The value of antimicrobial peptides in the age of resistance
M Magana, M Pushpanathan, AL Santos… - The lancet infectious …, 2020 - thelancet.com
Accelerating growth and global expansion of antimicrobial resistance has deepened the need
for discovery of novel antimicrobial agents. Antimicrobial peptides have clear advantages …
for discovery of novel antimicrobial agents. Antimicrobial peptides have clear advantages …
[HTML][HTML] Evaluation of Genetic Mutations Associated with Mycobacterium tuberculosis Resistance to Amikacin, Kanamycin and Capreomycin: A Systematic Review
Background Rapid molecular diagnostics for detecting multidrug-resistant and extensively
drug-resistant tuberculosis (M/XDR-TB) primarily identify mutations in Mycobacterium …
drug-resistant tuberculosis (M/XDR-TB) primarily identify mutations in Mycobacterium …
Options and limitations in clinical investigation of bacterial biofilms
M Magana, C Sereti, A Ioannidis… - Clinical Microbiology …, 2018 - Am Soc Microbiol
Bacteria can form single- and multispecies biofilms exhibiting diverse features based upon
the microbial composition of their community and microenvironment. The study of bacterial …
the microbial composition of their community and microenvironment. The study of bacterial …
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples
We present a one per cent measurement of the cosmic distance scale from the detections of
the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon …
the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon …
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function
We obtain constraints on cosmological parameters from the spherically averaged redshift-space
correlation function of the CMASS Data Release 9 (DR9) sample of the Baryonic …
correlation function of the CMASS Data Release 9 (DR9) sample of the Baryonic …
The clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: including covariance matrix errors
… matrix as given by the extra factor in m 2 compared with m 1 . In this plot, the factor m 1 is
the ratio between the dashed and dot–dashed lines, and m 2 is the ratio between the dotted …
the ratio between the dashed and dot–dashed lines, and m 2 is the ratio between the dotted …
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogues for cosmological analysis
We present large-scale structure catalogues from the completed extended Baryon Oscillation
Spectroscopic Survey (eBOSS). Derived from Sloan Digital Sky Survey (SDSS) IV Data …
Spectroscopic Survey (eBOSS). Derived from Sloan Digital Sky Survey (SDSS) IV Data …
High prevalence of dysfibrinogenemia among patients with chronic thromboembolic pulmonary hypertension
…, JJ Marsh, PG Chiles, MM Magaña… - Blood, The Journal …, 2009 - ashpublications.org
The mechanism by which chronic thromboembolic pulmonary hypertension (CTEPH) develops
after acute pulmonary thromboembolism is unknown. We previously reported that fibrin …
after acute pulmonary thromboembolism is unknown. We previously reported that fibrin …
Nonlinear model predictive control of a point absorber wave energy converter
M Richter, ME Magana, O Sawodny… - IEEE Transactions on …, 2012 - ieeexplore.ieee.org
This paper presents the application of nonlinear model predictive control (NMPC) to a point
absorber wave energy converter (WEC). Model predictive control (MPC) is generally a …
absorber wave energy converter (WEC). Model predictive control (MPC) is generally a …
The clustering of galaxies in the SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: constraints on primordial non-Gaussianity
… (2012), which assumed a flat geometry with Ω m = 0.274, but we adopt a flat geometry
with Ω m = 0.285 as our fiducial cosmology. In order to account for the difference, we assume …
with Ω m = 0.285 as our fiducial cosmology. In order to account for the difference, we assume …