Quasars as standard candles - III. Validation of a new sample for cosmological studies
A&A, 642 (2020) A150
Published online: 2020-10-13
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E S Kammoun, Z Igo, J M Miller, A C Fabian, M T Reynolds, A Merloni, D Barret, E Nardini, P O Petrucci, E Piconcelli, S Barnier, J Buchner, T Dwelly, I Grotova, M Krumpe, T Liu, K Nandra, A Rau, M Salvato, T Urrutia and J WolfMonthly Notices of the Royal Astronomical Society 522 (4) 5217 (2023)
https://doi.org/10.1093/mnras/stad952
S 8 increases with effective redshift in ΛCDM cosmology
S A Adil, Ö Akarsu, M Malekjani, E Ó Colgáin, S Pourojaghi, A A Sen and M M Sheikh-JabbariMonthly Notices of the Royal Astronomical Society: Letters 528 (1) L20 (2023)
https://doi.org/10.1093/mnrasl/slad165
(2023)
https://doi.org/10.2139/ssrn.4646868
Quasars as standard candles
Matilde Signorini, Guido Risaliti, Elisabeta Lusso, Emanuele Nardini, Giada Bargiacchi, Andrea Sacchi and Bartolomeo TrefoloniAstronomy & Astrophysics 676 A143 (2023)
https://doi.org/10.1051/0004-6361/202346104
Tensions with the flat ΛCDM model from high-redshift cosmography
G Bargiacchi, M G Dainotti and S CapozzielloMonthly Notices of the Royal Astronomical Society 525 (2) 3104 (2023)
https://doi.org/10.1093/mnras/stad2326
The most luminous blue quasars at 3.0 < z < 3.3
Bartolomeo Trefoloni, Elisabeta Lusso, Emanuele Nardini, Guido Risaliti, Giada Bargiacchi, Susanna Bisogni, Francesca M. Civano, Martin Elvis, Giuseppina Fabbiano, Roberto Gilli, Alessandro Marconi, Gordon T. Richards, Andrea Sacchi, Francesco Salvestrini, Matilde Signorini and Cristian VignaliAstronomy & Astrophysics 677 A111 (2023)
https://doi.org/10.1051/0004-6361/202346024
Current data are consistent with flat spatial hypersurfaces in the ΛCDM cosmological model but favor more lensing than the model predicts
Javier de Cruz Pérez, Chan-Gyung Park and Bharat RatraPhysical Review D 107 (6) (2023)
https://doi.org/10.1103/PhysRevD.107.063522
Fitting Type Ia Supernova Data to a Cosmological Model Based on Einstein–Newcomb–De Sitter Space
Vladimir N. YershovUniverse 9 (5) 204 (2023)
https://doi.org/10.3390/universe9050204
Cosmological redshift and Hubble tension explained by means of the FLRWT time-metric framework and transit physics in the IGM
Alessandro TrincheraFrontiers in Astronomy and Space Sciences 9 (2023)
https://doi.org/10.3389/fspas.2022.1014433
The jet emitting disk‐standard accretion disk model applied to the active galactic nuclei ultra violet–X‐ray correlation
S. Barnier, P.‐O. Petrucci, J. Ferreira and G. MarcelAstronomische Nachrichten 344 (4) (2023)
https://doi.org/10.1002/asna.20230020
Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius–luminosity relation luminosity distances
Narayan Khadka, Michal Zajaček, Raj Prince, Swayamtrupta Panda, Bożena Czerny, Mary Loli Martínez-Aldama, Vikram Kumar Jaiswal and Bharat RatraMonthly Notices of the Royal Astronomical Society 522 (1) 1247 (2023)
https://doi.org/10.1093/mnras/stad1040
Nonparametric analysis of the Hubble diagram with neural networks
Lorenzo Giambagli, Duccio Fanelli, Guido Risaliti and Matilde SignoriniAstronomy & Astrophysics 678 A13 (2023)
https://doi.org/10.1051/0004-6361/202346236
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https://doi.org/10.1007/978-981-16-4544-0_114-1
The intrinsic X-ray luminosity distribution of an optically selected SDSS quasar population
Amy L Rankine, James Aird, Angel Ruiz and Antonis GeorgakakisMonthly Notices of the Royal Astronomical Society 527 (3) 9004 (2023)
https://doi.org/10.1093/mnras/stad3686
Seven Hints That Early-Time New Physics Alone Is Not Sufficient to Solve the Hubble Tension
Sunny VagnozziUniverse 9 (9) 393 (2023)
https://doi.org/10.3390/universe9090393
Shadows of black holes at cosmological distances in the co-varying physical couplings framework
R R Cuzinatto, C A M de Melo and Juliano C S NevesMonthly Notices of the Royal Astronomical Society 526 (3) 3987 (2023)
https://doi.org/10.1093/mnras/stad2954
Constraining Coupling Constants’ Variation with Supernovae, Quasars, and GRBs
Rajendra GuptaSymmetry 15 (2) 259 (2023)
https://doi.org/10.3390/sym15020259
Tracking the spectral properties of ESO 511-G030 across different epochs
R. Middei, P.-O. Petrucci, S. Bianchi, et al.Astronomy & Astrophysics 672 A101 (2023)
https://doi.org/10.1051/0004-6361/202244022
Spectral energy distribution profiles from AGN accretion disc in multigap set-up
Marcel Štolc, Michal Zajaček, Bożena Czerny and Vladimír KarasMonthly Notices of the Royal Astronomical Society 522 (2) 2869 (2023)
https://doi.org/10.1093/mnras/stad1127
The universal shape of the X-ray variability power spectrum of AGN up to z ∼ 3
M. Paolillo, I. E. Papadakis, W. N. Brandt, et al.Astronomy & Astrophysics 673 A68 (2023)
https://doi.org/10.1051/0004-6361/202245291
Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
Maria Giovanna Dainotti, Giada Bargiacchi, Malgorzata Bogdan, Aleksander Lukasz Lenart, Kazunari Iwasaki, Salvatore Capozziello, Bing Zhang and Nissim FraijaThe Astrophysical Journal 951 (1) 63 (2023)
https://doi.org/10.3847/1538-4357/acd63f
Quasars: Standard Candles up to z = 7.5 with the Precision of Supernovae Ia
M. G. Dainotti, G. Bargiacchi, A. Ł. Lenart, S. Nagataki and S. CapozzielloThe Astrophysical Journal 950 (1) 45 (2023)
https://doi.org/10.3847/1538-4357/accea0