Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Apr-2024)

Result of query: info cati MSW2019] FieldN-WFC3 NNN$
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Details on Acronym:   [MSW2019]
  
[MSW2019] (Mutlu-Pakdil+Sand+Walker+, 2019)
Write:<<[MSW2019] FieldN-ACS NNNN>>
<<[MSW2019] FieldN-WFC3 NNN>>
<<[MSW2019] Leo V-NNN>>
N: 2466+1231+538+416+117
Object:*  (SIMBAD class: Star)
Note:HST (ACS and WFC3) and MMT Hectochelle observations of N=2466+1231+538+416+117 stars in Leo V.
The ACS central pointing of Leo V is referred to as Field 1 and the candidate debris stream as Field 2. Similarly, coordinated parallel observations with WFC3 were made in two additional fields.
in source:NAME Leo V
Ref:=2019ApJ...885...53M
byMUTLU-PAKDIL B. , SAND D.J., WALKER M.G., CALDWELL N., CARLIN J.L., COLLINS M.L., CRNOJEVIC D., MATEO M., OLSZEWSKI E.W., SETH A.C., STRADER J., WILLMAN B., ZARITSKY D.
 Astrophys. J., 885, 53-53 (2019)
  Signatures of tidal disruption in ultra-faint dwarf galaxies: a combined HST, Gaia, and MMT/Hectochelle study of Leo V.
oTables 2-3: <[MSW2019] FieldN-ACS NNNN> N=2466+1231. Tables 2-3: <[MSW2019] FieldN-WFC3 NNN> N=538+416. Table 6: <[MSW2019] LeoV-NNN> (Nos 0-116).
=E=Catalogue in electronic form as <J/ApJ/885/53/>
Originof the Acronym: S = Created by Simbad, the CDS Database