Details on Acronym: MOA
MOA (Microlensing Observations in Astrophysics) ***** Avoid the usage of MOA, prefer [BAD2001] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: MOA
MOA (Microlensing Observations in Astrophysics) Write:<<MOA -bin-N>>
<<MOA -bin-Na>>
<<MOA -bin-LNa>> (not recognised by Simbad, but found in literature) Object:Lev + * + Poss. Planet (SIMBAD class: Unknown = Object of Unknown Nature) Note:Binary microlensing events from the 2006-2007 MOA-II galactic bulge survey data.
First reference: arXiv:1203.4560. Ref:=arXiv:1203.4560 Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: MOA
MOA (Microlensing Observations in Astrophysics) Write:<<MOA -ip-NN>> N: 10 Object:Lev (SIMBAD class: LensingEv = (Micro)Lensing Event) Note:Search for planetary-mass lenses in the 2006-2007 MOA-II galactic bulge survey data. Ref:=2011Natur.473..349S bySUMI T. , KAMIYA K., BENNETT D.P., BOND I.A., ABE F., BOTZLER C.S., FUKUI A., FURUSAWA K., HEAMSHAW J.B., ITOW Y., KILMARTIN P.M., KORPELA A., LIN W., LING C.H., MASUDA K., MATSUBARA Y., MIYAKE N., MOTOMURA M., MURAKI Y., NAGAYA M., NAKAMURA S., OHNISHI K., OKUMURA T., PERROTT Y.C., RATTENBURY N., SAITO T., SAKO T., SULLIVAN D.J., SWEATMAN W.L., TRISTRAM P.J., YOCK P.C.M., (The MOA Collaboration), UDALSKI A., SZYMANSKI M.K., KUBIAK M., PIETRZYNSKI G., POLESKI R., SOSZYNSKI I., WYRZYKOWSKI L., ULACZYK K., (The OGLE Collaboration) Natur, 473, 349-352 (2011) Unbound or distant planetary mass population detected by gravitational microlensing. oTable 1: <MOA-ip-NN> (Nos 1-10). Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: MOA
MOA (Microlensing Observations in Astrophysics) Write:<<MOA YYYY-BLG-NNN>>
<<MOA YYYY-BLG-NNNa>>
<<MOA -YYYY-BLG-NNN>> (not recognised by Simbad, but found in literature)
<<MOA -YYYY-BLG-NNN-L>>
<<MOA -YYYY-BLG-NNN-La>>
<<MOA -YYYY-BLG-NNNL>>
<<MOA -YYYY-BLG-NNNLa>>
<<MOA -YYYY-BLG-NNN L>>
<<MOA -YYYY-BLG-NNN La>> Object:Microlensing Event + Planet (SIMBAD class: LensingEv = (Micro)Lensing Event) Note:Format found in literature for MOA microlensing events in the Galactic Bulge.
Only the first references using these formats are listed here. in source:NAME Galactic Bulge Ref:=2002MNRAS.331L..19B byBOND I.A. , ABE F., DODD R.J., HEARNSHAW J.B., KILMARTIN P.M., MASUDA K., MATSUBARA Y., MURAKI Y., NODA S., PETTERSON O.K.L., RATTENBURY N.J., REID M., SAITO T., SAITO Y., SAKO T., SKULJAN J., SULLIVAN D.J., SUMI T., WILKINSON S., YAMADA R., YANAGISAWA T., YOCK P.C.M. Mon. Not. R. Astron. Soc., 331, 19-23 (2002) Improving the prospects for detecting extrasolar planets in gravitational microlensing events in 2002. oTable 1, Fig.1: <MOA YYYY-BLG-NN> N=10. Ref:=2008ApJ...684..663B byBENNETT D.P. , BOND I.A., UDALSKI A., SUMI T., ABE F., FUKUI A., FURUSAWA K., HEARNSHAW J.B., HOLDERNESS S., ITOW Y., KAMIYA K., KORPELA A.V., KILMARTIN P.M., LIN W., LING C.H., MASUDA K., MATSUBARA Y., MIYAKE N., MURAKI Y., NAGAYA M., OKUMURA T., OHNISHI K., PERROTT Y.C., RATTENBURY N.J., SAKO T., SAITO T., SATO S., SKULJAN L., SULLIVAN D.J., SWEATMAN W.L., TRISTRAM P.J., YOCK P.C.M., KUBIAK M., SZYMANSKI M.K., PIETRZYNSKI G., SOSZYNSKI I., SZEWCZYK O., WYRZYKOWSKI L., ULACZYK K., BATISTA V., BEAULIEU J.P., BRILLANT S., CASSAN A., FOUQUE P., KERVELLA P., KUBAS D., MARQUETTE J.B. Astrophys. J., 684, 663-683 (2008) A low-mass planet with a possible Sub-Stellar-Mass host in microlensing event MOA-2007-BLG-192. o<MOA YYYY-BLG-NNN> N=1. Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: MOA
MOA (Microlensing Observations in Astrophysics) Write:<<MOA JHHMMSS.s+DDMMSS>> N: 167 Object:V* (SIMBAD class: Variable* = Variable Star) Note:The MOA project is surveying some 400000 stars in the SMC and 1400000 in the LMC.
2002MNRAS.331..609B: N=167 Binaries in the SMC.
2004MNRAS.348.1120N: N=29 V* in the LMC.
More catalogues are likely to follow. in source:Magellanic Clouds:LMC = LMC in source:Magellanic Clouds:SMC = SMC Ref:=2002MNRAS.331..609B byBAYNE G. , TOBIN W., PRITCHARD J.D., BOND I., POLLARD K.R., BESIER S.C., NODA S., SUMI T., YANAGISAWA T., SEKIGUCHI M., HONDA M., MURAKI Y., TAKEUTI M., HEARNSHAW J.B., KILMARTIN P.M., DODD R.J., SULLIVAN D.J., YOCK P.C.M. Mon. Not. R. Astron. Soc., 331, 609-614 (2002) The MOA catalogue of eclipsing binary stars in the Small Magellanic Cloud. oTable 1: <MOA JHHMMSS.s-DDMMSS> N=167. Ref:=2004MNRAS.348.1120N byNODA S. , TAKEUTI M., ABE F., BOND I.A., DODD R.J., HEARNSHAW J.B., HONDA M., HONMA M., JUGAKU J., KAN-YA Y., KATO Y., KILMARTIN P.M., MATSUBARA Y., MASUDA K., MURAKI Y., NAKAMURA T., OHNISHI K., REID M., RATTENBURY N.J., SAITO T., SAITO Y., SATO H., SEKIGUCHI M., SKULJAN J., SULLIVAN D.J., SUMI T., YAMADA R., YANAGISAWA T., YOCK P.C.M., YOSHIZAWA M. Mon. Not. R. Astron. Soc., 348, 1120-1134 (2004) Study of variable stars in the MOA data base: long-period red variables in the Large Magellanic Cloud - II. Multiplicity of the period-luminosity relation. oTables 3, B1, B2: <MOA JHHMMSS.s-DDMMSS> N=75+5+17. Dept of Physics & Astronomy, University of Canterbury, Christchurch, New Zealand =E=Catalogue in electronic form as J/MNRAS/331/609 Originof the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: MOA
MOA (Microlensing Observations in Astrophysics) ***** Avoid the usage of MOA, prefer [NTA2002] Originof the Acronym: A = Assigned by the author(s)
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