atmospheric probes to Jupiter and Titan, offering tantalizing glimpses of the atmospheres beneath their hazy cloud layers, in many cases surprising scientists by revealing compositional or structural elements markedly different than originally believed. These differences will shed light on how these objects formed and evolved. Leveraging the opportunity to use the soon-to-be decommissioned Cassini spacecraft as an atmospheric probe in its own right gave a remarkable data return about the upper atmosphere of Saturn, providing yet another piece of the puzzle of outer planet formation and evolution. The quantity of science returned during the EDL process has greatly improved our understanding of the atmospheres of our planetary neighbors. Blended with numerical models and remote observations, we have been able to construct profiles of many of our planetary neighbors, allowing for the design of new instruments, and new spacecraft to further exploration, while reducing uncertainty about the environment into which the probes will be entering. New spacecraft have a very clear heritage to some of these earliest explorers, and draw upon the lessons learned, and experience gained, in the delivery of spacecraft into a planet’s atmosphere.
DOI: 10.15468/dl.trhy8t
title: Occurrence Download

description: A dataset containing 109 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is Colombia",
 "TaxonKey is Citrullus lanatus (Thunb.) Matsum. & Nakai"
 ]
}

 The dataset includes 109 records from 24 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0104024-250525065834625/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.3535/aq3-8n1-den
title: Caligus elongatus Nordmann, 1832

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/ssw-11b-g3f
title: Chirundina indica Sewell, 1929

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.pvrneg
title: Atmospheric CO2 Ice in the Martian Polar Regions: Physical and Spectral Properties from Mars Climate Sounder Observation

description: CO2 ice clouds are important for the polar energy balance and carbon dioxide cycle on Mars. However, uncertainties remain regarding their physical and radiative properties, which control how polar CO2 clouds interact with the global Martian climate. Here, we use Mars Climate Sounder (MCS) observations of atmospheric radiance to estimate these bulk physical and radiative properties. We find that Martian CO2 clouds are typically composed of large particles from a narrow size distribution with an effective radius of 46 μm and an effective variance of 0.002 in the southern hemisphere, and an effective radius of 42 μm and an effective variance of 0.002 in the north. The similarity in sizes of CO2 ice particles in both hemispheres may be due to the fact that CO2 clouds tend to form near the same pressure level in each hemisphere, despite the higher surface pressures in the north. We use a simplified convective cooling model to show that the narrow effective variance we derive may be a consequence of the fact that CO2 is also the dominant atmospheric constituent on Mars, which allows CO2 ice particles to reach sizes of &gt; 10 μm within seconds. At the same time, the fact that the Martian atmosphere is so thin means that large particles fall rapidly to the surface, reducing the range of particle sizes that can remain in the atmosphere for any extended period of time. This study is part of ongoing work to add CO2 ice opacity profiles to the MCS retrieval pipeline.
DOI: 10.3535/276-91v-9rh
title: Calanus pacificus Brodsky, 1948

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/njw-y69-lvq
title: Senariellus liber (Brady, 1880)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/dpt-fmk-e3p
title: Asellus (Asellus) aquaticus aquaticus Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/gpb-40k-vjf
title: Caligus elongatus Nordmann, 1832

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/58h-5fc-499
title: Caligus curtus Müller O.F., 1785

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.15468/dl.493c32
title: Occurrence Download

description: A dataset containing 121 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is Ecuador",
 "TaxonKey is Myioborus miniatus (Swainson, 1827)",
 "Year 2024-2025"
 ]
}

 The dataset includes 121 records from 3 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0104023-250525065834625/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.3535/c0e-4qr-3sd
title: Candacia falcifera Farran, 1929

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/j2x-z83-5k3
title: Candacia cheirura Cleve, 1904

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.48577/jpl.0nqucm
title: Detection of the Silicate Precursor Silane in a Cold, Low-Metallicity Brown Dwarf

description: Within 20 pc of the Sun there are currently 29 known cold brown dwarfs - sources with measured distances and an estimated effective temperature between that of Jupiter (170K) and∼500K ([1]). These sources are almost all isolated and are the closest laboratories we have for detailed atmo- spheric studies of giant planets formed outside the solar system. Here we report JWST observations of one such source, WISEA J153429.75-104303.3 (W1534), which we confirm is a substellar mass member of the Galactic halo with a metallicity &lt;0.01×solar. Its spectrum reveals methane (CH4), water (H2O), and silane (SiH4) gas. Although SiH4 is expected to serve as a key reservoir for the cloud-forming element Si in gas giant worlds, it eluded detection until now because it is removed from observable atmospheres by the formation of silicate clouds at depth. These condensates are favored with increasing metallicity, explaining why SiH4 remains undetected on well studied, metal-rich solar system worlds like Jupiter and Saturn ([2]). On the metal-poor world W1534, we detect a clear signature of SiH4 cen- tered at∼4.55 µm with an abundance of 19±2 parts per billion (ppb). Our chemical modelling suggests that this SiH4 abundance may be quenched at∼kilobar levels just above the silicate cloud layers, whereupon verti- cal atmospheric mixing can transport SiH4 to the observable photosphere. The formation and detection of SiH4 demonstrates key coupled relation- ships between composition, cloud formation, and atmospheric mixing in cold brown dwarf and planetary atmospheres.
DOI: 10.3535/r2x-wwc-ege
title: Calanus helgolandicus (Claus, 1863)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/ska-9eh-clh
title: Calanus helgolandicus (Claus, 1863)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/6vh-g8p-cdg
title: Euchirella bella Giesbrecht, 1888

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/9j0-4y3-zev
title: Asellus (Asellus) aquaticus aquaticus Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/1pg-q9j-wm6
title: Asellus (Asellus) aquaticus aquaticus Linnaeus, 1758

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/khz-bey-ntc
title: Alloniscus marinus Collinge, 1920

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.