LensCLEANing JVAS B0218+357 to determine H0
| dc.creator | Wucknitz, Olaf | |
| dc.date | 2001-12-13 | |
| dc.date.accessioned | 2026-07-07T02:01:53Z | |
| dc.date.available | 2026-07-07T02:01:53Z | |
| dc.description | We use the radio ring in JVAS B0218+357 to constrain the mass models with LensCLEAN. H0 is determined from the resulting model and the time delay. B0218+357 is one of the best systems to reduce systematic errors in H0 and may thus be called a "golden lens". | |
| dc.description | to appear in "A New Era in Cosmology" proceedings, ASP conf. ser., 2 pages, Latex 2.09, uses newpasp.sty and epsf.sty, original full-length poster version available from http://www.hs.uni-hamburg.de/english/persons/wucknitz.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0112330 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0112330 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3913 | |
| dc.subject | Astrophysics | |
| dc.title | LensCLEANing JVAS B0218+357 to determine H0 | |
| dc.type | text |