bluuebunny/crossref_metadata_2025_split huggingface dataset:
Advanced Modeling of Interwell Fracturing Interference: An Eagle Ford Shale Oil Study - Refracturing
Authors: Morales Adrian , Zhang Ke , Gakhar Kush , Marongiu Porcu Matteo , Lee Don , Shan Dan , Malpani Raj , Pope Tim , Sobernheim David , Acock Andrew 
Published: January 2016

Abstract
This paper continues the investigation of interwell fracturing interference for an infill drilling scenario synthetic case based on Eagle Ford available public data and explores pressure and stress-sink mitigation strategies applied to the simulation cases developed in the previous publication (SPE 174902). Emphasis is given to refracturing scenarios, given the intrinsic restimulation value for depleted parent wells and the strategic importance due to the current low oil prices.
The stress and pressure depletion methodology is expanded in this paper, adding a refracturing scenario before the infill child well is stimulated. Changes in stress magnitudes and azimuths caused by new and reactivated fractures are calculated using a finite element model (FEM). After refracturing the parent well, modeling shows that stress deflection and repressurization of the originally depleted production zone will reduce subsequent fracture hits from infill wells.
The first mechanism to reduce fracture hits is the stress realignment, which promotes transverse fracture propagation from the infill well away from the parent well. The second fracture-hit-reduction mechanism is repressurization of depleted zones to hinder fracture propagation in lower-pressure zones. Prevention of fracture hits by active deflection results in an increased stimulated reservoir volume (SRV) for both the parent and child wells. Overall pad level and individual wellbore cumulative production experience a significant increase due to increased SRV. With proper reservoir and geomechanical data, this approach can be applied in a predictive manner to decrease fracture-hit risk and improve overall recovery.
This workflow represents the first comprehensive multidisciplinary approach to coupling geomechanical, complex hydraulic fracture models, and multiwell production simulation models aimed towards understanding fracture-hit reduction using refracturing. The workflow presented can be applied to study and design an optimum refracturing job to prevent potentially catastrophic fracture hits during refracturing operations.
THE PHASE SPACE OF
SpARCS CLUSTERS: USING HERSCHEL TO PROBE DUST TEMPERATURE AS A FUNCTION OF ENVIRONMENT AND ACCRETION HISTORY*
Authors: Noble A. G. , Webb T. M. A. , Yee H. K. C. , Muzzin A. , Wilson G. , Burg R. F. J. van der , Balogh M. L. , Shupe D. L. 
Published: January 2016

ABSTRACT
We present a five-band Herschel study (100–500 μm) of three galaxy clusters at

from the Spitzer Adaptation of the Red-Sequence Cluster Survey. With a sample of 120 spectroscopically confirmed cluster members, we investigate the role of environment on galaxy properties utilizing the projected cluster phase space (line-of-sight velocity versus clustercentric radius), which probes the time-averaged galaxy density to which a galaxy has been exposed. We divide cluster galaxies into phase-space bins of

, tracing a sequence of accretion histories in phase space. Stacking optically star-forming cluster members on the Herschel maps, we measure average infrared star formation rates, and, for the first time in high-redshift galaxy clusters, dust temperatures for dynamically distinct galaxy populations—namely, recent infalls and those that were accreted onto the cluster at an earlier epoch. Proceeding from the infalling to virialized (central) regions of phase space, we find a steady decrease in the specific star formation rate and increase in the stellar age of star-forming cluster galaxies. We perform a probability analysis to investigate all acceptable infrared spectral energy distributions within the full parameter space and measure a

drop in the average dust temperature of cluster galaxies in an intermediate phase-space bin, compared to an otherwise flat trend with phase space. We suggest one plausible quenching mechanism which may be consistent with these trends, invoking ram-pressure stripping of the warmer dust for galaxies within this intermediate accretion phase.
THE CARNEGIE HUBBLE PROGRAM: THE DISTANCE AND STRUCTURE OF THE SMC AS REVEALED BY MID-INFRARED OBSERVATIONS OF CEPHEIDS
Authors: Scowcroft Victoria , Freedman Wendy L. , Madore Barry F. , Monson Andy , Persson S. E. , Rich Jeff , Seibert Mark , Rigby Jane R. 
Published: January 2016

ABSTRACT
Using Spitzer observations of classical Cepheids we have measured the true average distance modulus of the Small Magellanic Cloud (SMC) to be

mag (corresponding to

kpc), which is 0.48 ± 0.01 mag more distant than the LMC. This is in agreement with previous results from Cepheid observations, as well as with measurements from other indicators such as RR Lyrae stars and the tip of the red giant branch. Utilizing the properties of the mid-infrared Leavitt Law we measured precise distances to individual Cepheids in the SMC, and have confirmed that the galaxy is tilted and elongated such that its eastern side is up to 20 kpc closer than its western side. This is in agreement with the results from red clump stars and dynamical simulations of the Magellanic Clouds and Stream.
MAGNETIC GRAIN TRAPPING AND THE HOT EXCESSES AROUND EARLY-TYPE STARS
Authors: Rieke G. H. , Gáspár András , Ballering N. P. 
Published: January 2016

ABSTRACT
A significant fraction of main sequence stars observed interferometrically in the near-infrared have slightly extended components that have been attributed to very hot dust. To match the spectrum appears to require the presence of large numbers of very small (<200 nm in radius) dust grains. However, particularly for the hotter stars, it has been unclear how such grains can be retained close to the star against radiation pressure force. We find that the expected weak stellar magnetic fields are sufficient to trap nm-sized dust grains in epicyclic orbits for a few weeks or longer, sufficient to account for the hot excess emission. Our models provide a natural explanation for the requirement that the hot excess dust grains be smaller than 200 nm. They also suggest that magnetic trapping is more effective for rapidly rotating stars, consistent with the average vsini measurements of stars with hot excesses being larger (at ∼2σ) than those for stars without such excesses.
MULTI-WAVELENGTH STUDY OF HESS J1741–302
Authors: Hare Jeremy , Rangelov Blagoy , Sonbas Eda , Kargaltsev Oleg , Volkov Igor 
Published: January 2016

ABSTRACT
We present the results of two Chandra X-ray Observatory (CXO) observations of TeV γ-ray source HESS J1741–302. We investigate whether there is any connection between HESS J1741−302 and the sources seen at lower energies. One of the brightest X-ray sources in the HESS J1741–302 field, CXOU J174112.1−302908, appears to be associated with a low-mass star (possibly representing a quiescent low-mass X-ray binary or cataclysmic variable (CV)), hence, it is unlikely to be a source of TeV γ-rays. In the same field we have potentially detected X-rays from WR 98a, which is likely to be a colliding wind binary with massive stars. No TeV emission has been reported so far from such systems although predictions have been made. Finally, we found that the previously reported Suzaku source, Suzaku J1740.5–3014 (which is not covered by the CXO observations), appears to be a hard X-ray source detected by INTERGAL ISGRI, which supports the magnetized CV classification but makes its association with the TeV emission unlikely. The young pulsar PSR B1737–30, so far undetected in X-rays and projected on the sky near the CV, may be the contributor of relativistic particles responsible for the TeV emission.
THE HYDROXYL–WATER MEGAMASER CONNECTION. I. WATER EMISSION TOWARD OH MEGAMASER HOSTS
Authors: Wiggins Brandon K. , Migenes Victor , Smidt Joseph M. 
Published: January 2016

ABSTRACT
Questions surround the connection of luminous extragalactic masers to galactic processes. The observation that water and hydroxyl megamasers rarely coexist in the same galaxy has given rise to a hypothesis that the two species appear in different phases of nuclear activity. The detection of simultaneous hydroxyl and water megamaser emission toward IC694 has called this hypothesis into question, but, because many megamasers have not been surveyed for emission in the other molecule, it remains unclear whether IC694 occupies a narrow phase of galaxy evolution or whether the relationship between megamaser species and galactic processes is more complicated than previously believed. In this paper, we present results of a systematic search for 22 GHz water maser emission among OH megamaser hosts to identify additional objects hosting both megamasers. Our work roughly doubles the number of galaxies searched for emission in both molecules, which host at least one confirmed maser. We confirm with a high degree of confidence (

) the detection of water emission toward IIZw96, firmly establishing it as the second object to cohost both water and hydroxyl megamasers after IC694. We find high luminosity, narrow features in the water feature in IIZw96. All dual megamaser candidates appear in merging galaxy systems suggestive that megamasers that coexistance may signal a brief phase along the merger sequence. A statistical analysis of the results of our observations provide possible evidence for an exclusion of H2O kilomasers among OH megamaser hosts.
SODIUM ABSORPTION SYSTEMS TOWARD SN Ia 2014J ORIGINATE ON INTERSTELLAR SCALES*
Authors: Maeda K. , Tajitsu A. , Kawabata K. S. , Foley R. J. , Honda S. , Moritani Y. , Tanaka M. , Hashimoto O. , Ishigaki M. , Simon J. D. , Phillips M. M. , Yamanaka M. , Nogami D. , Arai A. , Aoki W. , Nomoto K. , Milisavljevic D. , Mazzali P. A. , Soderberg A. M. , Schramm M. , Sato B. , Harakawa H. , Morrell N. , Arimoto N. 
Published: January 2016

ABSTRACT
Na i D absorbing systems toward Type Ia supernovae (SNe Ia) have been intensively studied over the last decade with the aim of finding circumstellar material (CSM), which is an indirect probe of the progenitor system. However, it is difficult to deconvolve CSM components from non-variable, and often dominant, components created by interstellar material (ISM). We present a series of high-resolution spectra of SN Ia 2014J from before maximum brightness to ≳250 days after maximum brightness. The late-time spectrum provides unique information for determining the origin of the Na i D absorption systems. The deep late-time observation allows us to probe the environment around the SN at a large scale, extending to ≳40 pc. We find that a spectrum of diffuse light in the vicinity, but not directly in the line of sight, of the SN has absorbing systems nearly identical to those obtained for the “pure” SN line of sight. Therefore, basically all Na i D systems seen toward SN 2014J must originate from foreground material that extends to at least ∼40 pc in projection and none at the CSM scale. A fluctuation in the column densities at a scale of ∼20 pc is also identified. After subtracting the diffuse, “background” spectrum, the late-time Na i D profile along the SN line of sight is consistent with profiles near maximum brightness. The lack of variability on a ∼1 year timescale is consistent with the ISM interpretation for the gas.
ABSORPTION OSCILLATOR STRENGTHS FOR THE
(3, 4, 6)–
(10, 13, 20)–
AND
(1)–
PROGRESSIONS IN N2
Authors: Lavín C. , Velasco A. M. 
Published: January 2016

ABSTRACT
Absorption oscillator strengths, calculated with the molecular quantum defect orbital method, for the

(3)–

= 0–12),

(4)–

= 0–12),

(6)–

= 0–12),

(10)–

= 0–12),

(13)–

= 0–12),

(20)–

= 0–12), and

(1)–

= 0–12) bands of molecular nitrogen are reported. The Rydberg–valence interaction between states of

symmetry has been treated through an interaction matrix that includes vibrational coupling. Due to the homogeneous interaction, the intensity distribution of the bands within each progression deviates from the Franck–Condon predictions. The present results for vibronic transitions from the

ground state agree rather well with reported high-resolution measurements. As far as we know, f-values for bands originating from v″ > 0 vibrational levels of the electronic ground state are reported here for the first time. These data may be useful in the interpretation of the extreme ultraviolet spectra from Earth’s and Titan’s atmospheres, in which several bands of the

and

progressions have been identified.
FERMI-LAT OBSERVATIONS OF SUPERNOVA REMNANT G5.7–0.1, BELIEVED TO BE INTERACTING WITH MOLECULAR CLOUDS
Authors: Joubert Timothy , Castro Daniel , Slane Patrick , Gelfand Joseph 
Published: January 2016

ABSTRACT
This work reports on the detection of γ-ray emission coincident with the supernova remnant (SNR) G5.7–0.1 using data collected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope. The SNR is believed to be interacting with molecular clouds, based on 1720 MHz hydroxyl (OH) maser emission observations in its direction. This interaction is expected to provide targets for the production of γ-ray emission from π
0-decay. A γ-ray source was observed in the direction of SNR G5.7–0.1, positioned near the bright γ-ray source SNR W28. We model the emission from radio to γ-ray energies using a one-zone model. Following consideration of both π
0-decay and leptonically dominated emission scenarios for the MeV–TeV source, we conclude that a considerable component of the γ-ray emission must originate from the π
0-decay channel. Finally, constraints were placed on the reported ambiguity of the SNR distance through X-ray column density measurements made using XMM-Newton observations. We conclude G5.7–0.1 is a significant γ-ray source positioned at a distance of ∼3 kpc with luminosity in the 0.1–100 GeV range of L

γ
≈ 7.4 × 1034 erg s−1.
A Common Genetic Variant in TLR1 Enhances Human Neutrophil Priming and Impacts Length of Intensive Care Stay in Pediatric Sepsis
Authors: Whitmore Laura C. , Hook Jessica S. , Philiph Amanda R. , Hilkin Brieanna M. , Bing Xinyu , Ahn Chul , Wong Hector R. , Ferguson Polly J. , Moreland Jessica G. 
Published: January 2016

Abstract
Polymorphonuclear leukocytes (PMN) achieve an intermediate or primed state of activation following stimulation with certain agonists. Primed PMN have enhanced responsiveness to subsequent stimuli, which can be beneficial in eliminating microbes but may cause host tissue damage in certain disease contexts, including sepsis. As PMN priming by TLR4 agonists is well described, we hypothesized that ligation of TLR2/1 or TLR2/6 would prime PMN. Surprisingly, PMN from only a subset of donors were primed in response to the TLR2/1 agonist, Pam3CSK4, although PMN from all donors were primed by the TLR2/6 agonist, FSL-1. Priming responses included generation of intracellular and extracellular reactive oxygen species, MAPK phosphorylation, integrin activation, secondary granule exocytosis, and cytokine secretion. Genotyping studies revealed that PMN responsiveness to Pam3CSK4 was enhanced by a common single-nucleotide polymorphism (SNP) in TLR1 (rs5743618). Notably, PMN from donors with the SNP had higher surface levels of TLR1 and were demonstrated to have enhanced association of TLR1 with the endoplasmic reticulum chaperone gp96. We analyzed TLR1 genotypes in a pediatric sepsis database and found that patients with sepsis or septic shock who had a positive blood culture and were homozygous for the SNP associated with neutrophil priming had prolonged pediatric intensive care unit length of stay. We conclude that this TLR1 SNP leads to excessive PMN priming in response to cell stimulation. Based on our finding that septic children with this SNP had longer pediatric intensive care unit stays, we speculate that this SNP results in hyperinflammation in diseases such as sepsis.
Molecular Mechanisms of Airway Hyperresponsiveness in a Murine Model of Steroid-Resistant Airway Inflammation
Authors: Manni Michelle L. , Mandalapu Sivanarayana , McHugh Kevin J. , Elloso M. Merle , Dudas Paul L. , Alcorn John F. 
Published: January 2016

AbstractIL-13 and IL-17A, produced mainly by Th2 and Th17 cells, respectively, have an influential role in asthma pathogenesis. We examined the role of IL-13 and IL-17A in mediating airway hyperresponsiveness (AHR), lung inflammation, and mucus metaplasia in a dual Th2/Th17 model of asthma. IL-13 and/or IL-17A were neutralized using mAbs. Th2/Th17 adoptive transfer induced a mixed asthma phenotype characterized by elevated eosinophilia and neutrophilia, tissue inflammation, mucus metaplasia, and AHR that were partially reversible with steroid treatment. Pulmonary inflammation and quasi-static lung compliance were largely unaffected by neutralization of IL-13 and/or IL-17A. However, neutralization of IL-13 alone or in combination with IL-17A significantly attenuated AHR and mucus metaplasia. Further, STAT6 activation was attenuated following IL-13 and IL-13/IL-17A Ab treatment. We next assessed the role of STAT6 in Th2/Th17-mediated allergic airway disease using STAT6−/− mice. STAT6−/− mice adoptively transferred with Th2/Th17 cells had decreased AHR compared with controls. These data suggest that IL-13 drives AHR and mucus metaplasia in a STAT6-dependent manner, without directly contributing to airway or tissue inflammation. IL-17A independently contributes to AHR, but it only partially mediates inflammation and mucus metaplasia in a mixed Th2/Th17 model of steroid-resistant asthma.
Analysis of sparse data in logistic regression in medical research
Authors: Devika S , Jeyaseelan L , Sebastian G 
Published: January 2016

Background and Objective:
In the analysis of dichotomous type response variable, logistic regression is usually used. However, the performance of logistic regression in the presence of sparse data is questionable. In such a situation, a common problem is the presence of high odds ratios (ORs) with very wide 95% confidence interval (CI) (OR: >999.999, 95% CI: <0.001, >999.999). In this paper, we addressed this issue by using penalized logistic regression (PLR) method.

Materials and Methods:
Data from case-control study on hyponatremia and hiccups conducted in Christian Medical College, Vellore, Tamil Nadu, India was used. The outcome variable was the presence/absence of hiccups and the main exposure variable was the status of hyponatremia. Simulation dataset was created with different sample sizes and with a different number of covariates.

Results:
A total of 23 cases and 50 controls were used for the analysis of ordinary and PLR methods. The main exposure variable hyponatremia was present in nine (39.13%) of the cases and in four (8.0%) of the controls. Of the 23 hiccup cases, all were males and among the controls, 46 (92.0%) were males. Thus, the complete separation between gender and the disease group led into an infinite OR with 95% CI (OR: >999.999, 95% CI: <0.001, >999.999) whereas there was a finite and consistent regression coefficient for gender (OR: 5.35; 95% CI: 0.42, 816.48) using PLR. After adjusting for all the confounding variables, hyponatremia entailed 7.9 (95% CI: 2.06, 38.86) times higher risk for the development of hiccups as was found using PLR whereas there was an overestimation of risk OR: 10.76 (95% CI: 2.17, 53.41) using the conventional method. Simulation experiment shows that the estimated coverage probability of this method is near the nominal level of 95% even for small sample sizes and for a large number of covariates.

Conclusions:
PLR is almost equal to the ordinary logistic regression when the sample size is large and is superior in small cell values.
Complications of chemoport in children with cancer: Experience of 54,100 catheter days from a tertiary cancer center of Southern India
Authors: Aparna S. , Ramesh S. , Appaji L. , Srivatsa Kavitha , Shankar Gowri , Jadhav Vinay , Babu Narendra 
Published: January 2016

Abstract
Background: Chemoport is an essential part of the management of children with cancer and provides long-term venous access. There are few studies from resource poor countries reporting complications of chemoport. Aims: This study was aimed at describing the complications of chemoport in patients with cancer. Materials and Methods: This retrospective observational study analyzed 200 patients <15 years of age who underwent chemoport insertion. The medical records of these patients were reviewed for the patient characteristics, diagnosis, nature of port use, port-related complications and their management. Results: A total of 209 ports were implanted in 200 patients and 24 ports were removed due to port-related complications. There were 122 boys and 78 girls whose ages ranged from 4 months to 13 years (median age 2.5 years). About72% of patients were <2 years old. The cumulative duration of catheterization was 54,100 days. Of 209 ports, there were 36 complications that led to the removal of 21 ports. Port-related infection was the most common infection observed in our study (0.66/1000 catheter days and 11.9%). Mechanical complications were seen in 9 patients. Venous thrombosis and skin necrosis occurred in one patient each. Conclusions: Use of chemoport is safe and is a boon for children with cancer in developing countries with incidence of complications similar to Western countries. Although use of chemoport is associated with complications, they are easily managed. With stringent catheter care by trained personnel, some complications can be prevented.
Transitions Into and Out of Census Disability
Authors: Krueger Kurt V. , Skoog Gary R. 
Published: January 2016

Abstract
This paper examines disability as measured and reported in three Census surveys: the American Community Survey (ACS), the Current Population Survey (CPS), and the Survey on Income Program Participation (SIPP). We focus on whether person-specific disability, as measured by the Census, is a permanent or a transitory condition. Survey data results regarding the incidence of Census-measured disability are shown both cross-sectionally and longitudinally. It is found from longitudinal CPS and SIPP responses that Census-measured disability is largely transitory. That finding empirically confirms the longstanding theoretical objections to the use of Census cross-section disability data along with a permanent disability assumption in worklife expectancy models; hence, any worklife expectancy model which assumes that Census disability measures are permanent conditions is misspecified and empirically invalid. Instead of using the permanent disability assumption, we use actual longitudinal disability transition probabilities and life table analysis to quantify the lifetime duration of disability as measured by the Census in total life years and working life years. We show that the realistic feature of disability transition dramatically lowers the effect of disability on worklife expectancy.