Article
Astronomy & Astrophysics
Ginevra Favole, Benjamin R. Granett, Javier Silva Lafaurie, Domenico Sapone
Summary: The study investigates the jackknife method for internal covariance estimation in large-scale structure surveys, exploring the impact of jackknife size and number of resamplings on the precision of the covariance estimate and errors in cosmological parameters. Results show that the baryon acoustic scale error estimate is independent of the jackknife scale, while the shift parameter a exhibits variations in error estimates from different datasets.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Boryana Hadzhiyska, Sonya Liu, Rachel S. Somerville, Austen Gabrielpillai, Sownak Bose, Daniel Eisenstein, Lars Hernquist
Summary: In this study, two galaxy models (Illustris'ING and SC-SAM) were compared for their predictions on large scale structure observables for stellar mass selected samples at z=0. The models show good agreement in two-point clustering and galaxy assembly bias, but differences in areas such as halo gas content correlation with environment and occupancy predictions for low-mass haloes. Higher order statistics help accurately describe the galaxy distribution and differentiate between models showing similar behavior in two-point statistics. SAMs are suggested as a promising method for generating mock catalogues for future cosmological surveys.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Sownak Bose, Boryana Hadzhiyska, Monica Barrera, Ana Maria Delgado, Fulvio Ferlito, Carlos Frenk, Cesar Hernandez-Aguayo, Lars Hernquist, Rahul Kannan, Ruediger Pakmor, Volker Springel, Simon D. M. White
Summary: Modern redshift surveys are mapping the distribution of galaxies on enormous distance scales. However, current hydrodynamical simulations cannot reach the volumes needed for upcoming surveys. A new, large volume hydrodynamical simulation called MillenniumTNG (MTNG) is able to accurately reproduce the observed clustering of galaxies, but there are discrepancies when separated by color. This is due to the quenching of satellite galaxies in the model.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
E. Perez-Hernandez, S. N. Kemp, V. H. Ramirez-Siordia, A. Nigoche-Netro
Summary: This study presents a comprehensive investigation of deep optical long-slit spectroscopy and deep broad-band photometry of NGC 6086. The results reveal the presence of two separate structures in NGC 6086 and the existence of an envelope. Additionally, the study finds radial discontinuity in the distribution of galaxies in the cluster A2162, indicating the need for further investigation of the cluster's kinematics.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Xue Ge, Qiu-Sheng Gu, Ruben Garcia-Benito, Shi-Ying Lu, Cheng-Long Lei, Nan Ding
Summary: This study presents observations of four dwarf lenticular galaxies with multiple star formation regions, showing that these galaxies exhibit significant rotation and follow the Kennicutt-Schmidt law in their star formation processes. The gas-phase metallicities in star-forming regions of these galaxies are lower, indicating that extended star formation may be related to abundant atomic hydrogen, a long dynamic time-scale, and a low-density environment.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Bruno J. De Bortoli, Juan P. Caso, Ana Ennis, Lilia P. Bassino
Summary: An analysis of the radial distribution of globular clusters in early-type galaxies (ETGs) reveals a second-order dependence on environmental density, indicating the evolution of the host galaxies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Shogo Masaki, Daichi Kashino, Shogo Shogo, Yen-Ting Lin
Summary: We propose a new subhalo abundance matching (SHAM) model that uses the virial mass of the main progenitor of each (sub)halo as a proxy for the observed galaxy stellar mass. This model can predict the two-point correlation functions depending on the chosen epoch. Applying this model to measured angular correlation functions, we find that it reproduces the observations well and is a better proxy for the galaxy stellar mass than the widely used V-peak model.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
M. Celeste Artale, Markus Haider, Antonio D. Montero-Dorta, Mark Vogelsberger, Davide Martizzi, Paul Torrey, Simeon Bird, Lars Hernquist, Federico Marinacci
Summary: The study examines the distribution and evolution of seven ionized metals in different cosmic structures and gas phases in a cosmological simulation. It reveals different patterns in the distribution and evolution of ionized metals, offering a new perspective on baryon distribution and evolution across cosmic time and providing new clues to the missing baryons problem.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
M. J. M. Marcha, I. W. A. Browne
Summary: Evidence for large-scale clustering is found among Fermi-selected BL Lac objects, but not among Fermi-selected FSRQs. High-latitude Fermi sources as a whole show a significant clustering signal on scales up to 30 degrees, while this signal may be washed out in FSRQs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Nagisa Hiroshima, Shin'ichiro Ando, Tomoaki Ishiyama
Summary: This article introduces a model for describing the properties of subhalo mass functions, and investigates the effects of Poisson fluctuation, host-mass scatter, and tidal evolution models on observables in the current Universe.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Juan P. Caso
Summary: The mass profile of NGC 3377, a moderately bright elliptical galaxy, is studied using a spherical Jeans analysis. The analysis suggests the presence of an intermediate mass dark matter halo.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Daniele Sorini, Romeel Dave, Weiguang Cui, Sarah Appleby
Summary: The study indicates that star formation in galaxies and AGN jets have significant impacts on the distribution of matter, especially causing baryon evacuation at different redshifts. In larger systems, AGN jets are particularly efficient in evacuating baryons, leading to the majority of baryonic mass being in the IGM.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Junkai Zhang, Stijn Wuyts, Callum Witten, Charlotte R. Avery, Lei Hao, Raman Sharma, Juntai Shen, Jun Toshikawa, Carolin Villforth
Summary: The study suggests that spheroidal 3D shapes of quiescent galaxies become more abundant at larger masses in the last half of cosmic history, with the most massive galaxies having the highest ex situ stellar mass fractions. Larger differences in shapes between observations and simulations are found at low to intermediate masses. The study also reveals an environmental influence on galaxy shape, with quiescent galaxies tending to be rounder in denser environments at higher masses.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Richard Watkins, Trey Allen, Collin James Bradford, Albert Ramon Jr, Alexandra Walker, Hume A. Feldman, Rachel Cionitti, Yara Al-Shorman, Ehsan Kourkchi, R. Brent Tully
Summary: We estimated the bulk flow in a volume of radii 150-200 h(-1) Mpc using the minimum variance method with data from the CosmicFlows-4 (CF4) catalogue. The addition of new data in the CF4 increased the estimate of the bulk flow in a sphere of radius 150 h(-1) Mpc compared to the CosmicFlows-3 (CF3). The bulk flow in CF4 has a low probability of occurring in the standard cosmological model, and on scales of 200 h(-1) Mpc, it is in even greater tension with the standard model.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Santiago Avila, Adrian Gutierrez Adame
Summary: The Fix and Pair techniques can reduce the variance in two-point statistics by modifying the initial conditions. This technique is also valid when there are local primordial nonGaussianities (PNG), reducing their variance without biasing the two-point statistics. By Matching the stochastic part of the initial conditions for different cosmologies, a large correlation between the statistics can be obtained, further reducing the uncertainty of the model testing.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Richard A. Battye, Michael L. Brown, Caitlin M. Casey, Ian Harrison, Neal J. Jackson, Ian Smail, Robert A. Watson, Christopher A. Hales, Sinclaire M. Manning, Chao-Ling Hung, Christopher J. Riseley, Filipe B. Abdalla, Mark Birkinshaw, Constantinos Demetroullas, Scott Chapman, Robert J. Beswick, Tom W. B. Muxlow, Anna Bonaldi, Stefano Camera, Tom Hillier, Scott T. Kay, Aaron Peters, David B. Sanders, Daniel B. Thomas, A. P. Thomson, Ben Tunbridge, Lee Whittaker
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2020)
Article
Astronomy & Astrophysics
Jiajun Zhang, Pablo Motta, Camila P. Novaes, Filipe B. Abdalla, Andre A. Costa, Bin Wang, Zhenghao Zhu, Chenxi Shan, Haiguang Xu, Elcio Abdalla, Luciano Barosi, Francisco A. Brito, Amilcar Queiroz, Thyrso Villela, Carlos A. Wuensche, Elisa G. M. Ferreira, Karin S. F. Fornazier, Alessandro Marins, Larissa Santos, Marcelo Vargas dos Santos, Ricardo G. Landim, Vincenzo Liccardo
Summary: This study introduces a method for generating mock maps of the 21 cm intensity mapping signal for the BINGO telescope and investigates the information about structure formation, Hi distribution, and Hi mass-halo mass relation contained in 21 cm intensity mapping observations. The results show that the theoretical calculation can fit the mock result at large scales but fails to provide an accurate fitting at small scales, indicating a poor understanding of the nonlinear distribution of Hi and its scale-dependent bias. The study also finds that the bias is highly sensitive to the method of populating Hi in halos, providing the potential for constraining the Hi distribution in halos through 21 cm intensity mapping observations. Furthermore, it is illustrated that the Finger-of-God effect can only be discriminated with thin frequency bins.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Vincenzo Liccardo, Eduardo J. de Mericia, Carlos A. Wuensche, Elcio Abdalla, Filipe B. Abdalla, Luciano Barosi, Francisco A. Brito, Amilcar Queiroz, Thyrso Villela, Michael W. Peel, Bin Wang, Andre A. Costa, Elisa G. M. Ferreira, Karin S. F. Fornazier, Camila P. Novaes, Larissa Santos, Marcelo dos Santos, Mathieu Remazeilles, Jiajun Zhang, Clive Dickinson, Stuart Harper, Ricardo G. Landim, Alessandro Marins, Frederico Vieira
Summary: In this study, we simulated the operation of the BINGO radio telescope and generated corresponding sky maps. We also evaluated the efficiency of the GNILC method using these maps. The results show that we have optimized the telescope design and demonstrated the feasibility of extracting cosmological signals using the GNILC method.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Elcio Abdalla, Elisa G. M. Ferreira, Ricardo G. Landim, Andre A. Costa, Karin S. F. Fornazier, Filipe B. Abdalla, Luciano Barosi, Francisco A. Brito, Amilcar R. Queiroz, Thyrso Villela, Bin Wang, Carlos A. Wuensche, Alessandro Marins, Camila P. Novaes, Vincenzo Liccardo, Chenxi Shan, Jiajun Zhang, Zhongli Zhang, Zhenghao Zhu, Ian Browne, Jacques Delabrouille, Larissa Santos, Marcelo dos Santos, Haiguang Xu, Sonia Anton, Richard Battye, Tianyue Chen, Clive Dickinson, Yin-Zhe Ma, Bruno Maffei, Eduardo J. de Mericia, Pablo Motta, Carlos H. N. Otobone, Michael W. Peel, Sambit Roychowdhury, Mathieu Remazeilles, Rafael M. Ribeiro, Yu Sang, Joao R. L. Santos, Juliana F. R. dos Santos, Gustavo B. Silva, Frederico Vieira, Jordany Vieira, Linfeng Xiao, Xue Zhang, Yongkai Zhu
Summary: The BINGO project is a unique radio telescope designed to study cosmology and astrophysics through observations of the redshifted 21-cm line of neutral hydrogen. It aims to detect the low redshift baryon acoustic oscillations (BAO) to constrain dark matter models and test the Lambda CDM model. The project utilizes intensity mapping to create a 3D map of the neutral hydrogen distribution and has the potential to discover fast radio bursts (FRBs) and other transients.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Karin S. F. Fornazier, Filipe B. Abdalla, Mathieu Remazeilles, Jordany Vieira, Alessandro Marins, Elcio Abdalla, Larissa Santos, Jacques Delabrouille, Eduardo Mericia, Ricardo G. Landim, Elisa G. M. Ferreira, Luciano Barosi, Amilcar R. Queiroz, Thyrso Villela, Bin Wang, Carlos A. Wuensche, Andre A. Costa, Vincenzo Liccardo, Camila Paiva Novaes, Michael W. Peel, Marcelo dos Santos, Jiajun Zhang
Summary: This paper investigates the ability of the BINGO survey to separate foreground signals in the observation of the redshifted 21 cm line. Through simulations and analysis of foreground residuals, the study demonstrates the recovery of the redshifted 21 cm signal and its non-Gaussian distribution. The results show that foreground contamination can be reduced below the cosmological signal and noise levels with the proposed methodology.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Carlos A. Wuensche, Thyrso Villela, Elcio Abdalla, Vincenzo Liccardo, Frederico Vieira, Ian Browne, Michael W. Peel, Christopher Radcliffe, Filipe B. Abdalla, Alessandro Marins, Luciano Barosi, Francisco A. Brito, Amilcar R. Queiroz, Bin Wang, Andre A. Costa, Elisa G. M. Ferreira, Karin S. F. Fornazier, Ricardo G. Landim, Camila P. Novaes, Larissa Santos, Marcelo dos Santos, Jiajun Zhang, Tianyue Chen, Jacques Delabrouille, Clive Dickinson, Giancarlo de Gasperis, Edmar C. Gurjao, Stuart Harper, Yin-Zhe Ma, Telmo Machado, Bruno Maffei, Eduardo J. de Mericia, Christian Monstein, Pablo Motta, Carlos H. N. Otobone, Luiz A. Reitano, Mathieu Remazeilles, Sambit Roychowdhury, Joao R. L. Santos, Alexandre J. R. Serres, Andreia P. Souza, Cesar Strauss, Jordany Vieira, Haiguang Xu
Summary: This paper introduces the design and current status of the BINGO radio telescope, which is aimed at detecting baryonic acoustic oscillations in the cosmological Hi signal. BINGO is carefully designed with non-cryogenic receivers and operates in a specific frequency range. Through laboratory and prototype testing, the performance of BINGO closely matches the expected results.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Andre A. Costa, Ricardo G. Landim, Camila P. Novaes, Linfeng Xiao, Elisa G. M. Ferreira, Filipe B. Abdalla, Bin Wang, Elcio Abdalla, Richard A. Battye, Alessandro Marins, Carlos A. Wuensche, Luciano Barosi, Francisco A. Brito, Amilcar R. Queiroz, Thyrso Villela, Karin S. F. Fornazier, Vincenzo Liccardo, Larissa Santos, Marcelo dos Santos, Jiajun Zhang
Summary: This study examines the fiducial setup and capabilities of the BINGO single-dish telescope in constraining cosmological parameters. The results show that combining BINGO with Planck data improves the precision of measurements and constraints on cosmological models. BINGO also provides valuable information on the distribution of neutral hydrogen and can help constrain alternative cosmological models.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Filipe B. Abdalla, Alessandro Marins, Pablo Motta, Elcio Abdalla, Rafael M. Ribeiro, Carlos A. Wuensche, Jacques Delabrouille, Karin S. F. Fornazier, Vincenzo Liccardo, Bruno Maffei, Eduardo J. de Mericia, Carlos H. N. Otobone, Juliana F. R. dos Santos, Gustavo B. Silva, Jordany Vieira, Joao A. M. Barretos, Luciano Barosi, Francisco A. Brito, Amilcar R. Queiroz, Thyrso Villela, Bin Wang, Andre A. Costa, Elisa G. M. Ferreira, Ricardo G. Landim, Camila Paiva Novaes, Michael W. Peel, Larissa Santos, Marcelo dos Santos, Jiajun Zhang
Summary: This paper presents the optical design for the BINGO telescope, including the arrangement of the horns in the focal plane and the properties of the intensity and polarization of the beams. Through modeling and optimization, an optimal configuration for the optical system is obtained, meeting the requirements for the experiment.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Camila P. Novaes, Jiajun Zhang, Eduardo J. de Mericia, Filipe B. Abdalla, Vincenzo Liccardo, Carlos A. Wuensche, Jacques Delabrouille, Mathieu Remazeilles, Larissa Santos, Ricardo G. Landim, Elcio Abdalla, Luciano Barosi, Amilcar Queiroz, Thyrso Villela, Bin Wang, Andre A. Costa, Elisa G. M. Ferreira, Alessandro Marins, Marcelo dos Santos
Summary: This study presents forecasts for measuring the transversal BAO signal during the operation of the BINGO radio telescope. Two clustering estimators, the two-point angular correlation function (ACF) and the angular power spectrum (APS), were used in combination with a template-based method to model the BAO information. The results show that both estimators perform better at higher redshifts, but the APS estimator provides slightly better estimates with smaller uncertainties. Instrumental noise has a greater impact on the results, while foreground residuals do not significantly affect the final uncertainties.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Eduardo. J. J. de Mericia, Larissa C. O. Santos, Carlos Alexandre Wuensche, Vincenzo Liccardo, Camila. P. P. Novaes, Jacques Delabrouille, Mathieu Remazeilles, Filipe. B. B. Abdalla, Chang Feng, Luciano Barosi, Amilcar Queiroz, Thyrso Villela, Bin Wang, Jiajun Zhang, Alessandro Marins, Andre. A. A. Costa, Elisa G. M. Ferreira, Ricardo. G. G. Landim, Marcelo. V. V. dos Santos
Summary: This work analyzes the performance of the GNILC method combined with a power spectrum debiasing procedure in order to optimize the removal of foreground emission and the recovery of the 21 cm signal in a simulated BINGO mission. The results show a near-optimal reconstruction of the HI signal with an average power spectrum reconstruction error of 3% using an 80-bin configuration. The GNILC method is robust against different synchrotron emission models and adding extra channel information can reduce the estimation error of the 21 cm signal.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
M. Brilenkov, K. S. F. Fornazier, L. T. Hergt, G. A. Hoerning, A. Marins, T. Murokoshi, F. Rahman, N. -O. Stutzer, Y. Zhou, F. . B. Abdalla, K. J. Andersen, R. Aurlien, R. Banerji, A. Basyrov, A. Battista, M. Bersanelli, S. Bertocco, S. Bollanos, L. P. L. Colombo, H. K. Eriksen, J. R. Eskilt, M. K. Foss, C. Franceschet, U. Fuskeland, S. Galeotta, M. Galloway, S. Gerakakis, E. Gjerlow, B. Hensley, D. Herman, T. D. Hoang, M. Ieronymaki, H. T. Ihle, J. B. Jewell, A. Karakci, E. Keihanen, R. Keskitalo, G. Maggio, D. Maino, M. Maris, S. Paradiso, B. Partridge, M. Reinecke, A. -S. Suur-Uski, T. L. Svalheim, D. Tavagnacco, H. Thommesen, M. Tomasi, D. J. Watts, I. K. Wehus, A. Zacchei
Summary: This paper addresses the important issue of how to define inputs in terms of sky model and instrument parameters in end-to-end simulations of high-sensitivity cosmic microwave background (CMB) experiments. The authors show that constrained and random simulations lead to significantly different correlation structures and quantify fundamentally different types of uncertainties. These different types of simulations have different and complementary scientific uses.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Multidisciplinary Sciences
Carlos A. Wuensche, Elcio Abdalla, Filipe Abdalla, Luciano Barosi, Bin Wang, Rui An, Joao A. M. Barretos, Richard Battye, Francisco A. Brito, Ian Browne, Daniel Correia, Andre A. Costa, Jacques Delabrouille, Clive Dickinson, Chang Feng, Elisa G. M. Ferreira, Karin Fornazier, Giancarlo De Gasperis, Priscila Gutierrez, Stuart Harper, Ricardo G. Landim, Vincenzo Liccardo, Yin-Zhe Ma, Telmo Machado, Bruno Maffei, Alessandro Marins, Milena M. M. Mendes, Eduardo Mericia, Christian Monstein, Pablo Motta, Camila Novaes, Carlos H. Otobone, Michael Peel, Amilcar R. Queiroz, Christopher Radcliffe, Mathieu Remazeilles, Rafael M. G. Ribeiro, Y. U. Sang, Juliana F. R. Santos, Larissa Santos, Marcelo Santos, Chenxi Shan, Gustavo B. Silva, Frederico Vieira, Jordany Vieira, Thyrso Villela, Linfeng Xiao, Weiqiang Yang, Jiajun Zhang, Xue Zhang, Zenghao Zhu
Summary: BINGO, a unique radio telescope designed to map the intensity of neutral hydrogen distribution at cosmological distances, aims to detect Baryon Acoustic Oscillations (BAO) in the frequency band of 980 MHz - 1260 MHz. The telescope, to be located in Paraiba, Brazil, consists of two 40m mirrors, a feedhorn array with 50 horns, and will work as a drift-scan instrument.
ANAIS DA ACADEMIA BRASILEIRA DE CIENCIAS
(2021)
Article
Astronomy & Astrophysics
C. G. Martz, B. R. McNamara, P. E. J. Nulsen, A. N. Vantyghem, M-J Gingras, Iu Babyk, H. R. Russell, A. C. Edge, M. McDonald, P. D. Tamhane, A. C. Fabian, M. T. Hogan
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
Gerrit Schellenberger, Laurence P. David, Jan Vrtilek, Ewan O'Sullivan, Jeremy Lim, William Forman, Ming Sun, Francoise Combes, Philippe Salome, Christine Jones, Simona Giacintucci, Alastair Edge, Fabio Gastaldello, Pasquale Temi, Fabrizio Brighenti, Sandro Bardelli
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron, Hakim Atek, Peter Capak, Iary Davidzon, Dominique Eckert, David Harvey, Anton M. Koekemoer, Claudia D. P. Lagos, Guillaume Mahler, Mireia Montes, Anna Niemiec, Mario Nonino, P. A. Oesch, Johan Richard, Steven A. Rodney, Matthieu Schaller, Keren Sharon, Louis-Gregory Strolger, Joseph Allingham, Adam Amara, Yannick Bahe, Celine Boehm, Sownak Bose, Rychard J. Bouwens, Larry D. Bradley, Gabriel Brammer, Tom Broadhurst, Rodrigo Canas, Renyue Cen, Benjamin Clement, Douglas Clowe, Dan Coe, Thomas Connor, Behnam Darvish, Jose M. Diego, Harald Ebeling, A. C. Edge, Eiichi Egami, Stefano Ettori, Andreas L. Faisst, Brenda Frye, Lukas J. Furtak, C. Gomez-Guijarro, J. D. Remolina Gonzalez, Anthony Gonzalez, Or Graur, Daniel Gruen, Hagan Hensley, Beryl Hovis-Afflerbach, Pascale Jablonka, Saurabh W. Jha, Eric Julio, Jean-Paul Kneib, Vasily Kokorev, David J. Lagattuta, Marceau Limousin, Anja von der Linden, Nora B. Linzer, Adrian Lopez, Georgios E. Magdis, Richard Massey, Daniel C. Masters, Matteo Maturi, Curtis McCully, Sean L. McGee, Massimo Meneghetti, Bahram Mobasher, Leonidas A. Moustakas, Eric J. Murphy, Priyamvada Natarajan, Mark Neyrinck, Kyle O'Connor, Masamune Oguri, Amanda Pagul, Jason Rhodes, R. Michael Rich, Andrew Robertson, Mauro Sereno, Huanyuan Shan, Graham P. Smith, Albert Sneppen, Gordon K. Squires, Sut-Ieng Tam, Celine Tchernin, Sune Toft, Keiichi Umetsu, John R. Weaver, R. J. van Weeren, Liliya L. R. Williams, Tom J. Wilson, Lin Yan, Adi Zitrin
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2020)