bluuebunny/crossref_metadata_2025_split huggingface dataset:
Postpartum meloxicam administration to sows but not split-suckling increases piglet growth and reduces clinical incidence of disease in suckling piglets
Authors: Arnaud Elisa A , Gardiner Gillian E , Halpin Keely M , Ribas Clément , O’ Doherty John V , Sweeney Torres , Lawlor Peadar G 
Published: August 2023

AbstractEach suckling pig should receive ≥200 g of colostrum within the first 24 h of life, but with increased litter size this is now difficult to achieve. The aim of this study was to assess the effect of split-suckling and postpartum meloxicam provision to sows as a means of ensuring adequate colostrum intake, on growth and health in pigs pre- and postweaning. One hundred and four sows (Large White × Landrace) and their litters, averaging 16.3 piglets born alive, were assigned to one of four treatments in a two-by-two factorial arrangement. Factors were provision of meloxicam (yes/no; Mel/N-Mel) and split-suckling (yes/no; Split/N-Split). Meloxicam was administered intramuscularly at 0.4 mg/kg body weight to sows on release of the placenta (~2 h postpartum). Split-suckling commenced 4 h after birth of the first piglet, with the six heaviest piglets removed from the sow for 1 h to allow the lightest piglets to suckle. This was repeated after 1.5 h. Pigs were weighed at birth and at days 1, 6, 14, and 27 after birth and at days 6, 14, 21, 28, 47, and 129 postweaning. Carcass data were collected at slaughter. Medication usage was recorded from birth to slaughter. There was a split-suckling by meloxicam interaction effect at days 1 to 6 (P &lt; 0.001) and days 6 to 14 (P &lt; 0.001) after birth. Meloxicam administration had no effect on average daily gain (ADG) when split-suckling was applied; however, when split-suckling was not applied, postpartum meloxicam administration increased ADG. There was a meloxicam × split-suckling interaction for ADG from weaning to day 6 postweaning (P = 0.03). Meloxicam increased ADG when split-suckling was applied but not in its absence. Carcass weight was increased by meloxicam (P = 0.01) but was not affected by split-suckling (P &gt; 0.05). Meloxicam use in sows reduced the number of clinical cases of disease (P = 0.04) in suckling pigs which tended to reduce the volume of antibiotics (P = 0.08) and anti-inflammatories (P = 0.08) administered. Split-suckling had no effect on medication usage in sows and piglets during lactation but increased their use from weaning to slaughter. In conclusion, postpartum administration of meloxicam to sows is an easily implemented strategy. It reduced clinical cases of disease, increased ADG in pigs during the first two weeks of life and early postweaning and increased carcass weight at slaughter. However, no split-suckling benefit was observed.
Utilizing a divalent metal ion transporter to control biogenic nanoparticle synthesis
Authors: Gangan Manasi Subhash , Naughton Kyle L , Boedicker James Q 
Published: August 2023

Abstract

Biogenic synthesis of inorganic nanomaterials has been demonstrated for both wild and engineered bacterial strains. In many systems the nucleation and growth of nanomaterials is poorly controlled and requires concentrations of heavy metals toxic to living cells. Here, we utilized the tools of synthetic biology to engineer a strain of Escherichia coli capable of synthesizing cadmium sulfide nanoparticles from low concentrations of reactants with control over the location of synthesis. Informed by simulations of bacterially-assisted nanoparticle synthesis, we created a strain of E. coli expressing a broad-spectrum divalent metal transporter, ZupT, and a synthetic CdS nucleating peptide. Expression of ZupT in the outer membrane and placement of the nucleating peptide in the periplasm focused synthesis within the periplasmic space and enabled sufficient nucleation and growth of nanoparticles at sub-toxic levels of the reactants. This strain synthesized internal CdS quantum dot nanoparticles with spherical morphology and an average diameter of approximately 3.3 nm.

One-Sentence Summary
Expression of a metal ion transporter regulates synthesis of cadmium sulfide nanoparticles in bacteria.
Actinomycosis of the paranasal sinuses: case report and literature review
Authors: Alqahtani Abdullah M , Alwadi Fahad A , Almahdi Mohammed 
Published: August 2023

Abstract
Actinomycosis is a chronic granulomatous condition caused by filamentous gram-positive anaerobic bacteria that colonizes the mouth, gastrointestinal tract and urogenital tract. Infection occurs through the mucosal surfaces, often resulting from dental procedures or trauma, primarily affecting the maxillary sinus. We report a case of Actinomyces sinusitis affecting the right maxillary and right ethmoidal sinuses of a 41-year-old woman. The diagnosis was made through a combination of histopathological report and computed tomography scan. The patient underwent endoscopic sinus surgery followed by long-term antibiotics for 6 months and reported improvement of her symptoms.
Giant gallbladder case report with vascular endothelial growth factor (VEGF) serum level and mRNA expression evaluation
Authors: Sapan Heber B , Rendy Leo , Tendean Michael , Panelewen Jimmy 
Published: August 2023

Abstract
Giant gallbladder (GGB) is a rare condition and its pathogenesis could not be explained clearly. It can result from cholelithiasis, chronic cholecystitis or neoplasm, but more rarely if created congenitally. Adequate vasculatization should support the development of this entity. A 47-year-old lady presented with a dull pain and right upper quadrant abdominal mass. A computed tomography scan showed 27 × 25 × 12 cms cystic mass expanding to the right illiac fossae, surrounded by a homogenous capsule. There were neither stones nor mass in the biliary tract and total cholecystectomy was done. Patient recovered well without signs of cholestasis 5 years postoperatively. A few cases of giant benign gall bladder have been reported in literature; however, no study has tried to investigate the mechanism of its etiology. To support the enlargement of the tissue or organ there must be some growth factors along with adequate vascularization. Vascular endothelial growth factor (VEGF) serum level and VEGF messenger ribonucleic acid (mRNA) gene expression were increased in this case. This GGB case suggests a congenital factor as its etiology. Cholecystectomy may relieve uncomfortable symptoms with good results. The incidence of GGB accompanied by increased serum VEGF levels and mRNA gene expression supports the hypothesis that VEGF plays a major role in supporting the vasculogenesis of GGBs.
Large bowel perforation secondary to endometriosis
Authors: Goriel Lawrence Y , Seok David J , Akrawe Silvy C , Goriel Yousif H 
Published: August 2023

Abstract
Endometriosis is described as the implantation of ectopic, viable endometrium. Among the complications associated with this phenomenon, ectopic foci that localizes to the bowel can result in many presentations. An uncommon presentation of such an occurrence is a mass effect on the colon causing an obstruction. This case report describes the progression of endometriosiscausing mass effect in the colon and resulting in perforated hollow viscous. Hence, this demonstrates the importance of maintaining endometriosis as a differential diagnosis in women of childbearing age presenting with bowel obstruction. Although the presence of endometriosis as a cause of bowel obstruction has been reported in the literature, the presentation of large bowel perforation is rare. In this case, an extremely rare presentation of sigmoid obstruction with transverse colonic perforation is observed.
Iatrogenic diaphragmatic herniation of the liver into the pericardium—a case report
Authors: Wood Phoebe C , Simpson Fraser H , Yuide Peter , Franz Robert 
Published: August 2023

Abstract
Iatrogenic diaphragmatic herniation is rare. This case is an example of herniation of the liver into the pericardial space post-transdiaphragmatic pericardial window formation for recurrent pericarditis. This case highlights that transdiaphragmatic herniation of intra-abdominal organs should be considered in patients presenting with gastrointestinal or cardiorespiratory symptoms with history of iatrogenic diaphragmatic defect.
Malignant primary melanoma of the colon: a case report
Authors: Foley Claire K , Hughes Marybeth S , Hehman Charles T 
Published: August 2023

Abstract
Melanoma is most associated with cancer of the skin. However, a small subset of these melanomas can be a primary malignancy of other mucosal membranes. A 55-year-old male presented to the gastroenterologist with 1 year of symptoms typical of colon cancer including bloating, abdominal pain and weight loss. He underwent colonoscopy and a mass was seen in the transverse colon that was later proven melanoma. A PET CT scan showed this was his only focus of disease. He then underwent a laparoscopic-assisted extended right hemicolectomy. He had an uneventful postoperative course. He was thoroughly examined for other sources of melanoma such as cutaneous, anal and uveal sources. He has recovered well at home and is receiving adjuvant pembrolizumab immunotherapy. Mucosal primary melanomas have a worse 5-year survival than primary cutaneous melanomas. A multi-disciplinary approach is necessary to treat and properly diagnose these malignancies.
Successful management of penetrating cardiac injury in a limited resource setting without cardiac surgical instruments and heart-lung machine
Authors: Ammannaya Ganesh Kumar K 
Published: August 2023

Abstract
Penetrating cardiac injuries (PCI) are often fatal and do not present enough time for effective referrals to higher centers. Most deaths occur in transit from a remote healthcare setting with limited resources. I present the first reported case of PCI in the medical literature to be managed successfully in the absence of heart-lung machine as well as dedicated cardiac surgical instruments and equipment, and which was further complicated by mediastinitis.
Antifungal susceptibility patterns for Aspergillus, Scedosporium, and Exophiala isolates recovered from cystic fibrosis patients against amphotericin B, and three triazoles and their impact after long-term therapies
Authors: Brito Devoto Tomás , Hermida-Alva Katherine , Posse Gladys , Finquelievich Jorge L , García-Effrón Guillermo , Cuestas María L 
Published: August 2023

Abstract
In cystic fibrosis (CF) patients, fungal colonization of the respiratory tract is frequently found. Aspergillus fumigatus, Scedosporium genus, and Exophiala dermatitidis are the most commonly isolated moulds from the respiratory tract secretions of CF patients. The aim of this 5-year surveillance study was to identify trends in species distribution and susceptibility patterns of 212 mould strains identified as Aspergillus spp., Scedosporium spp., and Exophiala spp., isolated from sputum of 63 CF patients who received long-term therapy with itraconazole (ITR) and/or voriconazole (VRC). The Aspergillus isolates were identified as members of the sections Fumigati (n = 130), Flavi (n = 22), Terrei (n = 20), Nigri (n = 8), Nidulantes (n = 1), and Usti (n = 1). Among the 16 species of the genus Scedosporium, 9 were S. apiospermum, 3 S. aurantiacum, and 4 S. boydii. Among the 14 Exophiala species, all were molecularly identified as E. dermatitidis. Overall, 94% (15/16) of Scedosporium spp., 50% (7/14) of E. dermatitidis, and 7.7% (14/182) of Aspergillus spp. strains showed high MIC values (≥8 µg/ml) for at least one antifungal. Particularly, 8.9% (19/212) of isolates showed high MIC values for amphotericin B, 11.7% (25/212) for ITR, 4.2% (9/212) for VRC, and 3.3% (7/212) for posaconazole. In some cases, such as some A. fumigatus and E. dermatitidis isolates recovered from the same patient, susceptibility to antifungal azoles decreased over time. We show that the use of azoles for a long time in CF patients causes the selection/isolation of mould strains with higher MIC values.
New radio lobes at parsec scale from the east–west protostellar jet RAFGL2591
Authors: Cheriyan A G , Vig S , Mohan Sreelekshmi 
Published: August 2023

ABSTRACT
RAFGL2591 is a massive star-forming complex in the Cygnus-X region comprising of a cluster of embedded protostars and young stellar objects located at a distance of 3.33 kpc. We investigate low-frequency radio emission from the protostellar jet associated with RAFGL2591 using the Giant Metrewave Radio Telescope (GMRT) at 325, 610, and 1280 MHz. For the first time, we have detected radio jet lobes in the east–west direction, labelled as GMRT-1 and GMRT-2. While GMRT-1 displays a flat radio spectral index of α = −0.10, GMRT-2 shows a steeply negative value of α = −0.62 suggestive of non-thermal emission. H2 emission maps show the presence of numerous knots, arcs, and extended emission towards the east–west jet, excited by the protostar VLA 3. In addition, we report a few H2 knots in the north-east and south-west for the first time. The radio lobes (GMRT-1 and GMRT-2) and H2 emission towards this region are understood in the context of the prominent east–west jet as well as its lesser-known sibling jet in the north-east and south-west direction. To model the radio emission from the lobes, we have employed a numerical model including both thermal and non-thermal emission and found number densities towards these lobes in the range 100–1000 cm−3. The misalignment of the east–west jet lobes exhibits a reflection symmetry with a bending of ∼20°. We attempt to understand this misalignment through precession caused by a binary partner and/or a supersonic side wind from source(s) in the vicinity.
The JWST FRESCO survey: legacy NIRCam/grism spectroscopy and imaging in the two GOODS fields
Authors: Oesch P A , Brammer G , Naidu R P , Bouwens R J , Chisholm J , Illingworth G D , Matthee J , Nelson E , Qin Y , Reddy N , Shapley A , Shivaei I , van Dokkum P , Weibel A , Whitaker K , Wuyts S , Covelo-Paz A , Endsley R , Fudamoto Y , Giovinazzo E , Herard-Demanche T , Kerutt J , Kramarenko I , Labbe I , Leonova E , Lin J , Magee D , Marchesini D , Maseda M , Mason C , Matharu J , Meyer R A , Neufeld C , Prieto Lyon G , Schaerer D , Sharma R , Shuntov M , Smit R , Stefanon M , Wyithe J S B , Xiao M 
Published: August 2023

ABSTRACT
We present the JWST cycle 1 53.8 h medium program FRESCO, short for ‘First Reionization Epoch Spectroscopically Complete Observations’. FRESCO covers 62 arcmin2 in each of the two GOODS/CANDELS fields for a total area of 124 arcmin2 exploiting JWST’s powerful new grism spectroscopic capabilities at near-infrared wavelengths. By obtaining ∼2 h deep NIRCam/grism observations with the F444W filter, FRESCO yields unprecedented spectra at R ∼ 1600 covering 3.8–5.0 µm for most galaxies in the NIRCam field of view. This setup enables emission line measurements over most of cosmic history, from strong PAH lines at z ∼ 0.2–0.5, to Pa α and Pa β at z ∼ 1–3, He i and [S iii] at z ∼ 2.5–4.5, H α and [N ii] at z ∼ 5–6.5, up to [O iii] and H β for z ∼ 7–9 galaxies. FRESCO’s grism observations provide total line fluxes for accurately estimating galaxy stellar masses and calibrating slit-loss corrections of NIRSpec/MSA spectra in the same field. Additionally, FRESCO results in a mosaic of F182M, F210M, and F444W imaging in the same fields to a depth of ∼28.2 mag (5σ in 0${_{.}^{\prime\prime}}$32 diameter apertures). Here, we describe the overall survey design and the key science goals that can be addressed with FRESCO. We also highlight several, early science results, including: spectroscopic redshifts of Lyman break galaxies that were identified almost 20 yr ago, the discovery of broad-line active galactic nuclei at z &gt; 4, and resolved Pa α maps of galaxies at z ∼ 1.4. These results demonstrate the enormous power for serendipitous discovery of NIRCam/grism observations.
Implications of z ≳ 12 JWST galaxies for galaxy formation at high redshift
Authors: Qin Yuxiang , Balu Sreedhar , Wyithe J Stuart B 
Published: August 2023

ABSTRACT
Using a semi-analytic galaxy formation model, we study analogues of eight z ≳ 12 galaxies recently discovered by James Webb Space Telescope (JWST). We select analogues from a cosmological simulation with a (311 cMpc)3 volume and an effective particle number of 1012 enabling the resolution of every atomic-cooling galaxy at z ≤ 20. We vary model parameters to reproduce the observed ultraviolet (UV) luminosity function at 5 &lt; z &lt; 13, aiming for a statistically representative high-redshift galaxy mock catalogue. Using the forward-modelled JWST photometry, we identify analogues from this catalogue and study their properties as well as possible evolutionary paths and local environment. We find faint JWST galaxies (MUV ≳ − 19.5) to remain consistent with the standard galaxy formation model and that our fiducial catalogue includes large samples of their analogues. The properties of these analogues broadly agree with conventional spectral energy distribution-fitting results, except for having systematically lower redshifts due to the evolving ultraviolet luminosity function, and for having higher specific star formation rates as a result of burstier histories in our model. On the other hand, only a handful of bright galaxy analogues can be identified for the observed z ∼ 12 galaxies. Moreover, in order to reproduce the z ≳ 16 JWST galaxy candidates, boosting star-forming efficiencies through reduced feedback regulation and increased gas depletion rate is necessary relative to models of lower redshift populations. This suggests star formation in the first galaxies could differ significantly from their lower redshift counterparts. We also find that these candidates are subject to low-redshift contamination, which is present in our fiducial results as both the dusty or quiescent galaxies at z ∼ 5.
On the origin of the evolution of the halo occupation distribution
Authors: Contreras Sergio , Zehavi Idit 
Published: August 2023

ABSTRACT
We use the TNG300 magnetohydrodynamic simulation and mock catalogues built using subhalo abundance matching (SHAM) to study the origin of the redshift evolution of the halo occupation distribution (HOD). We analyse stellar-mass selected galaxy samples with fixed number densities, spanning the redshift range 0 ≤ z ≤ 3. We measure their halo occupation functions and fit the HOD parameters to study their evolution over cosmic time. The TNG300 galaxy population strongly depends on the baryonic physics implemented in the simulation. In contrast, the galaxy population predicted by a basic SHAM model without scatter is a direct result of the cosmology of the dark matter simulation. We find that the HOD evolution is similar for both models and is consistent with a previous study of the HOD evolution in semi-analytical models. Specifically, this is the case for the ratio between the characteristic halo masses for hosting central and satellite galaxies. The only HOD parameter whose evolution varies across models is σlogM, which contains information about the stellar mass–halo mass relation of the galaxies but does not strongly impact galaxy clustering. We also demonstrate that the dependence on the specific values of the cosmological parameters is small. We conclude that the cosmology of the galaxy sample, i.e. the cosmological hierarchical growth of structure, and not the baryonic physics prescriptions, governs the evolution of the HOD for stellar mass-selected samples. These results have important implications for populating simulated light-cones with galaxies and can facilitate the interpretation of clustering data at different redshifts.
Optical and near-UV spectroscopic properties of low-redshift jetted quasars in the main sequence context
Authors: Mengistue Shimeles Terefe , Del Olmo Ascensión , Marziani Paola , Pović Mirjana , Martínez-Carballo María Angeles , Perea Jaime , Márquez Isabel 
Published: August 2023

ABSTRACT
This paper presents new optical and near-UV spectra of 11 extremely powerful jetted quasars, with radio to optical flux density ratio &gt;103, which concomitantly cover the low-ionization emission of Mg iiλ2800 and hβ as well as the Fe ii blends in the redshift range 0.35 ≲ z ≲ 1. We aim to quantify broad emission line differences between radio-loud (RL) and radio-quiet (RQ) quasars by using the 4D eigenvector 1 parameter space and its main sequence (MS) and to check the effect of powerful radio ejection on the low-ionization broad emission lines. The hβ and Mg iiλ2800 emission lines were measured by using non-linear multicomponent fittings as well as by analysing their full profile. We found that broad emission lines show large redward asymmetry both in hβ and Mg iiλ2800. The location of our RL sources in a UV plane looks similar to the optical one, with weak Fe iiUV emission and broad Mg iiλ2800. We supplement the 11 sources with large samples from previous work to gain some general inferences. We found that, compared to RQ, our extreme RL quasars show larger median hβ full width at half maximum (FWHM), weaker Fe ii emission, larger MBH, lower Lbol/LEdd, and a restricted bf space occupation in the optical and UV MS planes. The differences are more elusive when the comparison is carried out by restricting the RQ population to the region of the MS occupied by RL sources, albeit an unbiased comparison matching MBH and Lbol/LEdd suggests that the most powerful RL quasars show the highest redward asymmetries in hβ.
Searching for magnetic fields in pulsating A-type stars: the discovery of a strong field in the probable δ Sct star HD 340577 and a null result for the γ Dor star HR 8799
Authors: Hubrig S , Järvinen S P , Alvarado-Gómez J D , Ilyin I , Schöller M 
Published: August 2023

ABSTRACT
Numerous δ Sct and γ Dor pulsators are identified in the region of the Hertzsprung–Russell diagram that is occupied by chemically peculiar magnetic Ap stars. The connection between δ Sct and γ Dor pulsations and the magnetic field in Ap stars is however not clear: theory suggests for magnetic Ap stars some critical field strengths for pulsation mode suppression by computing the magnetic damping effect for selected p and g modes. To test these theoretical considerations, we obtained PEPSI spectropolarimetric snapshots of the typical Ap star HD 340577, for which δ Sct-like pulsations were recently detected in Transiting Exoplanet Survey Satellite data, and the γ Dor pulsator HR 8799, which is a remarkable system with multiple planets and two debris discs. Our measurements reveal the presence of a magnetic field with a strength of several hundred Gauss in HD 340577. The measured mean longitudinal field would be the strongest field measured so far in a δ Sct star if the pulsational character of HD 340577 is confirmed spectroscopically. No magnetic field is detected in HR 8799.