cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Oecobius navus Blackwall 1859
Creators: name: Fusco, Tommaso
name: Fattorini, Simone
name: Fortini, Lorenzo
name: Ruzzier, Enrico
name: Di Giulio, Andrea
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Oecobiidae
Oecobius
Oecobius navus

description: Oecobius navus Blackwall, 1859
Materials
Type status: Other material. Occurrence: recordedBy: Fattorini S., Di Giulio A.; individualCount: 1; sex: male; lifeStage: adult; occurrenceID: 58CC8F84-8A4C-5435-85BC-9B3CBE312942; Taxon: scientificName: Oecobius navus Blackwall, 1859; order: Araneae; family: Oecobiidae; genus: Oecobius; Location: country: Italy; countryCode: IT; stateProvince: Rome; county: Rome; municipality: Rome; locality: Appia Antica Regional Park, Rome; locationRemarks: San Sebastiano; decimalLatitude: 41.855733; decimalLongitude: 12.515114; geodeticDatum: WGS 84; Identification: identifiedBy: Tommaso Fusco; dateIdentified: 2022; Event: samplingProtocol: Pitfall traps; eventDate: 2014-06 - 09; Record Level: collectionID: Roma 3 _ 5.8
Distribution
Europe, northern Africa, South Africa, Turkey, Caucasus. Introduced to South Africa, China, Korea, Japan, New Zealand, Canada, USA, South America. Cosmopolitan (COS) chorotype.
description: Published as part of Fusco, Tommaso, Fattorini, Simone, Fortini, Lorenzo, Ruzzier, Enrico & Di Giulio, Andrea, 2024, Ground spiders (Chelicerata, Araneae) of an urban green space: intensive sampling in a protected area of Rome (Italy) reveals a high diversity and new records to the Italian territory, pp. e 122896 in Biodiversity Data Journal 12 on page e122896, DOI: 10.3897/BDJ.12.e122896
Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data
Creators: name: Garny, Mathias
name: Konstandin, Thomas
name: Sagunski, Laura
name: Viel, Matteo
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2020
Subjects: neutrino: mass
dimension: 1
error: statistical
power spectrum
flux
cosmic background radiation: temperature
conservation law
calibration
nonlinear
capture
satellite: Planck

description: We present an effective model for the one-dimensional Lyman-$\alpha$ flux power spectrum far above the baryonic Jeans scale. The main new ingredient is constituted by a set of two parameters that encode the impact of small, highly non-linear scales on the one-dimensional power spectrum on large scales, where it is measured by BOSS. We show that, by marginalizing over the model parameters that capture the impact of the intergalactic medium, the flux power spectrum from both simulations and observations can be described with high precision. The model displays a degeneracy between the neutrino masses and the (unknown, in our formalism) normalization of the flux power spectrum. This degeneracy can be lifted by calibrating one of the model parameters with simulation data, and using input from Planck CMB data. We demonstrate that this approach can be used to extract bounds on the sum of neutrino masses with comparably low numerical effort, while allowing for a conservative treatment of uncertainties from the dynamics of the intergalactic medium. An explorative analysis yields an upper bound of $0.16\,$eV at $95\%$ C.L. when applied to BOSS data at $3\leq z\leq 4.2$. We also forecast that if the systematic and statistical errors will be reduced by a factor two the upper bound will become $0.1\,$eV at $95\%$ C.L.
Tetrodotoxin identified in polyclad flatworms of temperate Eastern Australia
Creators: name: McNab, Justin Michael
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: Soft bodied marine invertebrates often possess bioactive secondary metabolites that they utilise in defensive or offensive contexts. These invertebrates utilise toxic secondary metabolites as chemical defenses and as venoms to enable them to become successful in their environments. The field of marine natural products often studies molecules isolated from invertebrates and one largely overlooked, yet prevalent group are flatworms of the order Polycladida. The potent neurotoxin tetrodotoxin is known to occur within this group in species of the suborder Acotylea, although its occurrence is only documented in polyclads from Asia and New Zealand. Herein, this thesis firstly reviews what is known about natural products isolated from polyclads from both Acotylea and Cotylea. Then, Australian polyclads from both Acotylea and Cotylea are tested for tetrodotoxin, to expand knowledge of this molecules distribution throughout the order. Finally, these results are discussed and future directions for study are given.
Alcelaphus Blainville 1816
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Alcelaphus

description: Alcelaphus Blainville, 1816. Bull. Sci. Soc. Philom. Paris, p. 75. COMMENT: Haltenorth, 1963:99, and Van Gelder, 1977, included Beatragus, Sigmoceros and Damaliscus in this genus, but have not been followed by recent authors; see Swanepoel et al., 1980, Ann. Transvaal Mus., 32(7):187. Formerly included Sigmoceros lichtensteini; see comment under Sigmoceros. ISIS NUMBER: 5301419009012000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 326, DOI: 10.5281/zenodo.7352976
description: {"references": ["Haltenorth, T. 1963. Klassifikation der Saugetiere: Artiodactyla I. Handbuch der Zoologie, 8 (32): 1 - 167.", "Swanepoel, P., R. H. N. Smithers, and I. L. Rautenbach. 1980. A checklist and numbering system of the extant mammals of the Southern African Subregion. Annals of the Transvaal Museum, 32: 155 - 196."]}
The Air Microwave Yield (AMY) experiment - A laboratory measurement of the microwave emission from extensive air showers
Creators: name: Louedec, K.
name: Alvarez-Muñiz, J.
name: Blanco, M.
name: Bohácová, M.
name: Buonomo, B.
name: Cataldi, G.
name: Coluccia, M. R.
name: Creti, P.
name: De Mitri, I.
name: Di Giulio, C.
name: Luis, P. Facal San
name: Foggetta, L.
name: Gaïor, R.
name: Garcia-Fernandez, D.
name: Iarlori, M.
name: Coz, S. Le
name: Letessier-Selvon, A.
name: Mariş, I. C.
name: Martello, D.
name: Mazzitelli, G.
name: Monasor, M.
name: Perrone, L.
name: Pesce, R.
name: Petrera, S.
name: Privitera, P.
name: Rizi, V.
name: Fernandez, G. Rodriguez
name: Salamida, F.
name: Salina, G.
name: Settimo, M.
name: Valente, P.
name: Vazquez, J. R.
name: Verzi, V.
name: Williams, C.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The AMY experiment aims to measure the microwave bremsstrahlung radiation (MBR) emitted by air-showers secondary electrons accelerating in collisions with neutral molecules of the atmosphere. The measurements are performed using a beam of 510 MeV electrons at the Beam Test Facility (BTF) of Frascati INFN National Laboratories. The goal of the AMY experiment is to measure in laboratory conditions the yield and the spectrum of the GHz emission in the frequency range between 1 and 20 GHz. The final purpose is to characterise the process to be used in a next generation detectors of ultra-high energy cosmic rays. A description of the experimental setup and the first results are presented.
description: 3 pages -- EPS-HEP'13 European Physical Society Conference on High Energy Physics (July, 18-24, 2013) at Stockholm, Sweden
RR Lyrae variables: visual and infrared luminosities, intrinsic colours, and kinematics
Creators: name: Dambis, A. K.
name: Berdnikov, L. N.
name: Kniazev, A. Y.
name: Kravtsov, V. V.
name: Rastorguev, A. S.
name: Sefako, R.
name: Vozyakova, O. V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use UCAC4 proper motions and WISE W1-band apparent magnitudes intensity-mean for almost 400 field RR Lyrae variables to determine the parameters of the velocity distribution of Galactic RR Lyrae population and constrain the zero points of the metallicity- relation and those of the period-metallicity--band and period-metallicity--band luminosity relations via statistical parallax. We find the mean velocities of the halo- and thick-disc RR Lyrae populations in the solar neighbourhood to be (U0(Halo), V0(Halo), W0(Halo)) = (-7 +/- 9, -214 +/- 10, -10 +/- 6) km/s and (U0(Disc), V0(Disc), W0(Disc)) =(-13 +/- 7, -37 +/- 6, -17 +/- 4) km/s, respectively, and the corresponding components of the velocity-dispersion ellipsoids, (sigma VR(Halo), sigma Vphi(Halo), sigma Vtheta(Halo)) = (153 +/- 9, 101 +/- 6, 96 +/- 5) km/s and (sigma VR(Disc), sigma Vphi(Disc), sigma Vtheta(Disc)) = (46 +/- 7, 37 +/- 5, 27 +/- 4) km/s, respectively. The fraction of thick-disc stars is estimated at 0.22 +/- 0.03. The corrected IR period-metallicity-luminosity relations are = -0.769 +0.088 [Fe/H]- 2.33 mathoprm log PF and = -0.825 + 0.088 [Fe/H] -2.33 mathoprm log PF, and the optical metallicity-luminosity relation, [Fe/H]-, is = +1.094 + 0.232 [Fe/H], with a standard error of +/- 0.089, implying an LMC distance modulus of 18.32 +/- 0.09, a solar Galactocentric distance of 7.73 +/- 0.36 kpc, and the M31 and M33 distance moduli of DM(M31) = 24.24 +/- 0.09 (D = 705 +/- 30 kpc) and DM(M33) = 24.36 +/- 0.09 (D = 745 +/- 31 kpc), respectively. Extragalactic distances calibrated with our RR Lyrae star luminosity scale imply a Hubble constant of ~80 km/s/Mpc. Our results suggest marginal prograde rotation for the population of halo RR Lyraes in the Milky Way.
description: 17 pages, 5 tables, 11 figures. To be published in the Monthly Notices of the Royal Astronomical Society
Lessons from the $B^{0,+}\to K^{*0,+}\mu^+\mu^-$ angular analyses
Creators: name: Ciuchini, Marco
name: Fedele, Marco
name: Franco, Enrico
name: Paul, Ayan
name: Silvestrini, Luca
name: Valli, Mauro
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2020
Subjects: * Automatic Keywords *
lepton: universality: violation
universality: violation
branching ratio: ratio
new physics
LHC-B
correlation
electron
muon

description: We perform an analysis within the Standard Model of $B^{0,+} \to K^{*0,+} \mu^+ \mu^-$ decays in light of the recent measurements from the LHCb experiment, showing that new data strengthen the need for sizable hadronic contributions and correlations among them. We then extend our analysis to New Physics via the Standard Model Effective Theory, and carry out a state-of-the-art fit of available $b \to s \ell^+ \ell^-$ data, including possible hadronic contributions. We find the case of a fully left-handed operator standing out as the simplest scenario with a significance of almost $6\sigma$.
Alcelaphus buselaphus
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Alcelaphus
Alcelaphus buselaphus

description: Alcelaphus buselaphus (Pallas, 1766). Misc. Zool., p. 7. TYPE LOCALITY: Probably Morocco. DISTRIBUTION: Senegal to W. Somalia to N. South Africato S. Angola;formerlyN. Africa. COMMENT: Includes tora; which according to PG is probably a separatespecies. Includes caama; see Ansell, 1972, Part. 15:53-54. PROTECTED STATUS: U.S. ESA- Endangered as A. b. swayneisubspeciesonly. U.S. ESA - Endangered as A. b. tora subspecies only. ISIS NUMBER: 5301419009012001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 326, DOI: 10.5281/zenodo.7352976
description: {"references": ["Ansell, W. F. H. 1972. Order Artiodactyla. Part 15. Pp. 1 - 84, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.) [issued 2 May 1972]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Mass Renormalization in String Theory: General States
Creators: name: Pius, Roji
name: Rudra, Arnab
name: Sen, Ashoke
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In a previous paper we described a procedure for computing the renormalized masses and S-matrix elements in bosonic string theory for a special class of massive states which do not mix with unphysical states under renormalization. In this paper we extend this result to general states in bosonic string theory, and argue that only the squares of renormalized physical masses appear as the locations of the poles of the S-matrix of other physical states. We also discuss generalizations to Neveu-Schwarz sector states in heterotic and superstring theories.
description: LaTeX file, 40 pages; v2: minor typos corrected
title: Die Kennzeichnung der Juden im Mittelalter; 1915
title: Ein Beitrag zur sozialen Geschichte des Judentums
titleType: Subtitle
Creators: name: Singermann, Felix
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Freiburg, Breisgau, Univ., Diss., 1914
Bipartite-Finsler spaces and the bumblebee model
Creators: name: Silva, J. Euclides G.
name: Almeida, C. A. S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present a proposal to include Lorentz-violating effects in gravitational field by means of the Finsler geometry. In the Finsler set up, the length of an event depends both on the point and the direction in the space-time. We briefly review the bumblebee model, where the Lorentz violation is induced by a spontaneous symmetry breaking due to the bumblebee vector field.The main geometrical concepts of the Finsler geometry are outlined. Using a Finslerian Einstein-Hilbert action we derive the bumblebee action from the bipartite Finsler function with a correction to the gravitational constant.
description: Presented at the Sixth Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 17-21, 2013
Auflösung von geländeseitig verursachten Antriebsverspannungen bei hochmobilen Arbeitsmaschinen
Creators: name: Herr, Stefan
name: Müller, Werner
name: Müller, Johannes
name: Eckloff, Udo
Publisher: name: KIT Scientific Publishing
Year: 2020
Subjects: Drehmoment
Drehmomentspitze
Peak
Verspannung
Antriebsstrang
Fahrantrieb
Allradantrieb

description: Bei schweren Arbeitsmaschinen, treten regelmäßig Antriebsverspannungen auf. Diese resultieren insbesondere daraus, dass herkömmliche Antriebsstränge mit Längs- und Querdifferenzialen systembedingt die auftretenden Drehzahlunterschiede im Gelände nicht ausgleichen können. Aktuell werden diesen Gegebenheiten durch Überdimensionierung der mechanischen Antriebsstränge kompensiert. Ziel des Projektes war, die straßen- und geländeseitig verursachten Antriebsverspannungen aktiv an den angetriebenen Rädern zu kompensieren, bevor sie in das Gesamtsystem eintreten können. Zentrales Element ist hierbei ein Planetengetriebe, dessen Hohlrad über eine hydraulische Einheit mit dem Fahrzeugrahmen verbunden ist. Über eine Ventilsteuerung der hydraulischen Einheit, lässt sich ein gezielter Freiheitsgrad in das Gesamtsystem einbringen. Durch die Entwicklung einer realen Antriebseinheit und Integration in eine Simulation eines schweren 8 × 8 Geländefahrzeugs konnte nachgewiesen werden, dass es möglich ist, diese Antriebsverspannungen im besten Fall komplett zu verhindern. Extern eingeprägte Drehmomentspitzen werden direkt am Rad gestoppt bevor Verspannungen entstehen können.
Ammodorcas Thomas 1891
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Ammodorcas

description: Ammodorcas Thomas, 1891. Proc. Zool. Soc. Lond., 1891:207, pl. 21, 22. REVIEWED BY: D. Ernst (DE). ISIS NUMBER: 5301419009021000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 326, DOI: 10.5281/zenodo.7352976
Spin Fluctuations and Frustrated Magnetism in the Multiferroic FeVO$_4$
Creators: name: Zhang, J.
name: Ma, L.
name: Dai, J.
name: Zhang, Y. P.
name: He, Z. Z.
name: Normand, B.
name: Yu, Weiqiang
Publisher: name: arXiv
Year: 2014
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report $^{51}$V nuclear magnetic resonance (NMR) studies on single crystals of the multiferroic material FeVO$_4$. The high-temperature Knight shift shows Curie-Weiss behavior, $^{51}K = a/(T + θ)$, with a large Weiss constant $θ\approx$ 116 K. However, the $^{51}$V spectrum shows no ordering near these temperatures, splitting instead into two peaks below 65 K, which suggests only short-ranged magnetic order on the NMR time scale. Two magnetic transitions are identified from peaks in the spin-lattice relaxation rate, $1/^{51}T_1$, at temperatures $T_{N1} \approx$ 19 K and $T_{N2} \approx$ 13 K, which are lower than the estimates obtained from polycrystalline samples. In the low-temperature incommensurate spiral state, the maximum ordered moment is estimated as 1.95$μ_B$/Fe, or 1/3 of the local moment. Strong low-energy spin fluctuations are also indicated by the unconventional power-law temperature dependence $1/^{51}T_1 \propto T^2$. The large Weiss constant, short-range magnetic correlations far above $T_{N1}$, small ordered moment, significant low-energy spin fluctuations, and incommensurate ordered phases all provide explicit evidence for strong magnetic frustration in FeVO$_4$.
description: 7 pages, 4 figures, published in Phys. Rev. B
Ammodorcas clarkei
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Ammodorcas
Ammodorcas clarkei

description: Ammodorcas clarkei (Thomas, 1891). Ann. Mag. Nat. Hist., ser. 6, 7: 304. TYPE LOCALITY: Somalia, Habergerhagi's Country, Buroa Wells. DISTRIBUTION: E. Ethiopia; N. Somalia. PROTECTED STATUS: U.S. ESA - Endangered as A. clarki (sic). ISIS NUMBER: 5301419009021001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 326, DOI: 10.5281/zenodo.7352976
Truncated affine Rozansky--Witten models as extended defect TQFTs
Creators: name: Brunner, Ilka
name: Carqueville, Nils
name: Fragkos, Pantelis
name: Roggenkamp, Daniel
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We apply the cobordism hypothesis with singularities to the case of affine Rozansky--Witten models, providing a construction of extended TQFTs that includes all line and surface defects. On a technical level, this amounts to proving that the associated homotopy 2-category is pivotal, and to systematically employing its 3-dimensional graphical calculus. This in particular allows us to explicitly calculate state spaces for surfaces with arbitrary defect networks. As specific examples we discuss symmetry defects which can be used to model non-trivial background gauge fields, as well as boundary conditions.
description: 79 pages
Philodromus rufus Walckenaer 1826
Creators: name: Fusco, Tommaso
name: Fattorini, Simone
name: Fortini, Lorenzo
name: Ruzzier, Enrico
name: Di Giulio, Andrea
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Philodromidae
Philodromus
Philodromus rufus

description: Philodromus rufus Walckenaer, 1826
Materials
Type status: Other material. Occurrence: recordedBy: Fattorini S., Di Giulio A.; individualCount: 1; sex: female; lifeStage: adult; occurrenceID: D5B984DE-B1E7-548F-912E-7C95C634A415; Taxon: scientificName: Philodromus rufus Walckenaer, 1826; order: Araneae; family: Philodromidae; genus: Philodromus; Location: country: Italy; countryCode: IT; stateProvince: Rome; county: Rome; municipality: Rome; locality: Appia Antica Regional Park, Rome; locationRemarks: Caffarella Nord; decimalLatitude: 41.867753; decimalLongitude: 12.512414; geodeticDatum: WGS 84; Identification: identifiedBy: Tommaso Fusco; dateIdentified: 2022; Event: samplingProtocol: Pitfall traps; eventDate: 2014-06 - 06; Record Level: collectionID: Roma 3 _ 5.8
Distribution
North America, Europe, Turkey, Caucasus, Russia (Europe to Far East), Kazakhstan, Iran, Central Asia, Mongolia, China, Korea, Japan. Holarctic (OLA) chorotype.
description: Published as part of Fusco, Tommaso, Fattorini, Simone, Fortini, Lorenzo, Ruzzier, Enrico & Di Giulio, Andrea, 2024, Ground spiders (Chelicerata, Araneae) of an urban green space: intensive sampling in a protected area of Rome (Italy) reveals a high diversity and new records to the Italian territory, pp. e 122896 in Biodiversity Data Journal 12 on page e122896, DOI: 10.3897/BDJ.12.e122896
An observational correlation between stellar brightness variations and surface gravity
Creators: name: Bastien, Fabienne A.
name: Stassun, Keivan G.
name: Basri, Gibor
name: Pepper, Joshua
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Surface gravity is one of a star's basic properties, but it is difficult to measure accurately, with typical uncertainties of 25-50 per cent if measured spectroscopically and 90-150 per cent photometrically. Asteroseismology measures gravity with an uncertainty of about two per cent but is restricted to relatively small samples of bright stars, most of which are giants. The availability of high-precision measurements of brightness variations for >150,000 stars provides an opportunity to investigate whether the variations can be used to determine surface gravities. The Fourier power of granulation on a star's surface correlates physically with surface gravity; if brightness variations on timescales of hours arise from granulation, then such variations should correlate with surface gravity. Here we report an analysis of archival data that reveals an observational correlation between surface gravity and the root-mean-square brightness variations on timescales of less than eight hours for stars with temperatures of 4500-6750K, log of surface gravities of 2.5-4.5 (cgs units), and having overall brightness variations <3 parts per thousand. A straightforward observation of optical brightness variations therefore allows a determination of the surface gravity with a precision of <25 percent for inactive Sun-like stars at main-sequence to giant stages of evolution.
description: Published in Nature (21 August 2013), 25 pages and 6 figures, including Supplementary Information. A machine-readable table containing flicker measurements for the asteroseismic sample is available in the online version of the paper
LTER Zöbelboden, Austria, Runoff Water Chemistry, 2013
Creators: name: Kobler, Johannes
name: Dirnböck, Thomas
name: Pröll, Gisela
Publisher: name: https://b2share.eudat.eu
Year: 2020

description: Runoff water chemistry data of the LTER station Zöbelboden from the year 2013
EFFICIENTNEXT: EFFICIENTNET FOR EMBEDDED SYSTEMS
Creators: name: Deokar, Abhishek Rajendra
Publisher: name: Purdue University Graduate School
Year: 2022
Subjects: Digital processor architectures
Other information and computing sciences not elsewhere classified
Electrical engineering not elsewhere classified

description: Convolutional Neural Networks have come a long way since AlexNet. Each year the limits of the state of the art are being pushed to new levels. EfficientNet pushed the performance metrics to a new high and EfficientNetV2 even more so. Even so, architectures for mobile applications can benefit from improved accuracy and reduced model footprint. The classic Inverted Residual block has been the foundation upon which most mobile networks seek to improve. EfficientNet architecture is built using the same Inverted Residual block. In this paper we experiment with Harmonious Bottlenecks in place of the Inverted Residuals to observe a reduction in the number of parameters and improvement in accuracy. The designed network is then deployed on the NXP i.MX 8M Mini board for Image classification.
Testing the nature of the supermassive black hole candidate in SgrA* with light curves and images of hot spots
Creators: name: Li, Zilong
name: Kong, Lingyao
name: Bambi, Cosimo
Publisher: name: arXiv
Year: 2014
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: General relativity makes clear predictions about the spacetime geometry around black holes. In the near future, new facilities will have the capability to explore the metric around SgrA$^*$, the supermassive black hole candidate at the Center of our Galaxy, and open a new window to test the Kerr black hole hypothesis. In this paper, we compute light curves and images associated with compact emission regions (hot spots) orbiting around Kerr and non-Kerr black holes. We study how the analysis of the properties of the radiation emitted by a hot spot can be used to test the Kerr nature of SgrA$^*$. We find that the sole observation of the hot spot light curve can at most constrain a combination of the black hole spin and of possible deviations from the Kerr solution. This happens because the same orbital frequency around a Kerr black hole can be found for a non-Kerr object with a different spin parameter. Second order corrections in the light curve due to the background geometry are typically too small to be identified. While the observation of the hot spot centroid track can potentially bound possible deviations from the Kerr solution, that is out of reach for the near future VLTI instrument GRAVITY. The Kerr black hole hypothesis could really be tested in the case of the discovery of a radio pulsar in a compact orbit around SgrA$^*$. Radio observations of such a pulsar would provide precise estimates of the mass and the spin of SgrA$^*$, and the combination of these measurements (probing the weak field) with the hot spot light curve information (probing the strong field) may constrain/find possible deviations from the Kerr solution with quite good precision.
description: 16 pages, 14 figures. v3: refereed version
Ammotragus Blyth 1840
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Ammotragus

description: Ammotragus Blyth, 1840. Proc. Zool. Soc. Lond., 1840:13. COMMENT: Ansell, 1972, Part 15:70, included Ammotragus in Capra; but see comment under Capra. ISIS NUMBER: 5301419009033000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 326, DOI: 10.5281/zenodo.7352976
description: {"references": ["Ansell, W. F. H. 1972. Order Artiodactyla. Part 15. Pp. 1 - 84, in The mammals of Africa: An identification manual (J. Meester and H. W. Setzer, eds.) [issued 2 May 1972]. Smithsonian Institution Press, Washington, D. C., not continuously paginated."]}
Squeezed States and Hermite polynomials in a Complex Variable
Creators: name: Ali, S. T.
name: Gorska, K.
name: Horzela, A.
name: Szafraniec, F. H.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Following the lines of the recent paper of J.-P. Gazeau and F. H. Szafraniec [J. Phys. A: Math. Theor. 44, 495201 (2011)], we construct here three types of coherent states, related to the Hermite polynomials in a complex variable which are orthogonal with respect to a non-rotationally invariant measure. We investigate relations between these coherent states and obtain the relationship between them and the squeezed states of quantum optics. We also obtain a second realization of the canonical coherent states in the Bargmann space of analytic functions, in terms of a squeezed basis. All this is done in the flavor of the classical approach of V. Bargmann [Commun. Pur. Appl. Math. 14, 187 (1961)].
description: 15 pages
Ammotragus lervia
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Ammotragus
Ammotragus lervia

description: Ammotragus lervia (Pallas, 1777). Spicil. Zool., 12: 12. TYPE LOCALITY: Algeria, Oran. DISTRIBUTION: N. Egypt to Morocco; Niger to Sudan; nerhaps S. Israel. Introduced to New Mexico and Texas (U.S.A.). COMMENT: Should be included in Hemitragus (PG). Reviewed by Gray and Simpson, 1980, Mamm. Species, 144:1-7. PROTECTED STATUS: CITES - Appendix III (Tunisia). ISIS NUMBER: 5301419009033001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on pages 326-327, DOI: 10.5281/zenodo.7352976
description: {"references": ["Gray, G. G., and C. D. Simpson. 1980. Ammotragus lervia. Mammalian Species, 144: 1 - 7."]}
The Angular Broadening of the Galactic Center Pulsar SGR J1745-29: A New Constraint on the Scattering Medium
Creators: name: Bower, Geoffrey C.
name: Deller, Adam
name: Demorest, Paul
name: Brunthaler, Andreas
name: Eatough, Ralph
name: Falcke, Heino
name: Kramer, Michael
name: Lee, K. J.
name: Spitler, Laura
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The pulsed radio emission from the Galactic Center (GC) magnetar SGR J1745-29 probes the turbulent, magnetized plasma of the GC hyperstrong scattering screen through both angular and temporal broadening. We present the first measurements of the angular size of SGR J1745-29, obtained with the Very Long Baseline Array and the phased Very Large Array at 8.7 and 15.4 GHz. The source sizes are consistent with the scatter--broadened size of Sagittarius A* at each frequency, demonstrating that SGR J1745-29 is also located behind the same hyperstrong scattering medium. Combining the angular broadening with temporal scattering obtained from pulsar observations provides a complete picture of the scattering properties. If the scattering occurs in a thin screen, then it must be at a distance Δ>~ 5 kpc. A best-fit solution for the distance of a thin screen is Δ=5.9 +/-0.3 kpc, consistent with being located in the Scutum spiral arm. This is a substantial revision of the previously held model in which the scattering screen is located very close to the GC. As also discussed in Spitler et al., these results suggest that GC searches can detect millisecond pulsars gravitationally bound to Sgr A* with observations at >~ 10 GHz and ordinary pulsars at even lower frequencies.
description: ApJL submitted
Aelurilus v-insignitus
Creators: name: Fusco, Tommaso
name: Fattorini, Simone
name: Fortini, Lorenzo
name: Ruzzier, Enrico
name: Di Giulio, Andrea
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Salticidae
Aelurilus
Aelurilus v-Insignitus

description: Aelurilus v-insignitus (Clerck, 1757)
Materials
Type status: Other material. Occurrence: recordedBy: Fattorini S., Di Giulio A.; individualCount: 1; sex: male; lifeStage: adult; occurrenceID: 51E35146-FE0E-52C0-8586-46720AA7B2DB; Taxon: scientificName: Aelurillus v-insignitus (Clerck, 1757); order: Araneae; family: Salticidae; genus: Aelurillus; Location: country: Italy; countryCode: IT; stateProvince: Rome; county: Rome; municipality: Rome; locality: Appia Antica regional Park, Rome; locationRemarks: Casal Verbeni; decimalLatitude: 41.815250; decimalLongitude: 12.552222; geodeticDatum: WGS 84; Identification: identifiedBy: Tommaso Fusco; dateIdentified: 2022; Event: samplingProtocol: Pitfall traps; eventDate: 2014-05 - 26; Record Level: collectionID: Roma 3 _ 5.8
Distribution
Europe, Turkey, Caucasus, Russia (Europe to Far East), Kazakhstan, Central Asia, China. Palaearctic (PAL) chorotype.
description: Published as part of Fusco, Tommaso, Fattorini, Simone, Fortini, Lorenzo, Ruzzier, Enrico & Di Giulio, Andrea, 2024, Ground spiders (Chelicerata, Araneae) of an urban green space: intensive sampling in a protected area of Rome (Italy) reveals a high diversity and new records to the Italian territory, pp. e 122896 in Biodiversity Data Journal 12 on page e122896, DOI: 10.3897/BDJ.12.e122896
Measurement of the $ν_μ$ flux and inclusive charged current cross section at T2K's near detector
Creators: name: Salzgeber, Melody Ravonel
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present the first measurement of the muon neutrino spectrum at the T2K near detector, ND280, using the data collected at the JPARC acc\ elerator facility in Tokai, Japan. ND280 is located 280 meters downstream from the target and 2.5$^\circ$ off-axis from the direction of the beam. The measured spectrum at ND280 constrains the flux and cross section uncertainties\ in the T2K oscillation analysis. We select inclusive charged-current (CC) events from muon \ neutrinos in ND280. These are separated into a charged current quasi-elastic (CCQE) enhanced sample and a CC non\ -QE sample. We then fit the muon spectrum for both samples to extract flux and cross section parameters, which are used as inputs into T2K's os\ cillation analysis. We separately produce a flux-averaged differential inclusive CC cross-se\ ction in the 2-dimensional plane of muon momentum and angle. For the cross-section measurement the flux is given by the MC and tuned to data from the NA61 experiment. We present the event selection, detector uncertainties, and final measurement result for both the spectrum and for the cross-section.
Antidorcas Sundevall 1847
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Antidorcas

description: Antidorcas Sundevall, 1847. Kongl. Svenska Vet.-Akad. Handl. Stockholm, for 1845, p. 271. ISIS NUMBER: 5301419009022000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 327, DOI: 10.5281/zenodo.7352976
K-theory, reality, and duality
Creators: name: Heard, Drew
name: Stojanoska, Vesna
Publisher: name: arXiv
Year: 2014
Subjects: subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics

description: We show that the real K-theory spectrum KO is Anderson self-dual using the method previously employed in the second author's calculation of the Anderson dual of Tmf. Indeed the current work can be considered as a lower chromatic version of that calculation. Emphasis is given to an algebro-geometric interpretation of this result in spectrally derived algebraic geometry. We finish by applying the result to a calculation of 2-primary Gross-Hopkins duality at height 1, and obtain an independent calculation of the group of exotic elements of the K(1)-local Picard group.
description: 24 pages; 6 figures. Updated to include reviewers comments, section 9 rewritten. Comments welcome
Intellection - A Bi-annual Interdisciplinary Research Journal
Creators: name: Islam, K M Baharul
Publisher: name: figshare
Year: 2022
Subjects: subject: Education
subject: Sociology
subject: FOS: Sociology
subject: 200101 Communication Studies
subject: FOS: Media and communications
subject: 200102 Communication Technology and Digital Media Studies
subject: 200199 Communication and Media Studies not elsewhere classified
subject: 200205 Culture, Gender, Sexuality
subject: FOS: Other humanities
subject: 220102 Business Ethics
subject: FOS: Philosophy, ethics and religion
subject: 130203 Economics, Business and Management Curriculum and Pedagogy
subject: FOS: Educational sciences
subject: Entertainment
subject: Gender studies
subject: Literature

description: Intellection- A Bi-annual Interdisciplinary Peer-Reviewed Research Journal Volume: X No 1, 2022 ISSN: 2319-8192 Published by: Barak Education Society A K Lane, Opp.Vivekananda Co-operative Society Hailakandi Road, P.O. Meherpur Silchar 788015 Assam India Tel: +91 9401425431, 9435072786, 9435370812
Quantum Control in the Cs 6S_{1/2} Ground Manifold Using rf and μw Magnetic Fields
Creators: name: Smith, A.
name: Anderson, B. E.
name: Sosa-Martinez, H.
name: Riofrío, C. A.
name: Deutsch, I. H.
name: Jessen, P. S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We implement arbitrary maps between pure states in the 16-dimensional Hilbert space associated with the ground electronic manifold of Cs. This is accomplished by driving atoms with phase modulated rf and μw fields, using modulation waveforms found via numerical optimization and designed to work robustly in the presence of imperfections. We evaluate the performance of a sample of randomly chosen state maps by randomized benchmarking, obtaining an average fidelity >99%. Our protocol advances state-of-the-art quantum control and has immediate applications in quantum metrology and tomography.
Near-Limb Zeeman and Hanle Diagnostics
Creators: name: Kim, I. S.
name: Alexeeva, I. V.
name: Bugaenko, O. I.
name: Popov, V. V.
name: Suyunova, E. Z.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: "Weak" magnetic-field diagnostics in faint objects near the bright solar disk are discussed in terms of the level of non-object signatures, in particular, of the stray light in telescopes. Calculated dependencies of the stray light caused by diffraction at the 0.5-, 1.6-, and 4-meter entrance aperture are presented. The requirements for micro-roughness of refractive and reflective primary optics are compared. Several methods for reducing the stray light (the Lyot coronagraphic technique, multiple stages of apodizing in the focal and exit pupil planes, apodizing in the entrance aperture plane with a special mask), and reducing the random and systematic errors are noted. An acceptable level of stray light in telescopes is estimated for the V-profile recording with a signal-to-noise ratio greater than three. Prospects for the limb chromosphere magnetic measurements are indicated.
description: 11 pages, 3 figures
NANOGrav results and LIGO-Virgo primordial black holes in axion-like curvaton model
Creators: name: Inomata, Keisuke
name: Kawasaki, Masahiro
name: Mukaida, Kyohei
name: Yanagida, Tsutomu T.
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2020
Subjects: black hole: primordial
perturbation: scalar
NANOGrav
curvaton
non-Gaussianity
LIGO
gravitational radiation: induced
axion
VIRGO
gravitational radiation
cosmological model
statistical analysis
gravitational radiation: background
gravitational radiation: emission

description: We discuss a possible connection between the recent NANOGrav results and the primordial black holes (PBHs) for the LIGO-Virgo events. In particular, we focus on the axion-like curvaton model, which provides a sizable amount of PBHs and GWs induced by scalar perturbations around the NANOGrav frequency range. The inevitable non-Gaussianity of this model suppresses the induced GWs associated with PBHs for the LIGO-Virgo events to be compatible with the NANOGrav results. We show that the axion-like curvaton model can account for PBHs for the LIGO-Virgo events and the NANOGrav results simultaneously.
Antidorcas marsupialis
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Antidorcas
Antidorcas marsupialis

description: Antidorcas marsupialis (Zimmermann, 1780). Geogr. Gesch. Mensch. Vierf. Thiere, 2:427. TYPE LOCALITY: South Africa, Cape of Good Hope. DISTRIBUTION: Former range included N. Namibia; S. Angola; South Africa; Botswana. COMMENT: Range now much diminished (RGVG). ISIS NUMBER: 5301419009022001001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 327, DOI: 10.5281/zenodo.7352976
Constraining Dark Energy through the Stability of Cosmic Structures
Creators: name: Pavlidou, V.
name: Tetradis, N.
name: Tomaras, T. N.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: For a general dark-energy equation of state, we estimate the maximum possible radius of massive structures that are not destabilized by the acceleration of the cosmological expansion. A comparison with known stable structures constrains the equation of state. The robustness of the constraint can be enhanced through the accumulation of additional astrophysical data and a better understanding of the dynamics of bound cosmic structures.
description: 11 pages, 1 figure
Antilocapra Ord 1818
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Bovidae
Antilocapra

description: Antilocapra Ord, 1818. J. Phys. Chim. Hist. Nat. Arts Paris, 87: 149. REVIEWED BY: J. Ramirez-Pulido (JRP). COMMENT: Included in a separate family, Antilocapridae, by Corbet and Hill, 1980:121, but see comment under Bovidae. ISIS NUMBER: 5301419008001000000.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Artiodactyla, pp. 315-343 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 327, DOI: 10.5281/zenodo.7352976
description: {"references": ["Corbet, G. B., and J. E. Hill. 1980. A world list of mammalian species. British Museum (Natural History), London, 226 pp."]}
Wash-In Leptogenesis
Creators: name: Domcke, Valerie Fiona
name: Kamada, Kohei
name: Mukaida, Kyohei
name: Schmitz, Kai
name: Yamada, Masaki
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2020
Subjects: * Automatic Keywords *
potential: chemical
equilibrium: chemical
temperature: high
temperature: low
CP: violation
leptogenesis
grand unified theory
baryogenesis
seesaw model
freeze-out
nonminimal
background
buildings
asymmetry
inflation
axion
TeV

description: We present a new leptogenesis mechanism based on the standard type-I seesaw model that successfully operates at right-handed-neutrino masses as low as a few 100 TeV. This mechanism, which we dub 'wash-in leptogenesis', does not require any CP violation in the neutrino sector and can be implemented even in the regime of strong washout. The key idea behind wash-in leptogenesis is to generalize standard freeze-out leptogenesis to a nonminimal cosmological background in which the chemical potentials of all particles not in chemical equilibrium at the temperature of leptogenesis are allowed to take arbitrary values. This sets the stage for building a plethora of new baryogenesis models where chemical potentials generated at high temperatures are reprocessed to generate a nonvanishing B-L asymmetry at low temperatures. As concrete examples, we discuss wash-in leptogenesis after axion inflation and in the context of grand unification.
Resenha - Tratato de Direito Antidiscriminatório
Creators: name: Lopes Ninomiya, Bruno
Publisher: name: figshare
Year: 2022
Subjects: subject: Law
subject: FOS: Law

description: O “Tratado de Direito Antidiscriminatório”, publicado em 2020 pela Editora Contracorrente, é o resultado de mais de vinte anos de pesquisa sobre as relações estruturais na sociedade no que tange à dois aspectos: a discriminação e a igualdade. Com exatas 783 páginas, a obra apresenta o direito antidiscriminatório desde um aspecto histórico-conceitual até na discussão aprofundada e detalhada das diferentes facetas da discriminação, que incluem, ainda, um paralelo às teorias da psicologia social.
Pulse Broadening Measurements from the Galactic Center Pulsar J1745--2900
Creators: name: Spitler, L. G.
name: Lee, K. J.
name: Eatough, R. P.
name: Kramer, M.
name: Karuppusamy, R.
name: Bassa, C. G.
name: Cognard, I.
name: Desvignes, G.
name: Lyne, A. G.
name: Stappers, B. W.
name: Bower, G. C.
name: Cordes, J. M.
name: Champion, D. J.
name: Falcke, H.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present temporal scattering measurements of single pulses and average profiles of PSR J1745--2900, a magnetar recently discovered only 3 arcsec away from Sagittarius A* (Sgr A*), from 1.2 - 18.95 GHz using the Effelsberg 100-m Radio Telescope, the Nançay Decimetric Radio Telescope, and the Jodrell Bank Lovell Telescope. Single pulse analysis shows that the integrated pulse profile above 2 GHz is dominated by pulse jitter, while below 2 GHz the pulse profile shape is dominated by scattering. The high dispersion measure and rotation measure of the magnetar suggest that it is close to Sgr A* (within ~0.1 pc). This is the first object in the GC with both pulse broadening and angular broadening measurements. We measure a pulse broadening spectral index of alpha = -3.8 +/- 0.2 and a pulse broadening time scale at 1 GHz of tau_GHz = 1.3 +/- 0.2 s, which is several orders of magnitude lower than the scattering predicted by the NE2001 model (Cordes and Lazio 2002). If this scattering timescale is representative of the GC as a whole, then previous surveys should have detected many pulsars. The lack of detections implies either our understanding of scattering in the GC is incomplete or there are fewer pulsars in the GC than previously predicted. Given that magnetars are a rare class of radio pulsar, we believe that there are many canonical and millisecond pulsars in the GC, and not surprisingly, scattering regions in the GC have complex spatial structures.
description: 6 pages, 4 figures, submitted to ApJL