about
OzDES multifibre spectroscopy for the Dark Energy Survey: first-year operation and resultsLocations of peculiar supernovae as a diagnostic of their originsSearching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up programPhotometric redshift analysis in the Dark Energy Survey Science Verification dataSN 2009ip à la PESSTO: no evidence for core collapse yet★Host galaxy identification for supernova surveysThe difference imaging pipeline for the transient search in the Dark Energy SurveyOzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data releaseHunting Gravitational Waves with Multi-Messenger Counterparts: Australia’s RoleDark Energy Survey Year 1 results: cross-correlation redshifts – methods and systematics characterizationDark Energy Survey Year 1 Results: redshift distributions of the weak-lensing source galaxiesSN 2008in—BRIDGING THE GAP BETWEEN NORMAL AND FAINT SUPERNOVAE OF TYPE IIPGRB 081008: from burst to afterglow and the transition phase in betweenDiscovery of a z = 0.65 post-starburst BAL quasar in the DES supernova fieldsRates of superluminous supernovae at z ∼ 0.2On the rates of type Ia supernovae in dwarf and giant hosts with ROTSE-IIIbThe exceptionally luminous type Ia supernova 2007ifAstronomical Image Subtraction by Cross‐ConvolutionReal-time detection and rapid multiwavelength follow-up observations of a highly subluminous type II-P supernova from the Palomar Transient Factory survey
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description
onderzoeker
@nl
researcher ORCID id 0000-0001-8315-4176
@en
name
Fang Yuan
@ast
Fang Yuan
@en
Fang Yuan
@es
Fang Yuan
@nl
type
label
Fang Yuan
@ast
Fang Yuan
@en
Fang Yuan
@es
Fang Yuan
@nl
prefLabel
Fang Yuan
@ast
Fang Yuan
@en
Fang Yuan
@es
Fang Yuan
@nl
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P21
P31
P496
0000-0001-8315-4176