Concurrent homozygous sickle‐cell disease and severe haemophilia A: Thromboelastography profiles

Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/148348/1/hae13692_am.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/148348/2/hae13692.pd

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.Comment: Replaced with published version. Added journal reference and DO

Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI. Supplemental material in the ancillary file

Utility of thromboelastography for the diagnosis of von Willebrand disease

Von Willebrand disease (VWD) is an inherited bleeding disorder that is caused by a quantitative or qualitative deficiency of von Willebrand factor (VWF). The National Heart, Lung, and Blood Institute (NHLBI) guidelines for the diagnosis of VWD state that a VWF activity (VWF:RCo) of <30 IU/dL or <50 IU/dL with symptoms of clinical bleeding are consistent with the diagnosis of VWD. However, current gold‐standard diagnostic testing takes days to have complete results. Thromboelastography (TEG) is a testing method that provides a graphical trace that represents the viscoelastic changes seen with fibrin polymerization in whole blood, therefore providing information on all phases of the coagulation process. This study describes the TEG characteristics in 160 patients who presented for workup of a bleeding disorder and a subset of those were subsequently diagnosed with VWD. The TEG parameters, K‐time (representing the dynamics of clot formation) and the maximal rate of thrombus generation (MRTG), were found to be sensitive in detecting patients with VWF:RCo <30 IU/dL. The TEG, unlike VWF:RCo, can be done in real time, and results are available to the clinician within an hour. This will definitely be beneficial in acute situations such as evaluation of and management of acute bleeding in patients with acquired deficiencies of VWF and may play an important role in the surgical management of patients with VWD.Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/149222/1/pbc27714_am.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/149222/2/pbc27714.pd

Utility of thromboelastography for the diagnosis of von Willebrand disease

Von Willebrand disease (VWD) is an inherited bleeding disorder that is caused by a quantitative or qualitative deficiency of von Willebrand factor (VWF). The National Heart, Lung, and Blood Institute (NHLBI) guidelines for the diagnosis of VWD state that a VWF activity (VWF:RCo) of <30 IU/dL or <50 IU/dL with symptoms of clinical bleeding are consistent with the diagnosis of VWD. However, current gold‐standard diagnostic testing takes days to have complete results. Thromboelastography (TEG) is a testing method that provides a graphical trace that represents the viscoelastic changes seen with fibrin polymerization in whole blood, therefore providing information on all phases of the coagulation process. This study describes the TEG characteristics in 160 patients who presented for workup of a bleeding disorder and a subset of those were subsequently diagnosed with VWD. The TEG parameters, K‐time (representing the dynamics of clot formation) and the maximal rate of thrombus generation (MRTG), were found to be sensitive in detecting patients with VWF:RCo <30 IU/dL. The TEG, unlike VWF:RCo, can be done in real time, and results are available to the clinician within an hour. This will definitely be beneficial in acute situations such as evaluation of and management of acute bleeding in patients with acquired deficiencies of VWF and may play an important role in the surgical management of patients with VWD.Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/149222/1/pbc27714_am.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/149222/2/pbc27714.pd