1. |
- Kanai, M, et al.
(author)
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- 2023
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swepub:Mat__t
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2. |
- Niemi, MEK, et al.
(author)
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- 2021
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swepub:Mat__t
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3. |
- Jung, Christian, et al.
(author)
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A comparison of very old patients admitted to intensive care unit after acute versus elective surgery or intervention
- 2019
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In: Journal of critical care. - : W B SAUNDERS CO-ELSEVIER INC. - 0883-9441 .- 1557-8615. ; 52, s. 141-148
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Journal article (peer-reviewed)abstract
- Background: We aimed to evaluate differences in outcome between patients admitted to intensive care unit (ICU) after elective versus acute surgery in a multinational cohort of very old patients (80 years; VIP). Predictors of mortality, with special emphasis on frailty, were assessed.Methods: In total, 5063 VIPs were induded in this analysis, 922 were admitted after elective surgery or intervention, 4141 acutely, with 402 after acute surgery. Differences were calculated using Mann-Whitney-U test and Wilcoxon test. Univariate and multivariable logistic regression were used to assess associations with mortality.Results: Compared patients admitted after acute surgery, patients admitted after elective surgery suffered less often from frailty as defined as CFS (28% vs 46%; p < 0.001), evidenced lower SOFA scores (4 +/- 5 vs 7 +/- 7; p < 0.001). Presence of frailty (CFS >4) was associated with significantly increased mortality both in elective surgery patients (7% vs 12%; p = 0.01), in acute surgery (7% vs 12%; p = 0.02).Conclusions: VIPs admitted to ICU after elective surgery evidenced favorable outcome over patients after acute surgery even after correction for relevant confounders. Frailty might be used to guide clinicians in risk stratification in both patients admitted after elective and acute surgery.
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4. |
- Selvavinayagam, Sivaprakasam T., et al.
(author)
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Platelet-Large Cell Ratio and Erythrocyte Sedimentation Rate are Surrogate Predictors of Latent Tuberculosis Infection
- 2024
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Other publication (other academic/artistic)abstract
- Aims: Prompt detection and treatment of latent tuberculosis infection (LTBI) holds the key to global TB elimination. The lack of an established test for predicting LTBI poses a substantial challenge in disease management. Here, we identified the biochemical and hematological markers of LTBI, and correlated their usefulness to discriminate LTBI from healthy controls. Main Methods: We conducted a cross-sectional investigation and correlated the various biochemical and hematological markers for detecting LTBI among household contacts (HHCs) of TB infection. Our study included 90 individuals – 30 healthy controls, 30 interferon-gamma release assay (IGRA) positive HHCs, and 30 IGRA-negative HHCs. Biomarkers were measured using designated auto analyzers. Key Findings: ESR, MPV, D-dimer, P-LCR, and PDW were significantly higher among LTBI subjects. ESR, PDW, and P-LCR were markedly associated with LTBI. Multivariate analysis showed that either ESR or P-LCR greater than their respective predetermined cut-off values showed higher odds of developing LTBI. Our study demonstrated that ESR and P-LCR are good surrogate markers for diagnosing LTBI. Also, significantly low ferritin in females and MCHC in males belonging to the HHC/IGRA-ve were observed. Significance: The ESR and P-LCR could aid in predicting LTBI among HHCs. Further, the low serum ferritin is associated with TB resisters.
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5. |
- Srinivasaragavan, Gokul P., et al.
(author)
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A Sensitive Search for Supernova Emission Associated with the Extremely Energetic and Nearby GRB 221009A
- 2023
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In: Astrophysical Journal Letters. - 2041-8205 .- 2041-8213. ; 949:2
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Journal article (peer-reviewed)abstract
- We report observations of the optical counterpart of the long gamma-ray burst GRB 221009A. Due to the extreme rarity of being both nearby (z = 0.151) and highly energetic (E ( gamma,iso) >= 10(54) erg), GRB 221009A offers a unique opportunity to probe the connection between massive star core collapse and relativistic jet formation across a very broad range of gamma-ray properties. Adopting a phenomenological power-law model for the afterglow and host galaxy estimates from high-resolution Hubble Space Telescope imaging, we use Bayesian model comparison techniques to determine the likelihood of an associated supernova (SN) contributing excess flux to the optical light curve. Though not conclusive, we find moderate evidence (K (Bayes) = 10(1.2)) for the presence of an additional component arising from an associated SN, SN 2022xiw, and find that it must be substantially fainter (<67% as bright at the 99% confidence interval) than SN 1998bw. Given the large and uncertain line-of-sight extinction, we attempt to constrain the SN parameters (M (Ni), M (ej), and E (KE)) under several different assumptions with respect to the host galaxy's extinction. We find properties that are broadly consistent with previous GRB-associated SNe: M (Ni) = 0.05-0.25 M (circle dot), M (ej) = 3.5-11.1 M (circle dot), and E (KE) = (1.6-5.2) x 10(52) erg. We note that these properties are weakly constrained due to the faintness of the SN with respect to the afterglow and host emission, but we do find a robust upper limit on M (Ni) of M (Ni) < 0.36 M (circle dot). Given the tremendous range in isotropic gamma-ray energy release exhibited by GRBs (seven orders of magnitude), the SN emission appears to be decoupled from the central engine in these systems.
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