cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.57780/esa-6zn2ipd
title: 094506

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: 10.3535/1eh-cdw-kwr
title: Crucigera inconstans Straughan, 1967

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/7jb-xr6-1fq
title: Capitella capitata (Fabricius, 1780)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-78vf5wg
title: 090042

description: We propose  to survey  the complete Galactic sample of confirmed massive binaryBe+sdO stars. We aim to probe the models which predicts that a significantfraction of Be-type stars have hot companions which were stripped of hydrogen bya mass exchange. These hot stripped companions with sdO spectral types  drivestellar winds which  collide and interact with the Be star winds and disks andhence have  unique signatures in their X-ray emission. The proposed survey willestablish X-ray properties of Be+sdO  binaries as needed to discriminate themfrom general OB star populations. The first X-ray survey of Be+sdO  binarieswill serve as important test on the physics of post-interaction binary stars andprovide critically important input to binary population synthesis models. [truncated! Please see actual data for full text]
DOI: 10.3535/456-avr-yga
title: Lanice conchilega (Pallas, 1766)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-7eva7qg
title: 093082

description: MS 22549-3712 is a unique AGN that shows both a quasi-periodic oscillation (QPO)and X-ray reflection and reverberation from the inner accretion disk. QPOs holdthe potential to probe General Relativity and the detailed physics of theaccretion process onto black holes and to provide independent constraints onthe black hole spin. Taking advantage of QPOs however requires a detailedunderstanding of the mechanism by which they are produced. We request deepsimultaneous observations of MS 22549-3712 using NuSTAR and XMM-Newton to takeadvantage of the X-ray reflection and reverberation in this AGN to probe theorigin of the QPO by studying how the QPO corresponds to variability of theinner accretion disk and/or corona. [truncated! Please see actual data for full text]
DOI: 10.3535/0sa-g69-a3n
title: Magelona papillicornis F. Müller, 1858

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/nvc-60q-bmx
title: Protula tubularia (Montagu, 1803)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-7onyuu5
title: 085178

description: Zetta Puppis observed every two years at 50 offset for the MOS off-patchresponse monitoring. PA should be fixed to 112 degrees
DOI: 10.3535/3q3-226-hqd
title: Tubificoides heterochaetus (Michaelsen, 1926)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/7tw-k9w-llp
title: Proteocephalus tetrastomus (Rudolphi, 1810) Willemse, 1969

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-9uk5sx7
title: 093079

description: The X-ray spectral analysis of new Compton thick (CT-) active galacticnuclei (AGN) represents a fundamental step to understand the physics of theobscuring material surrounding accreting supermassive black holes. Howeverat the present day CT-AGN remain extremely hard to detect. Implementinga previously successful machine learning algorithm we propose to target6 low-redshift candidate CT-AGN from the BAT 150-Month catalog for 30ks of NuSTAR and 25 ks of XMM-Newton time each. This analysis will helpdetermine the true intrinsic fraction of CT-AGN in the local universe andtheir contribution to the Cosmic X-ray Background (CXB). [truncated! Please see actual data for full text]
DOI: 10.57780/esa-b9uet1f
title: 092316

description: The Magellanic Clouds harbour a large sample of high-mass X-ray binary (HMXB)systems at a moderate and well known distance with low Galactic foregroundabsorption. In the course of the eROSITA all-sky surveys the Large MagellanicCloud is scanned frequently due to its close vicinity to the south eclipticpole. This provides the unique opportunity to find new low luminosity persistentHMXBs. We propose one 20 ks and two 60 ks XMM-Newton observations of three newlow luminosity persistent HMXBs. Optical spectra taken for one of the threetargets show the presence of a Be companion. Dedicated on-axis observations ofour three proposed systems will provide the unique opportunity to study thespectral and timing characteristics of this scarcely studied type of HMXB. [truncated! Please see actual data for full text]
DOI: 10.3535/96v-wak-967
title: Girardia Ball, 1974

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/wnx-7pj-jdh
title: Planariidae Stimpson, 1857

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-bot1oau
title: 093140

description: NuSTAR observations of the recent classical nova V1674 Her will test andconnect theories of intermediate polars (white dwarfs accreting througha disrupted disk and a magnetic stream) and of nova outbursts. The highenergy spectrum and the X-ray luminosity at quiescence allow to estimate thewhite dwarf mass the accretion rate and the accretion disk and columnparameters. Measuring the dependence of the spin period amplitude onenergy range will constrain the absorption effects and the geometry ofthe accretion columns. A coordinated XMM-Newton exposure will measureabsorption and complete the physical picture with the spectrum and thetiming of the residual soft emission from the polar caps. [truncated! Please see actual data for full text]
DOI: 10.3535/ama-19q-eha
title: Girardia Ball, 1974

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/l6y-v60-pah
title: Pygospio elegans Claparède, 1863

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-cd0sp7d
title: 092356

description: We propose 294 ks XMM-Newton EPIC observations on 15 X-ray luminous galaxyclusters detected in the first eROSITA All Sky Survey and are in the footprintsof Sunyaev-Zeldovich (SZ) surveys but without SZ detections. The m500 of the 15clusters scaled from X-ray luminosities are all  and amp gt 6e14 Msol which lie in a highcompleteness range of the two SZ surveys addressing questions relating to thecompleteness and selection biases in SZ and X-ray surveys. We will use theproposed data to obtain hydrostatic mass to investigate the selection biases inSZ and X-ray surveys and their impact on cosmology studies. Moreover we willalso measure other thermodynamic properties to explore the origins of SZnon-detections and discover new strong cool core clusters. [truncated! Please see actual data for full text]
DOI: 10.3535/dvs-008-9vy
title: Girardia Ball, 1974

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-cqjgs5l
title: 092157

description: Photospheres of sunlike stars have been found to display a smooth transition ofbeing dominated by spots or by faculae with the Sun sitting roughly in themiddle. We propose to characterize the coronae of four out of seven particularstars which have been identified to have different levels of spot- orfaculae-dominance on their surface. For this specific sample we haveinformation about the observed magnetic complexity from Zeeman-Doppler Imaging(ZDI) maps. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-dgsvr1c
title: 094507

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: 10.3535/8km-9xg-q8m
title: Eunice filamentosa Grube & Örsted in Grube, 1856

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/hls-cyl-bbr
title: Cura pinguis (Weiss, 1909)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-drqk7i9
title: 090122

description: We identified the transient object SRGt 062340.2-265715 as a bright (G virgul 12.5)nova-like cataclysmic variable (CV). A highly significant TESS period of 3.941hours (the orbital?) had disappeared when the object was reobserved with TESSlater. Located in very sparsely populated regions of X-ray/opticalcolor-magnitude diagrams the new object could be an X-ray underluminousintermediate polar an overluminous non-magnetic CV or a new type of CV. Wepropose XMM-Newton follow-up to search for spin- and orbital phase-dependentvariability and to perform time-resolved spectroscopy. We want to understandthe site of X-ray production and its modulation in the system (Lx = 4.8e32 erg/sat 495 pc) which was impossible to achieve with existing data and models. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613442_d13.v1
title: Additional file 5: of Tankyrase inhibition impairs directional migration and invasion of lung cancer cells by affecting microtubule dynamics and polarity signals

description: Raw data for Fig. S1. (XLSX 155 kb)
DOI: 10.3535/1eg-y09-zgy
title: Spathula truculenta Ball, 1977

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/2gn-41b-sna
title: Diversibipalium sumatrense (Loman, 1883)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-dxchln6
title: 092186

description: We ask for observations of a sample of luminous Ultraluminous X-ray Sourcesdiscovered duringthe first eROSITA All Sky Survey which are located in galaxies for which noprevious pointedX-ray observations exist. The aim of the proposal is to confirm these sources asULX characterizetheir spectral shape and variability and to perform a deeper X-ray study forthe most secure ofthese newly discovered ULX. [truncated! Please see actual data for full text]
DOI: 10.3535/jy8-peb-rmy
title: Crenobia alpina montenigrina (Mrazek, 1904)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/m58-vga-rr1
title: Girardia antillana Kenk, 1941

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-eke3j3a
title: 095186

description: 3C120 is a unique broad-line radio galaxy. Alongside the vast jets launched bythe supermassive black hole in its nucleus 3C120 possesses a compact X-rayemitting corona that irradiates the inner disk. This provides a unique view ofthe inner regions around the black hole in which the jet is launched and thecorona is formed. We propose four monthly 160ks observations of 3C120 withNuSTAR to be coordinated with ongoing monthly VLBA observations of the jet. Twoof these are to be simultaneous with 210ks XMM-Newton observations. Theseobservations will map the accretion geometry and trace the connection betweenthe accretion disk corona and jet. This comprehensive program will give usimportant new insight into how jets are launched by black holes. [truncated! Please see actual data for full text]
DOI: 10.3535/98r-lb3-msm
title: Hydroides alatalateralis (Jones, 1962)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-em0mumb
title: 088403

description: A new ULX was recently discovered in the nearby galaxy NGC 3621 in the archivalXMM-Newton data which shows extremely marked variability - unique among theknown ULXs - reminiscent of the so-called heartbeats a type of variabilitypattern observed in only a handful of systems. The archival data yieldedcontradictory information on the nature of the compact object powering XMMJ111816.0-324910 partly due to the limited quality of the data and to thelimited understanding of the heartbeat phenomenon. We propose a Target ofOpportunity observation of XMM J111816.0-324910 for a total of 120ks to obtaina better understanding of the properties of J1118 by means of detailed spectraland timing analysis. This ToO will be triggered based on approved Swift observations. [truncated! Please see actual data for full text]
DOI: 10.3535/hkp-skl-5gl
title: Filogranella elatensis Ben-Eliahu & Dafni, 1979

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/kh1-ay4-c4y
title: Serpula concharum Langerhans, 1880

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-g5ez5qp
title: 092184

description: Giant radio galaxies (GRGs) whose lobes can extend to megaparsec scales arerarely seen in the centers of galaxy clusters but in these rich environmentsthey raise important questions for AGN feedback models. With most of the energyof the jets dissipated in lobes far outside the cool core do such systemsrepresent a failure mode of feedback? If not how do these sources maintain thethermal balance of the ICM? As only a handful of cluster-central GRGs havemodern X-ray data we propose XMM snapshot observations of 11 GRGs inoptically-identified brightest cluster galaxies to confirm the presence of ahot ICM ascertain its basic properties and establish its morphology and wherepossible determine the thermodynamic state of the cluster core. [truncated! Please see actual data for full text]
DOI: 10.57780/esa-goxtkgh
title: 092065

description: X-ray tails of late-type cluster galaxies are rare. Detailed studies of thesesystems allow better understanding for ram-pressure stripping galaxy evolutionin clusters mixing of the stripped cold ISM with the hot ICM r^antmicro-physics and intracluster SF. Recently we discovered likely the longestX-ray tail ever known in the Virgo cluster. Our new Ha data also show thediffuse Ha emission in the same region spectroscopically confirmed to beassociated with the parent galaxy. We propose a new XMM observation to confirmthe X-ray tail and further explore the X-ray-Ha correlation in poor environmentto compare with that in rich cluster tails. Joint time with VLT/MUSE is alsorequested to study the kinematics and gas ionization conditions of the warm gas in the tail. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613442_d15.v1
title: Additional file 2: of Tankyrase inhibition impairs directional migration and invasion of lung cancer cells by affecting microtubule dynamics and polarity signals

description: Raw data for Fig.Â 1 . (XLSX 41 kb)
DOI: 10.3535/axq-ejt-70a
title: Hyalinoecia tubicola (O.F. Müller, 1776)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/fvr-kh3-qx5
title: Polycelis (Polycelis) pamirensis de Beauchamp, 1961

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-gwrneba
title: 092217

description: The circumgalactic medium (CGM) plays an instrumental role in galaxy evolution.From shallow archival data of Suzaku and XMM we have detected the extended(virgul150 kpc) and massive hot CGM of NGC 3221 an L* star-forming galaxy. There issuggestive evidence of cavities along the minor axis and super-virialtemperature within 100 kpc an indirect imprint of galactic outflow on the hotCGM. We would like to confirm our tentative yet exciting findings with deepdata. We ask for 430 ks XMM-Newton/EPIC time to precisely characterize theradial and angular profiles of surface brightness density temperaturepressure and entropy of the hot CGM of NGC 3221 through imaging spectroscopyand modeling. Our results would set the precedence for studying the hot CGM in the current and next decade. [truncated! Please see actual data for full text]
DOI: 10.3535/2es-xzq-wzq
title: Pseudovermilia fuscostriata ten Hove, 1975

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/s1d-w3p-vq5
title: Euniphysa aculeata Wesenberg-Lund, 1949

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-gxmm3f1
title: 090390

description: The fate of binary or multiple systems can be violent merger events with massexchange and the ejection of large scale outflows. One of the most recentlydiscovered merger candidates is our target TYC 597-735-1 which harbors a bluering nebular surrounding the rapidly rotating central source. A shortserendipitous Chandra observation suggests three X-ray sources associated withTYC 597-735-1. Here we propose a 50 ks follow-up observation to uncover theorigin of the X-ray emission magnetic activity or shocks  as both scenarioshave strong implications for the evolution of stellar merger remnants. [truncated! Please see actual data for full text]
DOI: 10.3535/xxx-jqe-e2m
title: Pomatostegus stellatus (Abildgaard, 1789)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/yab-gzn-lcm
title: Hyalinoecia tubicola (O.F. Müller, 1776)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-hhxqjph
title: 090041

description: The hot corona is central for our understanding of the X-ray emission of activegalactic nuclei (AGN). Beside its importance in fact we have very littleknowledge about the corona. The last years established a new viewing angle as afew observations allowed to observe the building of a hot corona especially inthe context of tidal disruption events. Unfortunately this observations had tofollow an opportunistic approach which substantially limits their significance.Here we propose a systematic monitoring of the building of a corona in ESO253-G003. ESO 253-G003 shows a strongly periodic disruption of its X-rayemission every virgul114 days and subsequent recovery of its X-ray emitting hotcorona within 20 days. This offers a unique opportunity to systematically monitor the raise of a corona. [truncated! Please see actual data for full text]
DOI: 10.3535/l1p-v81-5g3
title: Pseudovermilia fuscostriata ten Hove, 1975

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-hs9gjtk
title: 091659

description: We propose to monitor 1ES 2344+514 to better understand its intermittent extremestates. 1ES 2344+514 is a nearby BL Lac type object known for behaving as anextremely high-frequency peaked BL Lac object (EHBL) occasionally. During anX-ray flare in 1996 a shift of the synchrotron peak to frequencies above3*10**18 Hz was reported suggesting that the EHBL nature is correlated with theflux level. Still the small number of published MWL observations does not allowfor a coherent picture. In fact thanks to recent Xray observations we organizedin 2020 we reveal an EHBL behaviour during low activity while we also foundstrong flaring periods without EHBL characteristics. [truncated! Please see actual data for full text]
DOI: 10.3535/tah-102-w47
title: Gasterosteus

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/yeh-a1y-55c
title: Lagis koreni Malmgren, 1866

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-huvg5ql
title: 092414

description: Constraining the population of intermediate black holes (IMBHs) can help solveone of the long-standing problems in modern astrophysics the origin ofsupermassive black holes (SMBHs). Among the 305 optically selected IMBHcandidates (3e4 and amp lt MBH and amp lt 2e5 MSun) published to date which reside in galaxy centersand appear as weak type-I AGN only 24 are confirmed in X-rays and 23 more areawaiting confirmation with Chandra. We propose an XMM-Newton fulfil program for40 IMBH candidates to probe lower Eddington rates and BHs residing in non-dwarfhost galaxies. Our program will help to understand the masses of seed blackholes in the early Universe. [truncated! Please see actual data for full text]
DOI: 10.3535/019-8nd-kpp
title: Planariidae Stimpson, 1857

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/486-7aj-t4v
title: Nephtys caeca (Fabricius, 1780)

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.57780/esa-i3nfgye
title: 090065

description: The SMC is  hosting  more than a hundred  HMXBs  all  but one with Be companion stars and for half of them pulsations were discovered. During  the calibration  phase  of  the eROSITA  instrument the  Be/X-ray  binaryXMMUJ010429.4-723136 was observed and its pulsations were detected for the firsttime at 164s. The I-band OGLE light curve indicates a brightening of the sourcehappening in 2012 also matching with higher X-ray fluxes measured since then.Only eROSITA performed long observations of the source since 2012 enabling thedetection of pulsations. We are requesting 30ks observations with XMM-Newton inorder to confirm the long term spin-up trend suggested by the eROSITA datapossibly connected with the X-ray and optical brightening of the source from this last decade. [truncated! Please see actual data for full text]
DOI: 10.6084/m9.figshare.c.3613517_d1.v1
title: Additional file 1: of A meta-analysis of public microarray data identifies gene regulatory pathways deregulated in peripheral blood mononuclear cells from individuals with Systemic Lupus Erythematosus compared to those without

description: FDR-corrected p-values. (XLS 110 kb)
DOI: 10.3535/8ph-89b-tc1
title: Azygia lucii (Müller, 1776) Lühe, 1909

description: Digital Specimen for the physical specimen hosted at Naturalis Biodiversity Center.
DOI: 10.3535/sqm-zw8-76z
title: Cloeosiphon aspergillus (Quatrefages, 1865)

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