65 research outputs found
Rule-Based Cell Systems Model of Aging using Feedback Loop Motifs Mediated by Stress Responses
- Author
- A Alexander
- A Ben-Zvi
- A Bergman
- A Boveris
- A Kowald
- A Kowald
- A Kowald
- A Kriete
- A Kriete
- A Kriete
- A Navarro
- A Ramanathan
- A Sackmann
- A Sanz
- A Trifunovic
- AD de Grey
- AK Roy
- AL Alvers
- Andres Kriete
- AS Adler
- AS Adler
- B Bandy
- B Chance
- B Gerstbrein
- B Kosko
- B Mazumder
- B Onken
- BA Sokhansanj
- BA Sokhansanj
- BB Aldridge
- BB Aldridge
- BB Aldridge
- BS Berlett
- C Franceschi
- C Moraga
- C Soule
- CC Preston
- CH Yuh
- CJ Kenyon
- CJ Proctor
- CN Oliver
- CY Wang
- D Cristina
- D Harman
- D Steinsaltz
- DD Sarbassov
- DE Harrison
- DG Hardie
- DG Hardie
- DG Nicholls
- DJ Marcinek
- E Cevenini
- E Jeminez
- E Santini
- EA Shoubridge
- ED Smith
- EJ Brown
- EJ Lesnefsky
- EL Greer
- EM Crimmins
- ER Stadtman
- F Buttgereit
- F Robbesyn
- G Biswas
- G Rossolini
- G Sui
- GB West
- GB West
- GC Kujoth
- Glenn Booker
- GP Sykiotis
- H Bruunsgaard
- H de Jong
- H Wu
- H Xue
- HC Dan
- Herbert M. Sauro
- HF Kwok
- HM Sauro
- HR Warner
- I Luptak
- J Apfeld
- J Dong
- J Feret
- JD Mulligan
- JJ Pei
- JJ Tyson
- JK Park
- JM Zahn
- JM Zahn
- JP de Magalhaes
- JS Weitz
- JT Cunningham
- JW Shin
- JW Vaupel
- K Jaqaman
- K Khrapko
- K Kiselyov
- K Sachs
- KA Brand
- KA Janes
- KE Conley
- KE Conley
- KG Gadkar
- KS Echtay
- L Guarente
- L Zhuo
- LA Donehower
- LA Herndon
- M Brandfonbrener
- M Cloutier
- M D'Aurelio
- M Dajee
- M Greco
- M Helenius
- ME Sehl
- MI Aladjem
- MJ Munoz
- MK Shigenaga
- MM Sousa
- MP Duyao
- MT Lin
- MV Blagosklonny
- MV Miceli
- N Fedoroff
- N Friedman
- N Miyoshi
- N Sitte
- N Wiener
- NF Spencer
- NW Shock
- O Brandman
- P Du
- P Oberdoerffer
- PC Cogswell
- PC Supakar
- PF Chinnery
- PJW Y Woolf
- Q Zhang
- R Gunawan
- RA Butow
- RA Clark
- RS Balaban
- RS Sohal
- RS Sohal
- S Ghosh
- S Gonin-Giraud
- S Imoto
- S Marino
- S Welle
- SC Makrides
- SD Hursting
- SD Westerheide
- SM Jazwinski
- SM Schieke
- T Banno
- T Finkel
- T Finkel
- T Grune
- T Lu
- T Shioi
- T Toliver-Kinsky
- TB Kirkwood
- TJ Ross
- TL Kawahara
- VK Koltover
- W Wang
- William J. Bosl
- WJ Bosl
- Y Kamada
- Y Xu
- ZY Lu
- Publication venue
- Public Library of Science
- Publication date
- 01/01/2010
- Field of study
Investigating the complex systems dynamics of the aging process requires integration of a broad range of cellular processes describing damage and functional decline co-existing with adaptive and protective regulatory mechanisms. We evolve an integrated generic cell network to represent the connectivity of key cellular mechanisms structured into positive and negative feedback loop motifs centrally important for aging. The conceptual network is casted into a fuzzy-logic, hybrid-intelligent framework based on interaction rules assembled from a priori knowledge. Based upon a classical homeostatic representation of cellular energy metabolism, we first demonstrate how positive-feedback loops accelerate damage and decline consistent with a vicious cycle. This model is iteratively extended towards an adaptive response model by incorporating protective negative-feedback loop circuits. Time-lapse simulations of the adaptive response model uncover how transcriptional and translational changes, mediated by stress sensors NF-κB and mTOR, counteract accumulating damage and dysfunction by modulating mitochondrial respiration, metabolic fluxes, biosynthesis, and autophagy, crucial for cellular survival. The model allows consideration of lifespan optimization scenarios with respect to fitness criteria using a sensitivity analysis. Our work establishes a novel extendable and scalable computational approach capable to connect tractable molecular mechanisms with cellular network dynamics underlying the emerging aging phenotype
Time constraints on the tectonic evolution of the Eastern Sierras Pampeanas (Central Argentina)
- Author
- A Chincarini
- A Favetto
- A Guereschi
- A Guereschi
- A Guereschi
- A Lork
- A Pinan-Llamas
- A Steenken
- A Steenken
- A Steenken
- AD Huerta
- Alina Guereschi
- Andre Steenken
- BB Brito Neves
- BJA Willigers
- C Casquet
- C Simpson
- CE Gordillo
- CJ Adams
- CMA Powell
- CW Rapela
- CW Rapela
- CW Rapela
- CW Rapela
- CW Rapela
- EJ Llambías
- F Aceñolaza
- F Lucassen
- F Söllner
- FFM Almeida de
- G Franz
- GS Lister
- GW Wetherill
- IS Williams
- JA Dahlquist
- JD Keppie
- JDA Piper
- JE Otamendi
- JE Otamendi
- JE Otamendi
- JE Otamendi
- JE Otamendi
- JE Otamendi
- JG Meert
- JG Meert
- JJ Schwartz
- JJ Schwartz
- JR Booker
- Klaus Wemmer
- LC Silva da
- LP Black
- M Schaller
- MA Krol
- MAS Basei
- MG López de Luchi
- MG López de Luchi
- MG López de Luchi
- MM Pimentel
- MP Escayola
- MP Escayola
- Mónica G. López de Luchi
- P Ježek
- PA Cawood
- PA Cawood
- PC England
- PE Kraemer
- PR Leal
- PS Dahl
- PS Dahl
- R Frei
- R Frei
- R Lira
- R Scheepers
- R Unrug
- RA Jamieson
- RD Martino
- RD Martino
- RD Martino
- RD Martino
- RD Martino
- RD Martino
- RD Martino
- Robert Frei
- Roberto D. Martino
- S Kay
- Sergej Presnyakov
- Siegfried Siegesmund
- SJ Whitmeyer
- SL Baldwin
- UG Cordani
- VA Ramos
- VA Ramos
- VA Ramos
- VA Ramos
- W Barnett
- W Todt
- W YuanBao
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- Field of study
Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model
- Author
- Abbott Bp
- Abbott R
- Abbott Td
- Abraham S
- Acernese F
- Ackley K
- Adams C
- Adhikari Rx
- Adya Vb
- Affeldt C
- Agathos M
- Agatsuma K
- Aggarwal N
- Aguiar Od
- Aiello L
- Ain A
- Ajith P
- Allen G
- Allocca A
- Aloy Ma
- Altin Pa
- Amato A
- Anand S
- Ananyeva A
- Anderson Sb
- Anderson Wg
- Angelova Sv
- Antier S
- Appert S
- Arai K
- Araya Mc
- Areeda Js
- Arene M
- Arnaud N
- Aronson Sm
- Ascenzi S
- Ashton G
- Aston Sm
- Astone P
- Aubin F
- Aufmuth P
- AultONeal K
- Austin C
- Avendano V
- Avila-Alvarez A
- Babak S
- Bacon P
- Badaracco F
- Bader Mkm
- Bae S
- Baird J
- Baker Pt
- Baldaccini F
- Ballardin G
- Ballmer Sw
- Bals A
- Banagiri S
- Barayoga Jc
- Barbieri C
- Barclay Se
- Barish Bc
- Barker D
- Barkett K
- Barnum S
- Barone F
- Barr B
- Barsotti L
- Barsuglia M
- Barta D
- Bartlett J
- Bartos I
- Bassiri R
- Basti A
- Bawaj M
- Bayley Jc
- Bazzan M
- Becsy B
- Bejger M
- Belahcene I
- Bell As
- Beniwal D
- Benjamin Mg
- Berger Bk
- Bergmann G
- Bernuzzi S
- Berry Cpl
- Bersanetti D
- Bertolini A
- Betzwieser J
- Bhandare R
- Bidler J
- Biggs E
- Bilenko Ia
- Bilgili Sa
- Billingsley G
- Birney R
- Birnholtz O
- Biscans S
- Bischi M
- Biscoveanu S
- Bisht A
- Bitossi M
- Bizouard Ma
- Blackburn Jk
- Blackman J
- Blair Cd
- Blair Dg
- Blair Rm
- Bloemen S
- Bobba F
- Bode N
- Boer M
- Boetzel Y
- Bogaert G
- Bondu F
- Bonnand R
- Booker P
- Boom Ba
- Bork R
- Boschi V
- Bose S
- Bossilkov V
- Bosveld J
- Bouffanais Y
- Bozzi A
- Bradaschia C
- Brady Pr
- Bramley A
- Branchesi M
- Brau Je
- Breschi M
- Briant T
- Briggs Jh
- Brighenti F
- Brillet A
- Brinkmann M
- Brockill P
- Brooks Af
- Brooks J
- Brown Dd
- Brunett S
- Buikema A
- Bulik T
- Bulten Hj
- Buonanno A
- Buskulic D
- Bustillo Jc
- Buy C
- Byer Rl
- Cabero M
- Cadonati L
- Cagnoli G
- Cahillane C
- Callister Ta
- Calloni E
- Camp Jb
- Campbell Wa
- Cannon Kc
- Cao H
- Cao J
- Carapella G
- Carbognani F
- Caride S
- Carney Mf
- Carullo G
- Casentini C
- Castro Jmg
- Caudill S
- Cavaglia M
- Cavalier F
- Cavalieri R
- Cella G
- Cerda-Duran P
- Cesarini E
- Chaibi O
- Chakravarti K
- Chamberlin Sj
- Chan M
- Chao S
- Charlton P
- Chase Ea
- Chassande-Mottin E
- Chatterjee D
- Chaturvedi M
- Cheeseboro Bd
- Chen Hy
- Chen X
- Chen Y
- Cheng Hp
- Cheong Ck
- Chia Hy
- Chiadini F
- Chincarini A
- Chiummo A
- Cho G
- Cho Hs
- Cho M
- Christensen N
- Chu Q
- Chua S
- Chung Kw
- Chung S
- Ciani G
- Cieslar M
- Ciobanu Aa
- Ciolfi R
- Cipriano F
- Cirone A
- Clara F
- Clark Ja
- Clearwater P
- Cleva F
- Coccia E
- Cohadon Pf
- Cohen D
- Colleoni M
- Collette Cg
- Collins C
- Colpi M
- Cominsky Lr
- Constancio M
- Conti L
- Cooper Sj
- Corban P
- Corbitt Tr
- Cordero-Carrion I
- Corezzi S
- Corley Kr
- Cornish N
- Corre D
- Corsi A
- Cortese S
- Costa Ca
- Costa Cfd
- Cotesta R
- Coughlin Mw
- Coughlin Sb
- Coulon Jp
- Countryman St
- Couvares P
- Covas Pb
- Cowan Ee
- Coward Dm
- Cowart Mj
- Coyne Dc
- Coyne R
- Creighton Jde
- Creighton Td
- Cripe J
- Croquette M
- Crowder Sg
- Cullen Tj
- Cumming A
- Cunningham L
- Cuoco E
- D'Angelo B
- D'Antonio S
- Dal Canton T
- Dalya G
- Danilishin Sl
- Danzmann K
- Dasgupta A
- Datrier Leh
- Dattilo V
- Dave I
- Davier M
- Davis D
- Daw Ej
- De Laurentis M
- De Pietri R
- De Rosa R
- De Rossi C
- de Varona O
- DeBra D
- Deenadayalan M
- Degallaix J
- Del Pozzo W
- Deleglise S
- DeMarchi Lm
- Demos N
- Dent T
- DeSalvo R
- Dhurandhar S
- Di Fiore L
- Di Giorgio C
- Di Giovanni F
- Di Giovanni M
- Di Girolamo T
- Di Lieto A
- Di Pace S
- Di Palma I
- Di Renzo F
- Diaz Jc
- Diaz Mc
- Dietrich T
- DiFronzo C
- Ding B
- Divakarla Ak
- Dmitriev A
- Doctor Z
- Donovan F
- Dooley Kl
- Doravari S
- Dorrington I
- Downes Tp
- Drago M
- Driggers Jc
- Du Z
- Ducoin Jg
- Dupej P
- Durante O
- Dwyer Se
- Easter Pj
- Eddolls G
- Edo Tb
- Effler A
- Ehrens P
- Eichholz J
- Eikenberry Ss
- Eisenmann M
- Eisenstein Ra
- Errico L
- Essick Rc
- Estelles H
- Estevez D
- Etienne Zb
- Etzel T
- Evans M
- Evans Tm
- Fafone V
- Fairhurst S
- Fan X
- Farinon S
- Farr B
- Farr Wm
- Fauchon-Jones Ej
- Favata M
- Fays M
- Fazio M
- Fee C
- Feicht J
- Fejer Mm
- Feng F
- Fernandez-Galiana A
- Ferrante I
- Ferreira Ec
- Ferreira Ta
- Fidecaro F
- Fiori I
- Fiorucci D
- Fishbach M
- Fisher Rp
- Fishner Jm
- Fittipaldi R
- Fitz-Axen M
- Fiumara V
- Flaminio R
- Fletcher M
- Floden E
- Flynn E
- Fong H
- Font Ja
- Forsyth Pwf
- Fournier Jd
- Frasca S
- Frasconi F
- Frei Z
- Freise A
- Frey R
- Frey V
- Fritschel P
- Frolov Vv
- Fronze G
- Fulda P
- Fyffe M
- Gabbard Ha
- Gadre Bu
- Gaebel Sm
- Gair Jr
- Gammaitoni L
- Gaonkar Sg
- Garcia-Quiros C
- Garufi F
- Gateley B
- Gaudio S
- Gaur G
- Gayathri V
- Gemme G
- Genin E
- Gennai A
- George D
- George J
- Gergely L
- Ghonge S
- Ghosh A
- Ghosh A
- Ghosh S
- Giacomazzo B
- Giaime Ja
- Giardina Kd
- Gibson Dr
- Gill K
- Glover L
- Gniesmer J
- Godwin P
- Goetz E
- Goetz R
- Goncharov B
- Gonzalez G
- Gopakumar A
- Gossan Se
- Gosselin M
- Gouaty R
- Grace B
- Grado A
- Granata M
- Grant A
- Gras S
- Grassia P
- Gray C
- Gray R
- Greco G
- Green Ac
- Green R
- Gretarsson Em
- Grimaldi A
- Grimm Sj
- Groot P
- Grote H
- Grunewald S
- Gruning P
- Guidi Gm
- Gulati Hk
- Guo Y
- Gupta A
- Gupta A
- Gupta P
- Gustafson Ek
- Gustafson R
- Haegel L
- Halim O
- Hall Br
- Hall Ed
- Hamilton Ez
- Hammond G
- Haney M
- Hanke Mm
- Hanks J
- Hanna C
- Hannuksela Oa
- Hansen Tj
- Hanson J
- Harder T
- Hardwick T
- Haris K
- Harms J
- Harry Gm
- Harry Iw
- Hasskew Rk
- Haster Cj
- Haughian K
- Hayes Fj
- Healy J
- Heidmann A
- Heintze Mc
- Heitmann H
- Hellman F
- Hello P
- Hemming G
- Hendry M
- Heng Is
- Hennig J
- Hernandez Im
- Heurs M
- Hild S
- Hinderer T
- Hochheim S
- Hofman D
- Holgado Am
- Holland Na
- Holt K
- Holz De
- Hopkins P
- Horst C
- Hough J
- Howell Ej
- Hoy Cg
- Huang Y
- Hubner Mt
- Huerta Ea
- Huet D
- Hughey B
- Hui V
- Husa S
- Huttner Sh
- Huynh-Dinh T
- Idzkowski B
- Iess A
- Inchauspe H
- Ingram C
- Inta R
- Intini G
- Irwin B
- Isa Hn
- Isac Jm
- Isi M
- Iyer Br
- Jacqmin T
- Jadhav Sj
- Jani K
- Janthalur Nn
- Jaranowski P
- Jariwala D
- Jenkins Ac
- Jiang J
- Johnson Ds
- Jones Aw
- Jones Di
- Jones Jd
- Jones R
- Jonker Rjg
- Ju L
- Junker J
- Kalaghatgi Cv
- Kalogera V
- Kamai B
- Kandhasamy S
- Kang G
- Kanner Jb
- Kapadia Sj
- Karki S
- Kashyap R
- Kasprzack M
- Katsanevas S
- Katsavounidis E
- Katzman W
- Kaufer S
- Kawabe K
- Keerthana Nv
- Kefelian F
- Keitel D
- Kennedy R
- Key Js
- Khalili Fy
- Khan I
- Khan S
- Khazanov Ea
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- Khursheed M
- Kijbunchoo N
- Kim C
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- Kim W
- Kim Ws
- Kim Ym
- Kimball C
- King Pj
- Kinley-Hanlon M
- Kirchhoff R
- Kissel Js
- Kleybolte L
- Klika Jh
- Klimenko S
- Knowles Td
- Koch P
- Koehlenbeck Sm
- Koekoek G
- Koley S
- Kondrashov V
- Kontos A
- Koper N
- Korobko M
- Korth Wz
- Kovalam M
- Kozak Db
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- Krishnendu N
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- Lai Kh
- Lam Tl
- Landry M
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- Lasky Pd
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- London Lt
- Longo A
- Lorenzini M
- Loriette V
- Lormand M
- Losurdo G
- Lough Jd
- Lousto Co
- Lovelace G
- Lower Me
- Luck H
- Lumaca D
- Lundgren Ap
- Lynch R
- Ma Y
- Macas R
- Macfoy S
- MacInnis M
- Macleod Dm
- Macquet A
- Magana-Sandoval F
- Magee Rm
- Majorana E
- Maksimovic I
- Malik A
- Man N
- Mandic V
- Mangano V
- Mansell Gl
- Manske M
- Mantovani M
- Mapelli M
- Marchesoni F
- Marion F
- Marka S
- Marka Z
- Markakis C
- Markosyan As
- Markowitz A
- Maros E
- Marquina A
- Marsat S
- Martelli F
- Martin Iw
- Martin Rm
- Martinez V
- Martynov Dv
- Masalehdan H
- Mason K
- Massera E
- Masserot A
- Massinger Tj
- Masso-Reid M
- Mastrogiovanni S
- Matas A
- Matichard F
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- McCormick S
- McCuller L
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- McWilliams St
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- Merilh El
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- Messenger C
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- Meylahn F
- Miani A
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- Middleton H
- Milano L
- Miller L
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- Milovich-Goff Mc
- Minazzoli O
- Minenkov Y
- Mishkin A
- Mishra C
- Mistry T
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- Mitrofanov Vp
- Mitselmakher G
- Mittleman R
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- Ng Ky
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- O'Brien Bd
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- Ortega Lf
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- Ottaway Dj
- Overmier H
- Owen Bj
- Pace Ae
- Pagano G
- Page Ma
- Pagliaroli G
- Pai A
- Pai Sa
- Palamos Jr
- Palashov O
- Palomba C
- Pan H
- Panda Pk
- Pang Pth
- Pankow C
- Pannarale F
- Pant Bc
- Paoletti F
- Paoli A
- Parida A
- Parker W
- Pascucci D
- Pasqualetti A
- Passaquieti R
- Passuello D
- Patil M
- Patricelli B
- Payne E
- Pearlstone Bl
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- Pedersen Aj
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- Pedurand R
- Pele A
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- Perego A
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- Petermann J
- Pfeiffer Hp
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- Piccinni Oj
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- Piergiovanni F
- Pierro V
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- Pitkin M
- Plastino W
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- Wysocki Dm
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- Yancey Cc
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- Zhao G
- Zhou M
- Zhou Z
- Zhu Xj
- Zimmerman Ab
- Zucker Me
- Zweizig J
- Publication venue
- College Park, MD : American Physical Society
- Publication date
- 01/01/2019
- Field of study
We present results from a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to track spin wandering. This search improves on previous HMM-based searches of LIGO data by using an improved frequency domain matched filter, the J-statistic, and by analyzing data from Advanced LIGO's second observing run. In the frequency range searched, from 60 to 650 Hz, we find no evidence of gravitational radiation. At 194.6 Hz, the most sensitive search frequency, we report an upper limit on gravitational wave strain (at 95% confidence) of h095%=3.47×10-25 when marginalizing over source inclination angle. This is the most sensitive search for Scorpius X-1, to date, that is specifically designed to be robust in the presence of spin wandering. © 2019 American Physical Society
Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model
- Author
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- Wysocki Dm
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- Zimmerman Ab
- Zucker Me
- Zweizig J
- Publication venue
- 'American Physical Society (APS)'
- Publication date
- 01/01/2019
- Field of study
We present results from a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to track spin wandering. This search improves on previous HMM-based searches of LIGO data by using an improved frequency domain matched filter, the J-statistic, and by analyzing data from Advanced LIGO’s second observing run. In the frequency range searched, from 60 to 650 Hz, we find no evidence of gravitational radiation. At 194.6 Hz, the most sensitive search frequency, we report an upper limit on gravitational wave strain (at 95% confidence) of h95%0=3.47×10−25 when marginalizing over source inclination angle. This is the most sensitive search for Scorpius X-1, to date, that is specifically designed to be robust in the presence of spin wandering
First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary-Black-hole Merger GW170814
- Author
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- Publication venue
- IOP PUBLISHING LTD
- Publication date
- 01/05/2019
- Field of study
We present a multi-messenger measurement of the Hubble constant H 0 using the binary–black-hole merger GW170814 as a standard siren, combined with a photometric redshift catalog from the Dark Energy Survey (DES). The luminosity distance is obtained from the gravitational wave signal detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo Collaboration (LVC) on 2017 August 14, and the redshift information is provided by the DES Year 3 data. Black hole mergers such as GW170814 are expected to lack bright electromagnetic emission to uniquely identify their host galaxies and build an object-by-object Hubble diagram. However, they are suitable for a statistical measurement, provided that a galaxy catalog of adequate depth and redshift completion is available. Here we present the first Hubble parameter measurement using a black hole merger. Our analysis results in H0=75−32+40kms−1Mpc−1, which is consistent with both SN Ia and cosmic microwave background measurements of the Hubble constant. The quoted 68% credible region comprises 60% of the uniform prior range [20, 140] km s−1 Mpc−1, and it depends on the assumed prior range. If we take a broader prior of [10, 220] km s−1 Mpc−1, we find {H}_{0 {78}_{-24}^{+96}\,\mathrm{km}\,{{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1} (57% of the prior range). Although a weak constraint on the Hubble constant from a single event is expected using the dark siren method, a multifold increase in the LVC event rate is anticipated in the coming years and combinations of many sirens will lead to improved constraints on H 0
Search for gravitational waves associated with gamma-ray bursts detected by Fermi and Swift during the LIGO–Virgo run O3b
- Author
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- Zimmerman AB
- Zucker ME
- Zweizig J
- Publication venue
- 'American Astronomical Society'
- Publication date
- 01/01/2022
- Field of study
We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC–2020 March 27 17:00 UTC). We conduct two independent searches: a generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate
Anticonvulsant Level in Saliva, Serum, and Cerebrospinal Fluid
- Author
- Publication venue
- 'Wiley'
- Publication date
- Field of study
Teratogenic Activity and Metabolism of Primidone in the Mouse
- Author
- Publication venue
- 'Wiley'
- Publication date
- Field of study
A case with persistent nephrogenic diabetes insipidus following parathyroidectomy for hyperparathyrotiroidism
- Author
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- Field of study
Access related complications in anterior lumbar surgery performed by spinal surgeons
- Author
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- Field of study
- …