cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15468/dl.f8vdwz
title: Occurrence Download

description: A dataset containing 204 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Buteo buteo japonicus (Linnaeus, 1758)"
 ]
}

 The dataset includes 204 records from 22 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0037424-240229165702484/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48577/jpl.hm8pna
title: CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A

description: The mass distribution of dense cores is a potential key to understand the process of star formation. Applying dendrogram analysis to the CARMA-NRO Orion C18O (J=1{0) data, we identify 2342 dense cores, about 22 % of which have virial ratios smaller than 2, and can be classi ed as gravitationally bound cores. The derived core mass function (CMF) for bound starless cores which are not associated with protostars has a slope similar to Salpeter's initial mass function (IMF) for the mass range above1 M⊙, with a peak at   0.1 M⊙. We divide the cloud into four parts based on the declination, OMC- 1/2/3, OMC-4/5, L1641N/V380 Ori, and L1641C, and derive the CMFs in these regions. We find that starless cores with masses greater than 10 M⊙ exist only in OMC-1/2/3, whereas the CMFs in OMC-4/5, L1641N, and L1641C are truncated at around 5{10 M⊙. From the number ratio of bound starless cores and Class II objects in each subregion, the lifetime of bound starless cores is estimatedto be 5{30 free-fall times, consistent with previous studies for other regions. In addition, we discuss core growth by mass accretion from the surrounding cloud material to explain the coincidence of peak masses between IMFs and CMFs. The mass accretion rate required for doubling the core mass within a core lifetime is larger than that of Bondi-Hoyle accretion by a factor of order 2. This implies that more dynamical accretion processes are required to grow cores.
DOI: 10.15468/dl.hmsy84
title: Occurrence Download

description: A dataset containing 49162 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Pteridaceae",
 "Country is Brazil"
 ]
}

 The dataset includes 49162 records from 155 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0001524-170627171947987/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25549/independent-c69-44761
title: Attorney notes, 1991 Apr.-June

description: Collection of handwritten attorney notes, some with attached business cards (Sol Bernstein, Thomas W. Lorenzen, Charles M. Naumer, Philip A. Henning Jr.), with Los Angeles Police Department complaint database reports, phone message, 1991 April-June. PART OF A SERIES: The series relates to the work product of Sibley & Austin, whose staff contributed to the Commission's probe of excessive force allegations brought against the LAPD. Included in the series are memoranda, witness testimonies, interview summaries, copies of officers' background files, after-action summaries and reports, and notes taken by the firm. Materials relate to four major areas of study undertaken by the firm: the Justice for Janitors labor demonstration of 1990, the jail ward of County/USC Medical Center, Los Angeles city jails, and a review of the LAPD's Background Investigation Unit.
DOI: 10.48577/jpl.vkc4tg
title: Summary of the 51st U.S./Japan ASTER Science Team Meeting

description: The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) team organized a 3-day Science Team Workshop, held at Japan Space System’s (JSS) offices in Tokyo, Japan, on November 7-9. The meeting was attended by over 40 participants from Japan and the U.S, some of whom are shown in Figure 1 below. From the U.S., participants were from NASA/Jet Propulsion Laboratory (JPL), Goddard Space Flight Center (GSFC), NASA’s Land Processes Distributed Active Archive Center (LPDAAC), University of Arizona (UA), and University of Pittsburgh (UP). From Japan, participants were from Japan Space Systems (JSS), Ibaraki University (IU), Nagoya University (NU), University of Tokyo (UT), Tohoku University (TU), National Institute of Advanced Industrial Science and Technology (AIST), and University of Tsukuba (UT). The main objectives of this meeting were to discuss mission status, data products, science team projects, data calibration, validation, distribution, applications and end-of-mission plans. Another topic of immediate concern was NASA Headquarter’s recent Request For Information (RFI) for new science from drifting orbits of Terra, Aqua, and Aura; and the associated previous week’s workshop where each instrument team discussed the appropriate submissions with their constituency, and sought additional ideas for new science. With the 2023 Senior Review approaching, HQ has some important decisions to make regarding future funding for Terra, Aqua, and Aura.
DOI: 10.48577/jpl.az3qzd
title: Comparison of Antarctic iceberg observations by Cook in 1772-75, Halley in 1700, Bouvet in 1739, and Riou in 1789 with modern data

description: During Cook's 1772-75 Antarctic circumnavigation on the HMS Resolution, he recorded the positions of hundreds of icebergs. This paper compares Cook's observations and those of Halley in 1700, Bouvet in 1739, and Riou in 1789, with the Brigham Young University/National Ice Center (BYU/NIC) and the Alfred Wegener Institute data sets. Cook’s description of the iceberg plume east of the Amery Ice Shelf and the iceberg distributions in the Weddell, Ross and Amundsen Seas agree with modern data. In January 1774, Cook reached his farthest south on the shelf of the Amundsen Sea Embayment, the site of the current International Thwaites Glacier Collaboration field study. Cook’s largest iceberg had a 2.5-km diameter, where power-law models show that icebergs of this size or smaller comprise 92% of their total number. In the eastern Weddell, Cook’s observation of a sea-ice tongue with a much greater extent than in satellite imagery remains unexplained. Although Riou's icebergs lie 1000 km east of the BYU/NIC trajectories, application of the England and others (2020) fracture and drift model to the trajectories removes the discrepancy and means that all the ship observations are consistent with modern observations and theory.
DOI: 10.48577/jpl.r9a1ex
title: Assessing non-linear models for galaxy clustering II: model selection and forecsts for Stage IV surveys

description: Accurate modelling of non-linear scales in galaxy clustering will be crucial for data analysis of Stage IV galaxy surveys. A selection of competing non-linear models must be made based on validation studies. We provide a comprehensive set of forecasts of two different models for the halo redshift space power spectrum, namely the commonly applied TNS model and an effective field theory of large scale structure (EFTofLSS) inspired model. Using simulation data and a least-2 analysis,we determine ranges of validity for the models.We then conduct an exploratory Fisher analysis using the full anisotropic power spectrum to investigate parameter degeneracies.We proceed to perform an MCMC analysis utilising the monopole, quadrupole, and hexadecapole spectra, with a restricted range of scales for the latter in order to avoid biasing our growth rate, f , constraint.We find that the TNS model with a Lorentzian damping and standard Eulerian perturbative modelling outperforms other variants of the TNS model. Our MCMC analysis finds that the EFTofLSS-based model may provide tighter marginalised constraints on f at z = 0:5 and z = 1 than the TNS model, despite having additional nuisance parameters. However this depends on the range of scales used as well as the fiducial values and priors on the EFT nuisance parameters. Finally, we extend previous work to provide a consistent comparison between the Fisher matrix and MCMC forecasts using the multipole expansion formalism, and find good agreement between them.
DOI: 10.15468/dl.gvw559
title: Occurrence Download

description: A dataset containing 1 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Dendrobium praetermissum Seidenf."
 ]
}

 The dataset includes 1 records from 1 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0170025-230224095556074/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25549/independent-c69-46238
title: Reports (1-2 of 3) - A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988-11-18

description: Report: A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988 November 18.
DOI: 10.48577/jpl.4tdqpa
title: Tri-band receivers for the INAF radio telescopes: from procurement to acceptance tests

description: In less than 30 months, three different tri-band receivers have been developed for the three Italian radio telescopes. The receivers allow simultaneous observation of three different frequency bands: 18-26 GHz, 34-50 GHz and 80- 116 GHz. Each receiver delivers at its output ports a total of 112 GHz bandwidth in two polarizations. The receivers have been designed, fabricated and tested in KASI laboratories and will be mounted in the secondary foci of the INAF radio telescopes as soon as several upgrades to the infrastructures are completed.
DOI: 10.15468/dl.2gqtev
title: Occurrence Download

description: A dataset containing 21206 species occurrences available in GBIF matching the query:
{
 "and" : [
 "HasCoordinate is true",
 "TaxonKey is Amazilia rutila (Delattre, 1843)",
 "HasGeospatialIssue is false"
 ]
}

 The dataset includes 21206 records from 44 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0001524-170822121629195/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.25549/independent-c69-46241
title: Reports (1-2 of 3) - A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988-11-18

description: Report: A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988 November 18.
DOI: 10.48577/jpl.cmgcl8
title: Equilibrium Tidal Response of Jupiter: Detectability by Juno spacecraft

description: No abstract available.
DOI: 10.48577/jpl.e56nmc
title: THE NuSTAR EXTRAGALACTIC SURVEYS: X-RAY SPECTROSCOPIC ANALYSIS OF THE BRIGHT HARD-BAND SELECTED SAMPLE

description: We discuss the spectral analysis of a sample of 63 Active Galactic Nuclei (AGN) detected above a limiting ux of S(8 􀀀 24keV) = 7 10􀀀14 erg s􀀀1 cm􀀀2 in the multi-tiered NuSTAR Extragalactic Survey program. The sources span a redshift range z = 0􀀀2:1, and have a median redshift ⟨z⟩ = 0:58. The spectral analysis is performed in the broad-band energy range 0.5-24 keV, combining NuSTAR with Chandra and/or XMM-Newton data. As such this constitutes the largest sample of AGN se- lected at &gt; 10 keV to be homogeneously spectrally analyzed at such deep ux levels. Both empirical and physically motivated models are employed to account for the spectral complexity exhibited by the sources. We study the distribution of spectral parameters such as photon index, column density (NH) and re ection parameter, as well as both the unabsorbed and intrinsic coronal 10-40 keV lu- minosities. Heavily obscured (log[NH=cm􀀀2] 23) and Compton Thick (CT; log[NH=cm􀀀2] 24) AGN constitute 30% (19 sources) and 3% (2 sources) of the sample, respectively. The observed NH distribution is in fair agreement with predictions of Cosmic X-ray Background (CXB) popula- tion synthesis models. Properly accounting for the missed fraction of highly obscured AGN in a ux selected sample, we derive the intrinsic NH distribution. The intrinsic CT fraction relative to the total AGN population, is in the range 13-67%. The fraction of obscured and heavily obscured AGN {log(NH=cm􀀀2) 22 and log(NH=cm􀀀2) 23, respectively { show moderate anticorrelations with lu- minosity. These fractions are larger than the fractions of obscured and heavily obscured local (z &lt; 0:1) AGN. Despite the small sample size in relation to the large range in luminosity and redshift probed, this suggests a qualitative agreement with scenarios invoking two different AGN accretion modes.
DOI: 10.15468/dl.ug5yx4
title: Occurrence Download

description: A dataset containing 2979 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Choerodon fasciatus (Günther, 1867)"
 ]
}

 The dataset includes 2979 records from 65 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0049828-231120084113126/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48577/jpl.sxtvyz
title: Common Envelope Mass Ejection in Evolved Stars: Modeling the Dust Emission from post-RGB stars in the LMC

description: Common Envelope (CE) systems are the result of Roche lobe overflow in interacting binaries. Thesubsequent evolution of the CE, its ejection and the formation of dust in its ejecta while the primary is on the Red Giant Branch (RGB), gives rise to a recently identified evolutionary class – dusty post-RGBstars. Their spectral energy distributions (SEDs) suggest that their mass-ejecta are similar to dusty post-Asymptotic Giant Branch (post-AGB) stars. We have modeled the SEDs of a select sample of post-RGB and post-AGB stars in the Large Magellanic Cloud (LMC), quantified the total dust mass (and gas mass assuming gas-to-dust ratio) in the disks and shells and set constraints on the dust grain compositions and sizes. We find that the shell masses in the post-RGBs are generally less than those in post-AGBs, with the caveat that substantial amount of mass in both types of objects may lie in cold, extended shells. Our models suggest that circumstellar disks, when present, are geometrically thick structures with a substantial opening angle, consistent with numerical simulations of CE evolution(CEE). Comparison of our model dust masses with the predictions of dust production during CEE on the RGB suggest that CEE occurred near or at the tip of the RGB for our post-RGB sources. A surprising result is that some post-RGB stars harbor carbon-rich dust, believed to form when C/O &gt; 1, e.g. following triple-alpha nucleosynthesis and third dredge-up events in AGB stars. This anomalystrengthens the hypothesis that dusty post-RGBs are born in binary systems.
DOI: 10.25549/independent-c69-46340
title: Reports (1-2 of 3) - A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988-11-18

description: Report: A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988 November 18.
DOI: 10.48577/jpl.o8yuod
title: Distribution of Water Vapor in Molecular Clouds. II

description: No abstract available.
DOI: 10.15468/dl.fm5cwm
title: Occurrence Download

description: A dataset containing 1512 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Crypturellus cinereus (J.F.Gmelin, 1789)"
 ]
}

 The dataset includes 1512 records from 26 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0001525-150204170955391/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48577/jpl.hdyoui
title: Satellite Observations of the Tropical Terrestrial Carbon Balance and Interactions with the Water Cycle During the 21st Century

description: A constellation of satellites are now in orbit providing information about terrestrial carbon and water storage and fluxes. These combined observations show that the tropical biosphere has changed significantly in the last two decades from the combined effects of climate variability and land use. Large areas of forest have been cleared in both wet and dry forests, increasing the source of carbon to the atmosphere. Concomitantly, tropical fire emissions have declined, at least until 2016, from changes in land-use practices and rainfall, increasing the net carbon sink. Measurements of carbon stocks and fluxes from disturbance and recovery and of vegetation photosynthesis show significant regional variability of net biosphere exchange (NBE) and gross primary productivity (GPP) across the tropics and are tied to seasonal and interannual changes in water fluxes and storage. Comparison of satellite based estimates of evapotranspiration (ET), photosynthesis, and the deuterium content of water vapor with patterns of total water storage and rainfall demonstrate the presence of vegetation-atmosphere interactions and feedback mechanisms across tropical forests. However, these observations of stocks, fluxes and inferred interactions between them do not point unambiguously to either positive or negative feedbacks in carbon and water exchanges. These ambiguities highlight the need for assimilation of these new measurements with Earth System models for a consistent assessment of process interactions, along with focused field campaigns that integrate ground, aircraft and satellite measurements, to quantify the controlling carbon and water processes and their feedback mechanisms.
DOI: 10.25549/independent-c69-46337
title: Reports (1-2 of 3) - A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988-11-18

description: Report: A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988 November 18.
DOI: 10.48577/jpl.9vmaho
title: An Iwasawa-Taniguchi Effect for Compton-thick Active Galactic Nuclei

description: Here we present the first study of an Iwasawa-Taniguchi/‘X-ray Baldwin’ e↵ect forCompton-thick active galactic nuclei (AGN). We report a statistically significant anticorrelationbetween the rest-frame equivalent width (EW) of the narrow core of theneutral FeK↵ fluorescence emission line, ubiquitously observed in the reflection spectraof obscured AGN, and the mid-infrared 12 μm continuum luminosity (taken as aproxy for the bolometric AGN luminosity). Our sample consists of 68 Compton-thickAGN selected from pointed and deep-field observations covering a redshift range ofz ⇠ 0.0014 − 3.7. We employ a Monte Carlo-based fitting method, which returns aSpearman’s Rank correlation coefficient of ⇢ = −0.26 +0.11−0.13, significant to 98% confidence.The best fit found is log(EWFeK↵) / −0.10+0.04−0.04 log(L12 μm), which is consistentwith multiple studies of the X-ray Baldwin e↵ect for unobscured to mildly obscuredAGN. This is an unexpected result, as the FeK↵ line is conventionally thought tooriginate from the same region as the underlying reflection continuum, which togethermake up the reflection spectrum. Our result potentially decouples the neutral FeK↵line from the ‘composite’ reflection spectrum for Compton-thick AGN. We discuss furtherimplications this could have if confirmed on larger samples, including a systematicunder-estimation of the X-ray obscuration column density along the line of sight andhence the intrinsic luminosities and growth rates for the most infrared-luminous AGN.
DOI: 10.15468/dl.6zz5ew
title: Occurrence Download

description: A dataset listing the 88 species recorded in GBIF matching the query:
{
 "and" : [
 "Country is Mexico",
 "TaxonKey is Photinus Laporte, 1833"
 ]
}

 The dataset's 88 records were derived from 18 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0049806-231120084113126/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48577/jpl.r5tmkk
title: The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

description: The Effective Field Theory of Large-Scale Structure is a formalism that allows us to predict the clustering of Cosmological Large-Scale Structure in the mildly non-linear regime in an accurate and reliable way. After validating our technique against several sets of numerical simulations, we perform the analysis for the cosmological parameters of the DR12 BOSS data. We assume ΛCDM, a fixed value of the baryon/dark-matter ratio, Ωb/Ωc, and of the tilt of the primordial power spectrum, ns, and no significant input from numerical simulations. By using the one-loop power spectrum multipoles, we measure the primordial amplitude of the power spectrum, As, the abundance of matter, Ωm, and the Hubble parameter, H0, to about 13%, 3.2% and 3.2% respectively, obtaining ln(1010As) = 2.72 ± 0.13, Ωm = 0.309 ± 0.010, H0 = 68.5 ± 2.2 km/(s Mpc) at 68% confidence level. If we then add a CMB prior on the sound horizon, the error bar on H0 is reduced to 1.6%. These results are a substantial qualitative and quantitative improvement with respect to former analyses, and suggest that the EFTofLSS is a powerful instrument to extract cosmological information from Large-Scale Structure.
DOI: 10.15468/dl.q69jer
title: Occurrence Download

description: A dataset containing 185 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Asplenium dentatum L.",
 "HasGeospatialIssue is false",
 "HasCoordinate is true"
 ]
}

 The dataset includes 185 records from 11 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0001525-150316153013904/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48577/jpl.kaczvl
title: Observational Constraints on the Submesoscale Sea Surface Height Variance of Balanced Motion

description: A combination of in situ and remotely sensed observations are used to constrain the imprint of submesoscale turbulence in the sea surface height (SSH) field. The distribution of SSH variance across frequencies and wavenumbers is estimated by comparing an empirical model spectrum to two sets of observations. First, submesoscale SSH variance is constrained using a pair of GPS buoys spaced at about 10 km. From these data, one can estimate frequency spectra not only of SSH variance but also of the variance in the SSH difference between the buoys. The ratio between these two spectral estimates is sensitive to how much SSH variance is present in the submesoscale range and thus constrains the spectral roll-off of SSH variance in wavenumber space. Second, a combination of moored current meters and nadir altimetry is used to obtain an independent constraint. This constraint is enabled by geostrophy and the non-separability of the wavenumber–frequency spectrum of SSH variance revealed by the GPS data. The frequency spectra of kinetic energy and SSH variance follow different power laws, and the difference constrains the spectral content in wavenumber space, allowing for a constraint without the need to actually resolve the submesoscales in space. In all four locations studied, spanning the mid-latitude and subtropical ocean, these constraints indicate that the wavenumber spectral roll-off of submesoscale SSH variance is between about 𝑘−4 and 𝑘−5, where 𝑘 is the wavenumber. These estimates are consistent with previous observations, model results, and theoretical predictions. They provide for a strong prior for the interpretation of upcoming high-resolution satellite data.
DOI: 10.15468/dl.7mdq47
title: Occurrence Download

description: A dataset containing 0 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Dendrobium polyphyllum Schltr."
 ]
}

 The dataset includes 0 records from 0 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0170015-230224095556074/datasets/export for details.
DOI: 10.25549/independent-c69-46224
title: Reports (1-2 of 3) - A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988-11-18

description: Report: A review of administrative processes of the Tampa Police Department by the Police Foundation, 1988 November 18.