Abstract
We present a weak gravitational lensing measurement of the external convergence along the line of sight to the quadruply lensed quasar HE 0435-1223. Using deep r-band images from Subaru Suprime Cam, we observe galaxies down to a 3 sigma limiting magnitude of similar to 26 mag resulting in a source galaxy density of 14 galaxies per square arcminute after redshift-based cuts. Using an inpainting technique and multiscale entropy filtering algorithm, we find that the region in close proximity to the lens has an estimated external convergence of kappa = -0.012(-0.013)(+0.020) and is hence marginally underdense. We also rule out the presence of any halo with a mass greater than M-vir = 1.6 x 10(14)h(-1)M(circle dot) (68 per cent confidence limit). Our results, consistent with previous studies of this lens, confirm that the intervening mass along the line of sight to HE0435-1223 does not affect significantly the cosmological results inferred from the time-delay measurements of that specific object.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Physik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 530 Physik |
ISSN: | 0035-8711 |
Sprache: | Englisch |
Dokumenten ID: | 66699 |
Datum der Veröffentlichung auf Open Access LMU: | 19. Jul. 2019, 12:20 |
Letzte Änderungen: | 04. Nov. 2020, 13:48 |