Michael A. Strauss

Princeton University

H-index: 207

North America-United States

Description

Michael A. Strauss, With an exceptional h-index of 207 and a recent h-index of 111 (since 2020), a distinguished researcher at Princeton University,

His recent articles reflect a diverse array of research interests and contributions to the field:

Gemini Near Infrared Spectrograph--Distant Quasar Survey: Rest-Frame Ultraviolet-Optical Spectral Properties of Broad Absorption Line Quasars

Euclid preparation. The Near-IR Background Dipole Experiment with Euclid

2019 VZ50

Measurement of the Centrality Dependence of the Dijet Yield in p+ Pb Collisions at sNN= 8.16 TeV with the ATLAS Detector

A precise measurement of the Z-boson double-differential transverse momentum and rapidity distributions in the full phase space of the decay leptons with the ATLAS …

Observation of WZγ Production in pp Collisions at s= 13 TeV with the ATLAS Detector

A quasar-galaxy merger at : black hole mass and quasar properties from the NIRSpec spectrum

2017 BG231

Professor Information

University	Princeton University
Position	Professor of Astrophysical Sciences
Citations(all)	216829
Citations(since 2020)	67692
Cited By	158593
hIndex(all)	207
hIndex(since 2020)	111
i10Index(all)	926
i10Index(since 2020)	628
Email	Access Email
University Profile Page	Princeton University

Top articles of Michael A. Strauss

Gemini Near Infrared Spectrograph--Distant Quasar Survey: Rest-Frame Ultraviolet-Optical Spectral Properties of Broad Absorption Line Quasars

We present the rest-frame ultraviolet-optical spectral properties of 65 broad absorption line (BAL) quasars from the Gemini Near Infrared Spectrograph-Distant Quasar Survey (GNIRS-DQS). These properties are compared with those of 195 non-BAL quasars from GNIRS-DQS in order to identify the drivers for the appearance of BALs in quasar spectra. In particular, we compare equivalent widths and velocity widths, as well as velocity offsets from systemic redshifts, of principal emission lines. In spite of the differences between their rest-frame ultraviolet spectra, we find that luminous BAL quasars are generally indistinguishable from their non-BAL counterparts in the rest-frame optical band at redshifts . We do not find any correlation between BAL trough properties and the H-based supermassive black hole masses and normalized accretion rates in our sample. Considering the Sloan Digital Sky Survey quasar sample, which includes the GNIRS-DQS sample, we find that a monochromatic luminosity at rest-frame 2500 A of erg s is a necessary condition for launching BAL outflows in quasars. We compare our findings with other BAL quasar samples and discuss the roles that accretion rate and orientation play in the appearance of BAL troughs in quasar spectra.

Authors

Harum Ahmed,Ohad Shemmer,Brandon Matthews,Cooper Dix,Trung Ha,Gordon T Richards,Michael S Brotherton,Adam D Myers,WN Brandt,Sarah C Gallagher,Richard Green,Paulina Lira,Jacob N McLane,Richard M Plotkin,Donald P Schneider

Journal

arXiv preprint arXiv:2404.12343

Published Date

2024/4/18

Euclid preparation. The Near-IR Background Dipole Experiment with Euclid

Verifying the fully kinematic nature of the cosmic microwave background (CMB) dipole is of fundamental importance in cosmology. In the standard cosmological model with the Friedman-Lemaitre-Robertson-Walker (FLRW) metric from the inflationary expansion the CMB dipole should be entirely kinematic. Any non-kinematic CMB dipole component would thus reflect the preinflationary structure of spacetime probing the extent of the FLRW applicability. Cosmic backgrounds from galaxies after the matter-radiation decoupling, should have kinematic dipole component identical in velocity with the CMB kinematic dipole. Comparing the two can lead to isolating the CMB non-kinematic dipole. It was recently proposed that such measurement can be done using the near-IR cosmic infrared background (CIB) measured with the currently operating Euclid telescope, and later with Roman. The proposed method reconstructs the resolved CIB, the Integrated Galaxy Light (IGL), from Euclid's Wide Survey and probes its dipole, with a kinematic component amplified over that of the CMB by the Compton-Getting effect. The amplification coupled with the extensive galaxy samples forming the IGL would determine the CIB dipole with an overwhelming signal/noise, isolating its direction to sub-degree accuracy. We develop details of the method for Euclid's Wide Survey in 4 bands spanning 0.6 to 2 mic. We isolate the systematic and other uncertainties and present methodologies to minimize them, after confining the sample to the magnitude range with negligible IGL/CIB dipole from galaxy clustering. These include the required star-galaxy separation, accounting for …

Authors

A Kashlinsky,RG Arendt,MLN Ashby,F Atrio-Barandela,R Scaramella,MA Strauss,B Altieri,A Amara,S Andreon,N Auricchio,M Baldi,S Bardelli,R Bender,C Bodendorf,E Branchini,M Brescia,J Brinchmann,S Camera,V Capobianco,C Carbone,J Carretero,S Casas,M Castellano,S Cavuoti,A Cimatti,G Congedo,CJ Conselice,L Conversi,Y Copin,L Corcione,F Courbin,HM Courtois,A Da Silva,H Degaudenzi,AM Di Giorgio,J Dinis,F Dubath,X Dupac,S Dusini,A Ealet,M Farina,S Farrens,S Ferriol,M Frailis,E Franceschi,S Galeotta,B Gillis,C Giocoli,A Grazian,F Grupp,SVH Haugan,I Hook,F Hormuth,A Hornstrup,K Jahnke,E Keihänen,S Kermiche,A Kiessling,M Kilbinger,B Kubik,M Kunz,H Kurki-Suonio,S Ligori,PB Lilje,V Lindholm,I Lloro,D Maino,E Maiorano,O Mansutti,O Marggraf,K Markovic,N Martinet,F Marulli,R Massey,S Maurogordato,HJ McCracken,E Medinaceli,S Mei,Y Mellier,M Meneghetti,G Meylan,M Moresco,L Moscardini,E Munari,S-M Niemi,C Padilla,S Paltani,F Pasian,K Pedersen,WJ Percival,S Pires,G Polenta,M Poncet,LA Popa,F Raison,A Renzi,J Rhodes,G Riccio,E Romelli,M Roncarelli,E Rossetti,R Saglia,D Sapone,B Sartoris,M Schirmer,P Schneider,T Schrabback,A Secroun,G Seidel,M Seiffert,S Serrano,C Sirignano,G Sirri,L Stanco,C Surace,P Tallada-Crespí,AN Taylor,HI Teplitz,I Tereno,R Toledo-Moreo,F Torradeflot,I Tutusaus,L Valenziano,T Vassallo,A Veropalumbo,Y Wang,G Zamorani,J Zoubian,E Zucca,A Biviano,E Bozzo,C Burigana,C Colodro-Conde,D Di Ferdinando,G Fabbian,R Farinelli,J Graciá-Carpio,G Mainetti,M Martinelli,N Mauri,C Neissner,Z Sakr,V Scottez,M Tenti,M Viel,M Wiesmann,Y Akrami,V Allevato,S Anselmi,C Baccigalupi

Journal

arXiv preprint arXiv:2401.17945

Published Date

2024/1/31

2019 VZ50

2019 VZ50 - NASA/ADS Now on home page ads icon ads Enable full ADS view NASA/ADS 2019 VZ50 Li, X. ; Murayama, H. ; Waters, CZ ; Nakata, F. ; Ando, M. ; Reed, SL ; Koike, M. ; Hsieh, B. -C. ; Lin, Y. -T. ; Suto, Y. ; Plazas Malagón, AA ; Tanaka, M. ; Toba, Y. ; Mineo, S. ; Furusawa, H. ; Lupton, RH ; Ouchi, M. ; Simunovic, M. ; Miyatake, H. ; Terai, T. ; Lust, NB ; Turner, EL ; Fukuyama, H. ; Iwata, I. ; Bosch, J. ; Rykoff, ES ; Aikawa, R. ; Ito, K. ; Shibuya, T. ; Takita, S. ; Oguri, M. ; Osato, K. ; Yamamoto, N. ; Tang, S. ; Egami, E. ; Okabe, N. ; Yamada, Y. ; Furusawa, J. ; Komiyama, Y. ; Nishizawa, AJ ; Taranu, DS ; More, S. ; Kokubo, M. ; MacArthur, LA ; Takada, M. ; Morishima, T. ; Harikane, Y. ; Aihara, H. ; Okura, Y. ; Suzuki, N. and 20 more Abstract Publication: Minor Planet Electronic Circulars Pub Date: March 2024 DOI: 10.48377/MPEC/2024-F90 Bibcode: 2024MPEC....F...90. Keywords: Small Solar System bodies; 2019 …

Authors

X Li,H Murayama,CZ Waters,F Nakata,M Ando,SL Reed,M Koike,B-C Hsieh,Y-T Lin,Y Suto,AA Plazas Malagón,M Tanaka,Y Toba,S Mineo,H Furusawa,RH Lupton,M Ouchi,M Simunovic,H Miyatake,T Terai,NB Lust,EL Turner,H Fukuyama,I Iwata,J Bosch,ES Rykoff,R Aikawa,K Ito,T Shibuya,S Takita,M Oguri,K Osato,N Yamamoto,S Tang,E Egami,N Okabe,Y Yamada,J Furusawa,Y Komiyama,AJ Nishizawa,DS Taranu,S More,M Kokubo,LA MacArthur,M Takada,T Morishima,Y Harikane,H Aihara,Y Okura,N Suzuki,T Takata,T Kodama,M Yoshimi,H Ikeda,K Nakajima,PA Price,MA Strauss,H Uchiyama,Y-C Pan,B Vijarnwannaluk,Y AlSayyad,Y Ono,K Sugimori,Y Takagi,R Armstrong,K Mawatari,S Harasawa,T Yamashita,Y Liang,S Miyazaki

Journal

Minor Planet Electronic Circulars

Published Date

2024/3

Measurement of the Centrality Dependence of the Dijet Yield in p+ Pb Collisions at sNN= 8.16 TeV with the ATLAS Detector

The measurement of hard scatterings in proton-nucleus collisions has resulted in a greater understanding of both the proton and nuclear structure. ATLAS measured the centrality dependence of the dijet yield using 165 nb of +Pb data collected at = 8.16 TeV in 2016. The event centrality, which reflects the +Pb impact parameter, is characterized by the total transverse energy registered in the Pb-going side of the forward calorimeter. The central-to-peripheral ratio of the scaled dijet yields, , is evaluated, and the results are presented as a function of variables that reflect the kinematics of the initial hard parton scattering process. The shows a scaling with the Bjorken- of the parton originating from the proton, , while no such trend is observed as a function of . This analysis provides unique input to understanding the role of small proton spatial configurations in +Pb collisions by covering parton momentum fractions from the valence region down to and .

Authors

Georges Aad,Braden Keim Abbott,Kira Abeling,Nils Julius Abicht,Haider Abidi,Asmaa Aboulhorma,Halina Abramowicz,Henso Abreu,Yiming Abulaiti,Bobby Samir Acharya,Claire Adam Bourdarios,Leszek Adamczyk,Sagar Addepalli,Matt Addison,Jahred Adelman,Aytul Adiguzel,Tim Adye,Tony Affolder,Yoav Afik,Merve Nazlim Agaras,Jinky Agarwala,Anamika Aggarwal,Catalin Agheorghiesei,Ammara Ahmad,Faig Ahmadov,Waleed Syed Ahmed,Sudha Ahuja,Xiaocong Ai,Giulio Aielli,Arya Aikot,Malak Ait Tamlihat,Brahim Aitbenchikh,Iakov Aizenberg,Melike Akbiyik,Torsten Akesson,Andrei Akimov,Daiya Akiyama,Nilima Nilesh Akolkar,Konie Al Khoury,Gian Luigi Alberghi,Justin Albert,Pietro Albicocco,Guillaume Lucas Albouy,Sara Alderweireldt,Zackary Lee Alegria,Martin Aleksa,Igor Alexandrov,Calin Alexa,Theodoros Alexopoulos,Fabrizio Alfonsi,Malte Algren,Muhammad Alhroob,Babar Ali,Hanadi Ali,Shahzad Ali,Samuel William Alibocus,Malik Aliev,Gianluca Alimonti,Wael Alkakhi,Corentin Allaire,Benedict Allbrooke,Julia Frances Allen,Cristian Andres Allendes Flores,Philip Patrick Allport,Alberto Aloisio,Francisco Alonso,Cristiano Alpigiani,Manuel Alvarez Estevez,Adrian Alvarez Fernandez,Mario Alves Cardoso,Mariagrazia Alviggi,Mohamed Aly,Yara Do Amaral Coutinho,Alessandro Ambler,Christoph Amelung,Maximilian Amerl,Christoph Ames,Dante Amidei,Susana Patricia Amor dos Santos,Kieran Robert Amos,Viktor Ananiev,Christos Anastopoulos,Timothy Robert Andeen,John Kenneth Anders,Stefio Yosse Andrean,Attilio Andreazza,Stylianos Angelidakis,Aaron Angerami,Alexey Anisenkov,Alberto Annovi,Claire Antel,Matthew Thomas Anthony,Egor Antipov,Mario Antonelli,Fabio Anulli,Masato Aoki,Takumi Aoki,Javier Alberto Aparisi Pozo,Marco Aparo,Ludovica Aperio Bella,Christian Appelt,Aram Apyan,Nordin Aranzabal Barrio,Sergio Javier Arbiol Val,Chiara Arcangeletti,Ayana Tamu Arce,Eloisa Arena,Jean-Francois Arguin,Spyros Argyropoulos,Jan-Hendrik Arling,Olivier Arnaez,Hannah Arnold,Giacomo Artoni,Haruka Asada,Kanae Asai,Shoji Asai,Nedaa Alexandra Asbah,Jihad Assahsah,Ketevi Adikle Assamagan,Robert Astalos,Rose Atashi,Ryan Justin Atkin,Markus Julian Atkinson,Hicham Atmani,Prachi Atmasiddha,Kamil Augsten,Silvia Auricchio,Adrien Auriol,Volker Andreas Austrup,Giuseppe Avolio,Konstantinos Axiotis,Georges Azuelos,Dominik Babal,Henri Bachacou,Konstantinos Bachas,Alexander Bachiu,Karl Filip Backman,Anthony Badea,Paolo Bagnaia,Marzieh Bahmani,Daniel Bahner,Adam Bailey,Virginia Bailey,John Baines,Luke Baines,Keith Baker,Evelin Bakos,Debottam Bakshi Gupta,Veena Balakrishnan,Rahul Balasubramanian

Published Date

2023/9/7

A precise measurement of the Z-boson double-differential transverse momentum and rapidity distributions in the full phase space of the decay leptons with the ATLAS …

This paper presents for the first time a precise measurement of the production properties of the Z boson in the full phase space of the decay leptons. This is in contrast to the many previous precise unfolded measurements performed in the fiducial phase space of the decay leptons. The measurement is obtained from proton–proton collision data collected by the ATLAS experiment in 2012 at TeV at the LHC and corresponding to an integrated luminosity of 20.2 fb. The results, based on a total of 15.3 million Z-boson decays to electron and muon pairs, extend and improve a previous measurement of the full set of angular coefficients describing Z-boson decay. The double-differential cross-section distributions in Z-boson transverse momentum and rapidity are measured in the pole region, defined as GeV, over the range . The total uncertainty of the normalised cross-section measurements in the peak region of the …

Authors

ATLAS Collaboration atlas. publications@ cern. ch,G Aad,B Abbott,K Abeling,NJ Abicht,SH Abidi,A Aboulhorma,H Abramowicz,H Abreu,Y Abulaiti,AC Abusleme Hoffman,BS Acharya,C Adam Bourdarios,L Adamczyk,L Adamek,SV Addepalli,MJ Addison,J Adelman,A Adiguzel,T Adye,AA Affolder,Y Afik,MN Agaras,J Agarwala,A Aggarwal,C Agheorghiesei,A Ahmad,F Ahmadov,WS Ahmed,S Ahuja,X Ai,G Aielli,M Ait Tamlihat,B Aitbenchikh,I Aizenberg,M Akbiyik,TPA Åkesson,AV Akimov,D Akiyama,NN Akolkar,K Al Khoury,GL Alberghi,J Albert,P Albicocco,GL Albouy,S Alderweireldt,M Aleksa,IN Aleksandrov,C Alexa,T Alexopoulos,A Alfonsi,F Alfonsi,M Algren,M Alhroob,B Ali,HMJ Ali,S Ali,SW Alibocus,M Aliev,G Alimonti,W Alkakhi,C Allaire,BMM Allbrooke,JF Allen,CA Allendes Flores,PP Allport,A Aloisio,F Alonso,C Alpigiani,M Alvarez Estevez,A Alvarez Fernandez,MG Alviggi,M Aly,Y Amaral Coutinho,A Ambler,C Amelung,M Amerl,CG Ames,D Amidei,SP Amor Dos Santos,KR Amos,V Ananiev,C Anastopoulos,T Andeen,JK Anders,SY Andrean,A Andreazza,S Angelidakis,A Angerami,AV Anisenkov,A Annovi,C Antel,MT Anthony,E Antipov,M Antonelli,DJA Antrim,F Anulli,M Aoki,T Aoki,JA Aparisi Pozo,MA Aparo,L Aperio Bella,C Appelt,A Apyan,N Aranzabal,C Arcangeletti,ATH Arce,E Arena,J-F Arguin,S Argyropoulos,J-H Arling,AJ Armbruster,O Arnaez,H Arnold,ZP Arrubarrena Tame,G Artoni,H Asada,K Asai,S Asai,NA Asbah,K Assamagan,R Astalos,S Atashi,RJ Atkin,M Atkinson,NB Atlay,H Atmani,PA Atmasiddha,K Augsten,S Auricchio,AD Auriol,VA Austrup,G Avolio,K Axiotis,G Azuelos,D Babal,H Bachacou,K Bachas,A Bachiu,F Backman,A Badea,P Bagnaia,M Bahmani,AJ Bailey,VR Bailey,JT Baines,L Baines,C Bakalis,OK Baker,E Bakos

Journal

The European Physical Journal C

Published Date

2024/3/25

Observation of WZγ Production in pp Collisions at s= 13 TeV with the ATLAS Detector

This Letter reports the observation of W Z γ production and a measurement of its cross section using 140.1±1.2 fb− 1 of proton-proton collision data recorded at a center-of-mass energy of 13 TeV by the ATLAS detector at the Large Hadron Collider. The W Z γ production cross section, with both the W and Z bosons decaying leptonically, p p→ W Z γ→ ℓ′±ν ℓ+ ℓ− γ (ℓ (′)= e, μ), is measured in a fiducial phase-space region defined such that the leptons and the photon have high transverse momentum and the photon is isolated. The cross section is found to be 2.01±0.30 (stat)±0.16 (syst) fb. The corresponding standard model predicted cross section calculated at next-to-leading order in perturbative quantum chromodynamics and at leading order in the electroweak coupling constant is 1.50±0.06 fb. The observed significance of the W Z γ signal is 6.3 σ, compared with an expected significance of 5.0 σ.

Authors

Georges Aad,B Abbott,Kira Abeling,Nils Julius Abicht,SH Abidi,Asmaa Aboulhorma,Halina Abramowicz,Henso Abreu,Yiming Abulaiti,AC Abusleme Hoffman,Bobby Samir Acharya,C Adam Bourdarios,Leszek Adamczyk,Lukas Adamek,SV Addepalli,MJ Addison,Jahred Adelman,Aytül Adiguzel,Tim Adye,AA Affolder,Yoav Afik,Merve Nazlim Agaras,Jinky Agarwala,Anamika Aggarwal,Catalin Agheorghiesei,Ammara Ahmad,Faig Ahmadov,Waleed Syed Ahmed,Sudha Ahuja,Xiaocong Ai,Giulio Aielli,M Ait Tamlihat,Brahim Aitbenchikh,Iakov Aizenberg,Melike Akbiyik,TPA Åkesson,AV Akimov,Daiya Akiyama,Nilima Nilesh Akolkar,Konie Al Khoury,Gian Luigi Alberghi,Justin Albert,Pietro Albicocco,Guillaume Lucas Albouy,Sara Alderweireldt,Martin Aleksa,IN Aleksandrov,Calin Alexa,Theodoros Alexopoulos,Alice Alfonsi,Fabrizio Alfonsi,Malte Algren,Muhammad Alhroob,Babar Ali,HMJ Ali,Shahzad Ali,Samuel William Alibocus,Malik Aliev,Gianluca Alimonti,Wael Alkakhi,Corentin Allaire,BMM Allbrooke,Julia Frances Allen,CA Allendes Flores,Philip Patrick Allport,Alberto Aloisio,Francisco Alonso,Cristiano Alpigiani,M Alvarez Estevez,A Alvarez Fernandez,M Alves Cardoso,MG Alviggi,Mohamed Aly,Y Amaral Coutinho,Alessandro Ambler,Christoph Amelung,Maximilian Amerl,CG Ames,Dante Amidei,SP Amor Dos Santos,Kieran Robert Amos,Viktor Ananiev,Christos Anastopoulos,T Andeen,John Kenneth Anders,Stefio Yosse Andrean,Attilio Andreazza,Stylianos Angelidakis,Aaron Angerami,AV Anisenkov,Alberto Annovi,Claire Antel,Matthew Thomas Anthony,Egor Antipov,Mario Antonelli,DJA Antrim,Fabio Anulli,Masato Aoki,Takumi Aoki,JA Aparisi Pozo,MA Aparo,L Aperio Bella,Christian Appelt,Aram Apyan,N Aranzabal,Chiara Arcangeletti,ATH Arce,Eloisa Arena,Jean-Francois Arguin,Spyros Argyropoulos,Jan-Hendrik Arling,Olivier Arnaez,Hannah Arnold,ZP Arrubarrena Tame,Giacomo Artoni,Haruka Asada,Kanae Asai,Shoji Asai,Nedaa Alexandra Asbah,Jihad Assahsah,K Assamagan,Robert Astalos,S Atashi,Ryan Justin Atkin,M Atkinson,Naim Bora Atlay,Hicham Atmani,PA Atmasiddha,Kamil Augsten,Silvia Auricchio,AD Auriol,Volker Andreas Austrup,Giuseppe Avolio,Konstantinos Axiotis,Georges Azuelos,Dominik Babal,Henri Bachacou,Konstantinos Bachas,Alexander Bachiu,F Backman,Anthony Badea,Paolo Bagnaia,Marzieh Bahmani,AJ Bailey,VR Bailey,JT Baines,Luke Baines,Christos Bakalis,OK Baker,Evelin Bakos

Journal

Physical review letters

Published Date

2024/1/12

A quasar-galaxy merger at : black hole mass and quasar properties from the NIRSpec spectrum

We present JWST/NIRSpec integral field data of the quasar PJ308-21 at . As shown by previous ALMA and HST imaging, the quasar has two companion sources, interacting with the quasar host galaxy. The high-resolution G395H/290LP NIRSpec spectrum covers the wavelength range and shows the rest-frame optical emission of the quasar with exquisite quality ( per spectral element). Based on the H line from the broad line region, we obtain an estimate of the black hole mass . This value is within a factor of the H-based black hole mass from the same spectrum () and is consistent with a previous estimate relying on the MgII (). All these are within the dex intrinsic scatter of the adopted mass calibrations. The high Eddington ratio of PJ308-21 () is in line with the overall quasar population at . The relative strengths of the [OIII], FeII and H lines are consistent with the empirical "Eigenvector 1" correlations as observed for low redshift quasars. We find evidence for blueshifted [OIII] emission with a velocity offset km s from the systemic velocity and a km s. This may be the signature of an outflow from the nuclear region, despite the true values of and are likely more uncertain due to the blending with H and FeII lines. Our study demonstrates the unique capabilities of NIRSpec in capturing quasar spectra at cosmic dawn and studying their properties in unprecedented detail.

Authors

Federica Loiacono,Roberto Decarli,Marco Mignoli,Emanuele Paolo Farina,Eduardo Bañados,Sarah Bosman,Anna-Christina Eilers,Jan-Torge Schindler,Michael A Strauss,Marianne Vestergaard,Feige Wang,Laura Blecha,Chris L Carilli,Andrea Comastri,Thomas Connor,Tiago Costa,Massimo Dotti,Xiaohui Fan,Roberto Gilli,Hyunsung D Jun,Weizhe Liu,Alessandro Lupi,Madeline A Marshall,Chiara Mazzucchelli,Romain A Meyer,Marcel Neeleman,Roderik Overzier,Antonio Pensabene,Dominik A Riechers,Benny Trakhtenbrot,Maxime Trebitsch,Bram Venemans,Fabian Walter,Jinyi Yang

Journal

arXiv preprint arXiv:2402.13319

Published Date

2024/2/20

2017 BG231

2017 BG231 - NASA/ADS Now on home page ads icon ads Enable full ADS view NASA/ADS 2017 BG231 Suto, Y. ; Nakata, F. ; Nakajima, K. ; Armstrong, R. ; Yamauchi, A. ; Harasawa, S. ; Hsieh, B. -C. ; Lin, Y. -T. ; Okabe, N. ; Aihara, H. ; Kokubo, M. ; MacArthur, LA ; Yamamoto, N. ; Mawatari, K. ; Strauss, MA ; Furusawa, J. ; Yamashita, T. ; Osato, K. ; Plazas Malagón, AA ; Yamada, Y. ; Li, X. ; Furusawa, H. ; Komiyama, Y. ; Tang, S. ; Lust, NB ; Liang, Y. ; Ando, M. ; Ikeda, H. ; Lupton, RH ; Rykoff, ES ; Sugimori, K. ; Oguri, M. ; Pan, Y. -C. ; Terai, T. ; Ito, K. ; Mineo, S. ; Kodama, T. ; Bosch, J. ; Koike, M. ; Uchiyama, H. ; Vijarnwannaluk, B. ; Shibuya, T. ; AlSayyad, Y. ; Iwata, I. ; Takita, S. ; Suzuki, N. ; Takada, M. ; Turner, EL ; Takata, T. ; More, S. and 18 more Abstract Publication: Minor Planet Electronic Circulars Pub Date: March 2024 DOI: 10.48377/MPEC/2024-F77 Bibcode: 2024MPEC....F...77. Keywords: Small Solar System …

Authors

Y Suto,F Nakata,K Nakajima,R Armstrong,A Yamauchi,S Harasawa,B-C Hsieh,Y-T Lin,N Okabe,H Aihara,M Kokubo,LA MacArthur,N Yamamoto,K Mawatari,MA Strauss,J Furusawa,T Yamashita,K Osato,AA Plazas Malagón,Y Yamada,X Li,H Furusawa,Y Komiyama,S Tang,NB Lust,Y Liang,M Ando,H Ikeda,RH Lupton,ES Rykoff,K Sugimori,M Oguri,Y-C Pan,T Terai,K Ito,S Mineo,T Kodama,J Bosch,M Koike,H Uchiyama,B Vijarnwannaluk,T Shibuya,Y AlSayyad,I Iwata,S Takita,N Suzuki,M Takada,EL Turner,T Takata,S More,Y Takagi,CZ Waters,H Miyatake,T Morishima,E Egami,M Ouchi,SL Reed,DS Taranu,Y Okura,Y Ono,PA Price,M Tanaka,Y Harikane,Y Toba,H Murayama,AJ Nishizawa,S Miyazaki,M Simunovic

Journal

Minor Planet Electronic Circulars

Published Date

2024/3

Professor FAQs

What is Michael A. Strauss's h-index at Princeton University?

The h-index of Michael A. Strauss has been 111 since 2020 and 207 in total.

What are Michael A. Strauss's top articles?

The articles with the titles of

Gemini Near Infrared Spectrograph--Distant Quasar Survey: Rest-Frame Ultraviolet-Optical Spectral Properties of Broad Absorption Line Quasars

Euclid preparation. The Near-IR Background Dipole Experiment with Euclid

2019 VZ50

Measurement of the Centrality Dependence of the Dijet Yield in p+ Pb Collisions at sNN= 8.16 TeV with the ATLAS Detector

A precise measurement of the Z-boson double-differential transverse momentum and rapidity distributions in the full phase space of the decay leptons with the ATLAS …

Observation of WZγ Production in pp Collisions at s= 13 TeV with the ATLAS Detector

A quasar-galaxy merger at : black hole mass and quasar properties from the NIRSpec spectrum

2017 BG231

...

are the top articles of Michael A. Strauss at Princeton University.