Authors
R Abbott, H Abe, F Acernese, K Ackley, N Adhikari, RX Adhikari, VK Adkins, VB Adya, C Affeldt, D Agarwal, M Agathos, K Agatsuma, N Aggarwal, Odylio Denys de Aguiar, L Aiello, A Ain, P Ajith, T Akutsu, S Albanesi, RA Alfaidi, A Allocca, PA Altin, A Amato, C Anand, S Anand, A Ananyeva, SB Anderson, WG Anderson, M Ando, T Andrade, N Andres, M Andrés-Carcasona, T Andric, SV Angelova, 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, KG Arun, H Asada, Y Asali, G Ashton, Y Aso, M Assiduo, S Assis De Souza Melo, SM Aston, P Astone, F Aubin, K AultONeal, C Austin, S Babak, F Badaracco, MKM Bader, C Badger, S Bae, Y Bae, AM Baer, S Bagnasco, Y Bai, J Baird, R Bajpai, T Baka, M Ball, G Ballardin, SW Ballmer, A Balsamo, G Baltus, S Banagiri, B Banerjee, D Bankar, JC Barayoga, C Barbieri, R Barbieri, 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, BR Becher, B Bécsy, VM Bedakihale, Freija Beirnaert, M Bejger, I Belahcene, V Benedetto, D Beniwal, MG Benjamin, TF Bennett, JD Bentley, M BenYaala, S Bera, M Berbel, F Bergamin, BK Berger, S Bernuzzi, 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, G Billingsley, M Bilicki, S Bini, R Birney, O Birnholtz, S Biscans, M Bischi, S Biscoveanu, A Bisht, B Biswas, M Bitossi, MA Bizouard, JK Blackburn, CD Blair, DG Blair, RM Blair, F Bobba, N Bode
Publication date
2023/6/1
Journal
Astrophysical Journal
Volume
949
Issue
2
Pages
1-37
Publisher
IOP Publishing Ltd.
Description
The discovery of a gravitational wave (GW) signal from a binary neutron star (BNS) merger (Abbott et al. 2017a) and the kilonova emission from its remnant (Coulter et al. 2017; Abbott et al. 2017b) provided the first GW standard siren measurement of the cosmic expansion history (Abbott et al. 2017c). As pointed out by Schutz (1986), the GW signal from a compact binary coalescence directly measures the luminosity distance to the source without any additional distance calibrator, earning these sources the name “standard sirens”(Holz & Hughes 2005). Measuring the cosmic expansion as a function of the cosmological redshift is one of the key avenues with which to explore the constituents of the universe, along with the other canonical probes such as the cosmic microwave background (CMB; Spergel et al. 2003, 2007; Komatsu et al. 2011; Ade et al. 2014, 2016; Aghanim et al. 2020), baryon acoustic oscillations …
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R Abbott, H Abe, F Acernese, K Ackley, N Adhikari… - Astrophysical Journal, 2023