cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.57756/8m2a7x
title: LA-ICP-MS data from specimens NHMW-MIN-O1967 and O1969

description: <p>Laser Ablation – Inductively Coupled Plasma – Mass Spectrometry data from the meteorite samples NHMW-MIN-O1967 and O1969. Method and experimental conditions are provided in the related paper (Pittarello et al., submitted) and included in the data file.</p>
DOI: 10.57756/deu7jy
title: EMPA analysis of specimens NHMW-MIN-O1966 and O1968

description: <p>Electron microscope data of spot analysis of the major phases in the investigated samples.</p>
DOI: 10.57745/1m6s2d
title: Corpus_Expert_Links.tab

description: Ensemble des liens vers les documents du corpus thématique expert - Links to the documents of the expert thematic corpus
DOI: 10.57745/alcqve
title: Corpus_Manually_Annotated.zip

description: Zip des documents du corpus après pré-traitement et annotation manuelle (données d'entrée du processus de segmentation automatique) - Zip of the corpus documents after pre-processing and annotation
DOI: 10.57745/n3umhq
title: Corpus_Extracted_Segments.zip

description: Zip de 10 fichiers, au format texte, issus du processus de segmentation automatique avec les labels associés selon les 4 classes - Zip of 10 files, in text format, resulting from the automatic segmentation process with the associated labels according to the 4 classes (Verifiable, Non-verifiable, Informative and Not pertinent)
DOI: 10.57745/cd6unm
title: Read_Me.pdf

description: Annotation protocol with the definition of the terms used (segments, rules)
DOI: 10.57745/jzfmlu
title: Corpus_Extracted_Segments.zip

description: Zip de 10 fichiers, au format texte, issus du processus de segmentation automatique avec les labels associés selon les 4 classes - Zip of 10 files, in text format, resulting from the automatic segmentation process with the associated labels according to the 4 classes (Verifiable, Non-verifiable, Informative and Not pertinent)
DOI: 10.57745/kt6jab
title: Lisez_Moi.pdf

description: Protocole d’annotation avec la définition des différents termes employés (segments, règles)
DOI: 10.25403/upresearchdata.21960008
title: Task-based language teaching (TBLT) approach for language skills improvement

description: The dataset comprises data used to evaluate the effectiveness of task-based language teaching approach to improve the language skills of mature students. The study was a quasi-experimental study with a convergent parallel mixed method design. The data include a pretest and posttest in reading, writing and speaking. It also includes a pre-and post-intervention questionnaire, observational checksheets with graphs and a post-intervention interview summary.
DOI: 10.25403/upresearchdata.21960008.v1
title: Task-based language teaching (TBLT) approach for language skills improvement

description: The dataset comprises data used to evaluate the effectiveness of task-based language teaching approach to improve the language skills of mature students. The study was a quasi-experimental study with a convergent parallel mixed method design. The data include a pretest and posttest in reading, writing and speaking. It also includes a pre-and post-intervention questionnaire, observational checksheets with graphs and a post-intervention interview summary.
DOI: 10.5281/zenodo.7805150
title: Il torrente Parma nelle carte della Raccolta di Mappe e Disegni dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nelle carte della<em> Raccolta di Mappe e Disegni </em> dell'Archivio di Stato di Parma
DOI: 10.5281/zenodo.7805149
title: Il torrente Parma nelle carte della Raccolta di Mappe e Disegni dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nelle carte della<em> Raccolta di Mappe e Disegni </em> dell'Archivio di Stato di Parma
DOI: 10.5281/zenodo.7805141
title: Il torrente Parma nelle carte della Congregazione dei Cavamenti, serie Ponti e Strade dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nel fondo archivistico <em>Congregazione dei Cavamenti, </em>serie<em> Ponti e Strade </em> dell'Archivio di Stato di Parma
DOI: 10.5281/zenodo.7805140
title: Il torrente Parma nelle carte della Congregazione dei Cavamenti, serie Ponti e Strade dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nel fondo archivistico <em>Congregazione dei Cavamenti, </em>serie<em> Ponti e Strade </em> dell'Archivio di Stato di Parma
DOI: 10.34740/kaggle/dsv/5475798
title: AutoXGB
DOI: 10.5281/zenodo.7805126
title: Il torrente Parma nelle carte della Congregazione dei Cavamenti, serie Memoriali dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nel fondo archivistico <em>Congregazione dei Cavamenti, </em>serie<em> Memoriali </em> dell'Archivio di Stato di Parma
DOI: 10.5281/zenodo.7805125
title: Il torrente Parma nelle carte della Congregazione dei Cavamenti, serie Memoriali dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nel fondo archivistico <em>Congregazione dei Cavamenti, </em>serie<em> Memoriali </em> dell'Archivio di Stato di Parma
DOI: 10.57780/esa-00j8vop
title: 089069

description: The proposed observation of seven obscured AGN are necessary to obtain a complete and uniform coverage of the X-ray emission for the sample of Seyfert-2 galaxies from the 12micron galaxy sample openPar12MGSclosePar. Coupled with the broad-band X-ray observations available for the remaining 12MGS AGN comma  the proposed observations will allow us to investigate the column density distribution at low redshift for a complete and unbiased AGN sample openParbecause of its mid-IR selectionclosePar and to connect the accretion properties to those of the hosts by exploiting the unique multi-band characterization and coverage of the proposed sample.
DOI: 10.57780/esa-03gt22w
title: 085258

description: A 2001 XMM spectrum of radio-loud AGN 3C 223 revealed that the line-of-sight column density is significantly different from the average global column density. Two qualities make 3C 223 remarkabledoublePoint the implied obscuration geometry is a Compton-thick openPar>1.7 x 10elev24 cmelev-2closePar ring of gas embedded in a global Compon-thin openPar1.4 x 10elev23 cmelev-2closePar medium comma  and it is one of the very few radio loud Compton-thick AGN candidates known.
DOI: 10.57780/esa-0auwz64
title: 088191

description: IDCS J1426.5+3508 is arguably the most massive comma  very high redshift virialized cluster comma  with many galaxy redshifts comma  our strong and weak lensing data comma  our strong SZ detections comma  and a large X-ray flux from our Chandra observation. We propose a 194 ks observation to measure the global temperature and temperature profile comma  determine the metallicity comma  derive Y_X comma  find the density comma  pressure comma  and entropy profiles comma  and determine if this is a cool core or merging cluster. The pressure profile will be compared to our MUSTANG2 high resolution openPar9.closePar SZ image comma  providing a test for clumping. The abundance will test chemical evolution models for cluster galaxies given the early epoch. Even one high z comma  high mass relaxed cluster with an accurate mass can constrain LambdaCDM and non-gaussianity.
DOI: 10.57780/esa-0e0gl1x
title: 087080

description: Broadband X-ray spectra of polars and intermediate polars consist of multitemperature thermal plasma component comma its reflection from white dwarf  and  6.4 keV Fe fluorescence emission line. We propose simultaneous NuSTAR-XMM observation of CD Ind openParan asynchronous polarclosePar and Paloma openPara special IP evolving from IP to polarclosePar for the first time to robustly detect the reflection hump and resolve the 6.4 keV Fe fluorescence line. These observations will help us in having an idea of the geometry of accretion process. Also comma  we will determine the shock temperature to estimate the mass of WD and perform emission line spectroscopy to determine the temperature and density profile of the post-shock region.
DOI: 10.57780/esa-0epxgxl
title: 086037

description: V630 Cas is one of several long-period cataclysmic variables with rare comma  long-duration comma  dwarf nova outbursts. The characteristics of these outbursts are likely shaped by the large physical size of the accretion disks. Moreover comma  they often are luminous openPar> 10e33 ergs-sclosePar X-ray sources in quiescence comma  severely challenging the disk instability model. Here we propose an XMM-Newton observation of V630 Cas in quiescence to constrain the white dwarf mass and the accretion rate comma  possibly adding it to the list of troubling systems with a high accretion rate white dwarf with a large comma  quiescent accretion disk. We also propose to obtain fast UV photometry with the OM comma  since UV flickering is a key diagnostic of accretion for the related class of symbiotic stars.
DOI: 10.57780/esa-0g0qm1m
title: 084180

description: The mechanism of launching and powering relativistic jets in AGN is still not understood comma  but must link to the accretion flow. Evidence for this comes from the clear change in blazar jet properties at L-LEddvirgul0.01 comma  probably due to the accretion flow transition from a geometrically thick ADAF to a thin disc. There should be another transition at L-LEdd > 1 comma  where the accretion disc should puff up comma  but this is harder to study as few radio-loud AGN are super-Eddington. RX J0134.2-4258 is a robust super-Eddington NLS1 with L-LEddvirgul11 comma  the highest of all radio-loud AGN known. Therefore comma  we propose a joint XMM-Newton-NuSTAR program to study the accretion disc comma  corona and jet mechanism in this new radio-loud super-Eddington regime.
DOI: 10.57780/esa-0ofahe6
title: 086427

description: With the increase in sensitivity and resolution of the radio observations comma  in some late-type galaxies the so-called ..magnetic arms. have been detected in the interarm regions. Such magnetic arms are places of high ordering of the magnetic field. In We.zgowiec et al. openPar2016 comma  AA comma  585 comma  A3closePar comma  we presented that the strongly polarized radio emission comma  as well as a slight increase in the temperature of the hot gas in the areas of the magnetic arms of NGC comma 6946 may be caused by the magnetic reconnection processes. To further investigate this phenomenon we selected a sample of galaxies that show the magnetic arms and allow a detailed spectral analysis of the X-ray emission. The most exceptional among these galaxies is NGC comma 628 comma  with by far the lowest rotation velocity.
DOI: 10.57780/esa-0s00dhu
title: 084276

description: X-ray reverberation shows that the corona is compact comma  within 10 gravitational radii of the central black hole comma  and irradiates a disc that extends down to or near the ISCO. However comma  these results appear in tension with recent Swift disc reverberation results comma  where the time delay between X-rays and UV-optical is much larger than expected from the standard reprocessing model in which a compact corona irradiates and thermalizes a thin accretion disc. In order to explain these disc reverberation results comma  two suggestions have been madedoublePoint either openPar1closePar the thin disc is truncated with a hot inner flow or openPar2closePar absorption and scattering from the broad line region affect the time lag measurements. Neither of these two scenarios can be properly tested with Swift alone. XMM-Newton is required.
DOI: 10.57780/esa-0t9slb0
title: 088086

description: We propose an X-ray survey of six nearby polluted white dwarfs to detect high-rate accretion states indicated by both optical data and recent theoretical models of collisional cascades within their debris disks. The models predict that the collisionally generated gas will be subject to high and low states of accretion comma  where the fraction of time spent in the high and detectable states constrains the size of bodies initiating the cascade. The proposed observations will directly test these models comma  and thus provide valuable information on the nature of the openParas yet unseenclosePar parent bodies themselves. Only with X-ray observations can we directly detect ongoing accretion comma  and provide an invaluable and independent determination of mass accretion rates.
DOI: 10.57780/esa-199lyjw
title: 089242

description: As the largest and most energetic single objects in the Universe comma  giant radio galaxies openParGRGsclosePar comma  are of particular interest as they are less common but extreme examples of radio source evolution. No unified model has emerged to explain the properties of this extreme class of radio galaxies. Previous studies of GRGs are mostly at radio and optical bands comma  and there is a lack of systematic study of GRGs in X-rays. As the energetic radio jets of GRGs extend outwards comma  they interact with the surrounding medium. We select a complete sample of nearby GRGs and propose new XMM observations to complete the X-ray coverage of the sample to study the X-ray properties of GRGs and their environments comma  which helps to understand the processes responsible for the formation and evolution of GRGs.
DOI: 10.57780/esa-1al1z7t
title: 085220

description: NGC 1194 is one of the hardest AGN in the local sky and a rare example of a nearby Compton-thick Seyfert galaxy. This AGN houses a water maser comma  providing an intriguing possible origin for the Compton-thick gas. We request a joint 60 ks NuSTAR-XMM observation to build a model for this spectacular AGN. Availability of an accurate black hole mass and maser disk inclination give a solid framework of scale-size comma  Eddington ratio and orientation for interpretation of the X-ray data.
DOI: 10.57780/esa-1jlsvja
title: 088510

description: In the past decade comma  nearby dwarf galaxies have emerged as exciting observational laboratories for studying the still-mysterious origin of supermassive black holes in the early Universe and their impact on galaxies. This proposal aims for a 50 ks XMM-Newton program to obtain a deep X-ray spectrum of a recently discovered openParand heretefore uniqueclosePar candidate Compton-thick AGN in the nucleus of the nearby dwarf galaxy Mrk 462.
DOI: 10.57780/esa-1jy66ro
title: 084058

description: We propose to observe 3 X-ray luminous clusters which each have over 10elev10 Msun of cold molecular gas in their X-ray cool cores. The ALMA velocity and morphology data indicate that the cold gas is disturbed in these object. If comma  as Hitomi has shown in the Perseus cluster comma  the cold gas and ICM share the same velocity field comma  then we shall measure velocity broadening of the soft X-ray emission lines with the XMM RGS. We shall also measure or constrain mass cooling rates of the ICM below 1-2 keV.
DOI: 10.57780/esa-1k7w68r
title: 086131

description: We.ve shown in our recent X-ray studies of the Draco comma  Willman 1 comma  Sagittarius openParSgrclosePar dwarf spheroidal galaxies openPardSphsclosePar that the X-ray population in these very old and faint galaxies is very different from that in other Local Group galaxies and is dominated by accreting white dwarfs openParAWDsclosePardoublePoint at least four AWDs in the Draco dSph comma  one in Willman 1 dSph comma  and ten in the center of Sgr dSph. Optical and infrared studies show that the closet dwarf galaxy comma  Canis Major openParCMaclosePar comma  has an old massive core mainly populated by red giant branch openParRGBsclosePar stars. We propose to observe the center of CMa dwarf galaxy comma  which have not been yet observed in X- rays in order to analyse AWDs using X-ray and multi-wavelength data comma  and to perform a comparative study of the X-ray luminosity function of AWDs of dwarf galaxies.
DOI: 10.57780/esa-20xwivu
title: 088119

description: We propose mosaic observations of the massive comma  early-stage comma  binary merging cluster Abell 401 to probe the ICM out to the virial radius with essentially full azimuthal coverage. Simulations of structure formation predict relatively large numbers of cool gas clumps in such systems comma  with more clumps expected along filaments. Abell 401-Abell 399 is a perfect example of such a system comma  with the only intercluster filament detected by Planck. We will apply the X-COP method of combining X-ray and SZ observations to accurately determine the thermodynamic profiles of the ICM comma  with and without d_commaclump filteringd_comma comma  to measure the clumping factor and fraction of non-thermal pressure support both along and away from the putative cosmic filament and compare the results with expectations from simulations.
DOI: 10.57780/esa-251pday
title: 090399

description: eROSITA is performing multiple all-sky X-ray surveys until 2023 comma  and our team is systematically identifying rare accretion ignition-shut-down events - changing-look AGN - as they are transitioning.  To track how the X-ray corona comma  UV-optical accretion disk comma  and optical broad-line region respond to a sudden comma  major change in accretion rate comma  we propose joint ToO observations of XMM-Newton openParEPIC+OMclosePar and VLT openParFORS2closePar to obtain at least two observations per triggered object openParmaximum of 4 ignition events and 4 shutdown eventsclosePar.  We will constrain the extent of these drastic flux changes and yield crucial constraints on how the different structural AGN components respond to dramatic changes of the accretion rate.
DOI: 10.57780/esa-251q34n
title: 085039

description: TON 0599 is the flat spectrum radio quasar most recently detected in very high energy gamma rays. Analysis of the data taken during a flaring state revealed several interesting spectral featuresdoublePoint iclosePar apparent smooth spectral transition from the Fermi-LAT to MAGIC energy range comma  iiclosePar inverse Compton openParICclosePar peak between Fermi-LAT and MAGIC energy ranges comma  and iiiclosePar a spectral cut-off at few tens of GeV. Here we propose a monitoring campaign in order to study these spectral features in details. It will allow us to investigate the location of the gamma-ray emission region with respect to the broad line region and more detailed investigation of emission models. We also propose observations with XMM-Newton in order to investigate the transition from synchrotron to IC bump.
DOI: 10.57780/esa-28wbezj
title: 086335

description: Superclusters comma  as the largest cosmic structures comma  are important to study the evolution of galaxy clusters and groups comma  cosmic baryons openPare.g. comma  the warm hot intergalactic mediumclosePar and galaxy evolution. There have been few studies of superclusters in X-rays comma  while the X-ray data remain as the key to study the bulk of baryons in superclusters. We select the two richest superclusters from the SDSS-redMaPPer cluster catalog and propose XMM observations to map both of them. They are extreme mass concentrations with the total mass at least several times higher than well-known superclusters like A901-2. The XMM data will be used to map the mass distribution openParalong with our weak-lensing workclosePar comma  study merger dynamics and examine the cosmic filaments comma  and provide us important insights on superclusters.
DOI: 10.57780/esa-29g4atc
title: 086226

description: Outbursts of super-massive black holes openParSMBHsclosePar have a significant impact on structure formation and evolution. However comma  AGN heating from SMBHs has not been well studied in galaxy groups. The main reason is that groups are X-ray faint around the center comma  especially for those hosting strong radio AGN. We propose XMM observations of two nearby galaxy groups 3C 66B and IC 2476 comma  both of which host strong radio AGN comma  to study AGN feedback in groups. XMM.s high sensitivity at soft X-ray band makes it the best instrument for this project. The results will fill the little-explored regime of the  L_keyOpen radiokeyClose   -  L_keyOpen powerkeyClose   plane for galaxy groups and improve our understanding of AGN heating in groups.
DOI: 10.57780/esa-2d3f3xi
title: 086409

description: A population of intermediate black holes openParIMBHclosePar will allow us to solve one of the long-standing problems in modern astrophysics comma  the origin of supermassive black holes. Having analysed 1 million optical spectra comma  we identified 305 IMBH candidates openPar3e4-2e5 MSunclosePar comma  which reside in galaxy centers and pose as active galactic nuclei. With Chandra DDT and XMM-Newton AO-18 observations and mining X-ray data archives comma  we confirmed the AGN nature of 11 candidates comma  thus validating our IMBH search approach. Here we propose to observe 12 additional optically selected IMBH candidates to double the number of X-ray confirmed accreting IMBHs. This will enable detailed studies of the IMBH population and help to constrain the masses of ..seed. black holes in the early Universe.
DOI: 10.57780/esa-2v781eq
title: 089042

description: The HGPS revealed a point-like source we consider to be of high interestdoublePoint HESS J1828-099. It is one of only 17 sources in the HGPS with an angular size 0.07deg. This source is unique in the sense that it does not seem to have apparent associations at lower energies and it is not located in highly confused regions such as the Galactic Center. What is the nature of HESS J1828-099 questionMark Is it perhaps a young PWN comma  with dim counterpartsquestionMark Is it maybe a gamma-ray binaryquestionMark A supernova remnantquestionMark We aim at identifying the nature of the point-like unidentified source HESS J1828-099 in thecontext of a MWL campaign openParX-rays and radioclosePar. We will prove the non-thermal emission scenario making use of these three different frequencies.
DOI: 10.5281/zenodo.7805118
title: Il torrente Parma nelle carte della Congregazione dei Cavamenti, serie Canali e Torrenti dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nel fondo archivistico <em>Congregazione dei Cavamenti,</em> serie<em> Canali e Torrenti </em> dell'Archivio di Stato di Parma
DOI: 10.57780/esa-2zwuht6
title: 086062

description: We propose a 80 ks XMM-Newton monitoring campaign to cover 5 nights of VLTI-Gravity guaranteed time observations of Sgr A* comma  during the spring of 2021. At that time comma  Sgr A* will be visible from Paranal for virgul3.5-4 hr each night. Simultaneous X-ray and NIR observations will allow us to extract the best science from both European projects. This deep XMM-Newton exposure will also allow us to monitor the evolution of the reflection component off the clouds of the Sgr A molecular complex comma  therefore to further constrain Sgr A*.s past activity and the cloud 3-dimensional distribution.
DOI: 10.5281/zenodo.7805117
title: Il torrente Parma nelle carte della Congregazione dei Cavamenti, serie Canali e Torrenti dell'Archivio di Stato di Parma

description: Schedatura e metadatazione dei contenuti delle carte inerenti il corso del torrente Parma nel fondo archivistico <em>Congregazione dei Cavamenti,</em> serie<em> Canali e Torrenti </em> dell'Archivio di Stato di Parma