cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Musca molecular cloud: The perfect "filament" is still a sheet
Creators: name: Tritsis, A.
name: Bouzelou, F.
name: Skalidis, R.
name: Tassis, K.
name: Enßlin, T.
name: Edenhofer, G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The true 3-dimensional (3D) morphology of the Musca molecular cloud is a topic that has received significant attention lately. Given that Musca does not exhibit intense star-formation activity, unveiling its shape has the potential of also revealing crucial information regarding the physics that dictates the formation of the first generation of stars within molecular clouds. Here, we revisit the shape of Musca and we present a comprehensive array of evidence pointing towards a shape that is extended along the line-of-sight dimension: (a) 3D maps of differential extinction; (b) new non-local thermodynamic equilibrium radiative transfer simulations of CO rotational transitions from a sheet-like, magnetically-dominated simulated cloud; (c) an effective/critical density analysis of available CO observations; (d) indirect consequences that a filamentary structure would have had, from a theoretical star-formation perspective. We conclude that the full collection of observational evidence strongly suggests that Musca has a sheet-like geometry.
description: 13 pages, 14 figures. Accepted for publication in MNRAS
title: Ceci n’est pas une pipe: Disentangling measurement and reality in ex-post harmonization
Creators: name: Singh, Ranjit K.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Ex-Post Harmonization Adventures
subject: Comparability
subject: Survey Methodology
subject: FAIR Data Principles
subject: Open Data

description: The scores in our dataset are not reality itself; they are glimpses at reality through the lens of the respective measurement instrument. In research practice, that distinction sometimes takes a backseat. However, if we want to combine numerical scores of different instruments, then the relationship between measurement and reality becomes crucial.
description: Die Werte in unserem Datensatz bilden die Realität nur mittelbar ab; Sie erlauben uns lediglich den Blick durch die Linse des jeweiligen Messinstruments. In der Forschungspraxis tritt dieser Aspekt meist in den Hintergrund. Wenn wir jedoch numerische Werte, die mit verschiedenen Instrumenten gemessen wurden, kombinieren wollen, dann ist diese Beziehung zwischen Messung und Realität von zentraler Bedeutung.
description: GESIS Blog
Analyzing the memory ordering models of the Apple M1
Creators: name: Wrenger, Lars
name: Töllner, Dominik
name: Lohmann, Daniel
Publisher: name: Amsterdam : Elsevier
Year: 2024
Subjects: subject: Apple M1
subject: ARM
subject: Memory ordering
subject: TSO
subject: Dewey Decimal Classification::000 | Allgemeines, Wissenschaft::000 | Informatik, Wissen, Systeme::004 | Informatik

description: The Apple M1 ARM processor family incorporates two memory consistency models: the conventional ARM weak memory ordering and the Total store ordering (TSO) model from the x86 architecture utilized by Apple's x86 emulator, Rosetta 2. The presence of both memory ordering models on the same hardware enables us to thoroughly benchmark and compare their performance characteristics and worst-case workloads. In this paper, we assess the performance implications of TSO on the Apple M1 processor architecture. Based on the multi-threading workloads of the SPEC2017 CPU FP benchmark suite, our findings indicate that TSO is, on average, 8.94 percent slower than ARM's weaker memory ordering. Through synthetic benchmarks, we further explore the workloads that experience the most significant performance degradation due to TSO. We also take a deeper look into the specific atomic instructions provided by the ARMv8.3 specification and their synchronization overheads.
Challenging tumor hypoxia with a polymeric carrier system simultaneously encapsulating complementary therapeutic agents
Creators: name: Marco, Agnes
name: Mazza Arianna
name: Eszter, Kalydi
name: Szabolcs, Béni
name: Francesco, Manoli
name: Milo, Malanga
name: Julia, Manet Ilse Gert
Publisher: name: Zenodo
Year: 2022
Subjects: cyclodextrin polymers
combinatorial therapy
pdt
hypoxia

description: Nanotechnologies have been exploited for the co-administration of chemotherapeutics such as taxanes with a photosensitizer (PS) which produces singlet oxygen (1O2) upon irradiation with red light in the presence of molecular oxygen (O2) targeting cancer cells (photodynamic therapy, PDT). However, tumor tissues often suffer from hypoxic conditions, an inadequate supply of O2 compromising PDT efficacy and activating resistance to chemotherapy. The HypoCyclo project aims to develop a novel combination of chemo- and photo-therapies for the effective treatment of Breast Cancer (BC), bypassing hypoxia-derived limitations. We focused on cyclodextrin polymers (pCyD), biocompatible carriers able to improve the solubility and stability of hydrophobic drugs under physiological conditions and to host multiple functional agents outperforming current cancer treatments. We will discuss a multi-modal pCyD i) loaded with paclitaxel (PCX) as chemotherapeutic agent, ii) decorated with Chlorin e6 (Ce6) for PDT, and iii) functionalized with an Oxygen Releasing Agent (ORA) to supply O2 in situ. Preliminary data will be presented showing the NMR, UV-Vis and ESI-MS characterization of synthesized anthracene derivatives selected as suitable ORA due to their capacity to form endoperoxides photochemically by trapping 1O2 and releasing it upon cycloreversion. We will further provide evidences of the successful co-encapsulation of PCX, ORA and Ce6 into βCyD-polymer, without affecting the properties and efficacy of each component.
Sonnenfleckenzeichnung Nr. 15472.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 31.07.1943, 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. Später wurden ergänzende Angaben aufgrund auswärtiger Beobachtungen direkt auf der Fleckenzeichnung hinzugefügt. Unter Umständen sind Angaben zu Protuberanzen vermerkt
Sonnenfleckenzeichnung Nr. 3818.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 29.11.1951, erstellt als Beobachtung im Projektionsverfahren Nr. 2041 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Zusätzlich wurden ergänzende Angaben aufgrund weiterer Beobachtungen direkt auf der Fleckenzeichnung hinzugefügt. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
Capnia teresa Claassen 1924
Creators: name: Stewart, Kenneth W.
name: Drake, Eugene F.
name: Stark, Bill P.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Capniidae
Capnia
Capnia teresa

description: Capnia teresa Claassen 1924
(Figs. 3, 5, 6, 9, 38-43)
Distribution. California.
Material examined. California: San Bernadino Co., Forsee Creek, N 30 ° 09.431 ’ W 116 ° 55.885 ’, Elev. 1812m, 27-II-2008, E F. Drake, 16♂, 17♀, 1 pharate ♂ in exuvium, 3 reared ♂ with exuviae, 5 reared ♀ with exuviae, 6 pharate ♀ in exuviae (1 partially emerged), 2♂ larvae, 10♀ larvae.
Characters. Body length ♂ 6.0- 6.2mm, ♀ 6.8-6.9mm. Light to medium brown dorsally, ventrum lighter, little pattern except underlying muscles or developing adult pigment. Antennal segments 44-50, head capsule width ♂ 0.75mm, ♀ 0.87mm. Lacinia and mandibles as described for C. umpqua and C. ventura (Figs. 44-48, 50-53). Pronotum with setae scattered over surface and as a sparse marginal fringe. Mesosternal Y-arms typical of genus. Hind wingpads shallowly notched along inner margins; inside forewingpad length ♂ 0.84mm, ♀ 1.02- 1.08mm. Femora bear scattered surface bristles, and tibia with a silky outer fringe (Fig. 3). Abdominal segments with long surface hairs (Figs. 38-39). Sexual dimorphism evident. Male 10 th tergum with short, upturned posterior extension (Figs. 5, 6, 40); underlying developing epiproct visible in pharate or partially emerged individuals (Fig. 5). Female without upturned extension of 10 th tergum (Fig. 41). Cercal segments ♂ 30, ♀ 34; cercomeres with apical circlet of short and long bristles, longer dorsal and ventral bristle in lateral view, and no intercalary hairs (Figs. 9, 42, 43).
description: Published as part of Stewart, Kenneth W., Drake, Eugene F. & Stark, Bill P., 2011, Larvae Of Five Species Of The Winter Stonefly Genus Capnia (Plecoptera: Capniidae) From California, U. S. A., pp. 167-181 in Illiesia 7 (18) on page 175, DOI: 10.5281/zenodo.4760235
Sonnenfleckenzeichnung Nr. 3622.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 19.04.1951, erstellt von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
On the time evolution of the $M_{\rm d} - M_\star$ and $\dot M - M_\star$ correlations for protoplanetary discs: the viscous timescale increases with stellar mass
Creators: name: Somigliana, Alice
name: Toci, Claudia
name: Rosotti, Giovanni
name: Lodato, Giuseppe
name: Tazzari, Marco
name: Manara, Carlo
name: Testi, Leonardo
name: Lepri, Federico
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Large surveys of star-forming regions have unveiled power-law correlations between the stellar mass and the disc parameters, such as the disc mass $M_{\mathrm{d}} \propto {M_{\star}}^{λ_{\mathrm{m}}}$ and the accretion rate $\dot M \propto {M_{\star}}^{λ_{\mathrm{acc}}}$. The observed slopes appear to be increasing with time, but the reason behind the establishment of these correlations and their subsequent evolution is still uncertain. We conduct a theoretical analysis of the impact of viscous evolution on power-law initial conditions for a population of protoplanetary discs. We find that, for evolved populations, viscous evolution enforces the two correlations to have the same slope, $λ_{\mathrm{m}}$ = $λ_{\mathrm{acc}}$, and that this limit is uniquely determined by the initial slopes $λ_{\mathrm{m}, 0}$ and $λ_{\mathrm{acc}, 0}$. We recover the increasing trend claimed from the observations when the difference in the initial values, $δ_0 = λ_{\mathrm{m}, 0} - λ_{\mathrm{acc}, 0}$, is larger than $1/2$; moreover, we find that this increasing trend is a consequence of a positive correlation between the viscous timescale and the stellar mass. We also present the results of disc population synthesis numerical simulations, that allow us to introduce a spread and analyse the effect of sampling, which show a good agreement with our analytical predictions. Finally, we perform a preliminary comparison of our numerical results with observational data, which allows us to constrain the parameter space of the initial conditions to $λ_{\mathrm{m}, 0} \in [1.2, 2.1]$, $λ_{\mathrm{acc}, 0} \in [0.7, 1.5]$.
description: Accepted for publication in MNRAS. 14 pages, 8 figures
Sonnenfleckenzeichnung Nr. 134.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 08.06.1968, 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
Kein prahlendes, kein güldnes Zimmer
Creators: name: Spreng, Johann Jacob
Publisher: name: [s.n.]
Year: 1699
Subjects: Lyrik

description: mit Korrekturen von Spreng
description: Deutsch
description: Verzeichnung=Description=Inventaire April 2018 HAN-Katalogisierungsregeln Katalogisierung ab Original
Johanna Eleonore Gräfin zu Solms und Tecklenburg, Jeannettenruh in Wildenfels, eine poetische Erzählung, der hochgebohrnen Gräfin Frau Albertinen Charlotten, verwittwetten Gräfin zu Solms und Tecklenburg, <...> an Ihrem Jahrstage den 18. Novembris 1757 gewidmet
Creators: name: Spreng, Johann Jacob
Publisher: name: [s.n.]
Year: 1757
Subjects: Lyrik

description: Deutsch
description: Verzeichnung=Description=Inventaire April 2018 HAN-Katalogisierungsregeln Katalogisierung ab Original
ข้อจำกัดของการอุ้มบุญตามกฎหมายไทย: ศึกษากรณีผู้ที่มีสิทธิขอให้ดำเนินการให้หญิงอื่นตั้งครรภ์แทน
Creators: name: ปาริชาติ ม่วงศิริ
Publisher: name: สาขาวิชานิติศาสตร์ คณะมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา
Year: 2565
Subjects: คู่ชีวิต
คู่ชีวิตเพศเดียวกัน
อุ้มบุญ
Life Partner
Same-Sex Couple
Surrogacy

description: วารสารมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา, 16, 2, 224-251
Additional file 1 of A systematic analysis of splicing variants identifies new diagnoses in the 100,000 Genomes Project
Creators: name: Blakes, Alexander J. M.
name: Wai, Htoo A.
name: Davies, Ian
name: Moledina, Hassan E.
name: Ruiz, April
name: Thomas, Tessy
name: Bunyan, David
name: Thomas, N. Simon
name: Burren, Christine P.
name: Greenhalgh, Lynn
name: Lees, Melissa
name: Pichini, Amanda
name: Smithson, Sarah F.
name: Taylor Tavares, Ana Lisa
name: O’Donovan, Peter
name: Douglas, Andrew G. L.
name: Whiffin, Nicola
name: Baralle, Diana
name: Lord, Jenny
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Supplementary Figs. S1, S2, S3, S4.
Uniform Modelling of the Stellar Density of Thirteen Tidal Streams within the Galactic Halo
Creators: name: Patrick, Jeffrey M.
name: Koposov, Sergey E.
name: Walker, Matthew G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the results of fitting a flexible stellar stream density model to a collection of thirteen streams around the Milky Way, using photometric data from DES, DECaLS, and Pan-STARRS. We construct density maps for each stream and characterise their tracks on the sky, width, and distance modulus curves along the length of each stream. We use these measurements to compute lengths and total luminosities of streams and identify substructures. Several streams show prominent substructures, such as stream broadening, gaps, large deviations of stream tracks and sharp changes in stream densities. Examining the group of streams as a population, as expected we find that streams with globular cluster progenitors are typically narrower than those with dwarf galaxy progenitors, with streams around 100 pc wide showing overlap between the two populations. We also note the average luminosity of globular cluster streams is significantly lower than the typical luminosity of intact globular clusters. The likely explanation is that observed globular cluster streams preferentially come from lower luminosity and lower density clusters. The stream measurements done in a uniform manner presented here will be helpful for more detailed stream studies such as identifying candidate stream members for spectroscopic follow up and stellar stream dynamical modeling.
description: 25 pages, 40 figures, 4 tables. Accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 15469.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 28.07.1943, 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
Capnia umpqua Frison 1942
Creators: name: Stewart, Kenneth W.
name: Drake, Eugene F.
name: Stark, Bill P.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Capniidae
Capnia
Capnia umpqua

description: Capnia umpqua Frison 1942
(Figs. 10, 11, 20-25, 44-49, 56-59)
Distribution. California and Oregon.
Material examined. California: Orange Co., Trabuko Creek, Trabuko Canyon, 1 st concrete low water crossing, N 33 ° 40.29 ’ W 117 ° 32.45 ’, 5-IV-2005, K.W. Stewart and E.F. Drake, 8♂, 58♀, 1♂ reared with exuvium, 2♂ larvae, 1♀ larva. Same locality, 25-IV- 2005, E.F. Drake, 6♀. No other Capnia species collected at this locality.
Characters. Body length ♂ 5.0-6.0mm. Light to medium brown dorsally, ventrum lighter, little pattern except underlying muscles or developing adult pigment (Figs. 20, 23). Antennal segments 46- 48, head capsule width ♂ 0.75mm, ♀ 0.96mm. Lacinia triangular, palmate with longitudinally striate palm surface, broad apical teeth, ventral comb of 10-14 bristles and dorsal comb of 16-18 longer bristles (Fig. 44). Right mandible with apical teeth, molar pad of dense, stiff bristles, and inner band of hairs from base of apical teeth to molar pad (Figs. 45, 46). Left mandible with molar cup bordered by outer (dorsal) comb of curved teeth (Figs. 47, 48). Pronotum with scattered setae over surface and as a marginal fringe (Fig. 20). Mesosternal Y-arms with enclosed subtriangular area about 0.3 times the intercostal width (Fig. 22). Hind wingpads shallowly notched along inner margin (Fig. 20); inside forewingpad length ♂ 0.96mm, ♀ 1.08mm. Femora with scattered surface bristles, and tibia with a silky outer fringe (Fig. 21). Abdominal segments with long surface hairs (Fig. 56). Sexual dimorphism evident. Males with short posterior extension of 10 th tergum, triangular in dorsal and ventral views (Figs. 11, 23) with underlying developing narrow, tubular epiproct visible in pharate individuals (Figs. 11, 23); 10 th tergum in lateral view subtriangular, nearly straight dorsally, with slightly downturned tip (Figs. 10, 49). Female without posterior extension of 10 th tergum (Fig. 20). Cercal segments 28-30; cercomeres with apical circlet of short and long bristles, longer dorsal and ventral bristle in lateral view, and no intercalary hairs (Figs. 24, 25, 58, 59).
description: Published as part of Stewart, Kenneth W., Drake, Eugene F. & Stark, Bill P., 2011, Larvae Of Five Species Of The Winter Stonefly Genus Capnia (Plecoptera: Capniidae) From California, U. S. A., pp. 167-181 in Illiesia 7 (18) on page 175, DOI: 10.5281/zenodo.4760235
Data Driven Spectral Models For Apogee M Dwarfs
Creators: name: Birky, Jessica
name: Hogg, David W.
name: Burgasser, Adam J.
Publisher: name: Zenodo
Year: 2018
Subjects: APOGEE
M dwarfs
SDSS

description: The Cannon (Ness et al. 2015) is a flexible, data-driven spectral modeling and parameter inference framework, demonstrated on high-resolution Apache Point Galactic Evolution Experiment (APOGEE; λ/Δλ~22,500, 1.5-1.7µm) spectra of giant stars to estimate stellar labels (Teff, logg, [Fe/H], and chemical abundances) to precisions higher than the model-grid pipeline. The lack of reliable stellar parameters reported by the APOGEE pipeline for temperatures less than ~3550K (Schmidt et al. 2016), motivates the extension of this approach to M dwarf stars. Using a training set of 51 M dwarfs with spectral types ranging M0-M9 obtained from SDSS optical spectra, we demonstrate that The Cannon can infer spectral types to a precision of 0.6 types. We then use 30 M dwarfs ranging 3072 < Teff < 4131K, and -0.48 < [Fe/H] < 0.49 to train a two-parameter model precise to 44K and 0.05 dex respectively. Additionally we discuss the extension of a model to other labels, and the scientific objectives a data-driven pipeline could enable.
นางบุษมาลี: บทบาทตัวละครหญิงในละครนอกแบบหลวง เรื่องพระสมุท
Creators: name: นพวดี ไชยรัตน์
Publisher: name: คณะมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา
Year: 2565
Subjects: ตัวละครหญิง
บทบาท
ละครนอกแบบหลวง
Female protagonist
Character
Lakhon Nork Baep Luang

description: วารสารมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา, 16, 2, 252-276
ปัญหากฎหมายเกี่ยวกับโรงไฟฟ้าพลังงานนิวเคลียร์
Creators: name: กิตติคุณ มีนพัฒนสันติ
Publisher: name: คณะมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา
Year: 2565
Subjects: โรงไฟฟ้านิวเคลียร์
พลังงานนิวเคลียร์
กระแสไฟฟ้า
รังสี
วัสดุกัมมันตรังสี
เครื่องกำเนิดรังสี
วัสดุนิวเคลียร์
เชื้อเพลิงนิวเคลียร์
กากกัมมันตรังสี
Nuclear power plant
Nuclear energy
Electric current
Radiation
Radioactive substance
Radiation generator
Nuclear material
Nuclear fuel
Radioactive waste.

description: วารสารมนุษยศาสตร์และสังคมศาสตร์ มหาวิทยาลัยราชภัฏบ้านสมเด็จเจ้าพระยา, 16, 2, 277-296
The strong suppression of Galactic cosmic rays reaching AU Mic b, c and Prox Cen b
Creators: name: Mesquita, A. L.
name: Rodgers-Lee, D.
name: Vidotto, A. A.
name: Kavanagh, R. D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The propagation of Galactic cosmic rays is well understood in the context of the solar system but is poorly studied for M dwarf systems. Quantifying the flux of cosmic rays reaching exoplanets is important since cosmic rays are relevant in the context of life. Here, we calculate the Galactic cosmic ray fluxes in AU Mic and Prox Cen planetary systems. We propagate the Galactic cosmic rays using a 1D cosmic ray transport model. We find for Prox Cen b, AU Mic b and AU Mic c that the Galactic cosmic ray fluxes are strongly suppressed and are lower than the fluxes reaching Earth. We include in our models, for the first time for a star other than the Sun, the effect of radial particle drift due to gradients and curvatures in the stellar magnetic field. For Prox Cen we find that the inclusion of particle drift leads to less suppression of Galactic cosmic rays fluxes than when it is excluded from the model. In the case of AU Mic we explore two different wind environments, with a low and high stellar wind mass-loss rate. For AU Mic, the particle drift also leads to less suppression of the Galactic cosmic ray fluxes but it is only significant for the high mass-loss rate scenario. However, both wind scenarios for AU Mic suppress the Galactic cosmic rays strongly. Overall, careful modelling of stellar winds is needed to calculate the Galactic cosmic ray fluxes reaching exoplanets. The results found here can be used to interpret future exoplanet atmosphere observations and in atmospheric models.
description: 10 pages, 7 figures, accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 15446.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 05.07.1943, 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
Multi-wavelength study of blazar 4C +01.02 during its long-term flaring activity in 2014-2017
Creators: name: Zahoor, Malik
name: Zahir, Shah
name: Sahayanathan, Sunder
name: Iqbal, Naseer
name: Manzoor, Aaqib
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We conducted a detailed long-term spectral and temporal study of flat spectrum radio quasar 4C +01.02, by using the multi-wavelength observations from Fermi-LAT, Swift-XRT, and Swift-UVOT. The $2$-day bin $γ$-ray lightcurve in the 2014-2017 active state displays $14$ peak structures with a maximum integral flux $(\rm E > 100 \ MeV)$ of $\rm (2.5 \pm 0.2) \times 10^{-6}\ ph\ cm^{-2}\ s^{-1}$ at MJD 57579.1, which is approximately $61$ times higher than the base flux of $\rm (4.1 \pm 0.3) \times 10^{-8}\ ph\ cm^{-2}\ s^{-1}$, calculated by averaging the flux points when the source was in quiescent state. The shortest $γ$-ray variability of $0.66 \pm 0.08$ days is observed for the source. The correlation study between $γ$-ray spectral index and flux suggests that the source deviates from the usual trend of harder when brighter feature shown by blazars. To understand the likely physical scenario responsible for the flux variation, we performed a detailed broadband spectral analysis of the source by selecting different flux states from the multi-wavelength lightcurve. A single zone leptonic model was able to reproduce the broadband spectral energy distribution (SED) of each state. The parameters of the model in each flux state are determined using a $χ^2$ fit. We observed that the synchrotron, synchrotron-self-Compton (SSC), and External-Compton (EC) processes produce the broadband SED under varied flux states. The adjoining contribution of the seed photons from the broad-line region (BLR) and the IR torus for the EC process are required to provide adequate fits to the GeV spectrum in all the chosen states.
description: 12 Pages, 8 figures, Accepted for Publication in MNRAS
AGN X-ray Spectroscopy with Neural Networks
Creators: name: Parker, M. L.
name: Lieu, M.
name: Matzeu, G. A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We explore the possibility of using machine learning to estimate physical parameters directly from AGN X-ray spectra without needing computationally expensive spectral fitting. Specifically, we consider survey quality data, rather than long pointed observations, to ensure that this approach works in the regime where it is most likely to be applied. We simulate Athena WFI spectra of AGN with warm absorbers, and train simple neural networks to estimate the ionisation and column density of the absorbers. We find that this approach can give comparable accuracy to spectral fitting, without the risk of outliers caused by the fit sticking in a false minimum, and with an improvement of around three orders of magnitude in speed. We also demonstrate that using principal component analysis to reduce the dimensionality of the data prior to inputting it into the neural net can significantly increase the accuracy of the parameter estimation for negligible computational cost, while also allowing a simpler network architecture to be used.
description: 8 pages, 4 figures, accepted for publication in MNRAS
title: Die Messung sozialstruktureller Merkmale im Wandel der Zeit
Creators: name: Ortmanns, Verena
name: Schneider, Silke L.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Measurement
subject: Harmonization
subject: Comparability
subject: Social Structure
subject: Third Gender

description: Socio-structural characteristics such as marital status, education or employment are measured in many surveys. Like attitudes and values, they are affected by social change and therefore need to be adapted to changing realities as well as to how we look at them. An example is the discussion on the introduction of a third category for the question on respondents’ sex. At the same time, for comparisons of these characteristics across different surveys, it is helpful if they are measured and coded in a comparable way. These goals are obviously in conflict with each other. This blog post deals with the measurement and harmonization of socio-structural characteristics in the light of social change as also discussed in the recent virtual GESIS symposium "Socio structural characteristics in surveys: collection, coding, harmonization”.
description: Sozialstrukturelle Merkmale wie Familienstand, Bildung oder Erwerbstätigkeit werden in vielen Umfragen erfasst. Sie unterliegen, ähnlich wie Einstellungen und Werte auch, dem gesellschaftlichen Wandel und müssen daher an sich ändernde Realitäten und an unseren sich ebenfalls verändernden Blick auf diese angepasst werden. Beispielhaft kann hier die Diskussion zur Einführung einer dritten Geschlechtskategorie in Fragebögen genannt werden. Gleichzeitig ist es für den Vergleich dieser Merkmale zwischen verschiedenen Umfragen hilfreich, wenn sie vergleichbar gemessen und kodiert werden. Diese Ziele stehen in einem offensichtlichen Spannungsverhältnis zueinander. Dieser Beitrag widmet sich der Erhebung und Harmonisierung sozialstruktureller Merkmale im Licht des sozialen Wandels, wie sie kürzlich im virtuellen GESIS-Symposium „Sozialstrukturelle Merkmale in Umfragen: Erhebung, Kodierung, Harmonisierung“ diskutiert wurden.
description: GESIS Blog
Sonnenfleckenzeichnung Nr. 3739.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.08.1951, erstellt als Beobachtung im Projektionsverfahren Nr. 1962 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Zusätzlich wurden ergänzende Angaben aufgrund weiterer Beobachtungen direkt auf der Fleckenzeichnung hinzugefügt. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
De héroes y encrucijadas: el bivium, motivo ideológico y estructurador de las narraciones caballerescas espirituales del Siglo de Oro
Creators: name: Herrán Alonso, Emma
Publisher: name: Historias Fingidas
Year: 1970

description: Se analiza, a partir de la tradición literaria e iconográfica anterior, uno de los motivos más recurrentes de las narraciones caballerescas espirituales del Siglo de Oro: el del bivium o camino que se bifurca, que sirve de hilo conductor de la aventura llevando al protagonista, cual Hércules prodicus, tras la siempre difícil elección, por el camino bien sea de la virtud o del vicio. Las diferentes estrategias de los autores del Siglo de Oro permiten comprobar la flexibilidad de este motivo heredado, puesto por ellos al servicio no solo de una lectura edificante (ya sea de carácter doctrinal, filosófico o espiritual), sino también utilizado como elemento clave sobre el que reposa la estructura narrativa del relato. We analyze, from the previous literary tradition and iconography, one of the recurring motifs of spiritual chivalric narratives of the Golden Age: the bivium or road forks, serving thread of adventure bringing the protagonist, as Hercules prodicus, after the always difficult choice between the path of virtue or vice. The different strategies of the authors of the Golden Age allow us to check the flexibility of this inherited motif put by them in the service of not only an uplifting reading (either doctrinal, philosophical or spiritual nature), but also as a key element on which rests the narrative structure of the story.
description: Historias Fingidas, No. 1 (2013)
Catálogo descriptivo y analítico de textos breves en los libros de caballerías hispánicos (siglos XV-XVII): poesía y prosa
Creators: name: Campos García Rojas, Axayácatl
Publisher: name: Historias Fingidas
Year: 1970

description: Este trabajo constituye una presentación del Catálogo descriptivo de textos breves en los libros de caballerías hispánicos (siglos XV-XVII). Se expone un estado de la cuestión y cómo se inserta en los estudios actuales sobre literatura caballeresca. Se define lo que para los fines del proyecto se considera texto breve y las diversas variantes, formas y funciones que tiene al interior de la narración caballeresca. Asimismo, se describen los objetivos y alcances del catálogo conformado en una base de datos. Hay muestras de cómo están conformadas las fichas de datos, los aspectos considerados, el contexto de los textos breves, su forma y su función. This is a presentation of the Catálogo descriptivo de textos breves en los libros de caballerías hispánicos (siglos XV-XVII), and its backgound in terms of romances of chivalry studies. There is also a definition of «texto breve», the function and structure that it may have in the romance narrative. There are also two samples of how this catalogue will work and will be usefull for future research projects.
description: Historias Fingidas, No. 1 (2013)
Evidence of jet induced optical microvariability in radio-loud Narrow Line Seyfert 1 Galaxies
Creators: name: Ojha, Vineet
name: Jha, Vivek Kumar
name: Chand, Hum
name: Singh, Veeresh
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: To quantify the role of radio jets for Intra-Night Optical Variability (INOV) in Radio-Loud Narrow-Line Seyfert 1 (RLNLSy1) galaxies, we report the first systematic comparative INOV study of 23 RLNLSy1 galaxies, with 15 RLNLSy1s having confirmed detection of jets (jetted) and the remaining 8 RLNLSy1s having no detection of jets (non-jetted) based on their Very Long Baseline Array observations. We have monitored these two samples, respectively, in 37 and 16 sessions of a minimum 3-hour duration each. Based upon F$^η$-test at 99\% confidence level with a typical INOV amplitude ($ψ$) detection threshold of $>$ 3\%, we find the INOV duty cycles of 12\% for the sample of jetted RLNLSy1s, however, none of the sources showed INOV in the sample of non-jetted RLNLSy1s. Among the jetted RLNLSy1s, we find that the Duty Cycle (DC) for jetted $γ$-ray detected ($γ$-ray) RLNLSy1s is found to be 34\% in contrast to null INOV detection in the case of non-$γ$-ray RLNLSy1s. It suggests that instead of the mere presence of a jet, relativistic beaming plays a significant role for INOV in the case of low-luminous high accreting AGNs such as NLSy1s in which dilution of the AGN's non-thermal optical emission by the (much steadier) optical emission contributed by the nuclear accretion disc is quite likely. Our study of jetted $γ$-ray RLNLSy1s shows more frequent INOV detection for sources with higher apparent jet speed. Further, our results also suggest that among the NLSy1s, only jetted $γ$-ray RNLSy1 galaxies DC approaches blazar like DC.
description: 18 pages, 6 figures, and 5 tables. Accepted for publication in MNRAS
Capnia ventura Nelson & Baumann 1987
Creators: name: Stewart, Kenneth W.
name: Drake, Eugene F.
name: Stark, Bill P.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Capniidae
Capnia
Capnia ventura

description: Capnia ventura Nelson & Baumann 1987
(Figs. 12-14, 50-55, 60, 61)
Distribution. California.
Material examined. California: Orange Co., Silverado Creek, Silverado Canyon, concrete low water crossing about 4.67km above Forest Service Fire Gate, N 33 ° 44.43 ’ W 117 ° 32.44 ’, 6-IV-2004, K.W. Stewart and E.F. Drake, 4♂, 7♀, 5♂ larval exuviae, 10♀ larval exuviae (adults and exuviae all together on a floating board), 11♀ larvae. Silverado Creek, 91.4m above Forest Service Fire Gate, 574.5m Elev., N 33 ° 44.55 ’ W 117 ° 34.56 ’, 9-II-2005, E.F. Drake, 2♂, 4♂ larvae, 23♀ larvae. Same locality, 10-III-2005, E.F. Drake, 1♂ larva, 9♀ larvae. Same locality, 25-III-2005, E.F. Drake, 1♂ larva, 6♀ larvae. Same locality, 18-II- 2006, E.F. Drake, 3♂ reared with exuviae, 4♀ reared with exuviae. Same locality, 20-22-II-2006, 2♂, 3♀.
Characters. Body length ♂ 6.4-7.0mm, ♀ 7.2-7.3mm. Light to medium brown dorsally, ventrum lighter, little pattern except underlying muscles or adult pigment. Antennal segments ♂ 48-50, ♀ 48-52, head capsule width ♂ 0.75-0.81mm, ♀ 0.78-0.90mm. Lacinia triangular, palmate with longitudinally striate palm surface, broad apical teeth, ventral comb of about 10 bristles and dorsal comb of 16-18 longer bristles (Figs. 50, 51). Right mandible with apical teeth, molar pad of dense stiff bristles, and inner band of hairs from base of apical teeth to molar pad (Fig. 52). Left mandible with molar cup bordered by outer (dorsal) comb of curved teeth (Fig. 53). Pronotum with scattered setae over surface and as a marginal fringe (like Fig. 1). Mesosternal Y-arms and shallowly notched hind wingpads typical of genus; inside fore wingpad length ♂ 0.90-0.96mm, ♀ 1.02- 1.08mm. Leg setation typical of genus (like Figs. 2, 3). Abdominal segments with long surface and posterior fringe hairs (Fig. 57). Sexual dimorphism evident. Male with posterior extension of 10 th tergum nippleshaped in dorsal view with underlying developing tubular epiproct visible in pharate individuals (Fig. 12); 10 th tergum in lateral view with emarginated sides, cross-striated basal half, and narrowing apically (Figs. 54, 55). Female without posterior extension of 10 th tergum (Fig. 13). Cercal segments ♂ 30-32, ♀ 32; cercomeres with apical circlet of short and long bristles, longer dorsal and ventral bristle in lateral view, and no intercalary hairs (Figs. 60, 61).
description: Published as part of Stewart, Kenneth W., Drake, Eugene F. & Stark, Bill P., 2011, Larvae Of Five Species Of The Winter Stonefly Genus Capnia (Plecoptera: Capniidae) From California, U. S. A., pp. 167-181 in Illiesia 7 (18) on pages 175-178, DOI: 10.5281/zenodo.4760235
title: Apples and Oranges: How to find out if two questions measure the same concept?
Creators: name: Singh, Ranjit K.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Ex-Post Harmonization Adventures
subject: Comparability
subject: Survey Methodology
subject: FAIR Data Principles
subject: Open Data

description: We delve into an important but difficult matter in harmonization in general and ex-post harmonization in particular: How can we determine if two instruments measure the same concept? This is especially hard if the concepts are latent (i.e., not directly observable).
description: Wir beschäftigen uns mit einem wichtigen, aber schwierigen Aspekt von Harmonisierung und insbesondere der ex-post Harmonisierung: Wie können wir feststellen, ob zwei Instrumente das gleiche Konzept messen? Das ist eine besondere Herausforderung, wenn das Konzept latent (also nicht direkt beobachtbar) ist.
description: GESIS Blog
Additional file 1 of Benchmarking AutoML frameworks for disease prediction using medical claims
Creators: name: A. Romero, Roland Albert
name: Y. Deypalan, Mariefel Nicole
name: Mehrotra, Suchit
name: Jungao, John Titus
name: Sheils, Natalie E.
name: Manduchi, Elisabetta
name: Moore, Jason H.
Publisher: name: figshare
Year: 2022
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 1 ROC AUC performance of different AutoML models trained for various disease outcomes from non-stratified bootstrap samples. Median values are indicated by diamond markers and 95% CI limits are indicated by circles.
Vol'nyj proězd"
Creators: name: Cvetaeva, Marina
Publisher: name: [s.n.]
Year: 1924

description: Korrekturabzug, mit handschriftlichen Anmerkungen, Vanves 1938
description: Erschienen in: Sovremennye zapiski 21 (1924), S. 247-278
description: Marina Cvetaeva
description: Russisch
description: Verzeichnung=Description=Inventaire November 2018 HAN-Katalogisierungsregeln
title: The sum and its parts: The benefits of combining data from different surveys
Creators: name: Singh, Ranjit K.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Ex-Post Harmonization Adventures
subject: Comparability
subject: Survey Methodology
subject: FAIR Data Principles
subject: Open Data

description: Ex-post harmonization – combining data from different surveys – requires quite some effort. In this post, we explore the many reasons why it is still worth it. All benefits discussed here apply equally to large scale and smaller ex-post harmonization efforts.
description: Ex-post Harmonisierung – das Verbinden von Daten aus verschiedenen Umfragen – ist nicht unaufwändig. In diesem Post geht es um die vielen Gründe, warum es sich dennoch lohnt. Die Vorteile, die diskutiert werden, treffen gleichermaßen auf große wie kleine ex-post Harmonisierungsprojekte zu.
description: GESIS Blog
Dynamical Modelling and Emission Signatures of a Candidate Dual AGN with Precessing Radio Jets
Creators: name: Giri, Gourab
name: Dubey, Ravi Pratap
name: Rubinur, K.
name: Vaidya, Bhargav
name: Kharb, Preeti
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In this paper, we have modelled the dynamical and emission properties (in the presence of radiative losses and diffusive shock acceleration) of an observed S-shaped radio source (2MASX J12032061+131931) due to a precessing jet. In this regard, we have performed high-resolution 3D magnetohydrodynamic (MHD) simulations of a precessing jet in a galactic environment. We show the appearance of a distinct S-shape with two bright hotspots when the bow shock region weakens over time. The formed morphology is sensitive to the parameter selections. The increased interaction between the helical jet and the ambient medium and the deceleration of the jet due to MHD instabilities also greatly affect the resulting structure. Hence, kinematic models must be corrected for these deceleration effects in order to adequately predict the precession parameters. The synthetic spectral index map shows that the jet side and leading edges possess relatively steeper spectral index values than the jet ridge lines, whereas the hotspots show flat spectral index values. The jets are also found to be highly linearly polarized (up to 76%) and the magnetic field lines, in general, follow the jet locus which is formed due to the jet-ambient medium interaction. Diffusive shocks, in this context, keep the structure active during its course of evolution. Furthermore, we have demonstrated that these galaxies deviate significantly from the equipartition approximation leading to a discrepancy in their spectral and dynamical age.
description: 15 pages, 16 figures, 1 table Accepted for publication in the Monthly notices of the Royal Astronomical Society
การพัฒนากฎหมายเพื่อให้ตราสารทางการเงินที่ใช้ในการระดมทุนมีลักษณะเป็นตราสารเปลี่ยนมือ
Creators: name: ปกป้อง กลับวิเศษ
Publisher: name: Mae Fah Luang University
Year: 2017
Subjects: ตราสารเปลี่ยนมือ / การระดมทุน / ผู้ทรงตราสาร

description: MFU Connexion: Journal of Humanities and Social Sciences, 6, 2