cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Classification of cosmic structures for galaxies with deep learning: connecting cosmological simulations with observations
Creators: name: Inoue, Shigeki
name: Si, Xiaotian
name: Okamoto, Takashi
name: Nishigaki, Moka
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We explore the capability of deep learning to classify cosmic structures. In cosmological simulations, cosmic volumes are segmented into voids, sheets, filaments and knots, according to the distribution and kinematics of dark matter (DM), and galaxies are also classified according to the segmentation. However, observational studies cannot adopt this classification method using DM. In this study, we demonstrate that deep learning can bridge the gap between simulations and observations. Our models are based on three-dimensional convolutional neural networks and trained with data of the distribution of galaxies in a simulation to deduce the structure classes from the galaxies rather than DM. Our model can predict the class labels as accurate as a previous study using DM distribution for the training and prediction. This means that galaxy distribution can be a substitution for DM for the cosmic-structure classification, and our models using galaxies can be directly applied to wide-field survey observations. When observational restrictions are ignored, our model can classify simulated galaxies into the four classes with an accuracy (macro-averaged $F_{\rm 1}$-score) of 64 per cent. If restrictions such as limiting magnitude are considered, our model can classify SDSS galaxies at $\sim100~{\rm Mpc}$ with an accuracy of 60 per cent. In the binary classification distinguishing void galaxies from the others, our model can achieve an accuracy of 88 per cent.
description: 15 pages (+Appendices), 21 figures, accepted for publication in MNRAS
Four bright eclipsing binaries with gamma Doradus pulsating components: CM Lac, MZ Lac, RX Dra and V2077 Cyg
Creators: name: Southworth, John
name: Van Reeth, Timothy
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The study of pulsating stars in eclipsing binaries holds the promise of combining two different ways of measuring the physical properties of a star to obtain improved constraints on stellar theory. Gravity (g) mode pulsations such as those found in $γ$ Doradus stars can be used to probe rotational profiles, mixing and magnetic fields. Until recently few $γ$ Doradus stars in eclipsing binaries were known. We have discovered g-mode pulsations in four detached eclipsing binary systems from light curves obtained by the Transiting Exoplanet Survey Satellite (TESS) and present an analysis of their eclipses and pulsational characteristics. We find unresolved g-mode pulsations at frequencies 1--1.5 d$^{-1}$ in CM Lac, and measure the masses and radii of the component stars from the TESS data and published radial velocities. MZ Lac shows a much richer frequency spectrum, including pressure modes and tidally-excited g-modes. RX Dra is in the northern continuous viewing zone of TESS so has a light curve covering a full year, but shows relatively few pulsation frequencies. For V2077 Cyg we formally measure four pulsation frequencies, but the available data are inadequate to properly resolve the g-mode pulsations. V2077 Cyg also shows total eclipses, with which we obtain the first measurement of the surface gravity of the faint secondary star. All four systems are bright and good candidates for detailed study. Further TESS observations are scheduled for all four systems, with much improved temporal baselines in the cases of RX Dra and V2077 Cyg.
description: Accepted for publication in MNRAS. 11 pages, 8 figures, 5 tables. This is the authors' version of the accepted manuscript
Achillea distans Willd.
Creators: name: Info Flora
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Asteraceae
Achillea
Achillea distans

description: Achillea distans Willd.
Rainfarn-Wiesen-Schafgarbe
Art ISFS: 1300 Checklist: 1000250 Asteraceae Achillea Achillea millefolium aggr. Achillea distans Willd.
Bestimmungsschlüssel
Zusammenfassung
Artbeschreibung (nach Lauber & al. 2018): 20-80 cm hoch. Grundständige Blätter 3-8 cm breit. An den obersten 12 cm des Stängels unter dem Blütenstand 2-6 Blätter. Mittelrippe der Stängelblätter 2-4 mm breit, geflügelt und gezähnt. Blattabschnitte flach ausgebreitet, kaum bis über die Mitte geteilt, Zipfel und Zähne 0,3- 1 mm breit, 3eckig. Zungenblüten hellrosa bis purpurn. Früchte 2,5- 3 mm lang.
Blütezeit (nach Lauber & al. 2018): 7-8
Standort und Verbreitung in der Schweiz (nach Lauber & al. 2018): Lichte Wälder, Gebüsche / montan-alpin / Südliches TI (Generoso?)
Verbreitung global (nach Lauber & al. 2018): Mittel- und südosteuropäisch
Ökologische Zeigerwerte (nach Landolt & al. 2010) 334-32 + 3.h.2n=54
Ökologie
Lebensform Mehrjähriger Hemikryptophyt
Lebensraum Lebensraumnach Delarze & al. 2015
KEINE ANGABE
Ökologische Zeigerwerte nach Landolt & al. (2010)
BodenfaktorenKlimafaktorenSalztoleranzFeuchtezahl Fmässig feuchtLichtzahl LhalbschattigSalzzeichen--Reaktionszahl Rschwach sauer bis neutral (pH 4.5-7.5)Temperaturzahl Tunter-subalpin und ober-montanNährstoffzahl NnährstoffreichKontinentalitätszahl Ksubozeanisch bis subkontinental (mittlere Luftfeuchtigkeit, mässige Temperaturschwankungen und mässig tiefe Wintertemperaturen)
Nomenklatur
Gültiger Name (Checklist 2017):Achillea distansWilld.
Volksname Deutscher Name: Rainfarn-Wiesen-Schafgarbe Nom français: Achillée distante
Nome italiano: --
Übereinstimmung mit anderen Referenzwerken
RelationNomReferenzwerkeNo=Achillea distans Willd.Checklist 20171300=Achillea distans Willd.Flora Helvetica 20012122=Achillea distans Willd.Flora Helvetica 20122110=Achillea distans Willd.Flora Helvetica 20182110=Achillea distans Willd.Index synonymique 19961300=Achillea distans Willd.Landolt 19773178=Achillea distans Willd.SISF/ISFS 21300
= Taxon stimmt mit akzeptiertem Taxon überein (Checklist 2017)  Taxon enthält (neben anderen) auch das akzeptierte Taxon (Checklist 2017)
Status Indigenat: -
Liste der gefährdeten Pflanzen IUCN(nach Walter & Gillett 1997): Nein
description: Published as part of Info Flora, 2021,
Achillea erba-rotta All.
Creators: name: Info Flora
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Asteraceae
Achillea
Achillea erba-Rotta

description: Achillea erba-rotta All.
Art ISFS: 1350 Checklist: 1000260 Asteraceae Achillea Achillea erba-rotta All. Enthält: Achillea erba-rotta All. subsp. erba-rotta Achillea erba-rotta subsp. moschata (Wulfen) Vacc.
Bestimmungsschlüssel
ZusammenfassungKEINE ANGABE Status
Status IUCN: Nicht gefährdet
Nationale Priorität: 4 - Mässige nationale Priorität
Internationale Verantwortung: 3 - Hoch
Ökologie
Lebensraum Lebensraumnach Delarze & al. 2015
KEINE ANGABE
Ökologische Zeigerwerte nach Landolt & al. (2010)
BodenfaktorenKlimafaktorenSalztoleranzFeuchtezahl F--Lichtzahl L--Salzzeichen--Reaktionszahl R--Temperaturzahl T--Nährstoffzahl N--Kontinentalitätszahl K--
Nomenklatur
Gültiger Name (Checklist 2017):Achillea erba-rottaAll.
Volksname
Deutscher Name: -- Nom français: -- Nome italiano: --
Übereinstimmung mit anderen Referenzwerken
RelationNomReferenzwerkeNo=Achillea erba-rotta All.Checklist 20171350=Achillea erba-rotta All. s.l.SISF/ISFS 21350
= Taxon stimmt mit akzeptiertem Taxon überein (Checklist 2017)  Taxon enthält (neben anderen) auch das akzeptierte Taxon (Checklist 2017)
Kommentare aus der Checklist 2017 Wegfall des Ausdrucks s.l.: Die Art wurde bisher als "sensu lato" (s.l.) gekennzeichnet. Da die früher gleichlautende "sensu stricto-Art" (s.str.) in eine Unterart umbenannt wurde, erübrigt sich die Kennzeichnung s.l. Checklist
Status Indigenat: Indigen
Liste der gefährdeten Pflanzen IUCN(nach Walter & Gillett 1997): Nein
Status Rote Liste national 2016
Status IUCN: Nicht gefährdet
Zusätzliche InformationenKriterien IUCN: --
Status Rote Liste regional 2019
Biogeografische RegionenStatusKriterien IUCN
Status nationale Priorität /Verantwortung
Nationale Priorität4 - Mässige nationale PrioritätMassnahmenbedarf0 - Kein MassnahmebedarfInternationale Verantwortung3 - HochÜberwachung Bestände0 - Überwachung ist nicht nötig
Schutzstatus
Kein internationaler, nationaler oder kantonaler Schutz
description: Published as part of Info Flora, 2021,
Funambulus sublineatus
Creators: name: Wilson, Don E.
name: Thomas E. Lacher, Jr
name: Mittermeier, Russell A.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Funambulus
Funambulus sublineatus

description: 9. Dusky Palm Squirrel Funambulus sublineatus French: Ecureuil sombre / German: Dunkles Palmenhérnchen / Spanish: Ardilla de palma oscura Other common names: Dusky-striped Squirrel Taxonomy. Sciurus sublineatus Waterhouse, 1838, Nilgiri Hills, Madras, India. Two subspecies are recognized. Subspecies and Distribution. F.s.sublineatusWaterhouse,1838—SWIndia. F.s. obscurus Pelzeln & Kohl, 1886 — Sri Lanka. Descriptive notes. Head-body 110-130 mm, tail 94-135 mm; weight mean 44.1 g. The Dusky Palm Squirrel is the smallest species of the genus. It has three dorsal stripes, obscured by long brown fur. Venter is dull and drab andtail lacks a red mid-ventral stripe. Subspecies sublineatus has narrower dark brown stripes (3-5 mm) between the pale dorsal stripes than obscurus (6-8 mm). Habitat. Forests from near sea level to above ¢.2100 m. Near the Palni Mountains, in southern India, the Dusky Palm Squirrelis found in elevations of ¢.1372-2134 m,this is above elevations inhabited by the Indian Palm Squirrel (E palmarum). In Sri Lanka, it occurs in forest hills at elevations above ¢.610 m, but in the south-western part of the island it can be found in forests of the wet hilly country almostat sea level. Food and Feeding. There is no information available for this species. Breeding. There is no specific information available for this species, but one litter of the Dusky Palm Squirrel was recorded as consisting of two young. Activity patterns. There is no specific information available for this species, but the Dusky Palm Squirrel is diurnal and semi-arboreal, mostly within the scrub level ofthe forest. Movements, Home range and Social organization. There is no information available for this species. Status and Conservation. Classified as Vulnerable on The IUCN Red List. The Dusky Palm Squirrel has a severely fragmented distribution and is confined to riparian habitats, which are in a continuous decline. Major threats are habitat loss and degradation due to selective logging, reed collection for construction purposes, and forest fires, and the use of pesticides. The Dusky Palm Squirrel is not protected by any legislation. Bibliography. Hayssen et al. (1993), Johnsingh & Manjrekar (2015), Jordan et al. (2005h), Phillips (1980), Prater (1965), Rajamani et al. (2008a), Thorington et al. (2012).
description: Published as part of Don E. Wilson, Thomas E. Lacher, Jr & Russell A. Mittermeier, 2016, Sciuridae, pp. 648-837 in Handbook of the Mammals of the World – Volume 6 Lagomorphs and Rodents I, Barcelona :Lynx Edicions on page 716, DOI: 10.5281/zenodo.6840226
Radial velocities from far red spectra of Carina Arm O and early B stars
Creators: name: Drew, Janet E.
name: Parsons, Flora Blake
name: Mohr-Smith, Michael
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Massive O and early B stars are important markers of recent star formation and exert a significant influence on their environments during their short lives via photoionization and winds and when they explode as supernovae. In the Milky Way they can be detected at great distances but often lie behind large dust columns, making detection at short wavelengths difficult. In this study the use of the less extinguished far-red spectrum (8400 -- 8800 Å) for radial velocity measurement is examined. Results are reported for a sample of 164 confirmed OB stars within a 2-degree field positioned on the Carina Arm. Most stars are at distances between 3 and 6 kpc, and Westerlund 2 is at the field edge. The measured radial velocities have errors concentrated in the 3--10 km s$^{-1}$ range, with a systematic uncertainty of 2--3 km s$^{-1}$. These are combined with Gaia-mission astrometry to allow full space motions to be constructed. Up to 22 stars are likely to be runaways although 8 of them are as likely to be interloping (so far undetected) binaries. The mean azimuthal motion of the sample fits in with recent measurements of Galactic disk rotation. In the Galactocentric radial direction the mean motion indicates modest infall at a speed of $\sim$ 10 km s$^{-1}$. This experiment shows that weak Paschen lines in the far-red can yield credible radial velocity determination, offering the prospect of exploring OB-star kinematics over much more of the Galactic disk than has hitherto been possible.
description: 15 pages, 13 figures, 2 appendices -- accepted for publication in MNRAS, 19th July 2022
A transient ultraluminous X-ray source in NGC 55
Creators: name: Robba, A.
name: Pinto, C.
name: Pintore, F.
name: Rodriguez, G.
name: Ambrosi, E.
name: Barra, F.
name: Cusumano, G.
name: D'Aì, A.
name: Del Santo, M.
name: Kosec, P.
name: Marino, A.
name: Middleton, M.
name: Roberts, T.
name: Salvaggio, C.
name: Soria, R.
name: Wolter, A.
name: Walton, D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10$^{39}$ erg s$^{-1}$. The average number of ULXs per galaxy is still not well constrained, especially given the uncertainty on the fraction of ULX transients. Here, we report the identification of a new transient ULX in the galaxy NGC 55 (which we label as ULX-2), thanks to recent XMM-Newton and the Neil Gehrels Swift Observatory observations. This object was previously classified as a transient X-ray source with a luminosity around a few 10$^{38}$ erg s$^{-1}$ in a 2010 XMM-Newton observation. Thanks to new and deeper observations ($\sim$ 130 ks each), we show that the source reaches a luminosity peak $>1.6 \times 10^{39}$ erg s$^{-1}$. The X-ray spectrum of ULX-2 is much softer than in previous observations and fits in the class of soft ULXs. It can be well described using a model with two thermal components, as often found in ULXs. The time scales of the X-ray variability are of the order of a month and are likely driven by small changes in the accretion rate or due to super-orbital modulations, attributed to precession of the accretion disc, which is similar to other ULXs.
description: 6 pages, including 4 figures and 2 tables, accepted for pubblication in MNRAS
Achillea erba-rotta subsp. erba-rotta
Creators: name: Info Flora
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Asteraceae
Achillea
Achillea erba-Rotta
Achillea erba-Rotta all. subsp. erba-Rotta

description: Achillea erba-rotta All. subsp. erba-rotta
Unterart ISFS: 1400 Checklist: 1000270 Asteraceae Achillea Achillea erba-rotta All. Achillea erba-rotta All. subsp. erba-rotta
Bestimmungsschlüssel
ZusammenfassungKEINE ANGABE
Ökologie
Lebensraum Lebensraumnach Delarze & al. 2015
KEINE ANGABE
Ökologische Zeigerwerte nach Landolt & al. (2010)
BodenfaktorenKlimafaktorenSalztoleranzFeuchtezahl F--Lichtzahl L--Salzzeichen--Reaktionszahl R--Temperaturzahl T--Nährstoffzahl N--Kontinentalitätszahl K--
Nomenklatur
Gültiger Name (Checklist 2017):Achillea erba-rottaAll. subsp.erba-rotta
Volksname
Deutscher Name: -- Nom français: -- Nome italiano: --
Übereinstimmung mit anderen Referenzwerken
RelationNomReferenzwerkeNo=Achillea erba-rotta All. subsp. erba-rottaChecklist 20171400=Achillea erba-rotta All. s.str.Index synonymique 19961400=Achillea erba-rotta All. s.str.Landolt 19773184=Achillea erba-rotta All. s.str.SISF/ISFS 21400
= Taxon stimmt mit akzeptiertem Taxon überein (Checklist 2017)  Taxon enthält (neben anderen) auch das akzeptierte Taxon (Checklist 2017)
Kommentare aus der Checklist 2017 Wegfall des Ausdrucks s.str.: Alle "im engeren Sinn" (sensu stricto, s.str.) gefassten Arten werden neu in Unterarten mit gleichlautendem Unterart-Epithet gefasst (autonyme Unterart). Checklist
Status Indigenat: -
Liste der gefährdeten Pflanzen IUCN(nach Walter & Gillett 1997): Nein
description: Published as part of Info Flora, 2021,
Prosciurillus leucomus
Creators: name: Wilson, Don E.
name: Thomas E. Lacher, Jr
name: Mittermeier, Russell A.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Prosciurillus
Prosciurillus leucomus

description: 19. Whitsh Dwart Squirrel Prosciurillus leucomus French: Ecureuil givré / German: WeiRliches Sulawesi-Zwerghdrnchen / Spanish: Ardilla enana blanquecina Taxonomy. Sciurus leucomus S. Muller & Schlegel, 1844, “Celebes.” Restricted by A. B. Meyer in 1898 to Minahassa, northeast of Celebes (= Sulawesi), Indonesia. Two subspecies are recognized. Subspecies and Distribution. P.l.leucomusS.Muller&Schlegel,1844—NSulawesi(NpeninsulaandNCentralSulawesiProvinceexceptWofGorontaloProvince)andLembehI. P. l. occidentalis Meyer, 1898 — N Sulawesi (W of Gorontalo Province). Descriptive notes. Head-body 165-188 mm, tail 140-190 mm. No specific data are available for body weight. Dorsum of the Whitish Dwarf Squirrel is olive-brown, sometimes flecked with orange, buff, or black. Venter is reddish orange or ocherous, and tail is ringed black and buff with a black tuft at tip. Ears are black outside, with a prominent ear tuft, and bright ocherous inside. Habitat. Coastal lowlands and montane forests up to ¢.1700 m. Food and Feeding. There is no specific information available for this species, but it is thought that the Whitish Dwarf Squirrel consumes soft fruits and insects. Breeding. There is no specific information available for this species, but female Whitish Dwarf Squirrels have three pairs of teats, two inguinal and one post-axillary. Activity patterns. There is no specific information available for this species, but the Whitish Dwarf Squirrel appears to dwell in upper forest canopy. Movements, Home range and Social organization. There is no information available for this species. Status and Conservation. Classified as Data Deficient on The IUCN Red List. There is no sufficient information on the population size and trend for the Whitish Dwarf Squirrel. It is a forest obligate species that occurs at low densities and is threatened by habitat loss due to forest clearing. Bibliography. Meyer (1898), Musser et al. (2010), Ruedas & Suyanto (2008b), Thorington et al. (2012).
description: Published as part of Don E. Wilson, Thomas E. Lacher, Jr & Russell A. Mittermeier, 2016, Sciuridae, pp. 648-837 in Handbook of the Mammals of the World – Volume 6 Lagomorphs and Rodents I, Barcelona :Lynx Edicions on page 718, DOI: 10.5281/zenodo.6840226
Companion Mass Limits for 17 Binary Systems Obtained with Binary Differential Imaging and MagAO/Clio
Creators: name: Pearce, Logan A.
name: Males, Jared R.
name: Weinberger, Alycia J.
name: Long, Joseph D.
name: Morzinski, Katie M.
name: Close, Laird M.
name: Hinz, Philip M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Improving direct detection capability close to the star through improved star-subtraction and post-processing techniques is vital for discovering new low-mass companions and characterizing known ones at longer wavelengths. We present results of 17 binary star systems observed with the Magellan Adaptive Optics system (MagAO) and the Clio infrared camera on the Magellan Clay Telescope using Binary Differential Imaging (BDI). BDI is an application of Reference Differential Imaging (RDI) and Angular Differential Imaging (ADI) applied to wide binary star systems (2\arcsec $<Δρ<$ 10\arcsec) within the isoplanatic patch in the infrared. Each star serves as the point-spread-function (PSF) reference for the other, and we performed PSF estimation and subtraction using Principal Component Analysis. We report contrast and mass limits for the 35 stars in our initial survey using BDI with MagAO/Clio in L$^\prime$ and 3.95$μ$m bands. Our achieved contrasts varied between systems, and spanned a range of contrasts from 3.0-7.5 magnitudes and a range of separations from 0.2\arcsec to $\sim$2\arcsec. Stars in our survey span a range of masses, and our achieved contrasts correspond to late-type M dwarf masses down to $\sim$10 M$_{\rm{jup}}$. We also report detection of a candidate companion signal at 0.2\arcsec (18 AU) around HIP 67506 A (SpT G5V, mass $\sim$1.2\Msun), which we estimate to be ~60-90 M$_{\rm{jup}}$. We found that the effectiveness of BDI is highest for approximately equal brightness binaries in high-Strehl conditions.
description: 25 pages, 8 figures, 3 tables; Accepted to MNRAS
CLINICAL AND COMPUTER DIAGNOSTICS OF CONGENITAL ATRESIA OF THE EXTERNAL AUDITORY CANAL IN CHILDREN
Creators: name: Yusupova, S.R.
Publisher: name: Zenodo
Year: 2024

description: The results of computer studies of children with congenital atresia of the external auditory canal and an assessment of the types of hearing impairment are presented.

The studies were conducted in 67 children with congenital atresia of the external auditory canal in combination with an anomaly of the middle ear, aged from 1 to 16 years. Anomalies of the inner ear in children with atresia of the external auditory canal were identified in 4.5% cases. Among them: stenosis of the internal auditory canal - 1.5%, common cavity of the cochlea and vestibule - 1.5%, anomaly of the vestibule and semicircular canals - 1.5%.

Computer tomography of the temporal bones is a highly effective method for studying developmental anomalies of the external and middle ear in children, allowing to diagnose not only malformations of the external auditory canal, tympanic cavity, auditory ossicles, labyrinthine windows, facial nerve canal, but also structures of the inner ear.
Achillea filipendulina Lam.
Creators: name: Info Flora
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Asteraceae
Achillea
Achillea filipendulina

description: Achillea filipendulina Lam.
Gold-Schafgarbe
Art ISFS: 1550 Checklist: 1000300 Asteraceae Achillea Achillea filipendulina Lam.
Bestimmungsschlüssel
Zusammenfassung
Artbeschreibung (nach Lauber & al. 2018): 50-130 cm hoch, dünn anliegend behaart. Blätter fiederschnittig, Abschnitte gesägt. Blütenköpfe 50-500, in einer dichten, endständigen, 4-10 cm breiten Doldenrispe. Zungenblüten gelb.
Blütezeit (nach Lauber & al. 2018): 6-8
Standort und Verbreitung in der Schweiz (nach Lauber & al. 2018): Verwilderte Zierpflanze, Ruderalstellen /
Verbreitung global (nach Lauber & al. 2018): Kaukasisch
Ökologische Zeigerwerte (nach Landolt & al. 2010) 3 + w43-44 + 4.h
Ökologie
Lebensraum Lebensraumnach Delarze & al. 2015
KEINE ANGABE
Ökologische Zeigerwerte nach Landolt & al. (2010)
BodenfaktorenKlimafaktorenSalztoleranzFeuchtezahl F--Lichtzahl L--Salzzeichen--Reaktionszahl R--Temperaturzahl T--Nährstoffzahl N--Kontinentalitätszahl K--
Nomenklatur
Gültiger Name (Checklist 2017):Achillea filipendulinaLam.
Volksname Deutscher Name: Gold-Schafgarbe Nom français: Achillée à feuilles de fougère Nome italiano: Millefoglio a foglie di Filipendula
Übereinstimmung mit anderen Referenzwerken
RelationNomReferenzwerkeNo=Achillea filipendulina Lam.Checklist 20171550
= Taxon stimmt mit akzeptiertem Taxon überein (Checklist 2017)  Taxon enthält (neben anderen) auch das akzeptierte Taxon (Checklist 2017)
Kommentare aus der Checklist 2017 Neues Taxon: Gegenüber SISF-2 neu aufgenommener Neophyt. Checklist
Status Indigenat: Neophyt: nach der Entdeckung von Amerika in der Region aufgetreten (nach 1500)
Liste der gefährdeten Pflanzen IUCN(nach Walter & Gillett 1997): Nein
description: Published as part of Info Flora, 2021,
Schools as Community Hubs Development Framework: Workshop 2, Insights from Canada and the USA
Creators: name: CHANDLER, PHILIPPA
name: Cleveland, Benjamin
Publisher: name: University of Melbourne
Year: 2021
Subjects: Community planning

description: Insights from a research workshop (April 2021) with participants from Canada and the USA, examining the context, enablers and barriers to developing, implementing and sustaining schools as community hubs.
Linear change and minutes variability of solar wind velocity revealed by FAST
Creators: name: Liu, Li-Jia
name: Peng, Bo
name: Yu, Lei
name: Liu, Bin
name: Lu, Ji-Guang
name: Yu, Ye-Zhao
name: Xi, Hong-Wei
name: Xiong, Ming
name: Chang, O.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Observation of Interplanetary Scintillation (IPS) provides an important and effective way to study the solar wind and the space weather. A series of IPS observations were conducted by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The extraordinary sensitivity and the wide frequency coverage make FAST an ideal platform for IPS studies. In this paper we present some first scientific results from FAST observations of IPS with the L-band receiver. Based on the solar wind velocity fitting values of FAST observations on September 26-28, 2020, we found that the velocity decreases with increasing frequency linearly, which has not yet been reported in literature. And we have also detected a variation of solar wind velocity on a timescale of 3-5 minutes, which imply the slow change of the background solar wind, a co-existence of high- and low-speed streams, or a reflect of the quasi-periodic electron-density fluctuations.
description: 6 pages, 6 figures
Schools as Community Hubs Development Framework: Workshop 3, Insights from Europe and the UK
Creators: name: CHANDLER, PHILIPPA
name: Cleveland, Benjamin
Publisher: name: University of Melbourne
Year: 2022
Subjects: Community planning

description: Insights from a research workshop (April 2021) with participants from Europe and the UK, examining the context, enablers and barriers to developing, implementing and sustaining schools as community hubs.
Achillea millefolium subsp. millefolium
Creators: name: Info Flora
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Asteraceae
Achillea
Achillea millefolium
Achillea millefolium l. subsp. millefolium

description: Achillea millefolium L. subsp. millefolium
Unterart ISFS: 1701 Checklist: 1000340 Asteraceae Achillea Achillea millefolium aggr. Achillea millefolium L. Achillea millefolium L. subsp. millefolium
Bestimmungsschlüssel
ZusammenfassungKEINE ANGABE
Status Nationale Priorität: --
Internationale Verantwortung: --
Ökologie
Lebensraum Lebensraumnach Delarze & al. 2015
KEINE ANGABE
Ökologische Zeigerwerte nach Landolt & al. (2010)
BodenfaktorenKlimafaktorenSalztoleranzFeuchtezahl F--Lichtzahl L--Salzzeichen--Reaktionszahl R--Temperaturzahl T--Nährstoffzahl N--Kontinentalitätszahl K--
Nomenklatur
Gültiger Name (Checklist 2017):Achillea millefoliumL. subsp.millefolium
Volksname
Deutscher Name: -- Nom français: -- Nome italiano: --
Übereinstimmung mit anderen Referenzwerken
RelationNomReferenzwerkeNo=Achillea millefolium L. subsp. millefoliumChecklist 20171701=Achillea millefolium L. s.str.SISF/ISFS 21701
= Taxon stimmt mit akzeptiertem Taxon überein (Checklist 2017)  Taxon enthält (neben anderen) auch das akzeptierte Taxon (Checklist 2017)
Kommentare aus der Checklist 2017 Wegfall des Ausdrucks s.str.: Alle "im engeren Sinn" (sensu stricto, s.str.) gefassten Arten werden neu in Unterarten mit gleichlautendem Unterart-Epithet gefasst (autonyme Unterart). Checklist
Status Indigenat: Indigen
Liste der gefährdeten Pflanzen IUCN(nach Walter & Gillett 1997): Nein Status Rote Liste national
KEINE ANGABE
Status nationale Priorität /Verantwortung
Nationale Priorität--Massnahmenbedarf--Internationale Verantwortung--Überwachung Bestände--
Schutzstatus
Kein internationaler, nationaler oder kantonaler Schutz
description: Published as part of Info Flora, 2021,
Achillea millefolium
Creators: name: Info Flora
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Asteraceae
Achillea
Achillea millefolium

description: Achillea millefolium aggr.
Wiesen-Schafgarbe
Art ISFS: 1706 Checklist: 1000320 Asteraceae Achillea Achillea millefolium aggr. Enthält: Achillea collina Rchb. Achillea distans Willd. Achillea millefolium L. Achillea pratensis Saukel & R. Länger Achillea roseoalba Ehrend. Achillea setacea Waldst. & Kit. Achillea stricta Gremli
Bestimmungsschlüssel
Zusammenfassung
Artbeschreibung (nach Lauber & al. 2018): 15-80 cm hoch, nur im Blütenstand verzweigt, kurz behaart bis kahl. Blätter im Umriss lanzettlich bis lineal-lanzettlich, bis fast zum Mittelnerv 2-3fach fein fiederschnittig, jederseits mit 12-50 Abschnitten. Blütenköpfe zahlreich, in einer endständigen Doldenrispe. Durchmesser 4-8 mm, mit 4-6 Zungenblüten, innere Blüten röhrenförmig. Früchte eiförmig, ohne Pappus.
Status
Status IUCN: Nicht gefährdet
Ökologie
Lebensraum Lebensraumnach Delarze & al. 2015
KEINE ANGABE
Ökologische Zeigerwerte nach Landolt & al. (2010)
BodenfaktorenKlimafaktorenSalztoleranzFeuchtezahl F--Lichtzahl L--Salzzeichen--Reaktionszahl R--Temperaturzahl T--Nährstoffzahl N--Kontinentalitätszahl K--
Nomenklatur
Gültiger Name (Checklist 2017):Achillea millefoliumaggr.
Volksname Deutscher Name: Wiesen-Schafgarbe Nom français: Achillée millefeuille Nome italiano: Millefoglio montano
Übereinstimmung mit anderen Referenzwerken
RelationNomReferenzwerkeNo=Achillea millefolium aggr.Checklist 20171706=Achillea millefolium aggr.Flora Helvetica 20182105-2110<Achillea millefolium aggr.SISF/ISFS 21705
= Taxon stimmt mit akzeptiertem Taxon überein (Checklist 2017)  Taxon enthält (neben anderen) auch das akzeptierte Taxon (Checklist 2017)
Kommentare aus der Checklist 2017 Neues taxonomisches Konzept: Das neue Aggregat wird breiter als im SISF-2 gefasst, denn es enthält neu die zusätzliche Art A. pratensis Saukel & R. Länger. Checklist
Status Indigenat: Indigen
Liste der gefährdeten Pflanzen IUCN(nach Walter & Gillett 1997): Nein
Status Rote Liste national 2016
Status IUCN: Nicht gefährdet
Zusätzliche InformationenKriterien IUCN: --
Status Rote Liste regional 2019
Biogeografische RegionenStatusKriterien IUCNJura (JU)nicht gefährdet (Least Concern)Mittelland (MP)nicht gefährdet (Least Concern)Alpennordflanke (NA)nicht gefährdet (Least Concern)Alpensüdflanke (SA)nicht gefährdet (Least Concern)Östliche Zentralalpen (EA)nicht gefährdet (Least Concern)Westliche Zentralalpen (WA)nicht gefährdet (Least Concern)
Status nationale Priorität /Verantwortung
Keine nationale Priorität oder internationale Verantwortung
Schutzstatus
Kein internationaler, nationaler oder kantonaler Schutz
description: Published as part of Info Flora, 2021,
Gravitational wave of intermediate-mass black holes in Population III star clusters
Creators: name: Wang, Long
name: Tanikawa, Ataru
name: Fujii, Michiko
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Previous theoretical studies suggest that the Population III (Pop3) stars tend to form in extremely metal poor gas clouds with approximately $10^5 M_\odot$ embedded in mini dark matter halos. Very massive stars can form via multiple collisions in Pop3 star clusters and eventually evolve to intermediate-mass black holes (IMBHs). In this work, we conduct star-by-star $N$-body simulations for modelling the long-term evolution of Pop3 star clusters. We find that if the mini dark matter halos can survive today, these star clusters can avoid tidal disruption by the galactic environment and can efficiently produce IMBH-BH mergers among a wide range of redshift from 0 to 20. The average gravitational wave event rate is estimated to be $0.1-0.8~\mathrm{yr}^{-1} \mathrm{Gpc}^{-3}$, and approximately $40-80$ percent of the mergers occur at high redshift ($z>6$). The characteristic strain shows that a part of low-redshift mergers can be detected by LISA, TianQin, and Taiji, whereas most mergers can be covered by DECIGO and advanced LIGO/VIRGO/Kagra. Mergers with pair-instability BHs have a rate of approximately $0.01-0.15$~yr$^{-1}$~Gpc$^{-3}$, which can explain the GW190521-like events.
description: 15 pages, 11 figures, 4 tables, accepted for MNRAS
A new reference catalogue for the very metal-poor Universe: +150 OB stars in Sextans A
Creators: name: Lorenzo, Marta
name: Garcia, Miriam
name: Najarro, Francisco
name: Herrero, Artemio
name: Cerviño, Miguel
name: Castro, Norberto
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Local Group (LG) very metal-poor massive stars are the best proxy for the First Stars of the Universe and fundamental to modelling the evolution of early galaxies. These stars may follow new evolutionary pathways restricted to very low metallicities, such as chemically homogeneous evolution (CHE). However, given the great distance leap needed to reach very metal-poor galaxies of the LG and vicinity, no comprehensive spectroscopic studies have been carried out at metallicities lower than the Small Magellanic Cloud (SMC, Z = 1/5 Z$_{\odot}$) until now. After five observing campaigns at the 10.4-m Gran Telescopio Canarias, we have assembled a low-resolution (R $\sim$ 1000) spectroscopic collection of more than 150 OB stars in the 1/10 Z$_{\odot}$ galaxy Sextans A, increasing by an order of magnitude the number of massive stars known in this galaxy. The catalogue includes 38 BA-type supergiants, 4 red supergiants, and the first candidate 1/10 Z$_{\odot}$ binary systems, CHE sources and systems hosting stripped stars. The sample massive stars mainly overlap the higher concentrations of neutral gas of Sextans A. However, we find some sources in low HI column-density regions. The colour-magnitude diagram of the galaxy presents large dispersion, which suggests uneven, internal extinction in Sextans A. This is the largest catalogue of OB-type stars ever produced at sub-SMC metallicities. This sample constitutes a fundamental first step to unveiling the evolutionary pathways and fates of very metal-poor massive stars, analyzing the dependence of radiation-driven winds with metallicity, and studying binary systems in an environment analogue to the early Universe.
description: 56 pages, 39 figures Accepted in the Monthly Notices of the Royal Astronomical Society
Achillea millefolium subsp. sudetica J. Weiss
Creators: name: Info Flora
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Asterales
Asteraceae
Achillea
Achillea millefolium
Achillea millefolium subsp. sudetica (opiz) j. weiss

description: Achillea millefolium subsp. sudetica (Opiz) J. Weiss
Unterart ISFS: 1702 Checklist: 1000350 Asteraceae Achillea Achillea millefolium aggr. Achillea millefolium L. Achillea millefolium subsp. sudetica (Opiz) J. Weiss
Bestimmungsschlüssel
ZusammenfassungKEINE ANGABE
Status Nationale Priorität: --
Internationale Verantwortung: --
Ökologie
Lebensraum Lebensraumnach Delarze & al. 2015
KEINE ANGABE
Ökologische Zeigerwerte nach Landolt & al. (2010)
BodenfaktorenKlimafaktorenSalztoleranzFeuchtezahl F--Lichtzahl L--Salzzeichen--Reaktionszahl R--Temperaturzahl T--Nährstoffzahl N--Kontinentalitätszahl K--
Nomenklatur
Gültiger Name (Checklist 2017):Achillea millefoliumsubsp.sudetica(Opiz) J. Weiss
Volksname
Deutscher Name: -- Nom français: -- Nome italiano: --
Übereinstimmung mit anderen Referenzwerken
RelationNomReferenzwerkeNo=Achillea millefolium subsp. sudetica (Opiz) J. WeissChecklist 20171702=Achillea millefolium subsp. sudetica (Opiz) J. WeissSISF/ISFS 21702
= Taxon stimmt mit akzeptiertem Taxon überein (Checklist 2017)  Taxon enthält (neben anderen) auch das akzeptierte Taxon (Checklist 2017)
Status Indigenat: Indigen
Liste der gefährdeten Pflanzen IUCN(nach Walter & Gillett 1997): Nein Status Rote Liste national
KEINE ANGABE
Status nationale Priorität /Verantwortung
Nationale Priorität--Massnahmenbedarf--Internationale Verantwortung--Überwachung Bestände--
Schutzstatus
Kein internationaler, nationaler oder kantonaler Schutz
description: Published as part of Info Flora, 2021,
A Probabilistic Method of Background Removal for High Energy Astrophysics Data
Creators: name: Ehlert, Steven
name: Chen, Chien-Ting
name: Swartz, Doug A.
name: Hickox, Ryan C.
name: Lutovinov, Alexander A.
name: Semena, Andrey N.
name: Krivonos, Roman
name: Shtykovsky, Andrey E.
name: Tkachenko, Alexey
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a new statistical method for constructing background subtracted measurements from event list data gathered by X-ray and gamma ray observatories. This method was initially developed specifically to construct images that account for the high background fraction and low overall count rates observed in survey data from the Mikhail Pavlinsky ART-XC telescope aboard the Spektrum Röntgen Gamma (SRG) mission, although the mathematical underpinnings are valid for data taken with other imaging missions and analysis applications. This method fully accounts for the expected Poisson fluctuations in both the sky photon and non X-ray background count rates in a manner that does not result in unphysical negative counts. We derive the formulae for arbitrary confidence intervals for the source counts and show that our new measurement converges exactly to the standard background subtraction calculation in the high signal limit. Utilizing these results, we discuss several variants of images designed to optimize different science goals for both pointed and slewing telescopes. Using realistic simulated data of a galaxy cluster as observed by ART-XC we show that our method provides a more significant and robust detection of the cluster emission as compared to a standard background subtraction. We also demonstrate its advantages using real observations of a point source from the ART-XC telescope. These calculations may have widespread applications for a number of source classes observed with high energy telescopes.
description: 15 pages, 9 figures, Accepted for Publication in MNRAS
Tamiops rodolphii
Creators: name: Wilson, Don E.
name: Thomas E. Lacher, Jr
name: Mittermeier, Russell A.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Tamiops
Tamiops rodolphii

description: 27. Cambodian Striped Squirrel Tamiops rodolphii French: Ecureuil du Cambodge / German: Kambodscha-Zwergstreifenhérnchen / Spanish: Ardilla rayada de Camboya Taxonomy. Sciurus (Tamias) rodolphii Milne-Edwards, 1867, “near Saigon, Cochin Chi- na,” Vietnam. Two subspecies are recognized. Subspecies and Distribution. T. r. rodolphi Milne-Edwards, 1867 — Viet- nam, C & S Laos, SE Thailand, and Cam- bodia. T. rn elbeli Moore, 1958 — NE Thailand (Chaiyaphum & Khon Kaen provinces). Populations in E & NE Thailand (except Chaiyaphum and Khon Kaen provinces) are of uncertain subspecific affiliation. Descriptive notes. Head—body mean 117 mm (males) and 118 mm (females), tail mean 111 mm (males) and 108 mm (females); weight mean c.56 g. The Cambodian Striped Squirrel has a thin, pale brown longitudinal stripe dividing the mid-dorsal black stripe. Pairs of lateral stripes have the same pale brown color and are equally wide. Subspecies rodolphii has a dull brown nape and head, and a yellowish to orange venter. Subspecies elbeli has bright yellow-brown head and nape, and the line that divides the mid-dorsal stripe is a distinctive yellowish brown. Habitat. Semi-evergreen forests with preference for slightly degraded areas. Food and Feeding. There is no information available for this species. Breeding. There is no specific information available for this species, but female Cambodian Striped Squirrels have three pairs of teats, one pectoral and two inguinal. Activity patterns. There is no specific information available for this species, but the Cambodian Striped Squirrel is diurnal. Movements, Home range and Social organization. There is no information available for this species. Status and Conservation. Classified as Least Concern on The IUCN Red List. The Cambodian Striped Squirrel is widespread and very abundant in a variety of habitats. There are currently no major threats to this species. Bibliography. Duckworth & Lunde (2008c), Lekagul & McNeely (1977), Lunde & Nguyen Truong Son (2001), Thorington et al. (2012).
description: Published as part of Don E. Wilson, Thomas E. Lacher, Jr & Russell A. Mittermeier, 2016, Sciuridae, pp. 648-837 in Handbook of the Mammals of the World – Volume 6 Lagomorphs and Rodents I, Barcelona :Lynx Edicions on page 732, DOI: 10.5281/zenodo.6840226
Opportunities for coordinating multi-level climate action: an analysis of city climate action and national urban engagement
Creators: name: Dickey, Ariana
name: Hadfield, Paris
name: OKE, CATHY
name: Verbeeck, Jorn
Publisher: name: University of Melbourne
Year: 2021
Subjects: Land use and environmental planning
Urban and regional planning not elsewhere classified

description: This report provides insights into how cities are responding to local climate change mitigation and adaptation challenges across regions, globally, and how they align with the priorities of the Mission Innovation program - an intergovernmental platform that brings together governments, businesses, investors and academia to achieve the goals of the Paris Agreement by enabling widely affordable clean energy. This analysis draws on an existing database of city climate actions from a sample of 98 climate change mitigation and adaptation plans published since 2016 in English, originally compiled for the Global Covenant of Mayors (Hadfield et al., 2021). The report also explores how national governments are currently engaging cities in climate action and where gaps exist to better coordinate between them.
Cosmic Ray Rejection with Attention Augmented Deep Learning
Creators: name: Bhavanam, S. R.
name: Channappayya, Sumohana S.
name: Srijith, P. K.
name: Desai, Shantanu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: Cosmic Ray (CR) hits are the major contaminants in astronomical imaging and spectroscopic observations involving solid-state detectors. Correctly identifying and masking them is a crucial part of the image processing pipeline, since it may otherwise lead to spurious detections. For this purpose, we have developed and tested a novel Deep Learning based framework for the automatic detection of CR hits from astronomical imaging data from two different imagers: Dark Energy Camera (DECam) and Las Cumbres Observatory Global Telescope (LCOGT). We considered two baseline models namely deepCR and Cosmic-CoNN, which are the current state-of-the-art learning based algorithms that were trained using Hubble Space Telescope (HST) ACS/WFC and LCOGT Network images respectively. We have experimented with the idea of augmenting the baseline models using Attention Gates (AGs) to improve the CR detection performance. We have trained our models on DECam data and demonstrate a consistent marginal improvement by adding AGs in True Positive Rate (TPR) at 0.01% False Positive Rate (FPR) and Precision at 95% TPR over the aforementioned baseline models for the DECam dataset. We demonstrate that the proposed AG augmented models provide significant gain in TPR at 0.01% FPR when tested on previously unseen LCO test data having images from three distinct telescope classes. Furthermore, we demonstrate that the proposed baseline models with and without attention augmentation outperform state-of-the-art models such as Astro-SCRAPPY, Maximask (that is trained natively on DECam data) and pre-trained ground-based Cosmic-CoNN. This study demonstrates that the AG module augmentation enables us to get a better deepCR and Cosmic-CoNN models and to improve their generalization capability on unseen data.
description: 21 pages, 23 figures. Accepted in Astronomy and Computing
The Impact of Academic Freedom on Democracy in Africa
Creators: name: Kratou, Hajer
name: Laakso, Liisa
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Shared experiences but diversified developments make Africa an interesting region in which to investigate the impact of education on democracy, and the role of academic freedom in this impact. As building expertise takes time, we focus on the causality between past experience of academic freedom and electoral democracy. Our theory is that independent experts advocating free and fair elections are acclaimed, which makes rigging elections a costly strategy for rulers. Using the Varieties of Democracy (V-Dem) index of Academic Freedom, and the Generalized method of moments (GMM) technique to estimate a dynamic panel model, we find a positive impact of preceding academic freedom on the quality of elections after the Post-Cold war democratic transitions. The result is robust when we check reverse causality and country-specific effects such as the initial level of democracy or dependence on oil exportation. The analysis is robust to indicators measuring democracy by accountability of the executive and Polity2 and Freedom House Indices as alternatives to V-Dem measures of democracy. We discuss the observed heterogeneity of countries showing a counterintuitive relationship. The study highlights the significance of scholars as a channel through which education supports democracy.