Article
Astronomy & Astrophysics
Zhengyi Wang, Ji Yao, Xiangkun Liu, Dezi Liu, Zuhui Fan, Bin Hu
Summary: We conducted a forecast study on the cross-correlation between cosmic shear tomography from CSST and CMB lensing from AliCPT-1 in Tibet. By generating correlated galaxy and CMB lensing signals, we accounted for various sources of error and estimated the cross-spectra in four tomographic bins. The total cross-correlation SNR was found to be approximately 15 (AliCPT-1 '4 modules*yr') and 22 (AliCPT-1 '48 modules*yr').
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Marika Asgari, Indiarose Friswell, Mijin Yoon, Catherine Heymans, Andrej Dvornik, Benjamin Joachimi, Patrick Simon, Joe Zuntz
Summary: The study introduces a mitigation strategy to reduce the impact of non-linear galaxy bias on the joint cosmological analysis of weak lensing and galaxy surveys, utilizing Psi-statistic to minimize contributions from smallest physical scales and showing comparable constraining power to standard two-point galaxy clustering statistics. It demonstrates a significant decrease in bias on cosmological parameter S-8 when analyzing Psi-statistics compared to standard two-point correlation functions, highlighting the importance of moving towards new statistics less sensitive to smallest physical scales in 3 x 2pt analyses.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
A. Kovacs, P. Vielzeuf, I Ferrero, P. Fosalba, U. Demirbozan, R. Miquel, C. Chang, N. Hamaus, G. Pollina, K. Bechtol, M. Becker, A. Carnero Rosell, M. Carrasco Kind, R. Cawthon, M. Crocce, A. Drlica-Wagner, J. Elvin-Poole, M. Gatti, G. Giannini, R. A. Gruendl, A. Porredon, A. J. Ross, E. S. Rykoff, I Sevilla-Noarbe, E. Sheldon, B. Yanny, T. Abbott, M. Aguena, S. Allam, J. Annis, D. Bacon, G. Bernstein, E. Bertin, S. Bocquet, D. Brooks, D. Burke, J. Carretero, F. J. Castander, M. Costanzi, L. N. da Costa, M. E. S. Pereira, J. De Vicente, S. Desai, H. T. Diehl, J. Dietrich, A. Ferte, B. Flaugher, J. Frieman, J. Garcia-Bellido, E. Gaztanaga, D. Gerdes, T. Giannantonio, D. Gruen, J. Gschwend, G. Gutierrez, S. Hinton, D. L. Hollowood, K. Honscheid, D. Huterer, K. Kuehn, O. Lahav, M. Lima, M. March, J. Marshall, P. Melchior, F. Menanteau, R. Morgan, J. Muir, R. Ogando, A. Palmese, F. Paz-Chinchon, A. Pieres, A. Plazas Malagon, M. Rodriguez Monroy, A. Roodman, E. Sanchez, M. Schubnell, S. Serrano, M. Smith, E. Suchyta, G. Tarle, D. Thomas, C-H To, T. N. Varga, J. Weller
Summary: In this analysis, the CMB lensing signal from cosmic voids and superclusters is studied. The measured signal is lower than expected, particularly in the void centre region. The combination of voids and superclusters provides a 10.3 sigma detection, but the overall signal is 2.3 sigma weaker than expected.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Yin-Zhe Ma, Yan Gong, Tilman Troster, Ludovic Van Waerbeke
Summary: The study compared the universal pressure profile (UPP) with measurements of the thermal Sunyaev-Zeldovich (tSZ) effect and weak gravitational lensing, finding consistent UPP parameters under fixed cosmology. The most constrained parameters were the pressure profile concentration c(500) and shape index alpha.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Zhuoqi (Jackie) Zhang, Yuuki Omori, Chihway Chang
Summary: This study examines the probability density function of the cosmic microwave background (CMB) convergence field and finds that the overall distribution is slightly non-Gaussian due to primordial non-Gaussianities and contributions from structures at low redshifts. By modelling the distribution of galaxies and subtracting the late-time component from the original CMB lensing map, a high-redshift mass map is obtained, allowing for the direct study of early phases of structure formation. The detectability of non-Gaussianity signatures from non-linear structure formation at z > 1.2 is forecasted in this work, and it is found that current surveys may face challenges in detecting such signatures, while future experiments like the deep field of CMB-S4 will have the capability to make detections at & SIM;7 & sigma;.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Omar Darwish, Mathew S. Madhavacheril, Blake D. Sherwin, Simone Aiola, Nicholas Battaglia, James A. Beall, Daniel T. Becker, J. Richard Bond, Erminia Calabrese, Steve K. Choi, Mark J. Devlin, Jo Dunkley, Rolando Dunner, Simone Ferraro, Anna E. Fox, Patricio A. Gallardo, Yilun Guan, Mark Halpern, Dongwon Han, Matthew Hasselfield, J. Colin Hill, Gene C. Hilton, Matt Hilton, Adam D. Hincks, Shuay-Pwu Patty Ho, J. Hubmayr, John P. Hughes, Brian J. Koopman, Arthur Kosowsky, J. Van Lanen, Thibaut Louis, Marius Lungu, Amanda MacInnis, Loic Maurin, Jeffrey McMahon, Kavilan Moodley, Sigurd Naess, Toshiya Namikawa, Federico Nati, Laura Newburgh, John P. Nibarger, Michael D. Niemack, Lyman A. Page, Bruce Partridge, Frank J. Qu, Naomi Robertson, Alessandro Schillaci, Benjamin Schmitt, Neelima Sehgal, Cristobal Sifon, David N. Spergel, Suzanne Staggs, Emilie Storer, Alexander van Engelen, Edward J. Wollack
Summary: Using data from 2014 and 2015 seasons of observation with the ACT, cosmic microwave background lensing mass maps were constructed and a novel cleaning procedure was used to remove thermal SZ contamination. The cross-spectrum between the cleaned lensing map and the BOSS CMASS galaxy sample was detected at 10 sigma significance. These results lay the foundation for future lensing cross-correlation science with ACT data.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Qianjun Hang, Shadab Alam, Yan-Chuan Cai, John A. Peacock
Summary: In this study, the imprints of large-scale structures on the Cosmic Microwave Background (CMB) were studied through CMB lensing and Integrated Sachs-Wolfe (ISW) signals. The stacked CMB lensing signal was found to be consistent with data, while the stacked ISW signal did not show a significant signal from voids and the signal from clusters was weakly detected. These results strongly deviate from previous claims of ISW signals at levels exceeding the Lambda CDM prediction. The comparison with past work and possible explanations for this discrepancy were also discussed.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Cristian Barrera-Hinojosa, Baojiu Li, Yan-Chuan Cai
Summary: This research explores the possibility of detecting the gravitomagnetic field through cross-correlations. By cross-correlating the weak-lensing convergence field with the cosmic microwave background temperature map, the researchers were able to extract the gravitomagnetic effect. The study found that insufficient simulation resolution can introduce significant spurious correlations between the weak-lensing convergence field and the kinetic Sunyaev-Zel'dovich effect.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
A. Kovacs, N. Jeffrey, M. Gatti, C. Chang, L. Whiteway, N. Hamaus, O. Lahav, G. Pollina, D. Bacon, T. Kacprzak, B. Mawdsley, S. Nadathur, D. Zeurcher, J. Garcia-Bellido, A. Alarcon, A. Amon, K. Bechtol, G. M. Bernstein, A. Campos, A. Carnero Rosell, M. Carrasco Kind, R. Cawthon, R. Chen, A. Choi, J. Cordero, C. Davis, J. DeRose, C. Doux, A. Drlica-Wagner, K. Eckert, F. Elsner, J. Elvin-Poole, S. Everett, A. Ferte, G. Giannini, D. Gruen, R. A. Gruendl, I Harrison, W. G. Hartley, K. Herner, E. M. Huff, D. Huterer, N. Kuropatkin, M. Jarvis, P. F. Leget, N. MacCrann, J. McCullough, J. Muir, J. Myles, A. Navarro-Alsina, S. Pandey, J. Prat, M. Raveri, R. P. Rollins, A. J. Ross, E. S. Rykoff, C. Sanchez, L. F. Secco, I Sevilla-Noarbe, E. Sheldon, T. Shin, M. A. Troxel, I Tutusaus, T. N. Varga, B. Yanny, B. Yin, Y. Zhang, J. Zuntz, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, D. Brooks, D. Burke, J. Carretero, M. Costanzi, L. N. da Costa, M. E. S. Pereira, T. Davis, J. De Vicente, S. Desai, H. T. Diehl, I Ferrero, B. Flaugher, P. Fosalba, J. Frieman, E. Gaztanaga, D. Gerdes, T. Giannantonio, J. Gschwend, G. Gutierrez, S. Hinton, D. L. Hollowood, K. Honscheid, D. James, K. Kuehn, M. Lima, M. A. G. Maia, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Morgan, R. Ogando, F. Paz-Chinchon, A. Pieres, A. A. Plazas, M. Rodriguez Monroy, K. Romer, A. Roodman, E. Sanchez, M. Schubnell, S. Serrano, M. Smith, M. Soares-Santos, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, C-H To, J. Weller
Summary: The study confirms the detection of the Eridanus supervoid as a significant underdensity in the Cold Spot's direction, with a lower lensing signal amplitude than expected. The results emphasize the causal relation between these individually rare structures in the cosmic web and in the Cosmic Microwave Background, encouraging more detailed future surveys in the Cold Spot region.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Boryana Hadzhiyska, S. Yuan, C. Blake, D. J. Eisenstein, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, N. Emas, J. E. Forero-Romero, C. Garcia-Quintero, M. Ishak, S. Joudaki, E. Jullo, R. Kehoe, T. Kisner, A. Kremin, A. Krolewski, M. Landriau, J. U. Lange, M. Manera, R. Miquel, Jundan Nie, C. Poppett, A. Porredon, G. Rossi, R. Ruggeri, C. Saulder, M. Schubnell, G. Tarle, B. A. Weaver, E. Xhakaj, Zhimin Zhou
Summary: The joint analysis of different cosmological probes can provide valuable insights into the nature of the primordial Universe, dark energy, and dark matter. This study presents high-resolution weak lensing maps and accompanying mock catalogues, which can be used to study these cosmological problems in more detail.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Ji Yao, Huanyuan Shan, Pengjie Zhang, Xiangkun Liu, Catherine Heymans, Benjamin Joachimi, Marika Asgari, Maciej Bilicki, Hendrik Hildebrandt, Konrad Kuijken, Tilman Troster, Jan Luca van den Busch, Angus Wright, Ziang Yan
Summary: In this study, the impact of intrinsic alignments on the Kilo-Degree Survey (KiDS) galaxy lensing shear and Planck CMB lensing convergence cross-correlation is investigated and compared to previous treatments. The results show that using the IA self-calibration method can effectively break the degeneracy between CMB lensing and IA, providing the best-fit values. Moreover, appropriate treatment of the boost factor, cosmic magnification, and photometric redshift modeling is crucial for obtaining accurate IA and cosmological results.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Dongwoo T. Chung
Summary: The field of millimetre-wave line-intensity mapping is seeing increased experimental activity. A future photometric galaxy survey programme along with the Rubin Observatory Legacy Survey of Space and Time will enable cross-correlation detection and provide competitive constraints on cosmic molecular gas density and astrophysical parameters.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Jozef Bucko, Sambit K. Giri, Aurel Schneider
Summary: From observations at low and high redshifts, it is well known that the bulk of dark matter (DM) has to be stable or very long-lived, but the possibility of a small fraction or all of the DM decaying with a significantly longer half-life time than the age of the Universe is not ruled out. In this study, the researchers investigated models in which a fraction or all DM decays into radiation, focusing on the long-lived regime. They used data from the Kilo-Degree Survey (KiDS) for weak-lensing analysis and CMB data from Planck. The results showed that the constraints on DM decay are more stringent from CMB data than from weak-lensing data.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Leonardo Giani, Cullan Howlett, Rossana Ruggeri, Federico Bianchini, Khaled Said, Tamara M. Davis
Summary: We investigate the cross correlation between radial peculiar velocities (PV) and lensing convergence of cosmic microwave background (CMB) photons for the first time. The theoretical expectations for the signal and its covariance are derived and the detectability with existing and forthcoming surveys is assessed. The study reveals that such cross-correlations can improve constraints on gravitational models by breaking degeneracies with matter density. Additionally, the distance-scaling dispersion of peculiar velocities is identified as the main source of noise in the cross correlation. When assuming a redshift-independent scatter for PV, the study shows that the cross correlation may be detected in the future using PV measurements from DESI and convergence map from CMB-S4.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Qianjun Hang, Shadab Alam, John A. Peacock, Yan-Chuan Cai
Summary: Using data from the DESI Legacy Survey, research investigated the galaxy density field in tomographic slices covering the redshift range 0 < z < 0.8. Cross-correlation analysis of photometric redshifts and CMB maps revealed the growth of structure since z = 0.8. In the context of Lambda CDM, a reduction in fluctuation normalization or matter density was found to be necessary based on the results from lensing and CMB analysis.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)