D. H. Shoemaker
Massachusetts Institute of Technology
H-index: 131
North America-United States
Description
D. H. Shoemaker, With an exceptional h-index of 131 and a recent h-index of 91 (since 2020), a distinguished researcher at Massachusetts Institute of Technology, specializes in the field of Gravitational Wave detection.
His recent articles reflect a diverse array of research interests and contributions to the field:
GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run
arXiv: Ultralight vector dark matter search using data from the KAGRA O3GK run
Ultralight vector dark matter search using data from the KAGRA O3GK run
Multi-messenger Astrophysics of Black Holes and Neutron Stars as Probed by Ground-based Gravitational Wave Detectors: From Present to Future
LISA Definition Study Report
arXiv: LISA Definition Study Report
Search for gravitational-lensing signatures in the full third observing run of the LIGO-Virgo network
Search for eccentric black hole coalescences during the third observing run of LIGO and virgo
Professor Information
University | Massachusetts Institute of Technology |
|---|---|
Position | Senior Research Scientist (MIT) |
Citations(all) | 114153 |
Citations(since 2020) | 75828 |
Cited By | 0 |
hIndex(all) | 131 |
hIndex(since 2020) | 91 |
i10Index(all) | 305 |
i10Index(since 2020) | 261 |
University Profile Page | Massachusetts Institute of Technology |
Research & Interests List
Gravitational Wave detection
Top articles of D. H. Shoemaker
GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run
The second Gravitational-Wave Transient Catalog, GWTC-2, reported on 39 compact binary coalescences observed by the Advanced LIGO and Advanced Virgo detectors between 1 April 2019 15∶ 00 UTC and 1 October 2019 15∶ 00 UTC. Here, we present GWTC-2.1, which reports on a deeper list of candidate events observed over the same period. We analyze the final version of the strain data over this period with improved calibration and better subtraction of excess noise, which has been publicly released. We employ three matched-filter search pipelines for candidate identification, and estimate the probability of astrophysical origin for each candidate event. While GWTC-2 used a false alarm rate threshold of 2 per year, we include in GWTC-2.1, 1201 candidates that pass a false alarm rate threshold of 2 per day. We calculate the source properties of a subset of 44 high-significance candidates that have a …
Authors
R Abbott,TD Abbott,F Acernese,K Ackley,C Adams,N Adhikari,RX Adhikari,VB Adya,C Affeldt,D Agarwal,M Agathos,K Agatsuma,N Aggarwal,OD Aguiar,L Aiello,A Ain,P Ajith,S Albanesi,A Allocca,PA Altin,A Amato,C Anand,S Anand,A Ananyeva,SB Anderson,WG Anderson,T Andrade,N Andres,T Andrić,SV Angelova,S Ansoldi,JM Antelis,S Antier,S Appert,K Arai,MC Araya,JS Areeda,M Arène,N Arnaud,SM Aronson,KG Arun,Y Asali,G Ashton,M Assiduo,SM Aston,P Astone,F Aubin,C Austin,S Babak,F Badaracco,MKM Bader,C Badger,S Bae,AM Baer,S Bagnasco,Y Bai,J Baird,M Ball,G Ballardin,SW Ballmer,A Balsamo,G Baltus,S Banagiri,D Bankar,JC Barayoga,C Barbieri,BC Barish,D Barker,P Barneo,F Barone,B Barr,L Barsotti,M Barsuglia,D Barta,J Bartlett,MA Barton,I Bartos,R Bassiri,A Basti,M Bawaj,JC Bayley,AC Baylor,M Bazzan,B Bécsy,VM Bedakihale,M Bejger,I Belahcene,V Benedetto,D Beniwal,TF Bennett,JD Bentley,M Benyaala,F Bergamin,BK Berger,S Bernuzzi,CPL Berry,D Bersanetti,A Bertolini,J Betzwieser,D Beveridge,R Bhandare,U Bhardwaj,D Bhattacharjee,S Bhaumik,IA Bilenko,G Billingsley,S Bini,R Birney,O Birnholtz,S Biscans,M Bischi,S Biscoveanu,A Bisht,B Biswas,M Bitossi,M-A Bizouard,JK Blackburn,CD Blair,DG Blair,RM Blair,F Bobba,N Bode,M Boer,G Bogaert,M Boldrini,LD Bonavena,F Bondu,E Bonilla,R Bonnand,P Booker,BA Boom,R Bork,V Boschi,N Bose,S Bose,V Bossilkov,V Boudart,Y Bouffanais,A Bozzi,C Bradaschia,PR Brady,A Bramley,A Branch,M Branchesi,JE Brau,M Breschi,T Briant,JH Briggs,A Brillet,M Brinkmann
Journal
Physical Review D
Published Date
2024/1/5
arXiv: Ultralight vector dark matter search using data from the KAGRA O3GK run
Among the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for U (1) B− L gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the U (1) B− L gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM.
Authors
AG Abac,ML Chiofalo,G Nieradka,R Pegna,C North,R Bhandare,G Pierra,A Amato,JG Baier,D Chen,B Haskell,F Robinet,M Fyffe,M Arogeti,P Stevens,DD White,TF Davies,E Payne,M Wright,K Johansmeyer,K Hayama,P-F Cohadon,CG Collette,D Sellers,S Hoang,V Sipala,H Heitmann,T O'Hanlon,B Edelman,G McCarrol,AD Huddart,KD Sullivan,T Harder,A Garron,TA Clarke,YT Huang,J Junker,M Hennig,N Hirata,J Portell,R McCarthy,M Weinert,R Poulton,G Ballardin,D Bankar,A Bianchi,M Montani,CD Panzer,X Chen,R Takahashi,J Lange,K Schouteden,Yitian Chen,A Sasli,F Yang,LM Modafferi,ME Zucker,J O'Dell,D Lumaca,AP Spencer,M Millhouse,G Quéméner,M Norman,MJ Szczepańczyk,S-C Hsu,ST Countryman,C Chatterjee,AL James,KN Nagler,E Chassande-Mottin,W Kiendrebeogo,M Tacca,FJ Raab,TR Saravanan,VP Mitrofanov,S Bernuzzi,C Adamcewicz,L Conti,C Tong-Yu,J Golomb,X Li,A Perego,ERG von Reis,J Woehler,G Bogaert,F Fidecaro,B Shen,JM Ezquiaga,D Macri,V Juste,S Sachdev,JD Bentley,R Sturani,TP Lott IV,K Takatani,D Beniwal,U Dupletsa,A Boumerdassi,F Glotin,Y Lee,R Bhatt,A Couineaux,M Wade,N Kanda,J Novak,S Bini,I Ferrante,RA Alfaidi,N Johny,LE Sanchez,J Heinze,J Zhang,M Kinley-Hanlon,AJ Weinstein,T Sainrat,NN Janthalur,A Trovato,A Romero,K Tomita,DE McClelland,B Fornal,M Heurs,AM Gretarsson,A Chincarini,BB Lane,AE Romano,V Fafone,FY Khalili,F Linde,C Messick,A Heffernan,J Gargiulo,V JaberianHamedan,SW Reid,D Moraru,D Pathak,M Iwaya,G Grignani,T Yan,K AultONeal,SA Pai,Y Xu,IM Pinto,KW Chung,C Palomba,J Tissino,T Klinger,Ll M Mir,K Kwan,C Posnansky
Published Date
2024/3/5
Ultralight vector dark matter search using data from the KAGRA O3GK run
Among the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation time scale of DM.
Authors
AG Abac,R Abbott,H Abe,I Abouelfettouh,F Acernese,K Ackley,C Adamcewicz,S Adhicary,N Adhikari,RX Adhikari,VK Adkins,VB Adya,C Affeldt,D Agarwal,M Agathos,OD Aguiar,I Aguilar,L Aiello,A Ain,P Ajith,T Akutsu,S Albanesi,RA Alfaidi,A Al-Jodah,C Alléné,A Allocca,S Al-Shammari,PA Altin,S Alvarez-Lopez,A Amato,L Amez-Droz,A Amorosi,C Amra,S Anand,A Ananyeva,SB Anderson,WG Anderson,M Andia,M Ando,T Andrade,N Andres,M Andrés-Carcasona,T Andrić,J Anglin,S Ansoldi,JM Antelis,S Antier,M Aoumi,EZ Appavuravther,S Appert,SK Apple,K Arai,A Araya,MC Araya,JS Areeda,N Aritomi,F Armato,N Arnaud,M Arogeti,SM Aronson,KG Arun,G Ashton,Y Aso,M Assiduo,S Melo,SM Aston,P Astone,F Aubin,K AultONeal,G Avallone,S Babak,F Badaracco,C Badger,S Bae,S Bagnasco,E Bagui,Y Bai,JG Baier,R Bajpai,T Baka,M Ball,G Ballardin,SW Ballmer,S Banagiri,B Banerjee,D Bankar,P Baral,JC Barayoga,BC Barish,D Barker,P Barneo,F Barone,B Barr,L Barsotti,M Barsuglia,D Barta,SD Barthelmy,MA Barton,I Bartos,S Basak,A Basalaev,R Bassiri,A Basti,M Bawaj,P Baxi,JC Bayley,AC Baylor,M Bazzan,B Bécsy,VM Bedakihale,F Beirnaert,M Bejger,D Belardinelli,AS Bell,V Benedetto,D Beniwal,W Benoit,JD Bentley,M Ben Yaala,S Bera,M Berbel,F Bergamin,BK Berger,S Bernuzzi,M Beroiz,D Bersanetti,A Bertolini,J Betzwieser,D Beveridge,N Bevins,R Bhandare,U Bhardwaj,R Bhatt,D Bhattacharjee,S Bhaumik,S Bhowmick,A Bianchi,IA Bilenko,G Billingsley,A Binetti,S Bini,O Birnholtz,S Biscoveanu,A Bisht,M Bitossi,M-A Bizouard,JK Blackburn,CD Blair,DG Blair,F Bobba
Journal
arXiv preprint arXiv:2403.03004
Published Date
2024/3/5
Multi-messenger Astrophysics of Black Holes and Neutron Stars as Probed by Ground-based Gravitational Wave Detectors: From Present to Future
The ground-based gravitational wave (GW) detectors LIGO and Virgo have enabled the birth of multi-messenger GW astronomy via the detection of GWs from merging stellar-mass black holes (BHs) and neutron stars (NSs). GW170817, the first binary NS merger detected in GWs and all bands of the electromagnetic spectrum, is an outstanding example of the impact that GW discoveries can have on multi-messenger astronomy. Yet, GW170817 is only one of the many and varied multi-messenger sources that can be unveiled using ground-based GW detectors. In this contribution, we summarize key open questions in the astrophysics of stellar-mass BHs and NSs that can be answered using current and future-generation ground-based GW detectors, and highlight the potential for new multi-messenger discoveries ahead.
Authors
Alessandra Corsi,Lisa Barsotti,Emanuele Berti,Matthew Evans,Ish Gupta,Konstantinos Kritos,Kevin Kuns,Alexander H Nitz,Benjamin J Owen,Binod Rajbhandari,Jocelyn Read,Bangalore S Sathyaprakash,David H Shoemaker,Joshua R Smith,Salvatore Vitale
Journal
arXiv preprint arXiv:2402.13445
Published Date
2024/2/21
LISA Definition Study Report
The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves in the 0.1 mHz to 1 Hz frequency band which will enable the study of a vast number of objects ranging from Galactic binaries and stellar mass black holes in the Milky Way, to distant massive black-hole mergers and the expansion of the Universe. This definition study report, or Red Book, presents a summary of the very large body of work that has been undertaken on the LISA mission over the LISA definition phase.
Authors
Monica Colpi,Karsten Danzmann,Martin Hewitson,Kelly Holley-Bockelmann,Philippe Jetzer,Gijs Nelemans,Antoine Petiteau,David Shoemaker,Carlos Sopuerta,Robin Stebbins,Nial Tanvir,Henry Ward,William Joseph Weber,Ira Thorpe,Anna Daurskikh,Atul Deep,Ignacio Fernández Núñez,César García Marirrodriga,Martin Gehler,Jean-Philippe Halain,Oliver Jennrich,Uwe Lammers,Jonan Larrañaga,Maike Lieser,Nora Lützgendorf,Waldemar Martens,Linda Mondin,Ana Piris Niño,Pau Amaro-Seoane,Manuel Arca Sedda,Pierre Auclair,Stanislav Babak,Quentin Baghi,Vishal Baibhav,Tessa Baker,Jean-Baptiste Bayle,Christopher Berry,Emanuele Berti,Guillaume Boileau,Matteo Bonetti,Richard Brito,Riccardo Buscicchio,Gianluca Calcagni,Pedro R Capelo,Chiara Caprini,Andrea Caputo,Eleonora Castelli,Hsin-Yu Chen,Xian Chen,Alvin Chua,Gareth Davies,Andrea Derdzinski,Valerie Fiona Domcke,Daniela Doneva,Irna Dvorkin,Jose María Ezquiaga,Jonathan Gair,Zoltan Haiman,Ian Harry,Olaf Hartwig,Aurelien Hees,Anna Heffernan,Sascha Husa,David Izquierdo,Nikolaos Karnesis,Antoine Klein,Valeriya Korol,Natalia Korsakova,Thomas Kupfer,Danny Laghi,Astrid Lamberts,Shane Larson,Maude Le Jeune,Marek Lewicki,Tyson Littenberg,Eric Madge,Alberto Mangiagli,Sylvain Marsat,Ivan Martin Vilchez,Andrea Maselli,Josh Mathews,Maarten van de Meent,Martina Muratore,Germano Nardini,Paolo Pani,Marco Peloso,Mauro Pieroni,Adam Pound,Hippolyte Quelquejay-Leclere,Angelo Ricciardone,Elena Maria Rossi,Andrea Sartirana,Etienne Savalle,Laura Sberna,Alberto Sesana,Deirdre Shoemaker,Jacob Slutsky,Thomas Sotiriou,Lorenzo Speri,Martin Staab,Danièle Steer,Nicola Tamanini,Gianmassimo Tasinato,Jesus Torrado,Alejandro Torres-Orjuela,Alexandre Toubiana,Michele Vallisneri,Alberto Vecchio,Marta Volonteri,Kent Yagi,Lorenz Zwick
Journal
arXiv preprint arXiv:2402.07571
Published Date
2024/2/12
arXiv: LISA Definition Study Report
Abstract The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves in the 0.1 mHz to 1 Hz frequency band which will enable the study of a vast number of objects ranging from Galactic binaries and stellar mass black holes in the Milky Way, to distant massive black-hole mergers and the expansion of the Universe. This definition study report, or Red Book, presents a summary of the very large body of work that has been undertaken on the LISA mission over the LISA definition phase.
Authors
Monica Colpi,Jean-Philippe Halain,Philippe Jetzer,Michele Vallisneri,Waldemar Martens,Vishal Baibhav,Etienne Savalle,Pedro R Capelo,Andrea Sartirana,Ian Harry,Gianluca Calcagni,Carlos Sopuerta,Sascha Husa,Tyson Littenberg,Antoine Petiteau,Nicola Tamanini,Oliver Jennrich,Robin Stebbins,Alejandro Torres-Orjuela,Elena Maria Rossi,Daniela Doneva,Christopher Berry,Jacob Slutsky,William JosephWeber,Deirdre Shoemaker,Nora Lützgendorf,Hsin-Yu Chen,Paolo Pani,Ana Piris Niño,Gijs Nelemans,Anna Daurskikh,Jonathan Gair,Ivan Martin Vilchez,Eleonora Castelli,Maude Le Jeune,Tessa Baker,Valerie Fiona Domcke,Martin Hewitson,Valeriya Korol,Martin Staab,Germano Nardini,Alvin Chua,Astrid Lamberts,Martina Muratore,Lorenz Zwick,Kent Yagi,Riccardo Buscicchio,Atul Deep,Maarten van de Meent,Olaf Hartwig,David Shoemaker,Mauro Pieroni,Quentin Baghi,Pierre Auclair,Jesus Torrado,Marco Peloso,Andrea Maselli,Eric Madge,Richard Brito,Martin Gehler,Uwe Lammers,Linda Mondin,Manuel Arca Sedda,Guillaume Boileau,Ignacio Fernández Núñez,Chiara Caprini,Marta Volonteri,Gianmassimo Tasinato,Stanislav Babak,Antoine Klein,David Izquierdo,Matteo Bonetti,Nikolaos Karnesis,Emanuele Berti,Thomas Kupfer,Zoltan Haiman,Karsten Danzmann,Natalia Korsakova,Maike Lieser,Jonan Larrañaga,Danièle Steer,Pau Amaro-Seoane,Andrea Caputo,Josh Mathews,Gareth Davies,Ira Thorpe,Alberto Vecchio,Jean-Baptiste Bayle,Henry Ward,Andrea Derdzinski,Thomas Sotiriou,Jose María Ezquiaga,César García Marirrodriga,Lorenzo Speri,Angelo Ricciardone,Nial Tanvir,Hippolyte Quelquejay-Leclere,Alexandre Toubiana,Xian Chen,Alberto Sesana,Shane Larson,Eric Joffre,Marek Lewicki,Aurelien Hees,Adam Pound,Danny Laghi,Sylvain Marsat,Laura Sberna,Irna Dvorkin,Alberto Mangiagli,Anna Heffernan
Published Date
2024/2/12
Search for gravitational-lensing signatures in the full third observing run of the LIGO-Virgo network
Gravitational lensing by massive objects along the line of sight to the source causes distortions of gravitational wave-signals; such distortions may reveal information about fundamental physics, cosmology and astrophysics. In this work, we have extended the search for lensing signatures to all binary black hole events from the third observing run of the LIGO--Virgo network. We search for repeated signals from strong lensing by 1) performing targeted searches for subthreshold signals, 2) calculating the degree of overlap amongst the intrinsic parameters and sky location of pairs of signals, 3) comparing the similarities of the spectrograms amongst pairs of signals, and 4) performing dual-signal Bayesian analysis that takes into account selection effects and astrophysical knowledge. We also search for distortions to the gravitational waveform caused by 1) frequency-independent phase shifts in strongly lensed images, and 2) frequency-dependent modulation of the amplitude and phase due to point masses. None of these searches yields significant evidence for lensing. Finally, we use the non-detection of gravitational-wave lensing to constrain the lensing rate based on the latest merger-rate estimates and the fraction of dark matter composed of compact objects.
Authors
R Abbott,H Abe,F Acernese,K Ackley,S Adhicary,N Adhikari,RX Adhikari,VK Adkins,VB Adya,C Affeldt,D Agarwal,M Agathos,OD Aguiar,L Aiello,A Ain,P Ajith,T Akutsu,S Albanesi,RA Alfaidi,C Alléné,A Allocca,PA Altin,A Amato,S Anand,A Ananyeva,SB Anderson,WG Anderson,M Ando,T Andrade,N Andres,M Andrés-Carcasona,T Andrić,S Ansoldi,JM Antelis,S Antier,T Apostolatos,EZ Appavuravther,S Appert,SK Apple,K Arai,A Araya,MC Araya,JS Areeda,M Arène,N Aritomi,N Arnaud,M Arogeti,SM Aronson,H Asada,G Ashton,Y Aso,M Assiduo,S Melo,SM Aston,P Astone,F Aubin,K AultONeal,S Babak,F Badaracco,C Badger,S Bae,Y Bae,S Bagnasco,Y Bai,JG Baier,J Baird,R Bajpai,T Baka,M Ball,G Ballardin,SW Ballmer,G Baltus,S Banagiri,B Banerjee,D Bankar,JC Barayoga,BC Barish,D Barker,P Barneo,F Barone,B Barr,L Barsotti,M Barsuglia,D Barta,J Bartlett,MA Barton,I Bartos,S Basak,R Bassiri,A Basti,M Bawaj,JC Bayley,M Bazzan,B Bécsy,VM Bedakihale,F Beirnaert,M Bejger,I Belahcene,AS Bell,V Benedetto,D Beniwal,W Benoit,JD Bentley,M BenYaala,S Bera,M Berbel,F Bergamin,BK Berger,S Bernuzzi,M Beroiz,CPL Berry,D Bersanetti,A Bertolini,J Betzwieser,D Beveridge,R Bhandare,AV Bhandari,U Bhardwaj,R Bhatt,D Bhattacharjee,S Bhaumik,A Bianchi,IA Bilenko,M Bilicki,G Billingsley,S Bini,O Birnholtz,S Biscans,M Bischi,S Biscoveanu,A Bisht,B Biswas,M Bitossi,M-A Bizouard,JK Blackburn,CD Blair,DG Blair,RM Blair,F Bobba,N Bode,M Boër,G Bogaert,M Boldrini,GN Bolingbroke,LD Bonavena,R Bondarescu,F Bondu,E Bonilla,R Bonnand,P Booker
Journal
arXiv preprint arXiv:2304.08393
Published Date
2023/4/17
Search for eccentric black hole coalescences during the third observing run of LIGO and virgo
Despite the growing number of confident binary black hole coalescences 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 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 were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass ) binaries covering eccentricities up to 0.3 at 15 Hz orbital 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 an upper limit for the merger rate density of high-mass binaries with eccentricities at Gpc yr at 90\% confidence level.
Authors
AG Abac,R Abbott,H Abe,F Acernese,K Ackley,C Adamcewicz,S Adhicary,N Adhikari,RX Adhikari,VK Adkins,VB Adya,C Affeldt,D Agarwal,M Agathos,OD Aguiar,I Aguilar,L Aiello,A Ain,P Ajith,T Akutsu,S Albanesi,RA Alfaidi,A Al-Jodah,C Alléné,A Allocca,M Almualla,PA Altin,S Álvarez-López,A Amato,L Amez-Droz,A Amorosi,S Anand,A Ananyeva,R Andersen,SB Anderson,WG Anderson,M Andia,M Ando,T Andrade,N Andres,M Andrés-Carcasona,T Andrić,S Ansoldi,JM Antelis,S Antier,M Aoumi,T Apostolatos,EZ Appavuravther,S Appert,SK Apple,K Arai,A Araya,MC Araya,JS Areeda,N Aritomi,F Armato,N Arnaud,M Arogeti,SM Aronson,KG Arun,G Ashton,Y Aso,M Assiduo,S Melo,SM Aston,P Astone,F Aubin,K AultONeal,S Babak,A Badalyan,F Badaracco,C Badger,S Bae,S Bagnasco,Y Bai,JG Baier,R Bajpai,T Baka,M Ball,G Ballardin,SW Ballmer,G Baltus,S Banagiri,B Banerjee,D Bankar,P Baral,JC Barayoga,J Barber,BC Barish,D Barker,P Barneo,F Barone,B Barr,L Barsotti,M Barsuglia,D Barta,SD Barthelmy,MA Barton,I Bartos,S Basak,A Basalaev,R Bassiri,A Basti,M Bawaj,P Baxi,JC Bayley,AC Baylor,M Bazzan,B Bécsy,VM Bedakihale,F Beirnaert,M Bejger,AS Bell,V Benedetto,D Beniwal,W Benoit,JD Bentley,M Ben Yaala,S Bera,M Berbel,F Bergamin,BK Berger,S Bernuzzi,M Beroiz,CPL Berry,D Bersanetti,A Bertolini,J Betzwieser,D Beveridge,N Bevins,R Bhandare,AV Bhandari,U Bhardwaj,R Bhatt,D Bhattacharjee,S Bhaumik,A Bianchi,IA Bilenko,M Bilicki,G Billingsley,A Binetti,S Bini,O Birnholtz,S Biscans,M Bischi,S Biscoveanu,A Bisht,M Bitossi,M-A Bizouard,JK Blackburn
Journal
arXiv preprint arXiv:2308.03822
Published Date
2023/8/7
Professor FAQs
What is D. H. Shoemaker's h-index at Massachusetts Institute of Technology?
The h-index of D. H. Shoemaker has been 91 since 2020 and 131 in total.
What are D. H. Shoemaker's top articles?
The articles with the titles of
GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run
arXiv: Ultralight vector dark matter search using data from the KAGRA O3GK run
Ultralight vector dark matter search using data from the KAGRA O3GK run
Multi-messenger Astrophysics of Black Holes and Neutron Stars as Probed by Ground-based Gravitational Wave Detectors: From Present to Future
LISA Definition Study Report
arXiv: LISA Definition Study Report
Search for gravitational-lensing signatures in the full third observing run of the LIGO-Virgo network
Search for eccentric black hole coalescences during the third observing run of LIGO and virgo
...
are the top articles of D. H. Shoemaker at Massachusetts Institute of Technology.
What are D. H. Shoemaker's research interests?
The research interests of D. H. Shoemaker are: Gravitational Wave detection
What is D. H. Shoemaker's total number of citations?
D. H. Shoemaker has 114,153 citations in total.
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