cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.57780/esa-tg5lwiy
title: 090232

description: Changing-look AGN (CLAGN) are one of the most mysterious categories of AGNshowing strong variability and sudden state changes. Our search for possibleCLAGN candidates led to the discovery of 2MASXJ0817. The source is affected by avery small amount of intrinsic absorption and exhibits long-term X-rayvariability by a factor of 10 at least. The strong spectral changes in thesource are associated with intrinsic changes only (no absorption-inducedvariability was identified). We propose to monitor the source during AO21 witha total of 240 ks in a way that will allow us to probe changes in the inneraccretion flow on dynamical thermal and viscous timescales ranging from a fewks up to a year. The proposed campaign will shed light on the nature of the strong variability in this source. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-ujn4mog
title: 091579

description: Owing to their brightness and proximity Mrk421 and Mrk501 are among the blazarsthat can be studied with the greatest level of detail and thus excellentastrophysical laboratories to study the underlying physics of blazars. Werequest MAGIC observations to provide sensitive VHE coverage for themulti-instrument campaigns in 2023/2024. These MAGIC observations are needed tocharacterise with accuracy the high-energy bump and its temporal evolution withsimultaneous coverage for the low-energy bump. [truncated! Please see actual data for full text]
DOI: 10.3535/66f-tb6-s1k
title: Alentia gelatinosa (M. Sars, 1835)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wmg-q0d-qzb
title: Girardia tigrina (Girard, 1850)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-uo8txp5
title: 092256

description: Over recent years a dearth of planets with radii between 1.5 and 2 times thatof the Earth has been uncovered in the observed population of short periodplanets. Several nearby multi-planet systems have been discovered hostingplanets on both sides of this gap dubbed the radius valley. One of theleading mechanisms for forming the gap is the stripping of small H/He envelopesby X-ray and EUV-driven photoevaporation. Systems boasting planets on eitherside of the valley provide a powerful testing ground for this hypothesis as allplanets in the system have been subject to the same high-energy irradiationhistory. We propose XMM-Newton observations of five such systems spanning arange of system architectures as well as stellar ages and masses with the aim of determining which are compatible [truncated! Please see actual data for full text]
DOI: 10.3535/2dm-vl5-alj
title: Girardia tigrina (Girard, 1850)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-urm29x0
title: 092125

description: We propose a high-resolution spectral study of the transient black hole X-raybinary MAXI J1810-222 to clearly resolve and determine the nature of one of themost powerful and fastest wind ever observed in a Galactic accreting system. Werequest a 60 ks XMM-Newton observation when the source is either in soft orintermediate state to constrain the physical parameters of the wind with muchgreater accuracy than those derived from the available NICER spectra. Byanalysing these spectra we obtained evidence for a spectral-state dependentoutflow with mildly relativistic speed which would test current theoreticalmodels of winds formation in X-ray binaries. RGS is the only instrument able toresolve sharp features around 1 keV within our observing constraints. [truncated! Please see actual data for full text]
DOI: 10.3535/16b-f8z-lrq
title: Dugesia japonica Ichikawa & Kawakatsu, 1964

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/h3k-1ne-dm8
title: Pygospio elegans Claparède, 1863

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-uybye0t
title: 092000

description: We propose to observe 32 (28 with new exposures) among the brightest galaxygroups and clusters selected from the eFEDS sample with a total exposure time of226 ks.We will use the requested data to determine their temperatures to measure thespectral cross-calibration uncertainties between eROSITA and XMM-Newton.The size of the selected sample together with its temperature coverage willallow a firm constraint of any systematic difference between the two instrumentsand how this difference (if any) depends on the spectral temperature itself.Considering the current situation on the eROSITA} operations  we notice thatthe eFEDS exposure will be unmatched in the next future providing a unique sample to investigate any cross-calibration among X-ray instruments. [truncated! Please see actual data for full text]
DOI: 10.3535/qxa-9r3-23j
title: Hemiurus communis Odhner, 1905

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wfl-h1s-ybh
title: Polycelis (Polycelis) pamirensis de Beauchamp, 1961

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-v3a0wc6
title: 094504

description: The 10 deg2 Euclid Deep Fornax Field (EDFF) will be the foremost extragalacticmedium-area deep field due to its unique multi-lambda coverage. We aim toprovide the X-ray view by mapping the entire EDFF at 40ks depth for untoldlegacy value. The XMM data and associated surveys will enable major advances inthe study of AGN and galaxy clusters including: deep characterisation of Euclidclusters and their selection function  robust measures of cluster scalingrelations to z=1.5 and the group regime  the study of rare clusters and AGN in avariety of environments  and revealing the link between AGN feedback and starformation to z and amp gt 3. We will deliver a complete validated multi-lambda legacydataset that will greatly enhance the AGN and cluster science from the 15000 deg2 Euclid Wide survey. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-vb56f2u
title: 090303

description: Dust chemistry is a key tracer of structure formation and evolution. In AGN theorigin and properties of dust are uncertain. Dust could be associated to AGNwinds which would have important implications on the driving and impact of thewinds on their host galaxies. High-resolution X-ray spectroscopy is a novel andpowerful method for probing chemistry of dust. We find NGC 6860 an X-ray brightAGN is an ideal target for investigating the link between dust and winds. Itshows significant reddening and absorption by dust while being sufficientlybright for X-ray spectroscopy. We propose a 120 ks XMM-Newton observation tocarry out high-resolution X-ray spectroscopic study of dust and ionised winds inthis AGN. [truncated! Please see actual data for full text]
DOI: 10.3535/s1y-9x3-e1w
title: Nephtys hombergii Savigny in Lamarck, 1818

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-vgpcn5z
title: 092340

description: Galactic PeVatrons are a new exciting class in high energy astrophysicsfollowing the LHAASO discovery of 14 ultra-high-energy (UHE   and amp gt  100 TeV) sourcesin our galaxy. However the mechanism powering the majority of UHE sourcesremains a mystery. Common leptonic and hadronic accelerators include PWNe SNRsinteracting with clouds and star clusters. Surprisingly four of the LHAASOsources have no active particle accelerator candidates in their vicinity andremain mostly undetected below the UHE band. We propose an extensive X-raysurvey of these dark PeVatron accelerators utilizing XMM.s large FOV andspectro-imaging capability. Our program combined with the planned VERITAS TeVobservations will collect X-ray legacy data on the most energetic and enigmatic objects in our galaxy. [truncated! Please see actual data for full text]
DOI: 10.3535/a3p-jpl-gsr
title: Seidlia schmidti Zabusov, 1916

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-vzk10wm
title: 092226

description: The mass of supermassive black holes (BHs) correlates with the bulge mass orstellar velocity dispersion of their host galaxies. The co-evolution of BHs andgalaxies could explain these correlations but this picture was challenged by aseries of arguments. We propose to explore three local red nugget analogs thathave high velocity dispersion relative to their bulge mass. Based on theXMM-Newton observations we will build gravitating mass profiles and compute thedark matter halo mass of the galaxies. By utilizing X-ray and optical data andresults of numerical simulations we will probe (1) the tightness of thecorrelation between BHs and dark matter halos (2) explore whether BHs and theirhost galaxies grow in sync and (3) estimate the frequency of red nuggets in the local universe. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613622_d2.v1
title: Additional file 2: Table S1. of The common stress responsive transcription factor ATF3 binds genomic sites enriched with p300 and H3K27ac for transcriptional regulation

description: A list of unique genes containing overlapped ATF3 and p53 peaks where both ATF3 and p53 motifs are present. (XLSX 32 kb)
DOI: 10.3535/157-f45-7zj
title: Pseudovermilia fuscostriata ten Hove, 1975

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/ls2-6wa-296
title: Seidlia schmidti Zabusov, 1916

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wj5-50t-450
title: Streblospio shrubsolii (Buchanan, 1890)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-wfzz9n6
title: 092051

description: Ultraluminous X-ray sources (ULXs) are extragalactic X-ray sources possiblyhosting super-Eddington accreting black holes or neutron stars. The ULXpopulation shows sources with randomic long and short-term variability. Weselected the ten nearby ( and amp lt 20 Mpc) galaxies that most probably host ULXs and thatwere not observed in X-rays. We ask for snapshot (10 ks) observations tocomplete the census of ULXs in the nearby universe. [truncated! Please see actual data for full text]
DOI: 10.3535/gka-g3n-5xp
title: Vermiliopsis infundibulum (Philippi, 1844)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/sxb-22j-rny
title: Namanereis Chamberlin, 1919

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-wmh60mx
title: 092001

description: We propose to observe 8 galaxy groups with a total exposure time of 48 ks tocomplete observations for a flux limited sample consisting of 67 objects.We will use this well-defined sample to study the scaling law properties oflocal low-mass systems.Only with the requested observations we will be able to correct for sampleselection effects entering in the scaling relations increasing the constrainingpower by a factor of 2 compared to previous samples.Furthermore we will determine detailed thermodynamic profiles puttingconstraints on the feedback processes.Our AO21 proposal was accepted in the category C and with this proposal we would like to ensure that the complete sample gets observed because it is essential to have good data for all the systems. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-xchzvad
title: 088306

description: The afterglow of some nearby short GRBs displays a late-time rebrighteningvisible in the near-infrared a few days after the burst. HST observationsprovided convincing evidence that such late-time bump could be explained askilonova emission. This provides a direct link to neutron star (NS) mergers anda compelling proof for the synthesis of heavy nuclei through the rapid neutroncapture process (r-process). We propose a multi-wavelength follow-up campaign ofa nearby (z and amp lt 0.4) short GRB in order to detect the kilonova bump and constrainits properties. Multi-band observations and in particular X-rays are criticalto pin down the nature of the observed rebrightening and to distinguish it fromstandard afterglow emission. [truncated! Please see actual data for full text]
DOI: 10.3535/bpp-1w1-he0
title: Girardia paramensis Fuhrmann, 1912

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-xfzvkza
title: 093379

description: BPM16274 is the most frequently observed OM photometric calibration target andis used to monitor the degradation of the instrument. It was mostly observed atthe OM boresight prior to the damaging Jupiter observation in rev 3224 but ithas not been observed at the OM boresight since.  Since the OM boresight is in fact barely affected by the Jupiter patch a newobservation at the OM boresight will provide an important reference measurementof the degradation that can be reliably connected to the existing data from theOM boresight position while giving us a very useful comparison against the post-rev3224 data obtained at the offset positions. The proposed observation ofBPM16274 should yield data with  and amp lt virgul 1% statistical uncertainties. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613637_d1.v1
title: Additional file 1: of A large deletion in RPGR causes XLPRA in Weimaraner dogs

description: A Candidate genes for PRA exome screening (n = 346). B and C Primers used for breakpoint analysis (B) and qPCR (C) with their corresponding product size. (XLSX 19 kb)
DOI: 10.3535/9j7-q7q-mm3
title: Phagocata papillifera (Ijima & Kaburaki, 1916)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/ahn-6cj-fse
title: Tomopteris septentrionalis Steenstrup, 1849

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-xjzxnc2
title: 092259

description: The recent discovery of a Jupiter-sized planet orbiting a very young 11 Myr oldmid M dwarf is unprecedented in its promise for the investigation of how planetsaround low mass stars evolve. Substantial evolution of the planet.s atmosphereshrinking the overall planet radius is expected in its future. We propose anobservation with the XMM-Newton.s EPIC cameras to investigate the current levelof X-ray irradiation of the atmosphere that along with the EUV is thought todrive atmospheric mass loss particularly within the first few hundred Myr. Ourdirect measurement will be a key input to evolution simulations which we willrun to better understand this remarkable planet.s future. [truncated! Please see actual data for full text]
DOI: 10.3535/cnb-kls-hsp
title: Proceraea aurantiaca Claparède, 1868

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/g05-jly-phw
title: Cerebratulus [Renier], [1804]

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-xzzvdpa
title: 094502

description: The 10 deg2 Euclid Deep Fornax Field (EDFF) will be the foremost extragalacticmedium-area deep field due to its unique multi-lambda coverage. We aim toprovide the X-ray view by mapping the entire EDFF at 40ks depth for untoldlegacy value. The XMM data and associated surveys will enable major advances inthe study of AGN and galaxy clusters including: deep characterisation of Euclidclusters and their selection function  robust measures of cluster scalingrelations to z=1.5 and the group regime  the study of rare clusters and AGN in avariety of environments  and revealing the link between AGN feedback and starformation to z and amp gt 3. We will deliver a complete validated multi-lambda legacydataset that will greatly enhance the AGN and cluster science from the 15000 deg2 Euclid Wide survey. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613640_d1.v1
title: Additional file 2: of Reporting of harms outcomes: a comparison of journal publications with unpublished clinical study reports of orlistat trials

description: Reporting of AEs.xlsâ  , Table S2 Reporting of adverse events in Clinical Study Reports (CSRs) and journal articles for Olistat trials. (XLS 31 kb)
DOI: 10.3535/avb-zgz-aqj
title: Proceraea aurantiaca Claparède, 1868

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/z78-bh9-3m2
title: Streblospio shrubsolii (Buchanan, 1890)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-y4hzd5o
title: 092151

description: A dedicated monitoring campaign with XMM Swift NICER Chandra and eROSITA overthe past 4+ years has unveiled a surprising second outburst from the tidaldisruption event (TDE) AT2018fyk. This dramatic X-ray and UV re-brightening hasbeen interpreted as the signature of a repeating partial TDE. We are requestinga 30 ks XMM exposure of AT2018fyk during the upcoming accretion shut off phasewhich is estimated to occur during mid-late 2023. Our main goal is to track theX-ray spectral evolution during this second outburst and compare it with theprevious flare. While we currently continue to track AT2018fyk with NICER andSwift through GO and DDT programs only XMM has large enough effective area andsensitivity to facilitate a high signal-to-noise spectrum in the next low-flux state. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-zsr4zy5
title: 092248

description: Under the unified model of AGN the difference between between Seyfert 1 and 2AGN is explained as an effect of orientation relative to the observer. Seyfert2s are seen edge-on with the broad line region obscured by a dusty torus. Thistheory is motivated by the observation of ???hidden??? broad lines in someSeyfert 2s. However not all Seyfert 2s have polarized broad lines suggestingthat the unified model is incomplete and that there are physical differencesbetween some Seyfert 1s and 2s. We propose to extend a sample of ???true???Seyfert 2 candidates that have been observed by both SDSS and the Chandra X-rayObservatory by obtaining high-quality XMM-Newton spectra for 11 sources withinsufficient signal in the Chandra observations to place constraints on their absorption. [truncated! Please see actual data for full text]
DOI: 10.3535/d0y-w0k-dbx
title: Namanereis hummelincki (Augener, 1933)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/zra-ja0-v6r
title: Tomopteris nisseni Rosa, 1908

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-zud5sb3
title: 092110

description: Recent years have seen great controversy about the rotational state ofsolar-mass stars older than the Sun. After excluding observational biasesevidence solidifies that the stars expected to rotate slower than the Sun arenowhere to be found leading to theories that such stars may have a mostlyswitched-off dynamo and continue to coast with practically constant rotationperiods into their future. However age-rotation studies can only detect adearth of stars rotating slower than our Sun not the reason behind it. Incontrast X-ray observations can probe the state of the magnetic dynamo andreveal whether a switch-off really occurs. We therefore propose deep X-rayobservations of a small decisive sample of old sunlike stars to find out the reason behind the missing slow rotators. [truncated! Please see actual data for full text]
DOI: 10.3535/v1f-1yh-xly
title: Cura pinguis (Weiss, 1909)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/xr1-gln-ncp
title: Geoplana Müller, 1856

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.6084/m9.figshare.c.3613640_d2.v1
title: Additional file 3: of Reporting of harms outcomes: a comparison of journal publications with unpublished clinical study reports of orlistat trials

description: Reporting of SAEs.xlsâ  , Table S3 Reporting of serious adverse events (SAEs) in Clinical study reports (CSRs) and journal articles for Olistat trials. (XLS 65 kb)
DOI: 10.3535/6zl-0hv-9b8
title: Clitellata

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-zxb0n4s
title: 092128

description: The X-ray dim isolated neutron star (XDINS) population comprised of 7 objects could make up a significant part of the Galactic isolated neutron star (INS)population. To understand intrinsic properties birthrates and evolutionarylinks to other INS classes the sample must be increased. The eROSITA All-SkySurvey (eRASS) will unveil the elusive XDINS population beyond the solarvicinity. To confirm the XDINS nature for 7 candidates selected from the eRASSwe propose observations with XMM-Newton and the VLT aiming to increase theX-ray-to-optical flux ratio limits to improve localisations and to investigatethe X-ray spectral and temporal properties. This programme will double the knownpopulation and be the basis for future studies of the Galactic XDINS population. [truncated! Please see actual data for full text]
DOI: 10.3535/xpp-sga-b85
title: Clitellata

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/ys8-gsr-0vn
title: Nephtys hombergii Savigny in Lamarck, 1818

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/2cj-z77-5yj
title: Pentacoelum kazukolinda (Kawakatsu & Mitchell, 1984)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/gep-b3l-24w
title: Nephtys hombergii Savigny in Lamarck, 1818

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/rwp-7hc-kzd
title: Dugesia ryukyuensis Kawakatsu, 1976

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/1cg-a3b-yd6
title: Hediste diversicolor (O.F. Müller, 1776)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/xyt-6sp-q8z
title: Dugesia Girard, 1850

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/z3v-h2k-71t
title: Girardia Ball, 1974

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.6084/m9.figshare.c.3613640_d4.v1
title: Additional file 4: of Reporting of harms outcomes: a comparison of journal publications with unpublished clinical study reports of orlistat trials

description: SAEs Meta-Analysis results.xlsâ  , Table S4 SAEs Meta-Analysis results. (XLS 76 kb)
DOI: 10.3535/fjj-7b2-ebd
title: Dugesia benazzii Lepori, 1951

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/flv-khn-ves
title: Ectoplana undata Sluys, 1986

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wk5-kds-7z1
title: Trichuris Roederer, 1761

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/h7t-a38-kph
title: Dugesia novaguineana Kawakatsu, 1976

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/sc7-2ew-7p8
title: Perionyx violaceus Horst, 1894

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.6084/m9.figshare.c.3613661_d1.v1
title: Additional file 1: of Comparison of hemodynamic response to tracheal intubation and postoperative pain in patients undergoing closed reduction of nasal bone fracture under general anesthesia: a randomized controlled trial comparing fentanyl and oxycodone

description: The datasets generated and analysed during the current study. (XLSX 38 kb)