Pediatric Pulmonology Training in India: Current Status and Future Directions.

Respiratory illnesses are common causes of morbidity and mortality in children. Postgraduates in Pediatrics spent significant time in learning to manage respiratory disorders. Improved survival of preterm neonates, improved diagnosis and survival of chronic respiratory problems, and advances in diagnosis and therapeutics have increased the need for specialists trained in managing these patients. Training programs in Pediatric Pulmonology are evolving over the past few decades. In India, super-specialty training in Pediatric Pulmonology has grown over the past few years. There is a need to modify the training structure used in industrialized countries due to differences in patient population, priorities, and limited available resources and expertise. Formal training courses have been started in a limited number of institutions. There is a large gap between the need for a trained workforce and the available specialists in the limited number of institutions. The Indian Academy of Pediatrics National Respiratory Chapter (IAPNRC) has initiated a fellowship program to bridge the gap. Comprehensive training involving academic and hands-on training may go a long way to improve the care of children with acute and chronic respiratory problems. For sustainable development of the super specialty, there is a need to work towards creating Pediatric Pulmonology service departments in various institutions that may be responsible for comprehensive training and research activities to answer common research questions.

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM.

Transmission spectroscopy1-3 of exoplanets has revealed signatures of water vapour, aerosols and alkali metals in a few dozen exoplanet atmospheres4,5. However, these previous inferences with the Hubble and Spitzer Space Telescopes were hindered by the observations' relatively narrow wavelength range and spectral resolving power, which precluded the unambiguous identification of other chemical species-in particular the primary carbon-bearing molecules6,7. Here we report a broad-wavelength 0.5-5.5 µm atmospheric transmission spectrum of WASP-39b8, a 1,200 K, roughly Saturn-mass, Jupiter-radius exoplanet, measured with the JWST NIRSpec's PRISM mode9 as part of the JWST Transiting Exoplanet Community Early Release Science Team Program10-12. We robustly detect several chemical species at high significance, including Na (19σ), H2O (33σ), CO2 (28σ) and CO (7σ). The non-detection of CH4, combined with a strong CO2 feature, favours atmospheric models with a super-solar atmospheric metallicity. An unanticipated absorption feature at 4 µm is best explained by SO2 (2.7σ), which could be a tracer of atmospheric photochemistry. These observations demonstrate JWST's sensitivity to a rich diversity of exoplanet compositions and chemical processes.

Adding MR Diffusion Imaging and T2 Signal Intensity to Neck Imaging Reporting and Data System Categories 2 and 3 in Primary Sites of Postsurgical Oral Cavity Carcinoma Provides Incremental Diagnostic Value.

BACKGROUND AND PURPOSE: The NI-RADS lexicon doesn't use ADC parameters and T2 weighted signal for ascribing categories. We explored ADC, DWI, and T2WI to examine the diagnostic accuracy in primary sites of postsurgical oral cavity carcinoma in the Neck Imaging Reporting and Data System (NI-RADS) categories 2 and 3. MATERIALS AND METHODS: We performed a retrospective analysis in clinically asymptomatic post-surgically treated patients with oral cavity squamous cell carcinoma who underwent contrast-enhanced MRI between January 2013 and January 2016. Histopathology and follow-up imaging were used to ascertain the presence or absence of malignancy in subjects with "new enhancing lesions," which were interpreted according to the NI-RADS lexicon by experienced readers, including NI-RADS 2 and 3 lesions in the primary site. NI-RADS that included T2WI and DWI (referred to as NI-RADS A) and ADC (using the best cutoff from receiver operating characteristic curve analysis, NI-RADS B) was documented in an Excel sheet to up- or downgrade existing classic American College of Radiology NI-RADS and calculate diagnostic accuracy. RESULTS: Sixty-one malignant and 23 benign lesions included in the study were assigned American College of Radiology NI-RADS 2 (n = 33) and NI-RADS 3 (n = 51) categories. The recurrence rate was 90% (46/51) for NI-RADS three, 45% (15/33) for NI-RADS 2, and 73% (61/84) overall. T2WI signal morphology was intermediate in 45 subjects (53.5%) and restricted DWI in 54 (64.2%). Sensitivity, specificity, positive predictive value, negative predictive value, and accuracy of the American College of Radiology NI-RADS were the following: NI-RADS (75.4%, 78.3%, 90.1%, 54.5%, and 76.1%); NI-RADS A (79.1%, 81.2%, 91.9%, 59.1%, and 79.6%); and NI-RADS B (88.9%, 72.7%, 91.4%, 66.7%, and 85.1%), respectively. CONCLUSIONS: Adding MR imaging diagnostic characteristics like T2WI, DWI, and ADC to the American College of Radiology NI-RADS improved diagnostic accuracy and sensitivity.

Comparison of Manual Capsulorhexis and 25-Gauge Vitrectorhexis in Pediatric Cataract Surgery: A Pilot Study.

PURPOSE: To compare short-term visual outcomes (best corrected visual acuity [BCVA]), visual axis opacification, anterior (ACCC) and posterior (PCCC) continuous curvilinear capsulorhexis size, shape, and extension, and their decentration between manual capsulorhexis and 25-gauge vitrectorhexis in pediatric cataract surgery with intraocular lens (IOL) implantation. METHODS: Thirty eyes of children aged 3 to 8 years with developmental cataract were randomly selected for ACCC and PCCC by manual capsulorhexis forceps and 25-gauge vitrectomy cutter followed by IOL implantation and limited anterior vitrectomy. The size of the ACCC and PCCC was measured intraoperatively with calibrated capsulorhexis forceps. Patients were followed up for 3 months postoperatively and were evaluated for BCVA and visual axis opacification. Slit-lamp photographs of operated eyes were taken in retroillumination. The size in millimeters and decentration of the ACCC and PCCC from the center of the IOL were measured with the help of the Python imaging library. RESULTS: There was no statistically significant difference between BCVA (P > .05), visual axis opacification (P > .05), size of the ACCC (P > .05) and its decentration (P > .05), extension of the rhexis (P > .05), and size of the PCCC (P > .05) and its decentration (P > .05) between the two methods. CONCLUSIONS: In both groups, BCVA, visual axis opacification, and ACCC and PCCC size, shape, and decentration from the center of the IOL were comparable, making 25-gauge vitrectorhexis a good alternative to manual capsulorhexis. [J Pediatr Ophthalmol Strabismus. 2019;56(5):327-332.].

An absolute sodium abundance for a cloud-free 'hot Saturn' exoplanet.

Broad absorption signatures from alkali metals, such as the sodium (Na I) and potassium (K I) resonance doublets, have long been predicted in the optical atmospheric spectra of cloud-free irradiated gas giant exoplanets1-3. However, observations have revealed only the narrow cores of these features rather than the full pressure-broadened profiles4-6. Cloud and haze opacity at the day-night planetary terminator are considered to be responsible for obscuring the absorption-line wings, which hinders constraints on absolute atmospheric abundances7-9. Here we report an optical transmission spectrum for the 'hot Saturn' exoplanet WASP-96b obtained with the Very Large Telescope, which exhibits the complete pressure-broadened profile of the sodium absorption feature. The spectrum is in excellent agreement with cloud-free, solar-abundance models assuming chemical equilibrium. We are able to measure a precise, absolute sodium abundance of logεNa = [Formula: see text], and use it as a proxy for the planet's atmospheric metallicity relative to the solar value (Zp/Zʘ = [Formula: see text]). This result is consistent with the mass-metallicity trend observed for Solar System planets and exoplanets10-12.

Helium in the eroding atmosphere of an exoplanet.

Helium is the second-most abundant element in the Universe after hydrogen and is one of the main constituents of gas-giant planets in our Solar System. Early theoretical models predicted helium to be among the most readily detectable species in the atmospheres of exoplanets, especially in extended and escaping atmospheres 1 . Searches for helium, however, have hitherto been unsuccessful 2 . Here we report observations of helium on an exoplanet, at a confidence level of 4.5 standard deviations. We measured the near-infrared transmission spectrum of the warm gas giant 3 WASP-107b and identified the narrow absorption feature of excited metastable helium at 10,833 angstroms. The amplitude of the feature, in transit depth, is 0.049 ± 0.011 per cent in a bandpass of 98 angstroms, which is more than five times greater than what could be caused by nominal stellar chromospheric activity. This large absorption signal suggests that WASP-107b has an extended atmosphere that is eroding at a total rate of 1010 to 3 × 1011 grams per second (0.1-4 per cent of its total mass per billion years), and may have a comet-like tail of gas shaped by radiation pressure.

Ocular manifestations of tuberculosis.

Tuberculosis (TB) is a chronic debilitating infection which is caused by Mycobacteriumn tuberculosis and other mycobacteria. Mycobacterium tuberculosis affects predominantly the lungs although it can affect every organ of the body. Two billion people are affected by tuberculosis. Majority of tuberculosis cases and related deaths occur in Asia. Tuberculosis most commonly occurs in people belonging to the low socio-economic status. Crowding, poor healthcare, unemployment and poor knowledge about basic sanitation increase the risk of acquiring the infection. India is endemic for tuberculosis with 256/lakh population. TB can affect majority of the structures of the eye with marked variability of the lesions. This review will focus on the clinical presentation and management of ocular TB.

Comparative Analysis of Refractive and Topographic Changes in Early and Advanced Keratoconic Eyes Undergoing Corneal Collagen Crosslinking.

PURPOSE: To compare the refractive and topographic changes at 1 year in eyes with early and advanced keratoconus undergoing corneal collagen crosslinking (CXL). A prospective, nonrandomized comparative clinical intervention study. METHODS: Thirty eyes of patients with keratoconus underwent CXL. They were divided into 2 groups based on their mean central keratometry: group A [mean central K ≤ 53 diopters (D)] and group B (mean central K > 53 D). Uncorrected visual acuity (UCVA), best-corrected visual acuity (BCVA), refraction, topography, pachymetry, and endothelial cell counts were evaluated at baseline and at 1, 3, 6, and 12 months of follow-up. RESULTS: The mean baseline logarithm of the minimum angle of resolution (logMAR) UCVA and logMAR BCVA in group A was 1.007 ± 0.30 and 0.566 ± 0.21, respectively. The values improved to 0.727 ± 0.29 (P = 0.001) and 0.306 ± 0.15 (P = 0.001) at 1-year post CXL. The mean baseline logMAR UCVA and logMAR BCVA in group B were 1.040 ± 0.24 and 0.641 ± 0.25, respectively. It changed to 0.953 ± 0.26 (P = 0.054) and 0.633 ± 0.27 (P = 0.891) at 1 year. The improvement in the UCVA and BCVA was statistically significant in group A as compared with that in group B. The mean baseline flattest, steepest, central, and apical keratometry in group A were 48.7 ± 2.5 D, 54.9 ± 3.3 D, 49.5 ± 1.4 D, and 57.3 ± 2.3 D, respectively. At 12 months, the values changed to 47.8 ± 2.4 D, 54.1 ± 3.0 D, 48.8 ± 1.8 D, and 56.2 ± 2.7 D, the change being statistically significant for mean flat and apical K only (P < 0.05). All the 4 indices did not show any statistically significant difference at 12 months in group B (P > 0.05). CONCLUSIONS: Corneal CXL is more effective in improving the refractive and topographical parameters at 1 year when it is performed early in the course of the disease.

Sterile keratitis after corneal collagen crosslinking in a child.

Corneal collagen crosslinking (CXL) is a non invasive technique used in halting the progression of keratoconus. Complications with this modality are rare. We report a case of an 8-year-old child who developed sterile infiltrates in the immediate postoperative period after uneventful corneal collagen crosslinking for keratoconus. The infiltrates resolved with topical steroid therapy. There was also present coexisting vernal keratoconjunctivitis (VKC) which was controlled with topical 2% cyclosporine A eye drops prior to crosslinking treatment. This case highlights importance of controlling VKC prior to CXL in keratoconus as it adds to the risk of developing post operative sterile keratitis.

Reporting statistics in clinical trials published in Indian journals: a survey.

OBJECTIVES: Clinical trials are having very important place in the hierarchy of evidence based medicine. It has been observed that current methods of use and reporting of statistics of clinical trials are responsible for errors in the interpretation of results. So we decided to evaluate clinical trials published in three Indian journals of 2007 and 2008 to analyse statistical issues which may affect the interpretation of results. SETTINGS AND DESIGN: Retrospective observational study MATERIALS AND METHODS: We analyzed all the clinical trials (46) published in Indian pediatrics, Indian journal of pharmacology, journal of postgraduate medicine and of 2007-2008. RESULTS: We found that median number of end points reported in clinical trials was 4 and median number of end points which were used for testing of significance was also 4. (21) 45% of trials reported repeated measurement. 18 (39%) trials had three or more than three treatment groups. median number of test of significance was 15. post hoc subgroup analysis was done in 19% (9) of trials. P value was the sole criteria for interpretation of results in most of the trials, confidence interval was calculated in 11 (23%) trials. Baseline comparison between the study groups was done in 41 (89%) trials. in all cases comparison was done by statistical tests. Exact sample size was calculated in 18 (39%) trials. CONCLUSION: There are great chances of having error during the interpretation of results of these trials was because of multiple treatment groups, repeated measurements of endpoints, multiple tests of significance, over reliability on P value and less use of confidence interval. Statistical methods available for reducing chances of errors should be used and result should be interpreted accordingly.

Statistical reporting in Indian Pediatrics.

We analyzed 45 original articles from Indian Pediatrics for appropriateness of the statistical methods. Appropriate statistical tests (93%), no use of obscure test and use of exact P value were the positive findings observed. Sample size was calculated in 24% and confidence interval in 13%. There is a need to generate awareness regarding confidence interval and sample size calculations.