Spatially unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

dc.creator	Sorba, Robert
dc.creator	Sawicki, Marcin
dc.date.accessioned	2025-01-14T17:53:11Z
dc.date.available	2025-01-14T17:53:11Z
dc.date.issued	2018
dc.identifier.issn	0035-8711
dc.identifier.uri	https://dx.doi.org/10.1093/mnras/sty186
dc.identifier.uri	https://library2.smu.ca/xmlui/handle/01/32080
dc.description	Published version	en_CA
dc.description.provenance	Submitted by Anna Labrador (anna.labrador@smu.ca) on 2025-01-14T17:53:11Z No. of bitstreams: 1 Sawiki_Marcin_2018b.pdf: 10970867 bytes, checksum: 559647e7cb529c907caf8f15cc5495d0 (MD5)	en
dc.description.provenance	Made available in DSpace on 2025-01-14T17:53:11Z (GMT). No. of bitstreams: 1 Sawiki_Marcin_2018b.pdf: 10970867 bytes, checksum: 559647e7cb529c907caf8f15cc5495d0 (MD5) Previous issue date: 2018	en
dc.language.iso	en	en_CA
dc.publisher	Oxford University Press	en_CA
dc.title	Spatially unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem	en_CA
dc.type	Technical Report	en_CA
dcterms.bibliographicCitation	Monthly Notices of the Royal Astronomical Society 476 (2), p.1532-1547, 2018	en_CA