bluuebunny/crossref_metadata_2025_split huggingface dataset:
EFISIENSI PEMILIHAN ALTERNATIF PENYELESAIAN SENGKETA DALAM PENYELESAIAN SENGKETA WARALABA
Authors: Yuniarti Rahmi 
Published: May 2017

AbstractFranchise as a business contract between franchisor and frachisee which in the practice sometimes leads to a dispute. A dispute happens because their rights and obligations are not met. Dispute settlement businesses can choose a judiciary or non-judiciary institution. However, considering of the business continuity, the dispute must be resolved so each side can fulfill their needs to solve the dispute. The problems in this study are the factors that can arise disputes franchise and the efficiency of selecting alternatives of dispute resolution to resolve the dispute franchise. This type of the research used by the researcher is a normative legal research. This type of research is a descriptive research. The conclusions of this study are the factors that cause disputes franchise is the existence of rights and obligations are not met and fulfilled, and it happens mostly because the oversight and discontinuance of the franchise that are assumed not giving advantages or inflicting one of the parties. Moreover, there are possibilities of not keeping promises which have been decided before. Keywords: Alternative Dispute Resolution, Franchise Dispute AbstrakWaralaba sebagai suatu kontrak bisnis antara franchisor dan frachisee dalam pelaksanaannya tidak sedikit yang menimbulkan suatu sengketa. Suatu sengketa muncul dikarenakan adanya hak dan kewajiban yang tidak terpenuhi. Penyelesaian sengketa bisnis dapat memilih lembaga pengadilan atau lemabaga non-peradilan. Namun, dengan pertimbangan akan kelanjutan bisnis yang dijalani alternatif penyelesaian sengketa dianggap lebih dapat menyalurkan keinginan para pihak untuk menyelesaiakan sengketa bisnis. Permasalahan pada penelitian ini adalah faktor-faktor yang dapat menimbulkan sengketa waralaba dan efisiensi pemilihan alternatif penyelesaian sengketa untuk menyelesaikan sengketa waralaba. Jenis penelitian yang digunakan penulis dalam penelitian ini adalah bersifat penelitian hukum normatif. Tipe penelitian ini adalah penelitian deskriptif. Simpulan dari penelitian ini, faktor-faktor yang menyebabkan timbulnya sengketa waralaba adalah adanya suatu hak dan kewajiban yang tidak terpenuhi dan paling banyak terjadi dikarenakan pengawasan dan pemutusan hubungan waralaba yang dianggap merugikan salah satu pihak. Selain itu, ketidakpastian karena ada kemungkinan tidak ditepatinya janji serta risiko permintaan yang tidak sesuai dengan yang direncanakan. Kata Kunci: Penyelesaian Sengketa, Sengketa Waralaba
UPAYA PUSAT PELAPORAN DAN ANALISIS TRANSAKSI KEUANGAN DALAM PENANGGULANGAN TINDAK PIDANA PENCUCIAN UANG
Authors: Raharjo Eko 
Published: May 2017

The issue of crime not only from the public spotlight in the local and national level, but also a serious concern of the international community. One crime that is now often used as a discussion by scholars of law, economics and banking apparatus of government and law enforcement are on the money laundering crime (money laundering), especially with the notion that the Republic of Indonesia is "heaven" for these practices criminal offenses or the crime of money laundering. The legal issues increasingly into the spotlight with the inclusion of the Republic of Indonesia in the black list or black list. Keywords: Center for Financial Transaction Reporting and Analysis, Money Laundering
KEKUATAN HUKUM GROSSE AKTA NOTARIS SEBAGAI BENTUK SURAT AUTENTIK
Authors: Oktaviana Selvia 
Published: May 2017

Grosse certificates as a form letter is authentic deed that has a distinctive shape. The parties made an agreement in the form of grosse deed will be protected by law, because basically the purpose or rationale for creating grosse deed is to protect the lender in case of default and because of the executorial title. Keywords: Grosse of Deed, Letter Authentic, Notary
PELAKSANAAN SISTEM PEMERINTAHAN DESA BERDASARKAN UNDANG-UNDANG NOMOR 32 TAHUN 2004 DIDESA KALICINTA KECAMATAN KOTABUMI KABUPATEN LAMPUNG UTARA
Authors: Sari Erna , Neta Yulia 
Published: May 2017

Village Administration System implementation as stipulated in the Act Law Number 32 Year 2004 on Regional Government to give freedom to the village to have a genuine authority in managing the household itself. The village also has a delegated power as deconcentration of the government on it. As the embodiment of democracy, the rule penyelenggarakan village consultative body established villages or other designations in accordance with the culture that flourished in their local village, which serves as the regulatory agencies in the governance of the village. Keywords: Village, Village Governance System Implementation
PENGECUALIAN PERJANJIAN HAK KEKAYAAN INTELEKTUAL DALAM HUKUM PERSAINGAN USAHA
Authors: Hakim Dani Amran 
Published: May 2017

Law business competition in the country Indonesia know the exceptions to assert that a the rule of law expressed does not apply for those kind certain agents or behavior particular activity. Law competition business environment in general grant an exemption on the basis of agreement , for example agreement intellectual property rights (IPR). IPR is incentives and reason was given the right monopolizes and protection because IPR need resources and time in an effort to get it, based on article 50 alphabet b Law on Business Competition. An exemption based on article 50 alphabet b Law on Business Competition the elaborated competition supervisory commission by issuing commission rules business competition supervisory Law Number 2 of 2009 on Exceptions The Application of the Law Number 5 of 1999 on Prohibition of Monopoly and Unfair Business Competition of a Pertaining to Intellectual Property Rights Scope arrangement based on Commission Rules Business Competition Supervisory Number 2 of 2009 is: (1) the license agreement that is in scope patent, the right brand, copyright, the right industrial design, the right design the layout integrated circuit and the right trade. (2) Trademark and brand services. (3) the design layout integrated circuit. Keywords: Exeptions, Intellectal Property Rights, Business Competition Law
Application of a simplified method of chloroplast enrichment to small amounts of tissue for chloroplast genome sequencing
Authors: Sakaguchi Shota , Ueno Saneyoshi , Tsumura Yoshihiko , Setoguchi Hiroaki , Ito Motomi , Hattori Chie , Nozoe Shogo , Takahashi Daiki , Nakamasu Riku , Sakagami Taishi , Lannuzel Guillaume , Fogliani Bruno , Wulff Adrien S. , L'Huillier Laurent , Isagi Yuji 
Published: May 2017

Premise of the study:High‐throughput sequencing of genomic DNA can recover complete chloroplast genome sequences, but the sequence data are usually dominated by sequences from nuclear/mitochondrial genomes. To overcome this deficiency, a simple enrichment method for chloroplast DNA from small amounts of plant tissue was tested for eight plant species including a gymnosperm and various angiosperms.Methods:Chloroplasts were enriched using a high‐salt isolation buffer without any step gradient procedures, and enriched chloroplast DNA was sequenced by multiplexed high‐throughput sequencing.Results:Using this simple method, significant enrichment of chloroplast DNA‐derived reads was attained, allowing deep sequencing of chloroplast genomes. As an example, the chloroplast genome of the conifer Callitris sulcata was assembled, from which polymorphic microsatellite loci were isolated successfully.Discussion:This chloroplast enrichment method from small amounts of plant tissue will be particularly useful for studies that use sequencers with relatively small throughput and that cannot use large amounts of tissue (e.g., for endangered species).
The Dynamical History of Chariklo and Its Rings
Authors: Wood Jeremy , Horner Jonti , Hinse Tobias C. , Marsden Stephen C. 
Published: May 2017

Abstract
Chariklo is the only small solar system body confirmed to have rings. Given the instability of its orbit, the presence of rings is surprising, and their origin remains poorly understood. In this work, we study the dynamical history of the Chariklo system by integrating almost 36,000 Chariklo clones backward in time for 1 Gyr under the influence of the Sun and the four giant planets. By recording all close encounters between the clones and planets, we investigate the likelihood that Chariklo’s rings could have survived since its capture to the Centaur population. Our results reveal that Chariklo’s orbit occupies a region of stable chaos, resulting in its orbit being marginally more stable than those of the other Centaurs. Despite this, we find that it was most likely captured to the Centaur population within the last 20 Myr, and that its orbital evolution has been continually punctuated by regular close encounters with the giant planets. The great majority (>99%) of those encounters within 1 Hill radius of the planet have only a small effect on the rings. We conclude that close encounters with giant planets have not had a significant effect on the ring structure. Encounters within the Roche limit of the giant planets are rare, making ring creation through tidal disruption unlikely.
A Potential Recoiling Supermassive Black Hole, CXO J101527.2+625911
Authors: Kim D.-C. , Yoon Ilsang , Privon G. C. , Evans A. S. , Harvey D. , Stierwalt S. , Kim Ji Hoon 
Published: May 2017

Abstract
We have carried out a systematic search for recoiling supermassive black holes (rSMBH) using the Chandra Source and SDSS Cross-Match Catalog. From the survey, we have detected a potential rSMBH, CXO J101527.2+625911, at z = 0.3504. The source CXO J101527.2+625911 has a spatially offset (1.26 ± 0.05 kpc) active SMBH and kinematically offset broad emission lines (175 ± 25 km s−1 relative to the systemic velocity). The observed spatial and velocity offsets suggest that this galaxy could be an rSMBH, but we have also considered the possibility of a dual SMBH scenario. The column density toward the galaxy center was found to be Compton thin, but no X-ray source was detected. The non-detection of the X-ray source in the nucleus suggests that either there is no obscured actively accreting SMBH or that there exists an SMBH, but it has a low accretion rate (i.e., a low-luminosity AGN (LLAGN)). The possibility of the LLAGN was investigated and found to be unlikely based on the Hα luminosity, radio power, and kinematic arguments. This, along with the null detection of an X-ray source in the nucleus, supports our hypothesis that CXO J101527.2+625911 is an rSMBH. Our GALFIT analysis shows the host galaxy to be a bulge-dominated elliptical. The weak morphological disturbance and small spatial and velocity offsets suggest that CXO J101527.2+625911 could be in the final stage of a merging process and about to turn into a normal elliptical galaxy.
On the Origin of Sub-subgiant Stars. I. Demographics
Authors: Geller Aaron M. , Leiner Emily M. , Bellini Andrea , Gleisinger Robert , Haggard Daryl , Kamann Sebastian , Leigh Nathan W. C. , Mathieu Robert D. , Sills Alison , Watkins Laura L. , Zurek David 
Published: May 2017

Abstract
Sub-subgiants are stars that are observed to be redder than normal main-sequence stars and fainter than normal subgiant (and giant) stars in an optical color–magnitude diagram (CMD). The red straggler stars, which lie redward of the red giant branch, may be related and are often grouped together with the sub-subgiants in the literature. These stars defy our standard theory of single-star evolution and are important tests for binary evolution and stellar collision models. In total, we identify 65 sub-subgiants (SSG) and red stragglers (RS) in 16 open and globular star clusters from the literature; 50 of these, including 43 sub-subgiants, pass our strict membership selection criteria (though the remaining sources may also be cluster members). In addition to their unique location on the CMD, we find that at least 58% (25/43) of sub-subgiants in this sample are X-ray sources with typical 0.5–2.5 keV luminosities of order 1030–1031 erg s−1. Their X-ray luminosities and optical–to–X-ray flux ratios are similar to those of RS CVn active binaries. At least 65% (28/43) of the sub-subgiants in our sample are variables, 21 of which are known to be radial-velocity binaries. Typical variability periods are ≲15 days. At least 33% (14/43) of the sub-subgiants are Hα emitters. These observational demographics provide strong evidence that binarity is important for sub-subgiant formation. Finally, we find that the number of sub-subgiants per unit mass increases toward lower-mass clusters, such that the open clusters in our sample have the highest specific frequencies of sub-subgiants.
Descattering of Giant Pulses in PSR B1957+20
Authors: Main Robert , Kerkwijk Marten van , Pen Ue-Li , Mahajan Nikhil , Vanderlinde Keith 
Published: May 2017

Abstract
The interstellar medium scatters radio waves, which causes pulsars to scintillate. For intrinsically short bursts of emission, the observed signal should be a direct measurement of the impulse response function. We show that this is indeed the case for giant pulses from PSR B1957+20: from baseband observations at 327 MHz, we demonstrate that the observed voltages of a bright pulse allow one to coherently descatter nearby pulses. We find that while the scattering timescale is

, the power in the descattered pulses is concentrated within a span almost two orders of magnitude shorter, of

. This sets an upper limit to the intrinsic duration of the giant pulses. We verify that the response inferred from the giant pulses is consistent with the scintillation pattern obtained by folding the regular pulsed emission, and that it decorrelates on the same timescale, of

. In principle, with large sets of giant pulses, it should be possible to constrain the structure of the scattering screen much more directly than with other current techniques, such as holography on the dynamic spectrum and cyclic spectroscopy.
On the Assembly Rate of Highly Eccentric Binary Black Hole Mergers
Authors: Samsing Johan , Ramirez-Ruiz Enrico 
Published: May 2017

Abstract
In this Letter we calculate the fraction of highly eccentric binary black hole (BBH) mergers resulting from binary-single interactions. Using an N-body code that includes post-Newtonian correction terms, we show that

of all BBH mergers resulting from this channel will have an eccentricity

when coming into the LIGO frequency band. As the majority of BBH mergers forming in globular clusters are assembled through three-body encounters, we suggest that such interactions are likely to dominate the population of high-eccentricity BBH mergers detectable by LIGO. The relative frequency of highly eccentric events could eventually help to constrain the astrophysical origin of BBH mergers.
Magnetic Nulls and Super-radial Expansion in the Solar Corona
Authors: Gibson Sarah E. , Dalmasse Kevin , Rachmeler Laurel A. , Rosa Marc L. De , Tomczyk Steven , Toma Giuliana de , Burkepile Joan , Galloy Michael 
Published: May 2017

Abstract
Magnetic fields in the Sun’s outer atmosphere—the corona—control both solar-wind acceleration and the dynamics of solar eruptions. We present the first clear observational evidence of coronal magnetic nulls in off-limb linearly polarized observations of pseudostreamers, taken by the Coronal Multichannel Polarimeter (CoMP) telescope. These nulls represent regions where magnetic reconnection is likely to act as a catalyst for solar activity. CoMP linear-polarization observations also provide an independent, coronal proxy for magnetic expansion into the solar wind, a quantity often used to parameterize and predict the solar wind speed at Earth. We introduce a new method for explicitly calculating expansion factors from CoMP coronal linear-polarization observations, which does not require photospheric extrapolations. We conclude that linearly polarized light is a powerful new diagnostic of critical coronal magnetic topologies and the expanding magnetic flux tubes that channel the solar wind.