19 results on '"K Gendreau"'
Search Results
2. NGC 300 ULX1: spin evolution, super-Eddington accretion, and outflows
- Author
-
G Vasilopoulos, M Petropoulou, F Koliopanos, P S Ray, C B Bailyn, F Haberl, and K Gendreau
- Published
- 2019
- Full Text
- View/download PDF
3. X-ray Quasi-Periodic Eruptions from Two Previously Quiescent Galaxies
- Author
-
R Arcodia, A Merloni, K Nandra, J Buchner, M Salvato, D Pasham, R Remillard, J Comparat, G Lamer, G Ponti, A Malyali, J Wolf, Z Arzoumanian, D Bogensberger, D A H Buckley, K Gendreau, M Gromadzki, E Kara, M Krumpe, C Markwardt, M E Ramos-Ceja, A Rau, M Schramm, and A Schwope
- Subjects
Lunar And Planetary Science And Exploration - Abstract
Quasi-Periodic Eruptions (QPEs) are extreme high-amplitude bursts of X-ray radiation recurring every few hours and originating near the central supermassive black holes in galactic nuclei. It is currently unknown what triggers these events, how long they last and how they are connected to the physical properties of the inner accretion flows. Previously, only two such sources were known, found either serendipitously or in archival data, with emission lines in their optical spectra classifying their nuclei as hosting an actively accreting supermassive black hole. Here we present the detection of QPEs in two further galaxies, obtained with a blind and systematic search over half of the X-ray sky. The optical spectra of these galaxies show no signature of black hole activity, indicating that a pre-existing accretion flow typical of active nuclei is not required to trigger these events. Indeed, the periods, amplitudes and profiles of the newly discovered QPEs are inconsistent with current models that invoke radiation-pressure driven accretion disk instabilities. Instead, QPEs might be driven by an orbiting compact object. Furthermore, their observed properties require the mass of the secondary object to be much smaller than the main body and future X-ray observations may constrain possible changes in the period due to orbital evolution. This scenario could make QPEs a viable candidate for the electromagnetic counterparts of the so-called extreme mass ratio inspirals, with considerable implications for multi-messenger astrophysics and cosmology.
- Published
- 2021
- Full Text
- View/download PDF
4. A NICER View of a Highly Absorbed Flare in GRS 1915+105
- Author
-
J. Neilsen, Jeroen Homan, J. F. Steiner, G. Marcel, E. Cackett, R. A. Remillard, and K. Gendreau
- Subjects
Astronomy ,Astrophysics - Abstract
After 26 yr in outburst, the black hole X-ray binary GRS 1915+105 dimmed considerably in early 2018; its flux dropped sharply in mid-2019, and it has remained faint ever since. This faint period, the "obscured state," is punctuated by occasional X-ray flares, many of which have been observed by NICER as part of our regular monitoring program. Here we present detailed time-resolved spectroscopy of one bright flare, whose spectrum shows evidence of high column density partial covering absorption and extremely deep absorption lines (equivalent widths over 100 eV in some cases). We study the time-dependent ionization of the obscuring gas with xstar, ultimately attributing the absorption to a radially stratified absorber of density ∼10^(12)–10^(13) per cu.cm at ∼few ×10^(11) cm from the black hole. We argue that a vertically extended outer disk could explain this obscuration. We discuss several scenarios to explain the obscured state, including massive outflows, an increase in the mass accretion rate, and changes in the outer disk that herald the approach of quiescence, but none are entirely satisfactory. Alternative explanations, such as obscuration by the accretion stream impact point, may be testable with current or future data.
- Published
- 2020
- Full Text
- View/download PDF
5. A NICER Look at Strong X-ray Obscuration in the Seyfert-2 Galaxy NGC 4388
- Author
-
J M Miller, E Kammoun, R M Ludlam, K Gendreau, Z Arzoumanian, E Cackett, and F Tombesi
- Subjects
Astrophysics - Abstract
We present an analysis of the time-averaged spectrum of the Seyfert-2 active galaxy NGC 4388, obtained by NICER. The intrinsic strength of the reflection spectrum in NGC 4388, the large collecting area and favorable passband of NICER, and a net exposure of 105.6 ks yielded an exceptionally sensitive spectrum. Using two independent families of models, the intrinsic spectrum from the central engine is found to be highly obscured but not Compton-thick. Enforcing physical self-consistency within each model, the independent treatments give formally consistent results: = - N 2.67+ 10 cm- H 0.030.02 23 2 or = ´ -N 2.64+ 10 cm- H 0.03 0.03 23 2. Past measurements made with Suzaku and XMM-Newton are in broad agreement with these column density values. A more recent measurement with NuSTAR (in late 2013) recorded a column density about twice as large; the robustness of this variability is reinforced by the use of consistent models and procedures. The neutral FeKα line in the NICER spectrum is nominally resolved and consistent with an origin in the optical broad-line region). The data also require ionized absorption in the Fe K band, similar to the “warm absorbers” detected in Seyfert-1 active galactic nuclei. The low-energy spectrum is consistent with a set of ionized plasma components. We discuss these findings and note that the geometric inferences that derive from this analysis can be tested with XRISM and Athena.
- Published
- 2019
- Full Text
- View/download PDF
6. Impact of COVID-19 on Patient-Provider Communication in Critical Care: Case Reports
- Author
-
Stephanie J. Scibilia, Sarah K. Gendreau, Rachel Toran Towbin, and Mary Beth Happ
- Subjects
Intensive Care Units ,Critical Care ,Communication ,Critical Illness ,COVID-19 ,Humans ,General Medicine ,Critical Care Nursing ,Pandemics - Abstract
Introduction Communication impairment during mechanical ventilation and prolonged critical illness is extremely frustrating and frightening for patients and increases the risk for miscommunication, misinterpretation, and poor outcomes. The COVID-19 pandemic amplified patient communication impairment in intensive care units. This article presents 3 case examples from the experience of a team of hospital-based speech-language pathologists providing augmentative and alternative communication support resources and services to intensive care unit patients treated for COVID-19 during the first wave of the pandemic. Cases were selected to illustrate the protracted and complex in-hospital and rehabilitative recovery of critically ill patients with COVID-19, necessitating creative problem-solving and nursing collaborations with speech-language pathologists to support patient-provider communication. Clinical Findings The cases demonstrate (1) increased need for bilingual communication resources, (2) impaired cognitive and motor function associated with a variety of post–COVID-19 sequelae including severe critical illness myopathy, and (3) delayed transition to a speaking valve due to the secretion burden. Diagnoses COVID-19 and acute respiratory distress syndrome (all), cerebral microhemorrhage, multi-system organ failure, hypoxic brain injury, altered mental status, seizure, stroke. Interventions Multimodal and progressive augmentative and alternative communication interventions included low-technology strategies and simple communication boards, video language interpretation, tracheostomy speaking strategies, and a video intercom system. Outcomes All patients made progressive gains in communication ability. Conclusion Evaluation by augmentative and alternative communication specialists and progressive intervention from speech-language pathologists in collaboration with intensive care unit nurses can greatly improve patient-provider communication during treatment for and recovery from COVID-19 and other prolonged critical illnesses.
- Published
- 2022
7. Magnetar spin-down glitch clearing the way for FRB-like bursts and a pulsed radio episode
- Author
-
G. Younes, M. G. Baring, A. K. Harding, T. Enoto, Z. Wadiasingh, A. B. Pearlman, W. C. G. Ho, S. Guillot, Z. Arzoumanian, A. Borghese, K. Gendreau, E. Göğüş, T. Güver, A. J. van der Horst, C.-P. Hu, G. K. Jaisawal, C. Kouveliotou, L. Lin, and W. A. Majid
- Subjects
High Energy Astrophysical Phenomena (astro-ph.HE) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
Magnetars are a special subset of the isolated neutron star family, with X-ray and radio emission mainly powered by the decay of their immense magnetic fields. Many attributes of magnetars remain poorly understood: spin-down glitches or the sudden reductions in the star's angular momentum, radio bursts reminiscent of extra-galactic Fast Radio Bursts (FRBs), and transient pulsed radio emission lasting months to years. Here we unveil the detection of a large spin-down glitch event ($|\Delta\nu/\nu| = 5.8_{-1.6}^{+2.6}\times10^{-6}$) from the magnetar SGR~1935+2154 on 2020 October 5 (+/- 1 day). We find no change to the source persistent surface thermal or magnetospheric X-ray behavior, nor is there evidence of strong X-ray bursting activity. Yet, in the subsequent days, the magnetar emitted three FRB-like radio bursts followed by a month long episode of pulsed radio emission. Given the rarity of spin-down glitches and radio signals from magnetars, their approximate synchronicity suggests an association, providing pivotal clues to their origin and triggering mechanisms, with ramifications to the broader magnetar and FRB populations. We postulate that impulsive crustal plasma shedding close to the magnetic pole generates a wind that combs out magnetic field lines, rapidly reducing the star's angular momentum, while temporarily altering the magnetospheric field geometry to permit the pair creation needed to precipitate radio emission., Comment: 51 pages, 3 tables, 8 figures. Accepted for publication in Nature Astronomy
- Published
- 2022
- Full Text
- View/download PDF
8. NICER Monitoring of Supersoft X-Ray Sources
- Author
-
M. Orio, K. Gendreau, M. Giese, G. J. M. Luna, J. Magdolen, S. Pei, B. Sun, E. Behar, A. Dobrotka, J. Mikolajewska, Dheeraj R. Pasham, and T. E. Strohmayer
- Subjects
High Energy Astrophysical Phenomena (astro-ph.HE) ,Space and Planetary Science ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We monitored four supersoft sources - two persistent ones, CAL 83 and MR Vel, and the recent novae YZ Ret (Nova Ret 2020) and V1674 Her (Nova Her 2021) - with NICER. The two persistent SSS were observed with unvaried X-ray flux level and spectrum, respectively, 13 and 20 years after the last observations. Short period modulations of the supersoft X-ray source (SSS) appear where the spectrum of the luminous central source was fully visibl (in CAL 83 and V1674 Her) and were absent in YZ Ret and MR Vel, in which the flux originated in photoionized or shocked plasma, while the white dwarf (WD) was not observable. We thus suggest that the pulsations occur on, or very close to, the WD surface. The pulsations of CAL 83 were almost unvaried after 15 years, including an irregular drift of the $\simeq$67 s period by 2.1 s. Simulations, including previous XMM-Newton data, indicate actual variations in period length within hours, rather than an artifact of the variable amplitude of the pulsations. Large amplitude pulsations with a period of 501.53$\pm$0.30 s were always detected in V1674 Her, as long as the SSS was observable. This period seems to be due to rotation of a highly magnetized WD.We cannot confirm the maximum effective temperature of ($\simeq$145,000 K) previously inferred for this nova, and discuss the difficulty in interpreting its spectrum. The WD appears to present two surface zones, one of which does not emit SSS flux., in press in the Astrophysical Journal
- Published
- 2022
- Full Text
- View/download PDF
9. 310: Association Between Carbohydrate Intake and Serum Lipids
- Author
-
YouFu Li, David E. Chiriboga, Ira S. Ockene, Andrea R. Hafner, K Gendreau, Barbara C. Olendzki, Yunsheng Ma, and Wenjun Li
- Subjects
medicine.medical_specialty ,Endocrinology ,Epidemiology ,business.industry ,Internal medicine ,medicine ,Blood lipids ,business ,Carbohydrate intake - Published
- 2005
- Full Text
- View/download PDF
10. Influence of condensed gases on field emission and the performance of superconducting RF cavities
- Author
-
J. Sears, David Rubin, R. Noer, J. Kirchgessner, W. Hartung, Q.S. Shu, K. Gendreau, D. Moffat, and Hasan Padamsee
- Subjects
Materials science ,Niobium ,chemistry.chemical_element ,Particle accelerator ,Temperature cycling ,Electronic, Optical and Magnetic Materials ,law.invention ,Field electron emission ,Outgassing ,chemistry ,Electrical resistivity and conductivity ,law ,Physics::Accelerator Physics ,Electrical and Electronic Engineering ,Atomic physics ,Helium ,Microwave - Abstract
In a program to study the field emission (FE) and to improve the performance of one-cell 1500-MHz superconducting Nb microwave particle accelerator cavities, the authors recently achieved peak surface fields as high as 51 MV/m through the use of 1200 degrees C UHV annealing, methanol rinsing, and high-power He processing. Performance is limited by excess FE from localized points on the cavity walls. Cycling of these cavities to room temperature and admission of He processing gas frequently produce large changes in Q correlating with the appearance or disappearance of the dominant field emitter, suggesting that condensed residual and impurity gases play a significant role in enhancing FE. By intentionally condensing O/sub 2/ into a cold cavity, the authors have produced similar effects, increasing the dissipated power and reducing Q, each by an order of magnitude at the same field level. Preliminary tests have also been carried out with H/sub 2/ and water vapor. These results suggest that improvements in the outgassing and vacuum environment of these cavities may be important. >
- Published
- 1989
- Full Text
- View/download PDF
11. A Persistent Disk Wind in GRS 1915+105 with NICER.
- Author
-
J. Neilsen, E. Cackett, R. A. Remillard, J. Homan, J. F. Steiner, K. Gendreau, Z. Arzoumanian, G. Prigozhin, B. LaMarr, J. Doty, S. Eikenberry, F. Tombesi, R. Ludlam, E. Kara, D. Altamirano, and A. C. Fabian
- Published
- 2018
- Full Text
- View/download PDF
12. A NICER Spectrum of MAXI J1535–571: Near-maximal Black Hole Spin and Potential Disk Warping.
- Author
-
J. M. Miller, K. Gendreau, R. M. Ludlam, A. C. Fabian, D. Altamirano, Z. Arzoumanian, P. M. Bult, E. M. Cackett, J. Homan, E. Kara, J. Neilsen, R. A. Remillard, and F. Tombesi
- Published
- 2018
- Full Text
- View/download PDF
13. Quasi-periodic X-ray eruptions years after a nearby tidal disruption event.
- Author
-
Nicholl M, Pasham DR, Mummery A, Guolo M, Gendreau K, Dewangan GC, Ferrara EC, Remillard R, Bonnerot C, Chakraborty J, Hajela A, Dhillon VS, Gillan AF, Greenwood J, Huber ME, Janiuk A, Salvesen G, van Velzen S, Aamer A, Alexander KD, Angus CR, Arzoumanian Z, Auchettl K, Berger E, de Boer T, Cendes Y, Chambers KC, Chen TW, Chornock R, Fulton MD, Gao H, Gillanders JH, Gomez S, Gompertz BP, Fabian AC, Herman J, Ingram A, Kara E, Laskar T, Lawrence A, Lin CC, Lowe TB, Magnier EA, Margutti R, McGee SL, Minguez P, Moore T, Nathan E, Oates SR, Patra KC, Ramsden P, Ravi V, Ridley EJ, Sheng X, Smartt SJ, Smith KW, Srivastav S, Stein R, Stevance HF, Turner SGD, Wainscoat RJ, Weston J, Wevers T, and Young DR
- Abstract
Quasi-periodic eruptions (QPEs) are luminous bursts of soft X-rays from the nuclei of galaxies, repeating on timescales of hours to weeks
1-5 . The mechanism behind these rare systems is uncertain, but most theories involve accretion disks around supermassive black holes (SMBHs) undergoing instabilities6-8 or interacting with a stellar object in a close orbit9-11 . It has been suggested that this disk could be created when the SMBH disrupts a passing star8,11 , implying that many QPEs should be preceded by observable tidal disruption events (TDEs). Two known QPE sources show long-term decays in quiescent luminosity consistent with TDEs4,12 and two observed TDEs have exhibited X-ray flares consistent with individual eruptions13,14 . TDEs and QPEs also occur preferentially in similar galaxies15 . However, no confirmed repeating QPEs have been associated with a spectroscopically confirmed TDE or an optical TDE observed at peak brightness. Here we report the detection of nine X-ray QPEs with a mean recurrence time of approximately 48 h from AT2019qiz, a nearby and extensively studied optically selected TDE16 . We detect and model the X-ray, ultraviolet (UV) and optical emission from the accretion disk and show that an orbiting body colliding with this disk provides a plausible explanation for the QPEs., (© 2024. The Author(s).)- Published
- 2024
- Full Text
- View/download PDF
14. Characterization of a Modulated X-ray Source for Ion Mobility Spectrometry.
- Author
-
Reinecke T, Kenyon S, Gendreau K, and Clowers BH
- Subjects
- X-Rays, Explosive Agents analysis, Ion Mobility Spectrometry methods
- Abstract
As a highly deployed field instrument for the detection of narcotics, explosives, and chemical warfare agents, drift tube ion mobility spectrometry relies heavily upon the performance of the ionization source and mechanism of ion beam modulation. For this instrumental platform, ion chemistry plays a critical role in the performance of the instrument from a sensitivity and selectivity perspective; however, a range of instrumental components also occupy pivotal roles. Most notably, the mechanism of ion modulation or ion gating is a primary contributor to peak width in a drift tube ion mobility experiment. Unfortunately, physical ion gates rarely perform perfectly, and in addition to serving as physical impediments to ion transmission, their modulation also has undesirable field effects. Using a recently developed modulated, non-radioactive X-ray source, we detail the performance of an ion mobility spectrometry (IMS) system that is free of a gating structure and utilizes the pulsed nature of the modulated X-ray source (MXS) for both ion generation and initiation of the IMS experiment. After investigating the influence of pulse duration and spatial X-ray beam width on the analytical performance of the instrument, the possibility of using multiplexing with a shutterless system is explored. By increasing ion throughput, the observed multiplexing gain compared to a signal-averaged spectrum approaches the theoretical maximum and illustrates the capability of the MXS-IMS system to realize significant signal to noise improvements.
- Published
- 2022
- Full Text
- View/download PDF
15. Impact of COVID-19 on Patient-Provider Communication in Critical Care: Case Reports.
- Author
-
Scibilia SJ, Gendreau SK, Towbin RT, and Happ MB
- Subjects
- Communication, Critical Care, Critical Illness therapy, Humans, Intensive Care Units, Pandemics, COVID-19
- Abstract
Introduction: Communication impairment during mechanical ventilation and prolonged critical illness is extremely frustrating and frightening for patients and increases the risk for miscommunication, misinterpretation, and poor outcomes. The COVID-19 pandemic amplified patient communication impairment in intensive care units. This article presents 3 case examples from the experience of a team of hospital-based speech-language pathologists providing augmentative and alternative communication support resources and services to intensive care unit patients treated for COVID-19 during the first wave of the pandemic. Cases were selected to illustrate the protracted and complex in-hospital and rehabilitative recovery of critically ill patients with COVID-19, necessitating creative problem-solving and nursing collaborations with speech-language pathologists to support patient-provider communication., Clinical Findings: The cases demonstrate (1) increased need for bilingual communication resources, (2) impaired cognitive and motor function associated with a variety of post-COVID-19 sequelae including severe critical illness myopathy, and (3) delayed transition to a speaking valve due to the secretion burden., Diagnoses: COVID-19 and acute respiratory distress syndrome (all), cerebral microhemorrhage, multi-system organ failure, hypoxic brain injury, altered mental status, seizure, stroke., Interventions: Multimodal and progressive augmentative and alternative communication interventions included low-technology strategies and simple communication boards, video language interpretation, tracheostomy speaking strategies, and a video intercom system., Outcomes: All patients made progressive gains in communication ability., Conclusion: Evaluation by augmentative and alternative communication specialists and progressive intervention from speech-language pathologists in collaboration with intensive care unit nurses can greatly improve patient-provider communication during treatment for and recovery from COVID-19 and other prolonged critical illnesses., (©2022 American Association of Critical-Care Nurses.)
- Published
- 2022
- Full Text
- View/download PDF
16. X-ray quasi-periodic eruptions from two previously quiescent galaxies.
- Author
-
Arcodia R, Merloni A, Nandra K, Buchner J, Salvato M, Pasham D, Remillard R, Comparat J, Lamer G, Ponti G, Malyali A, Wolf J, Arzoumanian Z, Bogensberger D, Buckley DAH, Gendreau K, Gromadzki M, Kara E, Krumpe M, Markwardt C, Ramos-Ceja ME, Rau A, Schramm M, and Schwope A
- Abstract
Quasi-periodic eruptions (QPEs) are very-high-amplitude bursts of X-ray radiation recurring every few hours and originating near the central supermassive black holes of galactic nuclei
1,2 . It is currently unknown what triggers these events, how long they last and how they are connected to the physical properties of the inner accretion flows. Previously, only two such sources were known, found either serendipitously or in archival data1,2 , with emission lines in their optical spectra classifying their nuclei as hosting an actively accreting supermassive black hole3,4 . Here we report observations of QPEs in two further galaxies, obtained with a blind and systematic search of half of the X-ray sky. The optical spectra of these galaxies show no signature of black hole activity, indicating that a pre-existing accretion flow that is typical of active galactic nuclei is not required to trigger these events. Indeed, the periods, amplitudes and profiles of the QPEs reported here are inconsistent with current models that invoke radiation-pressure-driven instabilities in the accretion disk5-9 . Instead, QPEs might be driven by an orbiting compact object. Furthermore, their observed properties require the mass of the secondary object to be much smaller than that of the main body10 , and future X-ray observations may constrain possible changes in their period owing to orbital evolution. This model could make QPEs a viable candidate for the electromagnetic counterparts of so-called extreme-mass-ratio inspirals11-13 , with considerable implications for multi-messenger astrophysics and cosmology14,15 .- Published
- 2021
- Full Text
- View/download PDF
17. Stationary Computed Tomography for Space and other Resource-constrained Environments.
- Author
-
Cramer A, Hecla J, Wu D, Lai X, Boers T, Yang K, Moulton T, Kenyon S, Arzoumanian Z, Krull W, Gendreau K, and Gupta R
- Subjects
- Animals, Electrons, Humans, Phantoms, Imaging, Swine, X-Rays, Tomography, X-Ray Computed methods
- Abstract
Computed tomography (CT) is used to diagnose many emergent medical conditions, including stroke and traumatic brain injuries. Unfortunately, the size, weight, and expense of CT systems make them largely inaccessible for patients outside of major hospitals. We have designed a module containing multiple miniature x-ray sources that could allow for CT systems to be significantly lighter, smaller, and cheaper, and to operate without any moving parts. We have developed a novel photocathode-based x-ray source, created by depositing a thin film of magnesium on an electron multiplier. When illuminated by a UV LED, this photocathode emits a beam of electrons, with a beam current of up to 1 mA. The produced electrons are accelerated through a high voltage to a tungsten target. These sources are individually addressable and can be pulsed rapidly, through electronic control of the LEDs. Seven of these sources are housed together in a 17.5 degree arc within a custom vacuum manifold. A full ring of these modules could be used for CT imaging. By pulsing the sources in series, we are able to demonstrate x-ray tomosynthesis without any moving parts. With a clinical flat-panel detector, we demonstrate 3D acquisition and reconstructions of a cadaver swine lung.
- Published
- 2018
- Full Text
- View/download PDF
18. Association between dietary carbohydrates and body weight.
- Author
-
Ma Y, Olendzki B, Chiriboga D, Hebert JR, Li Y, Li W, Campbell M, Gendreau K, and Ockene IS
- Subjects
- Adult, Age Factors, Aged, Diet Surveys, Energy Intake, Exercise, Female, Glycemic Index, Humans, Longitudinal Studies, Male, Middle Aged, Sex Factors, Body Mass Index, Body Weight, Dietary Carbohydrates administration & dosage
- Abstract
The role of dietary carbohydrates in weight loss has received considerable attention in light of the current obesity epidemic. The authors investigated the association of body mass index (weight (kg)/height (m)(2)) with dietary intake of carbohydrates and with measures of the induced glycemic response, using data from an observational study of 572 healthy adults in central Massachusetts. Anthropometric measurements, 7-day dietary recalls, and physical activity recalls were collected quarterly from each subject throughout a 1-year study period. Data were collected between 1994 and 1998. Longitudinal analyses were conducted, and results were adjusted for other factors related to body habitus. Average body mass index was 27.4 kg/m(2) (standard deviation, 5.5), while the average percentage of calories from carbohydrates was 44.9 (standard deviation, 9.6). Mean daily dietary glycemic index was 81.7 (standard deviation, 5.5), and glycemic load was 197.8 (standard deviation, 105.2). Body mass index was found to be positively associated with glycemic index, a measure of the glycemic response associated with ingesting different types of carbohydrates, but not with daily carbohydrate intake, percentage of calories from carbohydrates, or glycemic load. Results suggest that the type of carbohydrate may be related to body weight. However, further research is required to elucidate this association and its implications for weight management.
- Published
- 2005
- Full Text
- View/download PDF
19. Evaluation of a guinea pig model to assess interference in the immunogenicity of different components of a combination vaccine comprising diphtheria, tetanus and acellular pertussis (DTaP) vaccine and haemophilus influenzae type b capsular polysaccharide conjugate vaccine.
- Author
-
Gupta RK, Anderson R, Cecchini D, Rost B, Xu J, Gendreau K, Saroff DL, Marchant C, and Siber GR
- Subjects
- Animals, Bacterial Capsules, Diphtheria-Tetanus-acellular Pertussis Vaccines, Disease Models, Animal, Drug Interactions, Guinea Pigs, Humans, Mice, Polysaccharides, Bacterial biosynthesis, Diphtheria-Tetanus-Pertussis Vaccine immunology, Haemophilus Vaccines immunology, Polysaccharides, Bacterial immunology, Vaccines, Combined immunology
- Abstract
A guinea pig model to assess the immunogenicity of a combination vaccine containing diphtheria, tetanus and acellular pertussis (DTaP) vaccine and Haemophilus influenzae type b (Hib) capsular polysaccharide conjugated to tetanus toxoid (HibT) was evaluated comparatively with the mouse immunogenicity test to study the effect of combining these antigens on the immunogenicity of various components. The immunogenicity test in mice was performed by subcutaneous injection of groups of 10 animals twice at an interval of four weeks with 1/10 of a single human dose of various formulations of combination vaccines, DTaP or HibT vaccine. The animals were bled at 4 and 6 weeks and IgG or total antibodies to various components were determined by ELISA or RIA. The guinea pig immunogenicity model included groups of animals injected subcutaneously twice at an interval of six weeks with 1.5 times the single human dose of various formulations. The animals were bled at 4, 6 and 8 weeks and serum samples were tested for antibodies to various components by ELISA, RIA and/or neutralization tests. Additionally, potency of tetanus and diphtheria components was assessed as per the US Food and Drug Administration's regulations. Aluminium phosphate (AIPO(4)) adsorbed HibT vaccine or HibT as a combination with AIPO(4)adsorbed DTaP vaccine showed significant increases in IgG antibodies to tetanus toxin in mice as well increased tetanus antitoxin levels in guinea pigs as compared to soluble HibT vaccine. In general, combining DTaP and HibT vaccines did not affect the antibody levels to tetanus and diphtheria toxoids whereas DTaP-HibT combination vaccine elicited significantly lower IgG antibodies to pertussis toxin and filamentous haemagglutinin than DTaP vaccine alone, particularly after first injection. Mice showed similar Hib antibody responses for the combination and HibT alone whereas guinea pigs consistently showed lower anamnestic responses to Hib for combination formulations than for HibT alone. Reducing the amount of HibT and/or tetanus toxoid in the combination formulations reduced this suppression of Hib antibody response in guinea pigs. Suppression of Hib antibody response in combination vaccines has also been reported from recent clinical trials. Based on the results from this study, it appears that the guinea pig model may be able to predict the human response to various components of combination vaccines., (Copyright 1999 The International Association for Biologicals.)
- Published
- 1999
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.