Piroxicam has antitumour effects in dogs with cancer, although side effects may limit its use. The purpose of this study was to retrospectively identify factors predisposing cancer‐bearing dogs to ...adverse events (AEs) following piroxicam therapy. Medical records of dogs presented to the Purdue Veterinary Teaching Hospital between 2005 and 2015 were reviewed, and 137 dogs met the criteria for study inclusion. Toxic effects of piroxicam in these dogs were graded according to an established system. Multivariate logistic regression was used to estimate the extent to which certain factors affected the risk for AEs. Age odds ratio (OR) 1.250, P = 0.009; 95% confidence interval (CI) 1.057–1.479 and concurrent use of gastroprotectant medications (OR 2.612, P = 0.025; 95% CI 1.127–6.056) significantly increased the risk for gastrointestinal AEs. The results of this study may help inform the risk versus benefit calculation for clinicians considering the use of piroxicam to treat dogs with cancer.
The study hypothesis is that higher doses of metronomic (low‐dose) chlorambucil will improve outcome without significantly worsening adverse events (AE). Retrospectively, 88 dogs were screened to ...assess for tolerability and response to chlorambucil utilizing retrospective and prospective data sets, comparing metronomic oral daily doses 4, 6 and 8 mg m2. There were 78 and 70 dogs in the tolerability and efficacy portions, respectively. The severity of gastrointestinal (GI) AE was significantly worse, and time to development of GI events was significantly shorter at 6 mg m2 than at 4 mg m2 (both P < 0.001). Chlorambucil was discontinued earlier in the dogs treated at the 6 mg m2 doses than in the dogs treated at 4 mg m2 (P = 0.015). Thrombocytopenia occurred significantly earlier at 8 mg m2 than at 4 mg m2 (P = 0.017). Higher doses of metronomic (low‐dose) chlorambucil did not provide improved responses and were associated with more AE.
Expression of histamine, serotonin, and KIT was evaluated in 61 archived feline mast cell tumors (MCTs) from the skin (n = 29), spleen (n = 17), and gastrointestinal (GI) tract (n = 15) using ...immunohistochemistry. Twenty-eight percent of cutaneous MCTs, 18% of splenic MCTs, and 53% of GI MCTs displayed histamine immunoreactivity. Serotonin immunoreactivity was detected in 3 GI and 1 cutaneous MCT. Sixty-nine percent of cutaneous MCTs, 35% of splenic MCTs, and 33% of GI MCTs were positive for KIT. Expression of these biogenic amines and KIT was less common than expected. Results of this study suggest heterogeneity in feline MCTs based on anatomic location. Further studies are needed to explain the significance of these differences.
The purpose of this study was to assess the toxicoses and antitumor activity of metronomic chlorambucil at a dosage of 4 mg m−2 daily in dogs with naturally occurring cancer. Thirty‐six dogs were ...enrolled in the study. The protocol was well tolerated with no grade 3 or 4 toxicoses noted. Complete remission was achieved, and lasted over 35 weeks in three dogs (mast cell tumour, soft tissue sarcoma and thyroid carcinoma). Partial remission was noted in 1 dog with histiocytic sarcoma (39 weeks duration) for an overall remission rate of 11% (4 of 36). Stable disease was noted in 17 dogs (47%) with various other cancers. The median progression‐free interval was 61 days, and the median survival time was 153 days. Chlorambucil given in a metronomic protocol showed antitumor activity in dogs with a variety of naturally occurring cancers.
We report optical and near-infrared observations of SN2012ca with the Public ESO Spectroscopy Survey of Transient Objects (PESSTO), spread over one year since discovery. The supernova (SN) bears many ...similarities to SN1997cy and to other events classified as Type IIn but which have been suggested to have a thermonuclear origin with narrow hydrogen lines produced when the ejecta impact a hydrogen-rich circumstellar medium (CSM). Our analysis, especially in the nebular phase, reveals the presence of oxygen, magnesium and carbon features. This suggests a core-collapse explanation for SN2012ca, in contrast to the thermonuclear interpretation proposed for some members of this group. We suggest that the data can be explained with a hydrogen- and helium-deficient SN ejecta (Type I) interacting with a hydrogen-rich CSM, but that the explosion was more likely a Type Ic core-collapse explosion than a Type Ia thermonuclear one. This suggests that two channels (both thermonuclear and stripped envelope core-collapse) may be responsible for these SN 1997cy-like events.
Vigilance in socially foraging animals (e.g., elk) may serve to detect predators (i.e., reduce predation risk) or to monitor the behavior of conspecifics (i.e., reduce conspecific risk and/or ...increase reproductive benefits). These potential benefits and costs of vigilance may not be equal among different genders and age classes foraging together. We observed male and female elk from 3 age classes (yearlings, nonreproductive, reproductive) during 2 seasons (calving season, breeding season) that vary in social interactions (i.e., conspecific risk) and in 2 regions of Yellowstone National Park that varied in predation risk due to density of wolves. This study was designed to determine the potential functional benefit of vigilance across a range of herd sizes. If vigilance serves to monitor the behavior of conspecifics, we expected it to increase in the fall breeding season along with aggressive behaviors, regardless of changes in predation risk. If vigilance serves to detect predators, we expected it to increase in regions with wolves regardless of changes in conspecific risk. Adult male vigilance and aggression increased during the fall breeding season, but yearling males had significantly lower levels of vigilance. Adult female vigilance increased during the calving season, with increasing predator encounter risk, decreasing herd size, and edge position within the herd. Yearling female vigilance decreased with herd size but was lower than adult females. We conclude that the primary benefit of vigilance for male elk is to monitor conspecifics, but the primary benefit of vigilance for female elk is to detect potential predators.
RNA secondary structure is required for the proper regulation of the cellular transcriptome. This is because the functionality, processing, localization and stability of RNAs are all dependent on the ...folding of these molecules into intricate structures through specific base pairing interactions encoded in their primary nucleotide sequences. Thus, as the number of RNA sequencing (RNA-seq) data sets and the variety of protocols for this technology grow rapidly, it is becoming increasingly pertinent to develop tools that can analyze and visualize this sequence data in the context of RNA secondary structure. Here, we present Sequencing Annotation and Visualization of RNA structures (SAVoR), a web server, which seamlessly links RNA structure predictions with sequencing data and genomic annotations to produce highly informative and annotated models of RNA secondary structure. SAVoR accepts read alignment data from RNA-seq experiments and computes a series of per-base values such as read abundance and sequence variant frequency. These values can then be visualized on a customizable secondary structure model. SAVoR is freely available at http://tesla.pcbi.upenn.edu/savor.
We present Keck LRIS spectroscopy and g-band photometry of the metal-poor, low-luminosity host galaxy of the super-Chandrasekhar-mass Type Ia supernova SN 2007if. Deep imaging of the host reveals its ...apparent magnitude to be mg = 23.15 ? 0.06, which at the spectroscopically measured redshift of z helio = 0.07450 ? 0.00015 corresponds to an absolute magnitude of Mg = --14.45 ? 0.06. Galaxy g -- r color constrains the mass-to-light ratio, giving a host stellar mass estimate of log(M */M ) = 7.32 ? 0.17. Balmer absorption in the stellar continuum, along with the strength of the 4000 A break, constrains the age of the dominant starburst in the galaxy to be t burst = 123+165 --77 Myr, corresponding to a main-sequence turnoff mass of M/M = 4.6+2.6 --1.4. Using the R 23 method of calculating metallicity from the fluxes of strong emission lines, we determine the host oxygen abundance to be 12 + log(O/H)KK04 = 8.01 ? 0.09, significantly lower than any previously reported spectroscopically measured Type Ia supernova host galaxy metallicity. Our data show that SN 2007if is very likely to have originated from a young, metal-poor progenitor.
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