cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.57780/esa-dtvd1y7
title: 093141

description: Following a series of remarkable recent discoveries we now know thatsome of the most luminous members of the ultraluminous X-ray source(ULX) population are actually powered by highly super-Eddington pulsars(i.e. neutron stars) making them the most extreme sustained accretorsknown. Six such systems are now known but NGC5907 ULX1 stands out asthe most luminous peaking at Lx ~ 1e41 erg/s. Here we propose a pair ofsimultaneous NuSTAR+XMM observations of NGC5907 ULX1. These will allowus to continue to track the long-term evolution of the neutron star spinhelp investigate why the pulsations are transient in some ULX pulsars andexplore the nature of the long-term 78d X-ray period present in this system. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-eon4hss
title: 092172

description: While recent studies have expanded our knowledge of dwarf galaxies and the AGNsresiding in them such work has rarely explored populations of pristine(low-metallicity) low-mass dwarfs and mergers and their interactions betweensuch dwarfs.  As such systems represent local analogues of the first galaxies arobust understanding of these targets is required to fully understand the firstbuilding blocks of all galaxies and the seeds from which all SMBHs arise. TheDwarf GIMLI Survey will utilize XMM-Newton to explore the X-ray properties of 10dwarf mergers in order to determine the source of activity suggested by theirmid-IR colors and compare the X-ray properties of this sample with that of acontrol sample of isolated pristine dwarfs. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-fm2qxre
title: 092392

description: Magnetic activity features are often variable and some systems show clearsinusoidal modulations. Such activity cycles can change the stellar X-ray to EUVemission (XUV henceforth) by factors of a few. This also changes the EUVirradiation of orbiting exoplanets. XUV irradiation drives planetary mass-lossand likely shapes the exoplanet population at large. Models predict that XUVirradiation and mass-loss rate are correlated i.e. can be challenged bymeasuring the mass-loss of the same exoplanet during different phases of thehost stars magnetic cycle. The 7 year optical cycle of GJ 436 allows thisexperiment if mirrored in X-rays. Existing X-ray data cover only a very limitedphase space. We propose two new 20 ks observations of GJ 436 to reliably discover the X-ray cycle of GJ 436. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-gzi6ej4
title: 093081

description: We propose to observe the X-ray brightest and one of the firstgamma-ray-detected BAL quasars B3 1520+437 simultaneously with NuSTARand XMM-Newton for exposures 40 ksec and 20 ksec respectively. Theproposed observations will allow us to (i) check whether strong soft X-rayabsorption one of the most prominent characteristics of most BAL quasarsalso exists in the polar outflows and to check whether face-on BAL quasarsare otherwise X-ray normal and (ii) precisely estimate the jet powerlocation of the emission region along the jet bulk Lorentz factor andproperties of the electron energy distribution. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-ix6t4wt
title: 093085

description: We propose contemporaneous NuSTAR and XMM-Newton observations of the recentlyclassified IMXB 4U 1210-64 for 40 ks. Taking advantage of the excellent timingand spectral resolution of NuSTAR we will perform broadband continuumspectroscopy and look for signatures of a NS or BH such as pulsations QPOs andCRSFs. With XMM-Newton we will probe the geometry and ionization structure ofthe accretion flow onto the compact object using the high spectral resolution ofRGS  measure the profile of the Fe Kalpha Fe XXV and Fe XXVI emission lines aswell as search for emission lines of lower Z ions. Our observation of 4U 1210-64holds broader astrophysical r^ance in characterizing the circumstellarenvironment in IMXBs and will be the first observation of 4U1210 with grating resolution. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-jbawuql
title: 092284

description: NGC 7793 P13 is one of the best suited ultra-luminous X-ray pulsars to studysuper-Eddington accretion due to its easly detectable pulsations when it isX-ray bright. In 2020/2021 it was in an off-state and no longer detected bySwift/XRT but continued to spin-up indicating continued high accretion.Currently the source is in an intermediate state clearly detected by Swift/XRTbut below its historically maximum luminosity. In this state continuedmonitoring of the pulse period and spectral evolution is very interesting as itallows us to investigate if there is any change in accretion rate or if allobserved variations are due to geometric effects. We propose to continue oursuccessful campaign to monitor P13 and other sources in NGC 7793 throughout AO 22 with 2x40 ks observations. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-lhg6kmw
title: 092283

description: Previous XMM-Newton observations have led to the detection of AGNs in 2 of 3gravitationally lensed Hyper Luminous Infrared Galaxies (HyLIRGs) with apparentIR luminosities >10^14 L_sun while X-ray emission from the third is consistentwith the prediction from its star formation rate (SFR) according to the localcalibration. We propose observations of 6 more such HyLIRGs at z~2.1-3.3 toobtain a statistically meaningful sample of X-ray detections. This sample willenable us to 1) tighten the relation between non-AGN X-ray emission and SFR 2)probe the presence of AGN over the rest-frame 2-35 keV range and 3) determinethe obscuration of AGNs and their potential impact on these extreme galaxies.The results will have strong implications for understanding the star formation and AGN co-evolution. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-macen54
title: 092084

description: Clusters of galaxies are great objects to study cosmology and astrophysics.There are many cluster samples selected from ICM-based observations (X-ray andSZ). However the ICM-based selections are also ICM-biased e.g. X-rayselections are biased to cool core clusters. The results from these ICM-biasedsample can affect the constraints on the cluster cosmology and baryon physics.We select an optically rich cluster sample from the redMaPPer catalog. We findmost of them that uncovered by modern X-ray telescope are X-ray faint clusters.We request XMM observations for them in order to have a complete and unbiasedview of ICM properties. The results will provide helpful guidance for futuresurveys. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-p9h92du
title: 092165

description: We propose 55 ks of XMM-Newton exposure for an Eddington-limited dust-obscuredgalaxy which may be at a key phase closest to the peak of both the black-holeand galaxy growth in the coevolution framework for supermassive black holes andgalaxies. This source was previously targeted with Chandra for 3 ks and showsheavy obscuration reaching the Compton-thick level yet has an unexpectedly highcount rate in the hard X-ray band. Previous observations of similar sources havebeen highly limited by the collected counts and thus our proposed targetprovides an unprecedentedly economical opportunity to probe detailed X-rayspectral features. The proposed observation will also constrain the precisecolumn density of our source and how ^ated its X-ray luminosity is compared to expectations. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-pp8ye74
title: 093279

description: With the launch of JWST we are finally in a position to determine if terrestrialexoplanets orbiting M dwarfs can develop and retain atmospheres in the presenceof their hosts harsh high-energy environments. Necessary to the interpretationof any planetary atmospheric data is the measured high-energy spectra from theUV to the X-ray of the M dwarf hosts. A JWST Cycle 2 Large program will surveynine rocky worlds orbiting nearby M dwarfs for the presence of atmospheres. OnlyHST can capture the critical UV information which we will supplement with X-rayobservations to provide a complete picture of the high-energy output of these Mdwarf hosts. We request 47 HST orbits to capture the UV spectra of these five Mdwarfs. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-q575peo
title: 092030

description: The galaxy cluster PLCK G165.7+67.0 (z=0.35) is in the top 1 % brightest sourcesin the Planck sky as a result of strong lensing of background star-forminggalaxies at z=2. The mass estimated from the lens model appears inconsistentwith the lack of X-ray detection in the ROSAT/RASS survey but may be explainedby a non-equilibrium state of the cluster as indicated by its bimodal galaxydistribution and extended radio halo as well as the presence of two NarrowAngle Tail (NAT) galaxies. We request a 75ks XMM observation to determine thecluster???s dynamic state which enables us to measure the position of the X-rayhalo(s) and to search for shocks. These complementary capabilities will greatlyaid the interpretation of the upcoming JWST observations of this cluster. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-tekwvsv
title: 092132

description: In the ROSAT all-sky survey we serendipitously discovered an extended (~22x8arcmin) irregular-shaped X-ray diffuse emission located in H-ATLAS GAMA12field. The only nearby galaxy overdensities are two small groups of 3 galaxieseach spectroscopically confirmed at z=0.073 and z=0.11 located at the edge ofthe X-ray emission. In addition an NVSS/FIRST radio-galaxy is located exactlyalong the direction that connects the two brightest spots of the X-ray emissionand is not detected in any optical-to-FIR band. We propose a very cheap XMMobservation (14ks) of the entire X-ray emission that may correspond to arelatively nearby unvirialized large-scale structure thanks to which we willmeasure its redshift disentangle its morphological components and unveil its emission mechanisms. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-w38fba1
title: 092312

description: The recent discovery of a new transiting planet with only 1.4  Rearth orbitinga nearby bright M star offers us the possibility to search for planetatmospheric features in an Earth-like atmosphere. This planet will be among thebest studied in the next years. As the star is part of the CARMENES guaranteedtime observations we have used a wealth of high-resolution spectroscopic dataof the star to determine a mass of 1.9 Earth masses. We intend to observe theplanet host star GJ 806 with XMM-Newton for a total of 15 ks to model thecoronal XUV emission that is arriving to the planet likely producingphotoevaporation. The XUV data are needed for complementing the search forplanet atmospheric features in the optical and near-infrared such as the He I 10830 triplet or H2O molecular lines. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-yjk5g5c
title: 092022

description: The high redshift (z=6.18) quasar CFHQS J142952+544717 shows an extreme X-rayluminosity which is caused by inverse Compton scattering of cosmic Microwavebackground (CMB) photons by the relativistic electrons of the quasars radio jet. As the density of CMB photons increases with increasing redshift such sourcesare more X-ray luminous  at higher redshifts to an amount which compensates foreffects of larger distance i.e. XMM-Newton should be able to detect suchCMB-driven X-ray luminous quasars at any redshift. We aim to measure X-rayluminosities of 24 high redshift (z>5.5) radio-detected quasars with the aim  tocharacterize the luminosity distribution and establishing further evidence forCMB-driven X-ray emission. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-yvhr8mz
title: 095419

description: #1 AT2023lli    #2 AT2024mvz#3 GRB241105A   #4 eRASSt_J032543-45124#5 EP240222a    #6 AT2022upj#8 OGLE16aaa    #9 EP241021a #10 AT 2018cqh  #11 EP250108a#12 AT2024xuo
DOI: 10.57780/esa-z2s5l8n
title: 092268

description: Radio-loud supermassive black holes (SMBHs) at the highest redshifts($zgtrsim6$) are some of the most intriguing targets for early Universe studiesas their radio properties may be the key to understanding early SMBH growth.Until recently however the known population of these objects was small butrecent targeted surveys have dramatically expanded this census. The X-rayproperties of these quasars are fundamentally important as they reveal both theoverall accretion processes in individual quasars and as a population the roleinverse Compton interactions with the CMB play in suppressing radio flux injets. We therefore propose a Fulfil Programme to complete the archive ofReionization-era radio-loud quasars. [truncated! Please see actual data for full text]
DOI: 10.5281/zenodo.14512504
title: Mass Spectrometry Data from Wastewater Ozonation with Internal Standards and QC in Positive and Negative Ionizations and DDA

description: Profile mass spectrometry data from influent and effluent of an ozonation treatment step. Internal standards were spiked to all samples both in positive and negative ionization modes. There are QC samples which were directly injected (only positive ionization) and all the other samples (i.e., QC, influent and effluent) are pre-treated with solid-phase extraction (SPE), so expect matrix suppression. The compounds used for internal standards and QC are given as .cvs files for convenience. Note that not all added compounds are detected due to their properties.

The data was acquired in an Agilent 6560 Ion Mobility QTOF coupled to an Agilent 1260 Infinity III LC. The mobile phase was water and acetonitrile, both with 0.1% formic acid. The gradient profile in %V (acetonitrile) was 0% for 5 minutes with rise to 100% until 18 minutes. 100% was kept until 25 minutes. Equilibration was then performed until 36 minutes but the data acquisition stopped at 30 minutes. The reverse phase column was an Waters XSelect HSS T3 3.5 µm 3x150mm. Data dependent acquisition (DDA) was performed by selecting the 3 most intense ions per cylcle with a lower limit of 5000 counts.
DOI: 10.5281/zenodo.14512505
title: Mass Spectrometry Data from Wastewater Ozonation with Internal Standards and QC in Positive and Negative Ionizations and DDA

description: Profile mass spectrometry data from influent and effluent of an ozonation treatment step. Internal standards were spiked to all samples both in positive and negative ionization modes. There are QC samples which were directly injected (only positive ionization) and all the other samples (i.e., QC, influent and effluent) are pre-treated with solid-phase extraction (SPE), so expect matrix suppression. The compounds used for internal standards and QC are given as .cvs files for convenience. Note that not all added compounds are detected due to their properties.

The data was acquired in an Agilent 6560 Ion Mobility QTOF coupled to an Agilent 1260 Infinity III LC. The mobile phase was water and acetonitrile, both with 0.1% formic acid. The gradient profile in %V (acetonitrile) was 0% for 5 minutes with rise to 100% until 18 minutes. 100% was kept until 25 minutes. Equilibration was then performed until 36 minutes but the data acquisition stopped at 30 minutes. The reverse phase column was an Waters XSelect HSS T3 3.5 µm 3x150mm. Data dependent acquisition (DDA) was performed by selecting the 3 most intense ions per cylcle with a lower limit of 5000 counts.
DOI: 10.5523/bris.3nmqsrbv5ruom2abn0ql6e8yh2
title: Avian Contact Study Questionnaire Data (May - July 2024)

description: Data collected from the Avian Contact Study (https://bristol.ac.uk/avian-contact) questionnaire between 15 May 2024 and 31 July 2024. First data release.
DOI: 10.60797/psy.2025.6.4.1
title: Данные по шкале «Экологическая сознательность» во всей выборке

description: Cifra. Психология, Выпуск 1 (6) 2025
DOI: 10.60797/psy.2025.6.4.2
title: Данные по шкале «Экологическая сознательность» по параллельным классам

description: Cifra. Психология, Выпуск 1 (6) 2025
DOI: 10.60797/psy.2025.6.4.3
title: Динамика по шкале «Экологическая сознательность» в группе участников лонгитюдного наблюдения

description: Cifra. Психология, Выпуск 1 (6) 2025
DOI: 10.5281/zenodo.14761448
title: Mnemiopsis leidyi chromosome-level genome annotation

description: This dataset contains the annotation information for the chromosome-level assembly of the genome of Mnemiopsis leidyi. The annoation was produced using the genome annotator pipline. For further details on the methods used please see the corresponding publication in GBE (doi:10.1093/gbe/evaf006).

The following files are availalable:

mnemiopsis.genome.v3.genome.fasta

The genome scaffolds in fasta format. Note the naming of scaffolds is different from the version deposited at ENA due to the addition of ENA specific IDs. Below files reference the short scaffold names as used in this file.

mnemiopsis.genome.v3.evm.cdna.fasta

Predicted transcribed regions in fasta format.

mnemiopsis.genome.v3.evm.cds.fasta

Preditcted coding sequences in fasta format.

mnemiopsis.genome.v3.evm.proteins.fasta

Translations of the predicted coding regions.

mnemiopsis.genome.v3.evm.gff3

Coordinates of all predicted genes in gff3 format.
DOI: 10.5281/zenodo.14761449
title: Mnemiopsis leidyi chromosome-level genome annotation

description: This dataset contains the annotation information for the chromosome-level assembly of the genome of Mnemiopsis leidyi. The annoation was produced using the genome annotator pipline. For further details on the methods used please see the corresponding publication in GBE (doi:10.1093/gbe/evaf006).

The following files are availalable:

mnemiopsis.genome.v3.genome.fasta

The genome scaffolds in fasta format. Note the naming of scaffolds is different from the version deposited at ENA due to the addition of ENA specific IDs. Below files reference the short scaffold names as used in this file.

mnemiopsis.genome.v3.evm.cdna.fasta

Predicted transcribed regions in fasta format.

mnemiopsis.genome.v3.evm.cds.fasta

Preditcted coding sequences in fasta format.

mnemiopsis.genome.v3.evm.proteins.fasta

Translations of the predicted coding regions.

mnemiopsis.genome.v3.evm.gff3

Coordinates of all predicted genes in gff3 format.
DOI: 10.15468/dl.8am7sm
title: Occurrence Download

description: A dataset containing 863 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Arapaima gigas (Schinz, 1822)"
 ]
}

 The dataset includes 863 records from 77 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0003756-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.bvqdxz
title: Occurrence Download

description: A dataset containing 74175 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Continent is Europe",
 "TaxonKey is Cobitis Linnaeus, 1758"
 ]
}

 The dataset includes 74175 records from 253 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0003755-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5519/qd.jif6rg2n
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (8818 records)
DOI: 10.15468/dl.95ev9u
title: Occurrence Download

description: A dataset containing 8234 species occurrences available in GBIF matching the query:
{
 "and" : [
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "TaxonKey is Pinus banksiana Lamb."
 ]
}

 The dataset includes 8234 records from 187 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0003760-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5519/qd.gs0b9qmw
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1 records)
DOI: 10.6084/m9.figshare.25559628
title: Exploring the Impact of Artificial Intelligence-Mediated Communication on Bias and Information Loss in Non-academic and Academic Writing Contexts (Without Data of Academic Texts)

description: Exploring the Impact of Artificial Intelligence-Mediated Communication on Bias and Information Loss in Non-academic and Academic Writing Contexts (Without Data of Academic Texts)
DOI: 10.6084/m9.figshare.25559628.v2
title: Exploring the Impact of Artificial Intelligence-Mediated Communication on Bias and Information Loss in Non-academic and Academic Writing Contexts (Without Data of Academic Texts)

description: Exploring the Impact of Artificial Intelligence-Mediated Communication on Bias and Information Loss in Non-academic and Academic Writing Contexts (Without Data of Academic Texts)
DOI: 10.6084/m9.figshare.25559628.v1
title: Exploring the Impact of Artificial Intelligence-Mediated Communication on Bias and Information Loss in Non-academic and Academic Writing Contexts (Without Data of Academic Texts)

description: Exploring the Impact of Artificial Intelligence-Mediated Communication on Bias and Information Loss in Non-academic and Academic Writing Contexts (Without Data of Academic Texts)
DOI: 10.6084/m9.figshare.28300685
title: <b>In-Situ Observation on the Influence of Internal Waves on Deep-Sea Sand Ripple Evolution in the Dongsha Region of the South China Sea</b>

description: The data used in this study were collected through field observations carried out in the Dongsha region of the South China Sea from August 16 to August 31 (~16 days). An in-situ observation quadripod for bottom boundary layer in abyssal sea developed by the our research team was deployed at the site (117°31E, 21°12N), with a water depth of approximately 720 m, to observe the hydrodynamics and sand ripples. The observation quadripod was instrumented with a 75 kHz Acoustic Doppler Current Profiler (ADCP), a 6 MHz Acoustic Doppler Velocimeter (ADV), a high-precision pressure sensor, and a deep-sea camera.
DOI: 10.15468/dl.wrcpbq
title: Occurrence Download

description: A dataset containing 8442 species occurrences available in GBIF matching the query:
{
 "ScientificName" : [
 "is Stictocephala bisonia Kopp & Yonke, 1977"
 ]
}

 The dataset includes 8442 records from 383 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0003764-250127130748423/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.34740/kaggle/dsv/12238257
title: Peer-to-Peer Boliviano (BOB) Exchange Data
DOI: 10.15468/dl.uxwmap
title: Occurrence Download

description: A dataset containing 0 species occurrences available in GBIF matching the query:
{
 "and" : [
 "TaxonKey is Nitzschia etoshensis Cholnoky, 1966",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "BasisOfRecord is one of (Specimen, Living Specimen, Observation, Human Observation, Machine Observation, Material sample, Literature Occurrence, Material citation, Occurrence evidence)",
 "Geometry POLYGON ((27.1586 -33.5889,28.2048 -32.9007,25.5395 -32.9007,25.5395 -34.1098,25.6468 -34.1222,25.7787 -34.0734,25.7098 -33.9109,25.8639 -33.797,26.4806 -33.8473,27.1586 -33.5889))"
 ]
}

 The dataset includes 0 records from 0 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0061748-250525065834625/datasets/export for details.
DOI: 10.15468/dl.46ndaw
title: Occurrence Download

description: A dataset containing 13481554 species occurrences available in GBIF matching the query:
{
 "Country" : [
 "is Austria"
 ]
}

 The dataset includes 13481554 records from 1606 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0061738-250525065834625/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.