bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH STRATEGI PENYEIMBANGAN ANTARA AKTIVITAS PEKERJAAN DAN KELUARGA TERHADAP KESEJAHTERAAN KELUARGA SUBJEKTIF PADA PEREMPUAN BEKERJA DI BOGOR: Analisis Structural Equation Modelling
Authors: Puspitawati Herien 
Published: March 2017

The main purpose of this research was to know the effect of working women’s strategy in balancing between work and family towards the subjective family well-being. The respondents were working women who work in full-time and had a husband and a child or children. This was a cross sectional study which was performed among 50 working women in Bogor in March 2005. Almost all respondents were experienced in working because they have been working for about 15 years. The families of all respondents were in middleupper class families. The results showed that most of respondents performed the strategy of balancing between work and family activities. The overall subjective family well-being was measured by respondents’ satisfaction towards their resources and conditions of physically, economically, socially, and psychologically. It was found that the strategic of women that tend to prioritize the family purposes had positive effect to the subjective family well-being.
TINGKAT KEPUASAN KELUARGA BERPENDAPATAN RENDAH TERHADAP SUMBERDAYA YANG DIMILIKI
Authors: Kusumo Rani Andriani Budi , Simanjuntak Megawati 
Published: March 2017

Family function as a system is very urged by what to be the aims of life and ownership of resources. Family’s aims can be reached when resources available. Satisfaction level on family’s resources ownership is influenced by family’s values. The aimed of this research were to identify the ownership of resources of low income family and to analyze the satisfaction level on resources ownership by low income family. This research was a cross sectional study in thirty poor families that lived in urban area. In low income family, resources ownership (especially physical resources) is limited. Average of income per capita per month was Rp 78.492,00. Income was used only for daily food consumption, just enough "to eat" and not considering family nutrient requirement aspects. Because of this economy limitedness, many families had childrens who dropped out school. In general, physical resources that owned by family can only fulfil half of samples’ expectation, while non physical resources factor in general can fulfil samples’ expectation. Samples’s age correlated positively with the satisfaction level, while education correlated negatively with satisfaction level. Family income not correlated with samples satisfaction level. Satisfaction was influenced by how the families managed the income to fulfill daily needs.
KUALITAS TUMBUH KEMBANG, PENGASUHAN ORANG TUA, DAN FAKTOR RISIKO KOMUNITAS PADA ANAK USIA PRASEKOLAH WILAYAH PEDESAAN DI BOGOR
Authors: Latifah Melly , Alfiasari Alfiasari , Hernawati Neti 
Published: March 2017

Every family wants to reach qualified children in conducting of child caring. Generally, this study aims to analyze: (i) quality of child development; (ii) quality of psychosocial environment of parenting practices; and (iii) quality of family life and community that identified become risk factors to child development. This article is a part of results of multiyears study that consists of data from first year study. The design of the first study is cross sectional study that involved 208 families in rural area who had preschool children. The sites of study are four villages in two sub districts (Ciawi and Ciampea) in Bogor. The sites chosen by purposive based on the ecological context. Meanwhile, the samples are chosen by random sampling the result of this study showed that in all of study sites, only 70% of the children that had high quality of developmental task. The other result showed that there were 71,6% families in Ciawi and 64,2% in Ciampea that had moderate quality of psychosocial environment of parenting practices. The level of stress and anxiety of mother gave significant negative effect to quality of parenting. There are some factors that identified will become risk factors of community to child development such as communication low level of education, low income, and low knowledge of parenting.
KUALITAS REMAJA DI KABUPATEN BANYUMAS
Authors: Suksmadi Ignatius , Sumarwan Ujang , Khomsan Ali , Hartoyo Hartoyo 
Published: March 2017

This research was aimed at analyzing indicator of early adolescent quality and factors affecting the early adolescent quality (EAQ). The study tried to create EAQ index and to analyze its effect to academic achievement. EAQ was measured by body mass index (physical dimension), intelligent quotient and emotional intelligent (nonphysical dimension). The index could show the different quality among public and private school. A crosssectional study was applied on this study. The location were purposively selected at five subdistricts, i.e., Purwokerto, Baturaden, Ajibarang, Rawalo, and Sumpiuh. Total samples of the study were 300 students of secondary school and their families. The sample were divided into public school samples (150 students) and private school samples (150 students). The study created the EAQ categorized in four category, i.e., high (7,7%), medium (71,3%), low (20,7%), and very low (0,3%). The study described that both student (public and private school) have significant differences on EAQ, academic achievement, school environment. Yet, the study found no significant differences of home environment between public and private school samples. The public school amples had the better EAQ, academic achievement, and school environment than the private school samples. The regression analysis showed that home and school environment, education investment factors affected EAQ. Academic achievement was influenced by EAQ, parent’s control on student time, school condition, student activity involvement, family monetary investment, year of schooling of mother, and student expectation.
ANALISIS TINGKAT KESEJAHTERAAN, SIKAP, PERILAKU, DAN TINGKAT KEPUASAN KELUARGA SASARAN PROGRAM KONVERSI MINYAK TANAH KE LPG DI KOTA BEKASI
Authors: Muflikhati Istiqlaliyah , Nurmayanti Novida , Alfiasari Alfiasari 
Published: March 2017

Substitution program of kerosene to LPG is one of the government programs, which is very important for energy policy in this country. The aims of this research were to analyze the socioeconomic characteristics of target family and to construct the strategies in order to increase the quality of program. The study was conducted using cross sectional design. It involved 60 families from two villages at Bekasi City as respondents. The result of the study showed that expenditure allocation for fuel in the family respondents decreased after the program. The family welfare was affected by decreasing of expenditures allocation for fuel, wives’s occupational status, wives’ educational level, and family’s attitude in this program. Meanwhile, wives’s occupational status and educational level also affected family’s attitude in the program. Moreover, family’s attitude in the program gave significant effect on the behavior of using LPG. Family’s Satisfaction level based on CSI showed that respondents were satisfied with this program.
Biossorção do corante índigo carmim por Pennisetum purpureum Schumach. 1827 (Poales: Poaceae) (Capim elefante)
Authors: Costa do Nascimento Aline Carla , Da Cruz Filho Iranildo José , Felix de Lima Valmir , Nascimento Junior Agrinaldo Jacinto do , Martins Marques Olga , Salgueiro Gondim Manuella Virginia 
Published: March 2017

As indústrias têxteis devem tratar seus efluentes antes do descarte em corpos hídricos. Esse tratamento objetiva majoritariamente a remoção de corantes, cuja interação com o meio ambiente pode causar grandes danos a natureza. A Biossorção tem se mostrado muitas vezes uma técnica econômica e eficaz na remoção de boa parte destes corantes. Deste modo propomos aplicar como biossorvente, o Pennisetum purpureum Schumach., 1827 (Poales: Poaceae) (Capim elefante), para tratar efluentes contendo o corante Índigo Carmim. Os ensaios de remoção do corante foram realizados em batelada nas seguintes condições: variando as temperaturas (30, 40, 60 e 100 ± 2 ºC); agitação constante de 150 rpm; pH 5,5; 0,5 g de biossorvente; e em diferentes concentrações de corante, de 25 a 65 mg·L-1. O mecanismo de biossorção foi bem descrito pelo modelo de Langmuir. A capacidade biossortiva máxima foi de 17,51 mg∙g-1. A investigação termodinâmica indicou que a biossorção é um processo favorável e espontâneo em temperaturas até 60 ºC, acima disso o sistema apresentou uma redução da capacidade biossortiva. Deste modo, a utilização de Pennisetum purpureum Schumach., 1827 (Poales: Poaceae) como biossorvente para a remoção do corante índigo carmim de efluentes têxteis se mostrou uma nova alternativa eficaz e econômica
Extinction in the Star Cluster SAI 113 and Galactic Structure in Carina
Authors: Carraro Giovanni , Turner David G. , Majaess Daniel J. , Baume Gustavo L. , Gamen Roberto , Lera José A. Molina 
Published: March 2017

Abstract
Photometric CCD UB VI

C
photometry obtained for 4860 stars surrounding the embedded southern cluster SAI 113 (Skiff 8) is used to examine the reddening in the field and derive the distance to the cluster and nearby van Genderen 1. Spectroscopic color excesses for bright cluster stars, photometric reddenings for A3 dwarfs, and dereddening of cluster stars imply that the reddening and extinction laws match results derived for other young clusters in Carina:

and

. SAI 113 displays features that may be linked to a history of dynamical interactions among member stars: possible circumstellar reddening and rapid rotation of late B-type members, ringlike features in star density, and a compact core, with most stars distributed randomly across the field. The group van Genderen 1 resembles a stellar asterism, with potential members distributed randomly across the field. Distances of 3.90 ± 0.19 kpc and 2.49 ± 0.09 kpc are derived for SAI 113 and van Genderen 1, respectively, with variable reddenings

ranging from 0.84 to 1.29 and 0.23 to 1.28. The SRC variables CK Car and EV Car may be outlying members of van Genderen 1, thereby of use for calibrating the period–luminosity relation for pulsating M supergiants. More importantly, the anomalous reddening and extinction evident in Carina and nearby regions of the Galactic plane in the fourth quadrant impact the mapping of spiral structure from young open clusters. The distribution of spiral arms in the fourth quadrant may be significantly different from how it is often portrayed.
Temporary Capture of Asteroids by an Eccentric Planet
Authors: Higuchi A. , Ida S. 
Published: March 2017

Abstract
We have investigated the probability of temporary capture of asteroids in eccentric orbits by a planet in a circular or eccentric orbit through analytical and numerical calculations. We found that, in the limit of the circular orbit, the capture probability is ∼0.1% of encounters to the planet’s Hill sphere, independent of planetary mass and semimajor axis. In general, temporary capture becomes more difficult as the planet’s eccentricity (

) increases. We found that the capture probability is almost independent of

until a critical value (

) that is given by ≃5 times the Hill radius scaled by the planet’s semimajor axis. For

, the probability decreases approximately in proportion to

. The current orbital eccentricity of Mars is several times larger than

. However, since the range of secular change in Martian eccentricity overlaps

, the capture of minor bodies by Mars in the past is not ruled out.
Low-frequency Carbon Radio Recombination Lines. II. The Diffuse Interstellar Medium
Authors: Salgado F. , Morabito L. K. , Oonk J. B. R. , Salas P. , Toribio M. C. , Röttgering H. J. A. , Tielens A. G. G. M. 
Published: March 2017

Abstract
In the second paper of the series, we have modeled low-frequency carbon radio recombination lines (CRRLs) from the interstellar medium. Anticipating the Low Frequency Array survey of Galactic CRRLs, we focus our study on the physical conditions of the diffuse, cold neutral medium. We have used the improved departure coefficients computed in the first paper of the series to calculate line-to-continuum ratios. The results show that the line width and integrated optical depths of CRRLs are sensitive probes of the electron density, gas temperature, and emission measure of the cloud. Furthermore, the ratio of CRRL to the [C ii] at the 158 μm line is a strong function of the temperature and density of diffuse clouds. Guided by our calculations, we analyze CRRL observations and illustrate their use with data from the literature.
Charged Particle Diffusion in Isotropic Random Magnetic Fields
Authors: Subedi P. , Sonsrettee W. , Blasi P. , Ruffolo D. , Matthaeus W. H. , Montgomery D. , Chuychai P. , Dmitruk P. , Wan M. , Parashar T. N. , Chhiber R. 
Published: March 2017

Abstract
The investigation of the diffusive transport of charged particles in a turbulent magnetic field remains a subject of considerable interest. Research has most frequently concentrated on determining the diffusion coefficient in the presence of a mean magnetic field. Here we consider the diffusion of charged particles in fully three-dimensional isotropic turbulent magnetic fields with no mean field, which may be pertinent to many astrophysical situations. We identify different ranges of particle energy depending upon the ratio of Larmor radius to the characteristic outer length scale of turbulence. Two different theoretical models are proposed to calculate the diffusion coefficient, each applicable to a distinct range of particle energies. The theoretical results are compared to those from computer simulations, showing good agreement.
Probing Large Galaxy Halos at Z ∼ 0 with Automated Lyα-absorption Matching
Authors: French David M. , Wakker Bart P. 
Published: March 2017

Abstract
We present initial results from an ongoing large-scale study of the circumgalactic medium in the nearby Universe (

10,000

), using archival Cosmic Origins Spectrograph spectra of background quasi-stellar objects. This initial sample contains 33 sightlines chosen for their proximity to large galaxies (

kpc) and high signal-to-noise ratios (S/N

10), yielding 48 Lyα absorption lines that we have paired with 33 unique galaxies, with 29 cases where multiple absorbers within a single sightline are paired with the same galaxy. We introduce a likelihood parameter to facilitate the matching of galaxies to absorption lines in a reproducible manner. We find the usual anti-correlation between Lyα equivalent width (EW) and impact parameter (ρ) when we normalize by galaxy virial radius (R
vir). Galaxies associated with a Lyα absorber are found to be more highly inclined than galaxies in the survey volume at a

confidence level (equivalent to

for a normal distribution). In contrast with suggestions in other recent papers of a correlation with azimuth angle for Mg ii absorption, we find no such correlation for Lyα.
The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group
Authors: Danieli Shany , van Dokkum Pieter , Merritt Allison , Abraham Roberto , Zhang Jielai , Karachentsev I. D. , Makarova L. N. 
Published: March 2017

Abstract
We obtained follow-up HST observations of the seven low surface brightness galaxies discovered with the Dragonfly Telephoto Array in the field of the massive spiral galaxy M101. Out of the seven galaxies, only three were resolved into stars and are potentially associated with the M101 group at D = 7 Mpc. Based on HST ACS photometry in the broad F606W and F814W filters, we use a maximum likelihood algorithm to locate the Tip of the Red Giant Branch in galaxy color–magnitude diagrams. Distances are

and

and we confirm that they are members of the M101 group. Combining the three confirmed low-luminosity satellites with previous results for brighter group members, we find the M101 galaxy group to be a sparsely populated galaxy group consisting of seven group members, down to M

V
= −9.2 mag. We compare the M101 cumulative luminosity function to that of the Milky Way and M31. We find that they are remarkably similar; in fact, the cumulative luminosity function of the M101 group gets even flatter for fainter magnitudes, and we show that the M101 group might exhibit the two known small-scale flaws in the ΛCDM model, namely “the missing satellite” problem and the “too big to fail” problem. Kinematic measurements of M101's satellite galaxies are required to determine whether the “too big to fail” problem does in fact exist in the M101 group.
Evolution of Binary Supermassive Black Holes in Rotating Nuclei
Authors: Rasskazov Alexander , Merritt David 
Published: March 2017

Abstract
The interaction of a binary supermassive black hole with stars in a galactic nucleus can result in changes to all the elements of the binary’s orbit, including the angles that define its orientation. If the nucleus is rotating, the orientation changes can be large, causing large changes in the binary’s orbital eccentricity as well. We present a general treatment of this problem based on the Fokker–Planck equation for f, defined as the probability distribution for the binary’s orbital elements. First- and second-order diffusion coefficients are derived for the orbital elements of the binary using numerical scattering experiments, and analytic approximations are presented for some of these coefficients. Solutions of the Fokker–Planck equation are then derived under various assumptions about the initial rotational state of the nucleus and the binary hardening rate. We find that the evolution of the orbital elements can become qualitatively different when we introduce nuclear rotation: (1) the orientation of the binary’s orbit evolves toward alignment with the plane of rotation of the nucleus and (2) binary orbital eccentricity decreases for aligned binaries and increases for counteraligned ones. We find that the diffusive (random-walk) component of a binary’s evolution is small in nuclei with non-negligible rotation, and we derive the time-evolution equations for the semimajor axis, eccentricity, and inclination in that approximation. The aforementioned effects could influence gravitational wave production as well as the relative orientation of host galaxies and radio jets.
&lt;i&gt;SIRT1&lt;/i&gt; gene polymorphisms associated with carcass traits in Luxi cattle
Authors: Liu Guifen , Zhao Hongbo , Tan Xiuwen , Cheng Haijian , You Wei , Wan Fachun , Liu Yifan , Song Enliang , Liu Xiaomu 
Published: March 2017

Abstract. SIRT1 is the gene that codes for Sirtuin 1, an NAD (nicotinamide adenine dinucleotide)-dependent class III histone deacetylase. This gene plays a key role in adipose tissue and muscle development in animals. Chinese Luxi cattle (n  =  169) were selected to identify SIRT1 SNPs (single nucleotide polymorphisms) and investigate the relationship of these SNPs with carcass traits. Five SNPs (g.-382G  >  A, g.-274C  >  G, g.17324T  >  C, g.17379A  >  G, and g.17491G  >  A) were identified by direct sequencing. SNPs g.-382G  >  A and g.-274C  >  G were located within the promoter region of this gene. SNP g.-382G  >  A was significantly associated with dressing percentage, meat percentage, and striploin and ribeye weights, and the g.-274C  >  G polymorphism had a strong effect on carcass, tenderloin, and high rib weights in Luxi cattle. These findings will provide possible clues for the biological roles of SIRT1 underlying beef cattle carcass traits.
Diatoms as a paleoproductivity proxy in the NW Iberian coastal upwelling system (NE Atlantic)
Authors: Zúñiga Diana , Santos Celia , Froján María , Salgueiro Emilia , Rufino Marta M. , De la Granda Francisco , Figueiras Francisco G. , Castro Carmen G. , Abrantes Fátima 
Published: March 2017

Abstract. The objective of the current work is to improve our understanding of how water column diatom's abundance and assemblage composition is seasonally transferred from the photic zone to seafloor sediments. To address this, we used a dataset derived from water column, sediment trap and surface sediment samples recovered in the NW Iberian coastal upwelling system. Diatom fluxes (2.2 (±5.6) 106 valves m−2 d−1) represented the majority of the siliceous microorganisms sinking out from the photic zone during all studied years and showed seasonal variability. Contrasting results between water column and sediment trap diatom abundances were found during downwelling periods, as shown by the unexpectedly high diatom export signals when diatom-derived primary production achieved their minimum levels. They were principally related to surface sediment remobilization and intense Minho and Douro river discharge that constitute an additional source of particulate matter to the inner continental shelf. In fact, contributions of allochthonous particles to the sinking material were confirmed by the significant increase of both benthic and freshwater diatoms in the sediment trap assemblage. In contrast, we found that most of the living diatom species blooming during highly productive upwelling periods were dissolved during sinking, and only those resistant to dissolution and the Chaetoceros and Leptocylindrus spp. resting spores were susceptible to being exported and buried. Furthermore, Chaetoceros spp. dominate during spring–early summer, when persistent northerly winds lead to the upwelling of nutrient-rich waters on the shelf, while Leptocylindrus spp. appear associated with late-summer upwelling relaxation, characterized by water column stratification and nutrient depletion. These findings evidence that the contributions of these diatom genera to the sediment's total marine diatom assemblage should allow for the reconstruction of different past upwelling regimes.
Control spectra for Quito
Authors: Aguiar Roberto , Rivas-Medina Alicia , Caiza Pablo , Quizanga Diego 
Published: March 2017

Abstract. The Metropolitan District of Quito is located on or very close to segments of reverse blind faults, Puengasí, Ilumbisí–La Bota, Carcelen–El Inca, Bellavista–Catequilla and Tangahuilla, making it one of the most seismically dangerous cities in the world. The city is divided into five areas: south, south-central, central, north-central and north. For each of the urban areas, elastic response spectra are presented in this paper, which are determined by utilizing some of the new models of the Pacific Earthquake Engineering Research Center (PEER) NGA-West2 program. These spectra are calculated considering the maximum magnitude that could be generated by the rupture of each fault segment, and taking into account the soil type that exists at different points of the city according to the Norma Ecuatoriana de la Construcción (2015). Subsequently, the recurrence period of earthquakes of high magnitude in each fault segment is determined from the physical parameters of the fault segments (size of the fault plane and slip rate) and the pattern of recurrence of type Gutenberg–Richter earthquakes with double truncation magnitude (Mmin and Mmax) is used.