10 research outputs found
Incidence and duration of total occlusion of the radial artery in newborn infants after catheter removal
- Author
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 01/01/1990
- Field of study
The incidence and duration of total occlusion of the radial artery after catheter removal was determined using repeated Doppler flow measurements. Thirty-two newborn infants with birthweights ranging from 945 g to 3890 g (median 1935 g) and gestational age ranging from 26 to 40 weeks (median 32 weeks) were studied. In 20 out of 32 infants (63%), complete occlusion of the radial artery occurred. The number of occlusions were not related to birthweight, gestational age or duration of cannulation. In all infants, blood flow in the radial artery resumed within 1-29 days after catheter removal. The duration of occlusion was directly related to the duration of cannulation and inversely related to birthweight. This study demonstrates a high frequency of total occlusion of the radial artery in newborn infants after percutaneous radial artery cannulation. In the majority of infants with a radial artert catheter, blood flow to the tissue distal to the cannulation site is dependent solely on the existence of an adequate arterial palmar collateral circulation
Recommended from our members
Toward an improved representation of middle atmospheric dynamics thanks to the ARISE project
- Author
- A Camara de la
- A Camara de la
- A Charlton
- A Hauchecorne
- A Hauchecorne
- A Hertzog
- A Hertzog
- A Pichon Le
- A Pichon Le
- A Pichon Le
- A Pichon Le
- A Pichon Le
- A Pichon Le
- A Pichon Le
- A Pichon Le
- A. Charlton-Perez
- A. Hauchecorne
- A. Le Pichon
- AJ Charlton-Perez
- AJ Charlton-Perez
- AJ Prata
- AK Smith
- AL Dabrowa
- B Bilitza
- C Bonadonna
- C Caudron
- C Claud
- C Millet
- C Pilger
- C Pilger
- C. F. Lee
- C. Millet
- C. Pilger
- CJ Wright
- CL Silva Da
- D Drob
- D Fee
- D Rind
- D Rind
- D Rind
- D Tailpied
- DC Fritts
- DC Fritts
- DD Sentman
- DJ Cecil
- DL Wu
- DN Green
- DP Drob
- DP Drob
- DWJ Thompson
- E Blanc
- E Blanc
- E Blanc
- E Blanc
- E Manzini
- E Marchetti
- E Marchetti
- E Marchetti
- E. Blanc
- E. Marchetti
- EP Gerber
- F Ardhuin
- F Ardhuin
- F Lefeuvre
- F Lott
- G Angot
- G Heinemann
- G Noer
- G Occhipinti
- G Ulivieri
- GJ Fishman
- HC Stenbaek-Nielsen
- HJ Christian
- IP Chunchuzov
- IP Chunchuzov
- J Artru
- J Artru
- J Chum
- J Chum
- J Lastovicka
- J Marty
- J Marty
- J Yue
- J. Chum
- J. D. Assink
- J. Kero
- J. Lastovicka
- JA Screen
- JB Orbaek
- JD Assink
- JD Assink
- JE Stopa
- JL Baray
- JM Lalande
- JR Holton
- JR Holton
- KW Hoppel
- L Costantino
- L Costantino
- L Goncharenko
- L Hoffmann
- L. Ceranna
- L. Eliasson
- L. G. Evers
- LG Evers
- LG Evers
- LJ Gallin
- LJ Liszka
- M Bertin
- M Diamantakis
- M Ern
- M Ern
- M Füllekrug
- M Garcés
- M Garcés
- M Landes
- M Ripepe
- M Rojo
- M Sigmond
- M. Ripepe
- MAH Hedlin
- MJ Alexander
- MJ Alexander
- MJ Alexander
- ML Chanin
- MP Baldwin
- MP Baldwin
- MP Hickey
- N Butchart
- N Mze
- N. B. Crosby
- N. Brachet
- N. Kämpfer
- N. Mze
- P Keckhut
- P Keckhut
- P. Blanc-Benon
- P. Heinrich
- P. J. Espy
- P. Keckhut
- P. S. M. Smets
- PSM Smets
- PSM Smets
- R Arechiga
- R Plougonven
- R Rüfenacht
- R. E. Hibbins
- R. Rüfenacht
- RA Vincent
- RD Ray
- RJ Wit de
- RJ Wit de
- RS Lindzen
- RS Matoza
- RS Matoza
- S Khaykin
- S Larquier de
- S. J. Gibbons
- S. Khaykin
- S. P. Näsholm
- SH Francis
- SJ Gibbons
- SM Khaykin
- SN Kulichkov
- T Dunkerton
- T Farges
- T Farges
- T Farges
- T Neubert
- T Neubert
- T Sindelarova
- T. Farges
- T. Kvaerna
- T. Sindelarova
- TA Shaw
- TA Shaw
- V Ramaswamy
- W Randel
- WK Hocking
- WL Donn
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 01/01/2018
- Field of study
This paper reviews recent progress toward understanding the dynamics of the middle atmosphere in the framework of the Atmospheric Dynamics Research InfraStructure in Europe (ARISE) initiative. The middle atmosphere, integrating the stratosphere and mesosphere, is a crucial region which influences tropospheric weather and climate. Enhancing the understanding of middle atmosphere dynamics requires improved measurement of the propagation and breaking of planetary and gravity waves originating in the lowest levels of the atmosphere. Inter-comparison studies have shown large discrepancies between observations and models, especially during unresolved disturbances such as sudden stratospheric warmings for which model accuracy is poorer due to a lack of observational constraints. Correctly predicting the variability of the middle atmosphere can lead to improvements in tropospheric weather forecasts on timescales of weeks to season. The ARISE project integrates different station networks providing observations from ground to the lower thermosphere, including the infrasound system developed for the Comprehensive Nuclear-Test-Ban Treaty verification, the Lidar Network for the Detection of Atmospheric Composition Change, complementary meteor radars, wind radiometers, ionospheric sounders and satellites. This paper presents several examples which show how multi-instrument observations can provide a better description of the vertical dynamics structure of the middle atmosphere, especially during large disturbances such as gravity waves activity and stratospheric warming events. The paper then demonstrates the interest of ARISE data in data assimilation for weather forecasting and re-analyzes the determination of dynamics evolution with climate change and the monitoring of atmospheric extreme events which have an atmospheric signature, such as thunderstorms or volcanic eruptions
Catheterization of posterior tibial artery leading to limb amputation
- Publication venue
- 'Wiley'
- Publication date
- Field of study
Radial artery blood pressure measurement in neonates: an accurate and convenient technique in clinical practice
- Author
- Publication venue
- 'Walter de Gruyter GmbH'
- Publication date
- Field of study
Seasonal variation in nitrate reductase activity and protein content in response to growth in transplanted trees at Fisher forest and Lion safari of U.P.
- Author
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- Field of study
Incidence and duration of total occlusion of the radial artery in newborn infants after catheter removal
- Author
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- Field of study
An Efficient 3-D Model for Global Circulation, Transport and Chemistry
- Author
- A Bott
- A Bucholtz
- A Slingo
- A Stohl
- AD Moura
- AH Oort
- AI Prados
- BA Boville
- BP Briegleb
- C Granier
- CB Leovy
- CE Johnson
- CM Spivakovsky
- DG Andrews
- DJ Allen
- DJ Jacob
- DJ Wuebbles
- DJ Wuebbles
- DL Baulch
- DL Baulch
- DM Cunnold
- DM Cunnold
- DR Legates
- DR Legates
- EL Fleming
- EN Lorenz
- EP Olaguer
- G Brasseur
- G Pitari
- GR Carmichael
- H Singh
- HB Singh
- HL Kuo
- I Fung
- J Lelieveld
- J Olson
- J Rudolph
- JA Logan
- JF Louis
- JGJ Olivier
- JL Stanford
- JM Prospero
- JM Roberts
- JP Peixoto
- JR Holton
- JR Holton
- JR Holton
- JR Holton
- JS Fuglestvedt
- JT Kiehl
- KH Rosenlof
- LJ Gray
- LJ Gray
- M Allen
- MA Geller
- ME McIntyre
- MG Schultz
- MW Gery
- NA McFarlane
- NM Donahue
- R Atkinson
- R Atkinson
- R Toumi
- RB Chatfield
- RD Martinez
- RE Newell
- RJ Reed
- RP Turco
- RP Wayne
- RR Garcia
- RR Garcia
- RS Lindzen
- S Houweling
- S Manabe
- SA McKeen
- SB Fels
- SN Pandis
- T Matsuno
- TA Staffelbach
- TJ Dunkerton
- UE Willie
- VI Fomichev
- W Zhong
- WB More
- WJ Randel
- World Meteorological Organization Atmospheric ozone
- World Meteorological Organization Scientific assessment of ozone depletion
- WR Stockwell
- Y Jiang
- Y Li
- Y Wang
- Y Wang
- Y Wang
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 01/01/2002
- Field of study
Recommended from our members
Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo
- Author
- Abac AG
- Abbott R
- Abe H
- Acernese F
- Ackley K
- Adamcewicz C
- Adhicary S
- Adhikari N
- Adhikari RX
- Adkins VK
- Adya VB
- Affeldt C
- Agarwal D
- Agathos M
- Aguiar OD
- Aguilar I
- Aiello L
- Ain A
- Ajith P
- Akutsu T
- Al-Jodah A
- Albanesi S
- Alfaidi RA
- Allocca A
- Alléné C
- Almualla M
- Altin PA
- Amato A
- Amez-Droz L
- Amorosi A
- Anand S
- Ananyeva A
- Andersen R
- Anderson SB
- Anderson WG
- Andia M
- Ando M
- Andrade T
- Andres N
- Andrić T
- Andrés-Carcasona M
- Ansoldi S
- Antelis JM
- Antier S
- Aoumi M
- Apostolatos T
- Appavuravther EZ
- Appert S
- Apple SK
- Arai K
- Araya A
- Araya MC
- Areeda JS
- Arellano FE Peña
- Aritomi N
- Armato F
- Arnaud N
- Arogeti M
- Aronson SM
- Arun KG
- Ashton G
- Aso Y
- Assiduo M
- Aston SM
- Astone P
- Aubin F
- AultONeal K
- Babak S
- Badalyan A
- Badaracco F
- Badger C
- Bae S
- Bagnasco S
- Bai Y
- Baier JG
- Bajpai R
- Baka T
- Ball M
- Ballardin G
- Ballmer SW
- Baltus G
- Banagiri S
- Banerjee B
- Bankar D
- Baral P
- Barayoga JC
- Barber J
- Barish BC
- Barker D
- Barneo P
- Barone F
- Barr B
- Barsotti L
- Barsuglia M
- Barta D
- Barthelmy SD
- Barton MA
- Bartos I
- Basak S
- Basalaev A
- Bassiri R
- Basti A
- Bawaj M
- Baxi P
- Bayley JC
- Baylor AC
- Bazzan M
- Bedakihale VM
- Beirnaert F
- Bejger M
- Bell AS
- Benedetto V
- Beniwal D
- Benoit W
- Bentley JD
- Bera S
- Berbel M
- Bergamin F
- Berger BK
- Bernuzzi S
- Beroiz M
- Berry CPL
- Bersanetti D
- Bertolini A
- Betzwieser J
- Beveridge D
- Bevins N
- Bhandare R
- Bhandari AV
- Bhardwaj U
- Bhatt R
- Bhattacharjee D
- Bhaumik S
- Bianchi A
- Bilenko IA
- Bilicki M
- Billingsley G
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- Bini S
- Birnholtz O
- Biscans S
- Bischi M
- Biscoveanu S
- Bisht A
- Bitossi M
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- Boschi V
- Bose S
- Bossilkov V
- Boudart V
- Bozzi A
- Boër M
- Bradaschia C
- Brady PR
- Braglia M
- Branch A
- Branchesi M
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- Briant T
- Brillet A
- Brinkmann M
- Brockill P
- Brooks AF
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- Brunett S
- Bruno G
- Bruntz R
- Bryant J
- Bucci F
- Buchanan J
- Bulashenko O
- Bulik T
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- Buonanno A
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- Buskulic D
- Bustillo J Calderón
- Buy C
- Bécsy B
- Cabras G
- Cabrita R
- Cadonati L
- Cagnoli G
- Cahillane C
- Callaghan JD
- Callister TA
- Calloni E
- Camp JB
- Canepa M
- Cannavacciuolo M
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- Capocasa E
- Capote E
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- Cesarini E
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- Chan C
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- Chanial P
- Chao S
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- Charlton P
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- Chiang C
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- Chiofalo ML
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- Cieślar M
- Cifaldi M
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- Clesse S
- Cleva F
- Coccia E
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- Croquette M
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- Dall’Osso S
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- Dartez LP
- Dasgupta A
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- Dattilo V
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- Davier M
- Davies GS Cabourn
- Davis D
- Davis MC
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- Dax M
- De Laurentis M
- De Lillo F
- De Marco F
- De Matteis F
- De Pietri R
- De Rosa R
- De Rossi C
- De Simone R
- de Souza Melo S Assis
- Deenadayalan M
- Degallaix J
- Del Favero V
- Del Pozzo W
- Dell’Aquila D
- Deléglise S
- Demos N
- Dent T
- Depasse A
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- Di Fiore L
- Di Fronzo C
- Di Giovanni F
- Di Giovanni M
- Di Girolamo T
- Di Lieto A
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- Diab R
- Diamond PZ
- Diaz J Casanueva
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- Ding J
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- Doctor Z
- Dohmen E
- Doleva PP
- Donahue L
- Donovan F
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- Dooney T
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- Drago M
- Driggers JC
- Drori Y
- Du H
- Ducoin J-G
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- Dupletsa U
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- e Melo I Tosta
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- Effler A
- Eichholz J
- Einsle H
- Eisenmann M
- Eisenstein RA
- Ejlli A
- Engelby E
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- Essick RC
- Estellés H
- Estevez D
- Etzel T
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- Hsieh H-F
- Hsiung C
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- Hsu W-F
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- Hu Q
- Huang HY
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- Huang Y-J
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- Hui DCY
- Hui V
- Hur R
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- Hübner MT
- Iakovlev A
- Iandolo GA
- Iess A
- III HW Cain
- Inayoshi K
- Inoue Y
- Iorio G
- Iosif P
- Irwin J
- Isi M
- Ismail MA
- Itoh Y
- Iwaya M
- Iyer BR
- JaberianHamedan V
- Jacqmin T
- Jacquet P-E
- Jadhav SJ
- Jadhav SP
- Jain D
- Jain T
- James AL
- James PA
- Jamshidi R
- Jan AZ
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- Kapasi DP
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- Klimenko S
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- Wysocki DM
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- Yamamoto K
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- Yamamoto TS
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- Yang Y-C
- Yang Yang
- Yang Yi
- Yap MJ
- Yarbrough Z
- Yeh S-W
- Yelikar AB
- Yeung SMC
- Yeung TY
- Yokoyama J
- Yokozawa T
- Yoo J
- Yu H
- Yuzurihara H
- Zadrożny A
- Zannelli AJ
- Zanolin M
- Zeeshan M
- Zelenova T
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- Zevin M
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- Zhang Yanqi
- Zhao C
- Zhao Yue
- Zhao Yuhang
- Zheng Y
- Zhong H
- Zhou R
- Zhu Z-H
- Zimmerman AB
- Zucker ME
- Zweizig J
- Álvarez-López S
- Publication venue
- The Astrophysical Journal
- Publication date
- 04/10/2024
- Field of study
Abstract
Despite the growing number of binary black hole coalescences confidently observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include the effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that have already been identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total source-frame mass M > 70 M
⊙) binaries covering eccentricities up to 0.3 at 15 Hz emitted gravitational-wave frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place a conservative upper limit for the merger rate density of high-mass binaries with eccentricities 0 < e ≤ 0.3 at 16.9 Gpc−3 yr−1 at the 90% confidence level.</jats:p
Recommended from our members
Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO
- Author
- Abbott R
- Abe H
- Acernese F
- Ackley K
- Adhicary S
- Adhikari N
- Adhikari RX
- Adkins VK
- Adya VB
- Affeldt C
- Agarwal D
- Agathos M
- Aguiar OD
- Aiello L
- Ain A
- Ajith P
- Akutsu T
- Al-Jodah A
- Albanesi S
- Alfaidi RA
- Allocca A
- Alléné C
- Almualla M
- Altin PA
- Amato A
- Amez-Droz L
- Amorosi A
- Anand S
- Ananyeva A
- Andersen R
- Anderson SB
- Anderson WG
- Andia M
- Ando M
- Andrade T
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- Andrić T
- Andrés-Carcasona M
- Ansoldi S
- Antelis JM
- Antier S
- Aoumi M
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- Zweizig J
- Publication venue
- The Astrophysical Journal Supplement Series
- Publication date
- 22/08/2023
- Field of study
Abstract
The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.</jats:p
Recommended from our members
Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo
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- Wysocki DM
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- Yadav N
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- Yamamoto K
- Yamamoto M
- Yamamoto T
- Yamamoto TS
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- Yamazaki R
- Yan S
- Yang FW
- Yang KZ
- Yang L-C
- Yang Y-C
- Yang Yang
- Yang Yi
- Yap MJ
- Yarbrough Z
- Yeh S-W
- Yelikar AB
- Yeung SMC
- Yeung TY
- Yokoyama J
- Yokozawa T
- Yoo J
- Yu H
- Yuzurihara H
- Zadrożny A
- Zannelli AJ
- Zanolin M
- Zeeshan M
- Zelenova T
- Zendri J-P
- Zevin M
- Zhang J
- Zhang L
- Zhang R
- Zhang T
- Zhang Ya
- Zhang Yanqi
- Zhao C
- Zhao Yue
- Zhao Yuhang
- Zheng Y
- Zhong H
- Zhou R
- Zhu Z-H
- Zimmerman AB
- Zucker ME
- Zweizig J
- Álvarez-López S
- Publication venue
- The Astrophysical Journal
- Publication date
- 27/09/2024
- Field of study
Abstract
Despite the growing number of binary black hole coalescences confidently observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include the effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that have already been identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total source-frame mass M > 70 M
⊙) binaries covering eccentricities up to 0.3 at 15 Hz emitted gravitational-wave frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place a conservative upper limit for the merger rate density of high-mass binaries with eccentricities 0 < e ≤ 0.3 at 16.9 Gpc−3 yr−1 at the 90% confidence level.</jats:p