cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
GLOBAL BIOETIKANING AХLOQIY MUAMMOLARI
Creators: name: G. J. Abdullayeva
name: D. G. Sattorova
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: Biotsyentrizm
simpozium
antropotsyentristik
sivilizatsiya
umuminsoniy
ta’limni ijtimoiylashtirish
YUNESKO
dyeontologiya
patyernalizm printsipi
passiv ishtirok
tibbiyot etikasida

description: Bioetikaning insonni uning hayoti va sog’ligiga tibbiyot va biologiyaning salbiy ta’siridan himoya qilish, tibbiyot etikasi faqat vrachlarga taalluqli ekanligi, bioetika qo’mitalari faylasuflar, ekologlar, huquqshunoslar, jamoatchilik vakillari, shahar ma’murlaridan shu bilan birga tibbiyot etikasi, vrachning majburiyatlari haqida, bioetika patsiyentlarning huquqlarini himoya qilishi yoritilgan
Sonnenfleckenzeichnung Nr. 15464.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.07.1943, erstellt von William Otto Brunner
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
БУГУНГИ ЗАМОНАВИЙ ТИББИЁТДА БИОЭТИКА: МУАММОЛАР, ЗИДДИЯТЛАР ВА МУЛОҲАЗАЛАР
Creators: name: Дилдор Ғаппоровна Сатторова
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: “Зарар етказманг”
“Доктор-файласуф”
“Пандемия”
биоахлоқ
компетентлик
“Шифокор-бемор”
трафарентацион
рақамлаштириш
диагноз қўйиш.

description: Инсон томонидан атрофдаги дунёни ўрганишнинг тубдан янги парадигмаси ,униилмий -техникавий тараққиёт шароитида сақлаш,шу жумладан инсон саломатлигинисақлаш ,шу қаторида фаол ривожланаётган илмий соҳа бўлган замонавий биоэтикани кўплаб йўналишлари ёритилган
Sonnenfleckenzeichnung Nr. 15489.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 17.08.1943, erstellt von William Brunner, Assistent
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
ВОПРОСЫ СОВЕРШЕНСТВОВАНИЯ ЗАКОНОДАТЕЛЬСТВА УЗБЕКИСТАНА О ПРЕСТУПЛЕНИЯХ В СФЕРЕ ТРАНСПЛАНТОЛОГИИ С УЧЕТОМ ЗАРУБЕЖНОГО ОПЫТА
Creators: name: Алишер Рустамович Мухамедов
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: преступления
регулирование отношений в области трансплантации органов и тканей человека
изъятие органов или тканей человека
общественно опасные деяния
достоинство граждан Республики Узбекистан.

description: Современные достижения медицины, такие как трансплантология, генетика, пересадка эмбриона и искусственное оплодотворение требуют тщательного правового регулирования. Однако, пока ни одно государство не приняло наиболее полного законодательства, предусматривающего как медицинскую, так и правовую регламентацию всех вопросов трансплантации органов и тканей. Актуальность данного вопроса требует к себе внимания, как медицинских работников, так и юристов; как практиков, так и ученых
description: Modern advances in medicine, such as transplantology, genetics, embryo transfer and artificial insemination require careful legal regulation. However, so far no state has adopted the most complete legislation providing for both medical and legal regulation of all issues of organ and tissue transplantation. The relevance of this issue requires the attention of both medical workers and lawyers; both practitioners and scientists
A Search for Exoplanets in Open Clusters and Young Associations based on TESS Objects of Interest
Creators: name: Sun, Qinghui
name: Wang, Sharon Xuesong
name: Gan, Tianjun
name: Mann, Andrew W.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the results of our search of planet candidates in Open Clusters and Young Stellar Associations based on the TESS Objects of Interest Catalog. We find one confirmed planet, one promising candidate, one brown dwarf, and three unverified planet candidates in a sample of 1229 Open Clusters from the second Gaia data release. We discuss individual planet-star systems based on their basic parameters, membership probability, and the observation notes from the ExoFOP-TESS website. We also find ten planet candidates (P $>$ 95%) in Young Stellar Associations by using the BANYAN $Σ$ Bayesian Algorithm. Among the ten candidates, five are known planet systems. We estimate the rotation periods of the host stars using the TESS light curves and estimate their ages based on gyrochronology. Two candidates with periodic variations are likely to be young planets, but their exact memberships to Young Stellar Associations remain unknown.
description: 3 figures, 3 tables, accepted for publication in Research in Astronomy and Astrophysics
Characterising Atmospheres of Cloudy Temperate Mini-Neptunes with JWST
Creators: name: Constantinou, Savvas
name: Madhusudhan, Nikku
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The upcoming James Webb Space Telescope (JWST) promises a generational shift in the study of temperate mini-Neptune atmospheres using transit spectroscopy. High-altitude clouds however threaten to impede their atmospheric characterisation by muting spectral features. In this study, we systematically investigate JWST instrument configurations for characterising cloudy mini-Neptune atmospheres, assessing the importance of instrument choice and wavelength coverage, focusing on NIRISS and NIRSpec. We consider two temperate mini-Neptunes orbiting nearby M dwarfs, K2-18 b and TOI-732 c, with equilibrium temperatures below 400 K, as case studies and assess observations using different instrument configurations with one transit per instrument. We find that their JWST transmission spectra with modest observing time and adequate wavelength coverage can provide precise abundance constraints of key molecules H2O, CH4, and NH3 even in the presence of clouds at significantly high altitudes. The best constraints are obtained by combining all three high-resolution NIRSpec gratings (G140H+G235H+G395H) that together span the ~1-5 $μ$m range. Single-transit observations with this three-instrument configuration allow precise abundance constraints for cloud-top pressures as low as 3 mbar and 0.1 mbar for K2-18 b and TOI-732 c, respectively, assuming a nominal 10x solar metallicity. The constraints vary with instrument combinations. We find that NIRSpec G235H+G395H is the optimal two-instrument configuration, while NIRISS or NIRSpec G235H is optimal for single-instrument observations. Absent high-altitude clouds, even single-instrument observations can provide good abundance constraints for these planets. Our findings underscore the promise of JWST transmission spectroscopy for characterising temperate mini-Neptunes orbiting nearby M dwarfs.
description: Accepted for publication in MNRAS, 19 pages, 12 figures
Sonnenfleckenzeichnung Nr. 77.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 03.04.1968, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1968

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
SNR G292.0+1.8: A Remnant of a Low-Mass Progenitor Stripped-Envelope Supernova
Creators: name: Temim, Tea
name: Slane, Patrick
name: Raymond, John C.
name: Patnaude, Daniel
name: Murray, Emily
name: Ghavamian, Parviz
name: Renzo, Mathieu
name: Jacovich, Taylor
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a study of the Galactic supernova remnant (SNR) G292.0+1.8, a classic example of a core-collapse SNR that contains oxygen-rich ejecta, circumstellar material, a rapidly moving pulsar, and a pulsar wind nebula (PWN). We use hydrodynamic simulations of the remnant evolution to show that the SNR reverse shock is interacting with the PWN and has most likely shocked the majority of supernova ejecta. In our models, such a scenario requires a total ejecta mass of $\lesssim 3\: \rm M_{\odot}$ and implies that there is no significant quantity of cold ejecta in the interior of the reverse shock. In light of these results, we compare the estimated elemental masses and abundance ratios in the reverse-shocked ejecta to nucleosynthesis models and find that they are consistent with a progenitor star with an initial mass of 12-16 $\: \rm M_{\odot}$. We conclude that the progenitor of G292.0+1.8 was likely a relatively low mass star that experienced significant mass loss through a binary interaction and would have produced a stripped-envelope supernova explosion. We also argue that the region known as the "spur" in G292.0+1.8 arises as a result of the pulsar's motion through the supernova ejecta and that its dynamical properties may suggest a line-of-sight component to the pulsar's velocity, leading to a total space velocity of $\sim 600\: \rm km\:s^{-1}$ and implying a significant natal kick. Finally, we discuss binary mass loss scenarios relevant to G292.0+1.8 and their implications for the binary companion properties and future searches.
description: 19 pages, 4 tables, 11 figures, accepted for publication in ApJ
Sonnenfleckenzeichnung Nr. 15476.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 04.08.1943, erstellt von William Otto Brunner
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt.
Zusätzlich ist notiert: Aufnahme in der Turmkuppel, Bildorientierung etwas unsicher)
Sonnenfleckenzeichnung Nr. 15435.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 24.06.1943, erstellt von William Otto Brunner
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
Sonnenfleckenzeichnung Nr. 15441.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 30.06.1943, erstellt von William Otto Brunner
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
Observation of biradical spin coupling through hydrogen bonds
Creators: name: He, Yang
name: Li, Na
name: Castelli, Ivano E.
name: Li, Ruoning
name: Zhang, Yajie
name: Zhang, Xue
name: Li, Chao
name: Wang, Bingwu
name: Gao, Song
name: Peng, Lianmao
name: Hou, Shimin
name: Shen, Ziyong
name: Lü, Jing-Tao
name: Wu, Kai
name: Hedegård, Per
name: Wang, Yongfeng
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Chemical Physics (physics.chem-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Investigation of intermolecular electron spin interaction is of fundamental importance in both science and technology.Here, radical pairs of all-trans retinoic acid molecules on Au(111) are created using an ultra-low temperature scanning tunneling microscope. Antiferromagnetic coupling between two radicals is identified by magnetic-field dependent spectroscopy.The measured exchange energies are from 0.1 to 1.0 meV. The biradical spin coupling is mediated through O-H$\cdots$O hydrogen bonds, as elucidated from analysis combining density functional theory calculation and a modern version of valence bond theory.
description: 10 pages with supplemental materials, PRL accepted
Sidydrassus Esyunin & Tuneva 2002
Creators: name: Fomichev, Alexander A.
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Gnaphosidae
Sidydrassus

description: Key to Sidydrassus species
Males
1 Median apophysis with a prolaterally bent branch (Figs 25, 29)........................................ S. shumakovi - Median apophysis without a prolaterally bent branch (Figs 13, 16, 20, 23, 31, 35).................................. 2 2 RTA 4 times shorter than tibia (Figs 31–33)............................................................ S. rogue - RTA as long as tibia or twice shorter than tibia (Figs 13–18)................................................... 3 3 RTA as long as tibia (Figs 13–15)............................................................ S. saiynovi sp. n. - RTA twice as short as tibia (Figs 16–18)....................................................... S. tianschanicus
Females (female of S. saiynovi sp. n. is unknown)
1 Epigynal fovea slit-shaped, not contiguous with the epigastric furrow (Figs 37–38)........................ S. shumakovi
- Epigynal fovea wide and round, contiguous with the epigastric furrow (Figs 40, 42)................................ 2
2 Epigynal fovea 2.1 times longer than wide, anterior and posterior receptacles equal in size (Figs 42–43)........................................................................................................ S. tianschanicus
- Epigynal fovea 1.7 times longer than wide, anterior receptacles significantly larger than the posterior ones (Figs 40–41)................................................................................................... S. rogue
Possible relationships within Sidydrassus
Of the four species currently assigned to the genus, S. saiynovi sp. n., S. tianschanicus, and S. rogue seem to be closely related as they are similar in having the median apophysis without a prolateral branch, similar proportions of the embolic base, the wide epigynal fovea, the diverging anterior receptacles and posterior receptacles without pronounced heads (Figs 13, 16, 20, 23, 31, 35, 40–43). The generotype, S. shumakovi, stays apart and possesses the median apophysis with a prolateral branch, the thick embolic base, the slit-shaped epigynal fovea, the converging anterior receptacles and the posterior receptacles with pronounced heads (Figs 25, 29, 37–39). Thus, all the Sidydrassus species can be divided into two species groups: the shumakovi -group (one species) and the tianschanicus -group (three species) (Table 1).
description: Published as part of Fomichev, Alexander A., 2022, A survey of the East Palaearctic Gnaphosidae (Araneae). 12. A review of Sidydrassus Esyunin & Tuneva, 2002, pp. 260-272 in Zootaxa 5194 (2) on pages 270-271, DOI: 10.11646/zootaxa.5194.2.7, http://zenodo.org/record/7147403
Sonnenfleckenzeichnung Nr. 26.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 29.01.1968, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1968

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Morpho-kinematic modeling of the expanding ejecta of the extremely slow nova V1280 Scorpii
Creators: name: Naito, Hiroyuki
name: Tajitsu, Akito
name: Ribeiro, Valèrio A. R. M.
name: Arai, Akira
name: Maehara, Hiroyuki
name: Kouzuma, Shinjirou
name: Iijima, Takashi
name: Okazaki, Atsuo T.
name: Watanabe, Makoto
name: Takagi, Seiko
name: Watanabe, Fumitake
name: Sakon, Itsuki
name: Sadakane, Kozo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Morphology of nova ejecta is essential for fully understanding the physical processes involved in nova eruptions. We studied the 3D morphology of the expanding ejecta of the extremely slow nova V1280 Sco with a unique light curve. Synthetic line profile spectra were compared to the observed [O III] 4959, 5007 and [N II] 5755 emission line profiles in order to find the best-fit morphology, inclination angle, and maximum expansion velocity of the ejected shell. We derive the best fitting expansion velocity, inclination, and squeeze as $V_{\rm exp} = 2100^{+100}_{-100}$ \,km\,s$^{-1}$, $i = 80^{+1}_{-3}$ deg, and $squ = 1.0^{+0.0}_{-0.1}$ using [O III] line profiles, and $V_{\rm exp} = 1600^{+100}_{-100}$ \,km\,s$^{-1}$, $i = 81^{+2}_{-4}$ deg, and $squ = 1.0^{+0.0}_{-0.1}$ using [N II] 5755 line profile. A high inclination angle is consistent with the observational results showing multiple absorption lines originating from clumpy gases which are produced in dense and slow equatorially focused outflows. Based on additional observational features such as optical flares near the maximum light and dust formation on V1280 Sco, a model of internal shock interaction between slow ejecta and fast wind proposed for the $γ$-ray emission detected in other novae seems to be applicable to this extremely slow and peculiar nova. Increasing the sample size of novae whose morphology is studied will be helpful in addressing long-standing mysteries in novae such as the dominant energy source to power the optical light at the maximum, optical flares near the maximum, clumpiness of the ejecta, and dust formation.
description: 21 pages, 8 figures, accepted for publication in ApJ
Towards the speed limit of high fidelity 2-qubit gates
Creators: name: Hegde, Swathi S
name: Zhang, Jingfu
name: Suter, Dieter
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Most implementations of quantum gate operations rely on external control fields to drive the evolution of the quantum system. Generating these control fields requires significant efforts to design the suitable control Hamiltonians. Furthermore, any error in the control fields reduces the fidelity of the implemented control operation with respect to the ideal target operation. Achieving sufficiently fast gate operations at low error rates remains therefore a huge challenge. In this work, we present a novel approach to overcome this challenge by eliminating, for specific gate operations, the time-dependent control fields entirely. This approach appears useful for maximising the speed of the gate operation while simultaneously eliminating relevant sources of errors. We present an experimental demonstration of the concept in a single nitrogen-vacancy (NV) center in diamond at room temperature.
description: Accepted in Physical Review Letters
ИССЛЕДОВАНИЕ КЛЮЧЕВЫХ ПРОБЛЕМ БИОЭТИКИ ИСЛАМЕ: СОВРЕМЕННОСТЬ
Creators: name: Замира Мухамеджановна Мухамедова
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: роль мусульманской биоэтики в развитии глобальной биоэтики
древние источники биоэтики ислама
исследование ключевых проблем биоэтики

description: В статье рассмотрена роль богатых философских и религиозных традиций, которые сохраняют в современной мусульманской биомедицинской этике основания и историческую преемственность с традиционной профессиональной медицинской этикой
Sonnenfleckenzeichnung Nr. 15479.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.08.1943, erstellt von William Otto Brunner
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Später wurden ergänzende Angaben aufgrund auswärtiger Beobachtungen direkt auf der Fleckenzeichnung hinzugefügt. Unter Umständen sind Angaben zu Protuberanzen vermerkt
The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 b
Creators: name: Hord, Benjamin J.
name: Colón, Knicole D.
name: Berger, Travis A.
name: Kostov, Veselin
name: Silverstein, Michele L.
name: Stassun, Keivan G.
name: Lissauer, Jack J.
name: Collins, Karen A.
name: Schwarz, Richard P.
name: Sefako, Ramotholo
name: Ziegler, Carl
name: Briceño, César
name: Law, Nicholas
name: Mann, Andrew W.
name: Ricker, George R.
name: Latham, David W.
name: Seager, Sara
name: Winn, Joshua N.
name: Jenkins, Jon M.
name: Bouma, Luke G.
name: Falk, Ben
name: Torres, Guillermo
name: Twicken, Joseph D.
name: Vanderburg, Andrew
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Hot Jupiters are generally observed to lack close planetary companions, a trend that has been interpreted as evidence for high-eccentricity migration. We present the discovery and validation of WASP-132 c (TOI-822.02), a 1.85 $\pm$ 0.10 $R_{\oplus}$ planet on a 1.01 day orbit interior to the hot Jupiter WASP-132 b. Transiting Exoplanet Survey Satellite (TESS) and ground-based follow-up observations, in conjunction with vetting and validation analysis, enable us to rule out common astrophysical false positives and validate the observed transit signal produced by WASP-132 c as a planet. Running the validation tools \texttt{vespa} and \texttt{triceratops} on this signal yield false positive probabilities of $9.02 \times 10^{-5}$ and 0.0107, respectively. Analysis of archival CORALIE radial velocity data leads to a 3$σ$ upper limit of 28.23 ms$^{-1}$ on the amplitude of any 1.01-day signal, corresponding to a 3$σ$ upper mass limit of 37.35 $M_{\oplus}$. Dynamical simulations reveal that the system is stable within the 3$σ$ uncertainties on planetary and orbital parameters for timescales of $\sim$100 Myr. The existence of a planetary companion near the hot Jupiter WASP-132 b makes the giant planet's formation and evolution via high-eccentricity migration highly unlikely. Being one of just a handful of nearby planetary companions to hot Jupiters, WASP-132 c carries with it significant implications for the formation of the system and hot Jupiters as a population.
description: 19 pages, 8 figures, Accepted for publication in AJ
Sonnenfleckenzeichnung Nr. 15432.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.06.1943, erstellt von William Otto Brunner
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
A BRST view of the spontaneous symmetry breaking
Creators: name: Amaral, R. L. P. G.
name: Lemes, V. E. R.
name: Ventura, O. S.
name: Vilar, L. C. Q.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: After the phase transition of a Grand Unified Theory (GUT), its single coupling splits into the couplings of the basic interactions. On the other side, the measurement of the Weinberg mixing angle in the eletroweak theory determines that the couplings associated to the SU(2) and U(1) symmetries were already distinct in its symmetric phase, before the electroweak breaking. This picture is consistent as we understand that such couplings evolve independently with the energy scale, meeting a common point together with the strong interaction coupling at the GUT scale. From a BRST symmetry point of view, this implies that each independent coupling should be associated to independent cocycles defined on a cohomological basis. The problem is that, before the GUT symmetry breaking, the BRST operator associated to this symmetric phase predicts a single Yang-Mills coupling. This sets the question of what should be the BRST operator of the asymmetric phase, that would allow for the splitting of this coupling but at the same time remain compatible with the BRST operator of the symmetric phase. In this work we proceed to answer this question.
description: 16 pages. No figures
ПАРАДИГМА БИОЭТИКИ В СФЕРЕ БИОЭТИЧЕСКОГО ОБРАЗОВАНИЯ
Creators: name: Фатима Ташпулатовна Худайбергенова
name: Дилором Арифовна Умарова
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: формирование биоэтической культуры будущих врачей
синтез естественных и гуманитарных дисциплин
биоэтика как феномен защиты фундаментальных моральных ценностей. вклад в развитие теоретических проблем биоэтики

description: В статье рассмотрены актуальные вопросы в философском обучении студентов-медиков, в формированиия биоэтической культуры будущих врачей. Приоритетом является формирование у них творческого мышления и научного мировоззрения в целях становления свободной и ответственной личности, способной конструктивно работать в проблемных ситуациях, сочетающей профессиональную компетентность с гражданской ответственностью
Sonnenfleckenzeichnung Nr. 15508.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 05.09.1943, erstellt von William Brunner, Assistent
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
PRISMA checklist and flowchart for ‘Elevated shock index and modified shock index are associated with mortality and major adverse cardiac events in patients with acute myocardial infarction: A systematic review and meta-analysis’
Creators: name: Pramudyo, Miftah
name: Putra, Iwan Cahyo Santosa
name: Kamarullah, William
name: Prameswari, Hawani Sasmaya
name: Saboe, Aninka
name: Akbar, Mohammad Rizki
Publisher: name: figshare
Year: 2022
Subjects: subject: 110201 Cardiology (incl. Cardiovascular Diseases)
subject: FOS: Clinical medicine
subject: Cardiology

description: This PRISMA 2020 checklist and flowchart were used to improve the transparency of our manuscript entitled Elevated shock index and modified shock index are associated with mortality and major adverse cardiac events in patients with acute myocardial infarction: A systematic review and meta-analysis. .
Sonnenfleckenzeichnung Nr. 15463.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 22.07.1943, erstellt von Max Waldmeier
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
Instability in the system of the distant post-AGB star LS III+52 24 (IRAS 22023+5249)
Creators: name: Klochkova, V. G.
name: Miroshnichenko, A. S.
name: Panchuk, V. E.
name: Tavolzhanskaya, N. S.
name: Yushkin, M. V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The optical spectra of the B-supergiant LS III+52 24 (IRAS 22023+5249) obtained at the 6-meter telescope BTA with a resolution R$\ge$60000 in 2010-2021 revealed signs of wind variability and velocity stratification in the extended atmosphere. The H$α$ and H$β$ lines have a P Cyg type profile; their wind absorption changes position in the range from $-270$ to $-290$ km/s. The intensity of the H$α$ emission reaches record values with respect to the local continuum: I/Icont $\approx$70. The stationary radial velocity according to the positions of symmetric forbidden emissions and permitted metal emissions was taken as the systemic velocity Vsys=$-149.6\pm$0.6 km/s. Based on the positions of absorptions of NII and OII ions, a time variability of the radial velocity in the range from $-127.2$ to $-178.3$ km/s was found for the first time for this star. This variability indicates the possible presence of a companion and/or atmospheric pulsations. The change of the oxygen triplet profile OI 7775 A due to the occurrence of unstable emission was registered. The set of interstellar absorptions of the NaI D-lines profile in the range from $-10.0$ to $-167.2$ km/s is formed in the Local Arm and subsequent arms of the Galaxy. The distance to the star, d$\ge$5.3 kpc, combined with the high systemic velocity, indicates that the star is located in the Galaxy beyond the Scutum-Crux arm.
description: 10 pages, 7 figures, accepted to Astronomy Reports
СОЦИОКУЛЬТУРНЫЙ ФЕНОМЕН БИОМЕДИЦИНСКОЙ ЭТИКИ
Creators: name: Сухроб Дустмурадович Норкулов
name: Феруза Садуллаевна Атамуратова
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: мораль
право
биоэтические комитеты
международные нормативные документы

description: В статье рассмотрена биомедицинская этика как социокультурный феномен, ее фундаментальной проблемой является защита прав человека (пациента) при медико-биологическом воздействии и манипуляции. Показано, что медицинская деятельность регламентируется двумя формами социального регулирования – моралью и правом, конкретными механизмами правовой защиты личности: этическими кодексами и законами, носящими как государственный, так и международный статус, системой биоэтических комитетов.
PRISMA 2020 Checklist and Flowchart
Creators: name: Pramudyo, Miftah
name: Putra, Iwan Cahyo Santosa
name: Kamarullah, William
name: Prameswari, Hawani Sasmaya
name: Saboe, Aninka
name: Akbar, Mohammad Rizki
Publisher: name: figshare
Year: 2022
Subjects: subject: 110201 Cardiology (incl. Cardiovascular Diseases)
subject: FOS: Clinical medicine
subject: Cardiology

description: This PRISMA 2020 checklist and flowchart were used to improve the transparency of our manuscript entitled Elevated shock index and modified shock index are associated with mortality and major adverse cardiac events in patients with acute myocardial infarction: A systematic review and meta-analysis. .
Akamboja Roza & Quintino & Mermudes & Silveira 2017, gen. nov.
Creators: name: Roza, André Silva
name: Quintino, Hingrid Yara Souza
name: Mermudes, José Ricardo Miras
name: Silveira, Luiz Felipe Lima Da
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Phengodidae
Akamboja

description: Key to species of Akamboja gen. nov.
1 Pronotum dark brown (Figs 27 and 30)....................................................................2
1’ Pronotum light brown (Fig. 2)............................................................................3
2 Elytron reaches the anterior margin of the second abdominal segment (Fig. 27); lateral region of the head sparsely setose posterior to eyes (Fig. 35); vertex occupying? of head in dorsal view (Fig. 36); specimens from Andradas (Fig. 36)......................................................................................... Akamboja tenebrae sp. nov.
2’ Elytron reaches the anterior margin of the third abdominal segment (Fig. 30); lateral region of the head densely setose posterior to eyes (Fig. 40); vertex occupying 1/2 of head in dorsal view (Fig. 41); specimens from Dores do Rio Preto......................................................................................... Akamboja caparaoensis sp. nov.
3 Eyes occupying two thirds the head width, in lateral view (Figs 5 and 26); apical maxillary palpomere 3.5x longer than subapical (Figs 5 and 26).....................................................................................4
3’ Eyes occupying half head width, in lateral view (Fig. 24); apical maxillary palpomere 4.5x longer than subapical (Fig. 24); specimens from Teresópolis, Itatiaia and São José do Barreiro (altitudinal range 1,200 to 1,900 m)...................................................................................................... Akamboja cleidae sp. nov.
4 Specimens larger (4.1–4.5 mm); elytron large, reaching the posterior margin of the fourth segment of abdomen; vertex occupying? of head in dorsal view (Fig. 31); specimens from Itatiaia, from 1,280 to 1,440 m ..... Akamboja monteirorum sp. nov.
4’ Specimens smaller (3.3–3.8 mm); elytron small, reaching the anterior margin of the third segment of abdomen; vertex occupying? of head in dorsal view (Fig. 6); specimens from Teresópolis and Tijuca, from 200 to 900 m ..................................................................................................... Akamboja minimum sp. nov.
description: Published as part of Roza, André Silva, Quintino, Hingrid Yara Souza, Mermudes, José Ricardo Miras & Silveira, Luiz Felipe Lima Da, 2017, Akamboja gen. nov., a new genus of railroad-worm beetle endemic to the Atlantic Rainforest, with five new species (Coleoptera: Phengodidae, Mastinocerinae), pp. 501-523 in Zootaxa 4306 (4) on pages 504-505, DOI: 10.11646/zootaxa.4306.4.3, http://zenodo.org/record/845117
The $κ$-model, a minimal model alternative to dark matter. Application to the galactic rotation problem
Creators: name: Pascoli, G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The determination of the velocities, accelerations and the gravitational field intensity at a given location in a galaxy could potentially be achieved in an unexpected manner with the environment of the observer, for instance, the local mean mass density in the galaxy. This idea, mathematically supported by the asymmetric distance concept, is illustrated here by a study regarding the rotation of spiral galaxies. This suggestion is new in the astrophysics field (in the following, it is called the \k{appa}-model) and could help to mimic the main effects seen in modified Newtonian dynamics (MOND) theory, modified gravity (MOG) models, or other related models built with the aim of eliminating dark matter that are already well-established theories. Thus, starting from two selected examples of galaxies, in section 5, we show that there is an equivalence between MOND and the \k{appa}-model. In particular, on the opposite side, we have the speculative nature of the dominant paradigm, the elusive dark matter, a matter whose properties always remain undefined despite intense theoretical, experimental and observational efforts for over 50 years.
description: 23 pages, 20 figures, accepted for publication in Astrophysics and Space Science
Sonnenfleckenzeichnung Nr. 15496.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 24.08.1943, erstellt von William Brunner, Assistent
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
ТИББИЙ ТАЪЛИМДА ШИФОКОР КАСБИНИ ШАКЛЛАНТИРИШДА БИОЭТИКАНИНГ ЎРНИ
Creators: name: Наргиза Акмаловна Умирзакова
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: биоэтика
биотиббиёт
шифокор ахлоқи
касбий компетенциялар
шифокор касби

description: Бугунги кунда жамият тараққиётида илм-фан кашфиётлари, шу жумладан тиббий-биологик фанларда янги биотиббий технологиялар ва тадқиқотларда эришилган ютуқлар тиббиётнинг фан ва фаолият шакли сифатидаги қиёфасини тубдан ўзгартириб, янги аввал бўлмаган муаммоларни келтириб чиқарди. Мақолада тиббий таълимда шифокор касбини шакллантиришда биоэтика фанининг ўрни тўғрисида сўз боради
Sonnenfleckenzeichnung Nr. 15501.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 29.08.1943, erstellt von William Otto Brunner
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
Detecting PAHs in high-z galaxies in proxy: Modelling physical conditions in an extremely strong damped Lyman-alpha absorber towards QSO SDSS J1143+1420 at z=2.323
Creators: name: Shaw, Gargi
name: Ranjan, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We explore indirect methods to detect Polycyclic Aromatic Hydrocarbons (PAHs) in gas-rich, absorption-selected galaxies at high redshift. We look at the optical VLT/X-shooter observations of an intervening, extremely strong damped Lyman-alpha absorber (or ESDLA, with log(N(HI))>~21.7)) towards QSO SDSS J1143+1420 at redshift, z(ESDLA)=2.323. Literature studies have shown that this ESDLA contains signatures of dust and diffuse molecular hydrogen and it was specifically chosen for our study due to its close spatial proximity (impact parameter, rho=0.6+/-0.3 kpc) with its associated galaxy. There is no direct detection of PAHs emission in the limited observations of infrared(IR)-spectra along this sight-line. Hence, we use CLOUDY numerical simulation modelling to indirectly probe the presence of PAH in the ESDLA. We note that PAHs need to be included in the models to reproduce the observed column densities of warm H2 and CI. Thus, we infer the presence of PAHs indirectly in our ESDLA, with an abundance of PAH/H = 10^(-7.046). We also measure a low 2175 A bump strength (E(bump)~0.03-0.19 mag) relative to star-forming galaxies by modelling extinction of QSO spectra by dust at the absorber rest-frame. This is consistent with the low PAH abundance obtained indirectly using CLOUDY modelling. Our study highlights the usage of CLOUDY modelling to indirectly detect PAH in high-redshift gas-rich absorption-selected galaxies.
description: 6 pages, 3 figures, 3 tables
ФАРМАЦЕВТИЧЕСКАЯ ЭТИКА КАК ОБЛАСТЬ НАУЧНОГО ПОЗНАНИЯ БИОЭТИКИ И ПРАВА
Creators: name: Мухамедова Замира Мухамеджановна
Publisher: name: Academic research in educational sciences
Year: 2022
Subjects: талидамидовая катастрофа
предотвращение негативных эффектов действия лекарств
массовое отравление лекарственным препаратом в Японии
правила GCP
проведение обязательной этической экспертизы участвующих в клинических испытаниях лекарств

description: В статье рассмотрены некоторые причины, которые привели к пониманию необходимости радикального изменения структуры взаимоотношений между наукой и практической медициной в контексте предотвращения негативных эффектов действия лекарств и становления фармацевтической биоэтики, которая изучает моральные, правовые, социальные, экологические и юридические проблемы, возникающие при создании, клинических испытаниях, регистрации, производстве, розничной реализации и доведении до потребителя лекарств и аптечной продукции.
Anisotropic carrier dynamics in a laser-excited Fe$_{1}$/(MgO)$_{3}$(001) heterostructure from real-time time-dependent DFT
Creators: name: Shomali, Elaheh
name: Gruner, Markus E.
name: Pentcheva, Rossitza
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The interaction of a femtosecond optical pulse with a Fe$_{1}$/(MgO)$_{3}$(001) metal/oxide heterostructure is investigated using time-dependent density functional theory (TDDFT) calculations in the real-time domain. We systematically study electronic excitations as a function of laser frequency, peak power density and polarization direction. While spin-orbit coupling is found to result in only a small time-dependent reduction of magnetization (less than 10%), we find a marked anisotropy in the response to in-plane and out-of-plane polarized light, which changes its character qualitatively depending on the excitation energy: the Fe-layer is efficiently addressed at low frequencies by in-plane polarized light, whereas for frequencies higher than the MgO band gap, we find a particularly strong response of the central MgO-layer for cross-plane polarized light. For laser excitations between the charge transfer gap and the MgO band gap, the interface plays the most important role, as it mediates concerted transitions from the valence band of MgO into the $3d$ states of Fe closely above the Fermi level and from the Fe-states below the Fermi level into the conduction band of MgO. As these transitions can occur simultaneously altering charge balance of the layers, they could potentially lead to an efficient transfer of excited carriers into the MgO bulk, where the corresponding electron and hole states can be separated by an energy which is significantly larger than the photon energy.
description: Phys. Rev. B, accepted for publication
The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study
Creators: name: Page, K. L.
name: Beardmore, A. P.
name: Osborne, J. P.
name: Munari, U.
name: Ness, J. -U.
name: Evans, P. A.
name: Bode, M. F.
name: Darnley, M. J.
name: Drake, J. J.
name: Kuin, N. P. M.
name: O'Brien, T. J.
name: Orio, M.
name: Shore, S. N.
name: Starrfield, S.
name: Woodward, C. E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: On 2021 August 8, the recurrent nova RS Ophiuchi erupted again, after an interval of 15.5 yr. Regular monitoring by the Neil Gehrels Swift Observatory began promptly, on August 9.9 (0.37 day after the optical peak), and continued until the source passed behind the Sun at the start of November, 86 days later. Observations then restarted on day 197, once RS Oph emerged from the Sun constraint. This makes RS Oph the first Galactic recurrent nova to have been monitored by Swift throughout two eruptions. Here we investigate the extensive X-ray datasets from 2006 and 2021, as well as the more limited data collected by EXOSAT in 1985. The hard X-rays arising from shock interactions between the nova ejecta and red giant wind are similar following the last two eruptions. In contrast, the early super-soft source (SSS) in 2021 was both less variable and significantly fainter than in 2006. However, 0.3-1 keV light-curves from 2021 reveal a 35 s quasi-periodic oscillation consistent in frequency with the 2006 data. The Swift X-ray spectra from 2021 are featureless, with the soft emission typically being well parametrized by a simple blackbody, while the 2006 spectra showed much stronger evidence for superimposed ionized absorption edges. Considering the data after day 60 following each eruption, during the supersoft phase the 2021 spectra are hotter, with smaller effective radii and lower wind absorption, leading to an apparently reduced bolometric luminosity. We explore possible explanations for the gross differences in observed SSS behaviour between the 2006 and 2021 outbursts.
description: 21 pages, 16 colour figures, accepted for publication in MNRAS. Table 1 in full is included as an ancillary PDF (will be supplementary online material when published by MNRAS)