cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.c.3613547_d4.v1
title: Additional file 5: Table S4. of miR-155 in the progression of lung fibrosis in systemic sclerosis

description: miRNA expression in PBMC by Nanostring analysis. Data are expressed as counts ofgenes and fold-change of the average on PBMC in SSc-ILD compared to the average of the controls (column U). (XLSX 167Â kb)
DOI: 10.3535/dfk-e60-bvp
title: Spiraserpula minuta (Straughan, 1967)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/flt-ez0-sef
title: Spirobranchus corniculatus (Grube, 1862)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-mrmf24p
title: 094501

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: 10.3535/42t-adt-xsq
title: Filograna Berkeley, 1835

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-mzqmujk
title: 092118

description: Contrary to expectations from current stellar evolutionary models recentobservations uncovered the ejection of shells of material by massive stars inthe years before the supernova (SN) explosion. The physical mechanism behind theimpulsive mass ejection synchronized with the stellar core-collapse is unclear.Here we propose a coordinated XMM-NuSTAR effort to map the evolution of thebroad-band X-ray spectrum of 1 nearby (d and amp lt  50 Mpc) or X-ray bright (Fx and amp gt 3 x 10^-13erg/s/cm2) strongly interacting SN and enable progress. Our program has theimmediate goal to characterize the medium around strongly interacting SNe whichoriginate from stellar progenitors with the most extreme mass loss beforeexplosion. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-n0hsc7j
title: 092149

description: Very High Energy (VHE  and amp gt 50 GeV) gamma rays provide a direct view of the mostextreme environments inour Galaxy and are an excellent probe of non-thermal astrophysical processes.Studies of the non-thermal Galacticsource population are essential to understand where and how the bulk of thecosmic rays are accelerated in ourGalaxy. Fermi has produced the first uniform survey of the entire Galactic planeat  and amp gt 50GeV detecting more than25% unidentified sources. We propose to observe with XMM-Newton the 2 spectrallyharder and thus most extreme objects in the Fermi sample. The study of these sources with XMM-Newton will unveil new sites of particle acceleration and will allow us to understand the physics behind VHE emitters. [truncated! Please see actual data for full text]
DOI: 10.3535/4ss-q6g-xlv
title: Diversibipalium Kawakatsu, Ogren, Froehlich & Sasaki, 2002

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/saf-00h-em2
title: Hydroides elegans (Haswell, 1883) [nomen protectum]

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-nyfo0p1
title: 092211

description: Understanding the 3D structure of disc winds is vital for constraining theirenergetics but in most sources we only have one sightline through the wind.Her X-1 is a unique X-ray binary with a warped precessing disc providing timevariable sightlines. A disc wind was detected during Her X-1 Main High statevarying in time due to the changes in our sightline over the precession cycle.Hence we can uniquely sample the vertical wind structure seen to weaken atgreater heights above the disc. An archival Short High state observation shows astronger wind than those during Main High - we are sampling lower wind heightsabove the disc. We propose 3x80 ks XMM and 1x25 ks Chandra exposures duringShort High to understand the 3D wind structure at all heights and constrain its energetics. [truncated! Please see actual data for full text]
DOI: 10.3535/twa-gzm-zpj
title: Maldane sarsi Malmgren, 1865

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/w46-z3m-tzn
title: Maldane sarsi Malmgren, 1865

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-oq93nb3
title: 092074

description: The impact of projection effects on optical photometric galaxy clusterselection has recently been clarified at z virgul 0.1 using extensive spectroscopy ofputative member galaxies. The projected fraction of photometrically associatedgalaxies has been constrained in bins as a function of richness along with therelations between photometric and spectroscopically corrected richness andvelocity dispersion. We propose XMM-Newton observations of a complete sub-sampleof these clusters at high richness to obtain low-scatter X-ray mass proxies.These measurements will provide independent complementary information onprojection effects and crucially will allow the scatter of spectroscopicallycorrected richness with mass to be quantified. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613547_d6.v1
title: Additional file 6: Table S5. of miR-155 in the progression of lung fibrosis in systemic sclerosis

description: miRNA expression in lung fibroblasts by Nanostring analysis. Healthy control lung fibroblasts (HC) and SSc-ILD lung fibroblasts were stimulated with media, interleukin-13 (IL-13), interferon alpha (IFN), and TGF-beta for 18Â hours. Data are expressed as counts of gene expression. (XLSX 56Â kb)
DOI: 10.3535/7nf-1sd-tbc
title: Filograna Berkeley, 1835

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/e7k-tne-3bs
title: Notaulax phaeotaenia (Schmarda, 1861)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-oyhyf7e
title: 092410

description: Knowledge of the structure and kinematics of gas around supermassive black holesis vital to understanding accretion and thus AGN feedback. To this end we the AGN STORM 2 team have conducted the largest multi-missionand multi-wavelength campaign of an AGN to date.This includes a Large 198-orbit Hubble Space Telescope Program an XMM-NewtonProgram (AO20) a Swift Key Project and monitoring withNICER and optical ground based facilities. The prime AGN STORM 2 campaign (fromDec 2020-Feb 2022) revealed a wealth of information on [truncated! Please see actual data for full text]
DOI: 10.3535/bah-2z7-54m
title: Maldane sarsi Malmgren, 1865

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-pm3dsuj
title: 092004

description: HD168112 is an eccentric wide O + O binary known for its synchrotron radioemission. The relativistic electrons responsible for this emission areaccelerated by the strong shocks between the stellar winds of both components.These shocks heat the post-shock plasma leading to a strong X-ray emission thatvaries with orbital separation d. We propose to investigate the impact of thepopulation of relativistic electrons on the hydrodynamic shocks and the X-rayemission. For this purpose we propose to collect XMM-Newton observations ofHD168112 during its next periastron passage in March 2023. We will search fordeviations of the X-ray luminosity over the 1/d relation for adiabatic shocksand constrain any hard X-ray tail due to non-thermal X-rays produced via inverse Compton scattering. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-qbrbq7b
title: 093080

description: Eclipsing Cataclysmic Variables (CVs) provide an unique opportunity toinvestigate deeply into their X-ray emitting regions by disentangling thesoft X-ray emission and the hard X-ray emission. The proposal requestssimultaneous NuSTAR and XMM observations of two eclipsing CVs: UU Aqra nova-like variable and V902 Mon an intermediate polar. The jointobservations are requested over the two orbital cycles of the source:29 ks for UU Aqr and 59 ks for V902 Mon each with NuSTAR and XMM. Theobservations would be used to detect X-ray eclipses and infer the originof the hard X-rays [truncated! Please see actual data for full text]
DOI: 10.3535/8xf-0xp-wld
title: Pygospio elegans Claparède, 1863

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/azz-kzk-c0a
title: Phagocata kawakatsui Okugawa, 1956

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-qpk87ly
title: 094353

description: We propose to invest 2.2Ms of XMM time to obtain the first X-raycharacterization of a sample of 15 hyper-luminous quasars at z=2-4. The maingoals are i) to detect the UFO features and derive the wind detection rate in alarge sample at these luminosities/redshift  ii) to investigate their launchingmechanism by exploring correlations between wind and accretion properties in aluminosity/accretion range unexplored so far  iii) to characterize through windmodels the physical properties of the nuclear winds derive their energetics andcompare them with the large-scale outflows  iv) to explore the connectionbetween the presence of nuclear winds and other X-ray properties. This programwill provide the community with the legacy sample for the study of SMBH accretion and ejection beyond z=2. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613577_d3.v1
title: Additional file 8: Table S2. of Insistence on sameness relates to increased covariance of gray matter structure in autism spectrum disorder

description: Subcortical-Cortical Region X Region Pairs with Significant (corrected) Correlations with IS. (XLSX 88.0 KB)
DOI: 10.3535/fqv-pf0-4bh
title: Korotkevitschia pelagica (Korotkevich, 1961)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/rz2-3dg-let
title: Vermiliopsis infundibulum (Philippi, 1844)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-r05fbsm
title: 092025

description: PG1448+273 is a luminous NLS1 thought to be accreting at the Eddington limit.An XMM observation in 2017 discovered an ultra fast outflow (v=0.1c) in PG1448via a deep Fe absorption trough at 7.5 keV. A 2022 NuSTAR observation thenrevealed a drastic increase in wind velocity to 0.3c coincident with apronounced drop in flux. Here we wish to further understand the extremevariability of the disk wind through 3x80ks and 3x50ks simultaneous XMM andNuSTAR observations to determine the wind changes in velocity and outflow ratevs flux. A 40x1ks Swift daily monitoring campaign is proposed to monitor the UVto X-ray SED over the XMM window to help determine how the wind reacts to thecontinuum. The observations will test the physics of accretion disk winds near the Eddington limit. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613547_d7.v1
title: Additional file 2: Table S2. of miR-155 in the progression of lung fibrosis in systemic sclerosis

description: List of mRNA gene expression in SSc-ILD compared to healthy controls. In sequence: gene symbol, gene name, and average fold-change expression in SSc-ILD compared to healthy controls. (XLSX 15Â kb)
DOI: 10.3535/1ez-dbd-mrp
title: Dero pectinata Aiyer, 1929

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/8wx-k6f-w0w
title: Polydora Bosc, 1802

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-r90wyyr
title: 090123

description: We propose to observe 8 galaxy groups with a total exposure time of 68 ks tocomplete observations for a flux limited sample consisting of 67 objects. Wewill use this well-defined sample to study the scaling law properties of locallow-mass systems. Only with the requested observations we will be able tocorrect for sample selection effects entering in the scaling relationsincreasing the constraining power by a factor of 2 compared to previous samples.Furthermore we will determine detailed thermodynamic profiles within R2500(i.e. the region where simulations differs more noticeably) putting constraintson the feedback processes. [truncated! Please see actual data for full text]
DOI: 10.3535/gge-3tq-d55
title: Serpula jukesii Baird, 1864

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/yff-8p4-mqx
title: Polydora ciliata (Johnston, 1838)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-rbanb2u
title: 091241

description: Masquerading BL Lacs are an elusive class of blazars which comprises ofFSRQs appearing as disguised BL Lac objects. In this work we will unveila potential target in an attempt to understand the nature of these sourcesand how they fit in the blazar population. We propose this source to beobserved with NuSTAR and XMM-Newton to help us construct a multiwavelengthSpectral Energy Distribution. This will assist us in revealing some essentialcharacteristics of this intriguing object. As the recent detection ofhigh-energy neutrinos by IceCube in the direction of TXS 0506+056 showsthese masquerading BL Lacs may be responsible for the astrophysical IceCubeneutrino flux proving that there is more to them than meets the eye. [truncated! Please see actual data for full text]
DOI: 10.3535/acx-xr1-ce7
title: Cura pinguis (Weiss, 1909)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/zfa-73s-x39
title: Capitella capitata (Fabricius, 1780)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-rc420iq
title: 091619

description: The goal of this proposal is a detailed long-term study of the temporal andspectral behaviour of the blazar 1ES 1959+650 to investigate further featuresseen in past campaigns with MAGIC and build-up a legacy data sample. After a low state since 2002 bright outbursts in 2016 were surrounded by intermediateactivity (2015-2018). Past observations have revealed a peak-shift towardshigher energies hinting an EHBL-like nature fast intra-night and long-termvariabilityas well as complex correlation patterns between wavebands. These features challenge simple one-zone synchrotron self-Compton models and suggest amore complex emission region. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-s4je6ab
title: 094503

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.3613547_d8.v1
title: Additional file 1: Table S1. of miR-155 in the progression of lung fibrosis in systemic sclerosis

description: The 185 differential miRNA expression (present in ≥25 % of samples, q 80 % of samples, p
DOI: 10.3535/ps2-ncm-rmq
title: Cura pinguis (Weiss, 1909)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-sbjy6mc
title: 092331

description: NGC 3516 is a remarkable Seyfert-1 galaxy which over the last decade hasundergone major spectral transformations classifying it as a changing-look AGN.Understanding the nature and origin of spectral variability in suchchanging-look AGN would provide key insights into the accretion-outflowmechanism. Swift monitoring of NGC 3516 shows dramatic flux rises and declinesduring its changing-look state. We propose ToO observations with XMM NuSTARand HST triggered using Swift monitoring to catch NGC 3516 at a high fluxlevel to be able to carry out the first high resolution X-ray and UVspectroscopy of its winds during the changing-look state. The proposedobservations would enable us to ascertain the role of winds in the transformation of NGC 3516. [truncated! Please see actual data for full text]
DOI: 10.3535/gmn-w37-zpy
title: Proteocephalus tetrastomus (Rudolphi, 1810) Willemse, 1969

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/t1h-gz1-bf7
title: Polycelis nigra (Müller, 1774)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-sd3wy04
title: 092068

description: Massive relic galaxies (MRGs) are local analogs of the high-redshift rednuggets.. thought to represent the progenitors of today.s early-type galaxies(ETGs). X-ray observation of the hot diffuse gas of MRGs is the most viablemeans to measure the global mass properties but only a few MRGs have beenidentified as suitable for such analysis. To remedy this we constructed asample of MRGs to map in detail their X-ray emission. We propose a snapshotsurvey of the 4 MRGs in the sample which lack X-ray data. Deep follow-upexposures with XMM-Newton and Chandra of promising targets will then be soughtto map their stellar gas and DM profiles to establish if high haloconcentrations are typical for MRGs and if their inner mass profiles differ from those of local ETGs. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613583_d2.v1
title: Additional file 1: Table S1. of Fatty acid kinase A is an important determinant of biofilm formation in Staphylococcus aureus USA300

description: Complete list of SNPs in genes representing divergent alleles in UAS391 and TCH1516 and their putative gene functions. TCH1516 was used as a reference for comparison with the allelic change in UAS391. Nucleotide changes in bold red represent the common SNPs in both FPR3757 and TCH1516 as compared to UAS391 (also in TableÂ 2). (XLSX 14 kb)
DOI: 10.3535/fbz-z8v-vxd
title: Thelepus thoracicus (Grube, 1869)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/ytd-t33-g29
title: Spirobranchus Blainville, 1818

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-su35evd
title: 092002

description: The binary zeta Tau was recently found to be a gamma Cas analog. Its X-rayspectrum however displays a unique feature amongst those objects: an extremeabsorption linked to the edge-on orientation of its disk. This provides aunique opportunity to draw final conclusions on the origin of the gamma Casphenomenon. [truncated! Please see actual data for full text]
DOI: 10.3535/yej-6kr-h2g
title: Branchiomma nigromaculatum (Baird, 1865)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-swxg32s
title: 092017

description: MACS J1931.8-2634 is a star-forming galaxy cluster at zvirgul0.35. Thearchival Chandra CCD spectra suggest a rather low level of metallicity inthe intracluster media out to virgul400 kpc. No other metal abundances weremeasured with the CCD data. AGN bubbles might explain the observed abundancebut it is unclear whether dust plays an essential role. Here we propose toobserve this target using mainly RGS with a total exposure of 188 ks.We will accurately measure the metal abundances of O Ne and Fe. Thisenables us to verify whether metals in the cluster core are locked into dustand moved away towards the cluster outskirt. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613577_d5.v1
title: Additional file 6: Table S1. of Insistence on sameness relates to increased covariance of gray matter structure in autism spectrum disorder

description: Subcortical-Subcortical Region X Region Pairs with Significant (corrected) Correlations with IS. (XLSX 45.6 KB)
DOI: 10.3535/1wg-bg9-df7
title: Pygospio elegans Claparède, 1863

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/qf6-m82-vdt
title: Magelona hartmanae Jones, 1978

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-tan53xy
title: 088335

description: We aim to study the cooling emission of highly magnetized neutron stars in Be/X-ray binaries. For this we need to increase our sample with high-qualitypost-outburst spectra. We require the flexibility of Swift to monitor thebehavior of the next potential target and the exceptional sensitivity and largeeffective area of XMM-Newton to study the low X-ray luminosity regime of thesource. These new observations will provide key additional data to i) betterconstrain the temporal evolution of the crust temperature in highly magnetizedaccreting NSs and ii) use the observed cooling curves as input into our 2Dcrust cooling model which incorporates magnetic fields. This is required tounderstand the role of such magnetic fields on the crust heating/cooling scenario of accreting NSs [truncated! Please see actual data for full text]
DOI: 10.3535/8th-v74-9kl
title: Seidlia auriculata (Ijima & Kaburaki, 1916)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wa6-qmq-g1l
title: Protula tubularia (Montagu, 1803)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-td42qs3
title: 093083

description: The X-ray emission from AGN is believed to be generated from the tiny regionsurrounding the SMBH namely the corona. The cutoff energy in the AGN X-rayspectrum (at a few hundred keV) can be used to probe the coronal properties.However only lower limits to the cutoff energy of low-redshift AGN weremeasured due to the limited bandpass (up to 80 keV). High-z quasarsinstead are the best targets to constrain the cutoff energy thanks tothe cosmological redshifting. So far only four z and amp gt 1 quasars have theircutoff energy constrained. Here we propose other four z and amp gt 1 quasars toincrease the current sample size to statistically constrain the AGN coronalproperties and thus better understand the physics of coronal Comptonization. [truncated! Please see actual data for full text]
DOI: 10.3535/32a-5xl-nsr
title: Alentia gelatinosa (M. Sars, 1835)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/cbh-rv6-h11
title: Spiraserpula plaiae Pillai & Ten Hove, 1994

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