Zobrazeno 1 - 10
of 232
pro vyhledávání: '"D. Fassnacht"'
Autor:
Devon M Powell, Simona Vegetti, J P McKean, Cristiana Spingola, Hannah R Stacey, Christopher D Fassnacht
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 516, 1808-1828. Oxford University Press
We investigate the mass structure of a strong gravitational lens galaxy at $z=0.350$, taking advantage of the milli-arcsecond (mas) angular resolution of very long baseline interferometric (VLBI) observations. In the first analysis of its kind at thi
Autor:
Geoff C-F Chen, Christopher D Fassnacht, Sherry H Suyu, Léon V E Koopmans, David J Lagattuta, John P McKean, Matt W Auger, Simona Vegetti, Tommaso Treu
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2022, Vol.513(2), pp.2349-2359 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 513(2), 2349-2359. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 513(2), 2349-2359. Oxford University Press
Strongly lensed quasars can provide measurements of the Hubble constant ($H_{0}$) independent of any other methods. One of the key ingredients is exquisite high-resolution imaging data, such as Hubble Space Telescope (HST) imaging and adaptive-optics
Autor:
Anowar J. Shajib, Pritom Mozumdar, Geoff C.-F. Chen, Tommaso Treu, Michele Cappellari, Shawn Knabel, Sherry H. Suyu, Vardha N. Bennert, Joshua A. Frieman, Dominique Sluse, Simon Birrer, Frederic Courbin, Christopher D. Fassnacht, Lizvette Villafaña, Peter R. Williams
Strong-lensing time delays enable measurement of the Hubble constant ($H_{0}$) independently of other traditional methods. The main limitation to the precision of time-delay cosmography is mass-sheet degeneracy (MSD). Some of the previous TDCOSMO ana
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e9be2bc1a37c21f3fcf8dd3064b93d1
http://arxiv.org/abs/2301.02656
http://arxiv.org/abs/2301.02656
While the direct detection of the dark-matter particle remains very challenging, the nature of dark matter could be possibly constrained by comparing the observed abundance and properties of small-scale sub-galactic mass structures with predictions f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5086d2770bc9bdea773f1282c509531c
Autor:
M N Laskowski, A Müller, P Trotzke, K Ali, D Fassnacht, M de Zwaan, M Brand, M Häder, M Kyrios
Publikováno v:
Suchttherapie.
Autor:
Daniel Gilman, Tommaso Treu, G. Despali, Christopher D. Fassnacht, Jonathan P. Coles, Frederic Courbin, Anupreeta More, Hyungsuk Tak, Matthew W. Auger, Hum Chand, Matteo Frigo, Philip J. Marshall, M. Millon, Dominique Sluse, A. Galan, L. Van de Vyvere, Geoff C. F. Chen, Joshua Yao-Yu Lin, Da Xu, Anowar J. Shajib, Philipp Denzel, Xuheng Ding, Ji Won Park, Simona Vegetti, Simon Birrer, Stefan Hilbert, Liliya L. R. Williams, Vivien Bonvin, Prasenjit Saha, S. R. Kumar
Publikováno v:
Monthly Notices of the Royal Astronomical Society
In recent years, breakthroughs in methods and data have enabled gravitational time delays to emerge as a very powerful tool to measure the Hubble constant $H_0$. However, published state-of-the-art analyses require of order 1 year of expert investiga
H0LiCOW XII. Lens mass model of WFI2033-4723 and blind measurement of its time-delay distance and H0
Autor:
Alessandro Sonnenfeld, Sherry H. Suyu, Simon Birrer, Kenneth C. Wong, Geoff C. F. Chen, Aleksi Halkola, James H. H. Chan, Tommaso Treu, Anowar J. Shajib, Matthew W. Auger, Léon V. E. Koopmans, Dominique Sluse, Christopher D. Fassnacht, Philip J. Marshall, Vivien Bonvin, Cristian E. Rusu, Frederic Courbin, Stefan Hilbert
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 498(1), 1440-1468. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We present the lens mass model of the quadruply-imaged gravitationally lensed quasar WFI2033-4723, and perform a blind cosmographical analysis based on this system. Our analysis combines (1) time-delay measurements from 14 years of data obtained by t
Autor:
Lu Shen, Brian C. Lemaux, Roy R. Gal, Adam Tomczak, Gordon K. Squires, Debora Pelliccia, Po-Feng Wu, Denise Hung, Christopher D. Fassnacht, N. Miller, Lori M. Lubin, Dale D. Kocevski, John McKean
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 494(4), 5374-5395. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 494(4), 5374-5395. Oxford University Press
In this study we investigate 179 radio-IR galaxies drawn from a sample of spectroscopically-confirmed galaxies that are detected in radio and mid-infrared (MIR) in the redshift range of $0.55 \leq z \leq 1.30$ in the Observations of Redshift Evolutio
Autor:
Giulia Despali, Simona Vegetti, Simon D M White, Devon M Powell, Hannah R Stacey, Christopher D Fassnacht, Francesca Rizzo, Wolfgang Enzi
Publikováno v:
Despali, G, Vegetti, S, White, S D M, Powell, D M, Stacey, H R, Fassnacht, C D, Rizzo, F & Enzi, W 2022, ' Detecting low-mass haloes with strong gravitational lensing I : the effect of data quality and lensing configuration ', Monthly Notices of the Royal Astronomical Society, vol. 510, no. 2, pp. 2480-2494 . https://doi.org/10.1093/mnras/stab3537
Monthly Notices of the Royal Astronomical Society (MNRAS)
Monthly Notices of the Royal Astronomical Society (MNRAS)
This paper aims to quantify how the lowest halo mass that can be detected with galaxy-galaxy strong gravitational lensing depends on the quality of the observations and the characteristics of the observed lens systems. Using simulated data, we measur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6418e3e8f3400aec5b6bf054b6bfb416
https://curis.ku.dk/ws/files/319534456/stab3537.pdf
https://curis.ku.dk/ws/files/319534456/stab3537.pdf
Autor:
Santiago Avila, Carlos E. Cunha, Anupreeta More, Issha Kayo, David J. Brooks, S. Desai, Philip J. Marshall, Peter Doel, Simon Birrer, Josh Frieman, E. Suchyta, Kyler Kuehn, M. Smith, Ofer Lahav, Daniel Gruen, F. Ostrovski, G. Tarle, Matthew W. Auger, Sherry H. Suyu, E. Bertin, Juan Garcia-Bellido, T. M. C. Abbott, Veronica Motta, M. Carrasco Kind, Cristian E. Rusu, D. W. Gerdes, Christopher D. Fassnacht, J. Carretero, James H. H. Chan, E. J. Sanchez, Adriano Agnello, B. Flaugher, I. Sevilla-Noarbe, Richard G. McMahon, Flavia Sobreira, A. Carnero Rosell, Anowar J. Shajib, B. Hoyle, Marcos Lima, Jennifer L. Marshall, D. L. Hollowood, Peter Melchior, N. Kuropatkin, Frederic Courbin, G. Gutierrez, G. Meylan, M. March, M. E. C. Swanson, A. R. Walker, E. Buckley-Geer, David J. James, Tom Shanks, Timo Anguita, L. N. da Costa, Felipe Menanteau, M. A. G. Maia, J. De Vicente, Pablo Fosalba, Ramon Miquel, Tommaso Treu, Paul L. Schechter, Thomas E. Collett, J. Annis, N. D. Morgan, Marcelle Soares-Santos, S. Allam, Robert A. Gruendl, Huan Lin, C. Lemon, W. G. Hartley, Masamune Oguri, A. A. Plazas, V. Scarpine
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Monthly Notices of the Royal Astronomical Society, 2021, Vol.501(2), pp.2833-2835 [Peer Reviewed Journal]
Universidade de São Paulo (USP)
instacron:USP
Monthly Notices of the Royal Astronomical Society, 2021, Vol.501(2), pp.2833-2835 [Peer Reviewed Journal]
The paper ‘Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars’ was published in MNRAS, 483, 4, 5649–5671 (2019). The coordinate values of the image positions in table 4 were wrongly