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A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403 : Robust characterization of the cluster mass distribution from VLT/MUSE deep observations. / Bergamini, P.; Rosati, P.; Vanzella, E.; Caminha, G. B.; Grillo, C.; Mercurio, A.; Meneghetti, M.; Angora, G.; Calura, F.; Nonino, M.; Tozzi, P.
I:
Astronomy & Astrophysics, Bind 645, A140, 27.01.2021.
Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt
Harvard
Bergamini, P, Rosati, P, Vanzella, E, Caminha, GB, Grillo, C, Mercurio, A, Meneghetti, M, Angora, G, Calura, F, Nonino, M & Tozzi, P 2021, '
A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403: Robust characterization of the cluster mass distribution from VLT/MUSE deep observations',
Astronomy & Astrophysics, bind 645, A140.
https://doi.org/10.1051/0004-6361/202039564APA
Bergamini, P., Rosati, P., Vanzella, E., Caminha, G. B., Grillo, C., Mercurio, A., Meneghetti, M., Angora, G., Calura, F., Nonino, M., & Tozzi, P. (2021).
A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403: Robust characterization of the cluster mass distribution from VLT/MUSE deep observations.
Astronomy & Astrophysics,
645, [A140].
https://doi.org/10.1051/0004-6361/202039564Vancouver
Bergamini P, Rosati P, Vanzella E, Caminha GB, Grillo C, Mercurio A o.a.
A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403: Robust characterization of the cluster mass distribution from VLT/MUSE deep observations.
Astronomy & Astrophysics. 2021 jan. 27;645. A140.
https://doi.org/10.1051/0004-6361/202039564Author
Bergamini, P. ; Rosati, P. ; Vanzella, E. ; Caminha, G. B. ; Grillo, C. ; Mercurio, A. ; Meneghetti, M. ; Angora, G. ; Calura, F. ; Nonino, M. ; Tozzi, P. / A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403 : Robust characterization of the cluster mass distribution from VLT/MUSE deep observations. I: Astronomy & Astrophysics. 2021 ; Bind 645.
Bibtex
@article{6c4f744ac514447aa10bb541f6e69428,
title = "A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403: Robust characterization of the cluster mass distribution from VLT/MUSE deep observations",
abstract = "We present a new high-precision parametric strong lensing model of the galaxy cluster MACS J0416.1-2403, at z=0.396, which takes advantage of the MUSE Deep Lensed Field (MDLF), with 17.1 h integration in the northeast region of the cluster, and Hubble Frontier Fields data. We spectroscopically identify 182 multiple images from 48 background sources at 0.9 ",
keywords = "galaxies: clusters: general, gravitational lensing: strong, cosmology: observations, dark matter, galaxies: kinematics and dynamics, LENSES",
author = "P. Bergamini and P. Rosati and E. Vanzella and Caminha, {G. B.} and C. Grillo and A. Mercurio and M. Meneghetti and G. Angora and F. Calura and M. Nonino and P. Tozzi",
year = "2021",
month = jan,
day = "27",
doi = "10.1051/0004-6361/202039564",
language = "English",
volume = "645",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",
}
RIS
TY - JOUR
T1 - A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403
T2 - Robust characterization of the cluster mass distribution from VLT/MUSE deep observations
AU - Bergamini, P.
AU - Rosati, P.
AU - Vanzella, E.
AU - Caminha, G. B.
AU - Grillo, C.
AU - Mercurio, A.
AU - Meneghetti, M.
AU - Angora, G.
AU - Calura, F.
AU - Nonino, M.
AU - Tozzi, P.
PY - 2021/1/27
Y1 - 2021/1/27
N2 - We present a new high-precision parametric strong lensing model of the galaxy cluster MACS J0416.1-2403, at z=0.396, which takes advantage of the MUSE Deep Lensed Field (MDLF), with 17.1 h integration in the northeast region of the cluster, and Hubble Frontier Fields data. We spectroscopically identify 182 multiple images from 48 background sources at 0.9
AB - We present a new high-precision parametric strong lensing model of the galaxy cluster MACS J0416.1-2403, at z=0.396, which takes advantage of the MUSE Deep Lensed Field (MDLF), with 17.1 h integration in the northeast region of the cluster, and Hubble Frontier Fields data. We spectroscopically identify 182 multiple images from 48 background sources at 0.9
KW - galaxies: clusters: general
KW - gravitational lensing: strong
KW - cosmology: observations
KW - dark matter
KW - galaxies: kinematics and dynamics
KW - LENSES
U2 - 10.1051/0004-6361/202039564
DO - 10.1051/0004-6361/202039564
M3 - Journal article
VL - 645
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
SN - 0004-6361
M1 - A140
ER -
