Weak lensing by galaxy troughs in DES Science Verification data - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2016

Weak lensing by galaxy troughs in DES Science Verification data

D. Gruen
  • Function : Author
O. Friedrich
  • Function : Author
A. Amara
  • Function : Author
D. Bacon
  • Function : Author
C. Bonnett
  • Function : Author
W. Hartley
  • Function : Author
B. Jain
  • Function : Author
M. Jarvis
  • Function : Author
T. Kacprzak
  • Function : Author
E. Krause
  • Function : Author
A. Mana
  • Function : Author
E. Rozo
  • Function : Author
E. S. Rykoff
  • Function : Author
S. Seitz
  • Function : Author
E. Sheldon
  • Function : Author
M. A. Troxel
  • Function : Author
V. Vikram
  • Function : Author
T. M. C. Abbott
  • Function : Author
F. B. Abdalla
  • Function : Author
S. Allam
  • Function : Author
R. Armstrong
  • Function : Author
M. Banerji
  • Function : Author
A. H. Bauer
  • Function : Author
M. R. Becker
  • Function : Author
A. Benoit-Lévy
  • Function : Author
G. M. Bernstein
  • Function : Author
R. A. Bernstein
  • Function : Author
S. L. Bridle
  • Function : Author
D. Brooks
  • Function : Author
E. Buckley-Geer
  • Function : Author
D. L. Burke
  • Function : Author
D. Capozzi
  • Function : Author
A. Carnero Rosell
  • Function : Author
M. Carrasco Kind
  • Function : Author
J. Carretero
  • Function : Author
M. Crocce
  • Function : Author
C. E. Cunha
  • Function : Author
C. B. d'Andrea
  • Function : Author
L. N. da Costa
  • Function : Author
D. L. Depoy
  • Function : Author
S. Desai
  • Function : Author
H. T. Diehl
  • Function : Author
J. P. Dietrich
  • Function : Author
P. Doel
  • Function : Author
T. F. Eifler
  • Function : Author
A. Fausti Neto
  • Function : Author
E. Fernandez
  • Function : Author
B. Flaugher
  • Function : Author
P. Fosalba
  • Function : Author
J. Frieman
  • Function : Author
D. W. Gerdes
  • Function : Author
R. A. Gruendl
  • Function : Author
G. Gutierrez
  • Function : Author
K. Honscheid
  • Function : Author
D. J. James
  • Function : Author
K. Kuehn
  • Function : Author
N. Kuropatkin
  • Function : Author
O. Lahav
  • Function : Author
T. S. Li
  • Function : Author
M. Lima
  • Function : Author
M. A. G. Maia
  • Function : Author
M. March
  • Function : Author
P. Martini
  • Function : Author
P. Melchior
  • Function : Author
C. J. Miller
  • Function : Author
R. Miquel
  • Function : Author
J. J. Mohr
  • Function : Author
B. Nord
  • Function : Author
R. Ogando
  • Function : Author
A. A. Plazas
  • Function : Author
K. Reil
  • Function : Author
A. K. Romer
  • Function : Author
A. Roodman
  • Function : Author
M. Sako
  • Function : Author
E. Sanchez
  • Function : Author
V. Scarpine
  • Function : Author
M. Schubnell
  • Function : Author
I. Sevilla-Noarbe
  • Function : Author
R. C. Smith
  • Function : Author
M. Soares-Santos
  • Function : Author
F. Sobreira
  • Function : Author
E. Suchyta
  • Function : Author
M. E. C. Swanson
  • Function : Author
G. Tarle
  • Function : Author
J. Thaler
  • Function : Author
D. Thomas
  • Function : Author
A. R. Walker
  • Function : Author
R. H. Wechsler
  • Function : Author
J. Weller
  • Function : Author
Y. Zhang
  • Function : Author
J. Zuntz
  • Function : Author

Abstract

We measure the weak lensing shear around galaxy troughs, I.e. the radial alignment of background galaxies relative to underdensities in projections of the foreground galaxy field over a wide range of redshift in Science Verification data from the Dark Energy Survey. Our detection of the shear signal is highly significant (10σ-15σ for the smallest angular scales) for troughs with the redshift range z ∈ [0.2, 0.5] of the projected galaxy field and angular diameters of 10 arcmin…1°. These measurements probe the connection between the galaxy, matter density, and convergence fields. By assuming galaxies are biased tracers of the matter density with Poissonian noise, we find agreement of our measurements with predictions in a fiducial Λ cold dark matter model. The prediction for the lensing signal on large trough scales is virtually independent of the details of the underlying model for the connection of galaxies and matter. Our comparison of the shear around troughs with that around cylinders with large galaxy counts is consistent with a symmetry between galaxy and matter over- and underdensities. In addition, we measure the two-point angular correlation of troughs with galaxies which, in contrast to the lensing signal, is sensitive to galaxy bias on all scales. The lensing signal of troughs and their clustering with galaxies is therefore a promising probe of the statistical properties of matter underdensities and their connection to the galaxy field.
Fichier principal
Vignette du fichier
stv2506.pdf (1.64 Mo) Télécharger le fichier
Origin : Publisher files allowed on an open archive

Dates and versions

insu-03747402 , version 1 (08-08-2022)

Identifiers

Cite

D. Gruen, O. Friedrich, A. Amara, D. Bacon, C. Bonnett, et al.. Weak lensing by galaxy troughs in DES Science Verification data. Monthly Notices of the Royal Astronomical Society, 2016, 455, pp.3367-3380. ⟨10.1093/mnras/stv2506⟩. ⟨insu-03747402⟩
13 View
13 Download

Altmetric

Share

Gmail Facebook X LinkedIn More