New Constraints on Ω<sub><i>M</i></sub>, Ω<sub>Λ</sub>, and<i>w</i>from an Independent Set of 11 High‐Redshift Supernovae Observed with the<i>Hubble Space Telescope</i>
R. A. KnopG. AlderingR. AmanullahP. AstierG. BlancM. S. BurnsA. ConleyS. E. DeustuaM. DoiR. EllisS. FabbroG. FolatelliA. S. FruchterG. GaraviniS. GarmondK. GartonR. GibbonsG. GoldhaberA. GoobarD. E. GroomD. HardinI. HookD. A. HowellA. G. KimB. C. LeeC. LidmanJ. MendezS. NobiliP. E. NugentR. PainN. PanagiaC. R. PennypackerS. PerlmutterR. QuimbyJ. RauxN. RegnaultP. Ruiz‐LapuenteG. SaintonB. SchaeferK. SchahmanecheE. SmithA. L. SpadaforaV. StanishevM. SullivanN. A. WaltonL. WangW. M. Wood‐VaseyN. Yasuda(The Supernova Cosmology Project)
2003en
ABI
Аннотация
Accepted for publication in Astrophysical Journal; For data tables and full-resolution figures, see http://supernova.lbl.gov
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
2 та иқтибос0 та фойдаланилган манба