MACHO LMC 23 , the SIMBAD biblio

MACHO LMC 23 , the SIMBAD biblio (14 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST00:12:50

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2000ApJ...542..281A 8 33 826 The MACHO project: microlensing results from 5.7 years of Large Magellanic Cloud observations. ALCOCK C., ALLSMAN R.A., ALVES D.R., et al.
2002A&A...393..129J 19 31 Microlensing towards the Large Magellanic Cloud. JETZER P., MANCINI L. and SCARPETTA G.
2004A&A...427...61M 18 38 LMC self-lensing from a new perspective. MANCINI L., CALCHI NOVATI S., JETZER P., et al.
2004ApJ...601L.151A 11 25 The stellar halo in the Large Magellanic Cloud: mass, luminosity, and microlensing predictions. ALVES D.R.
2004MNRAS.347..213R 23 9 Statistical interpretation of Large Magellanic Cloud microlensing candidates. RAHVAR S.
2004MNRAS.352..233B 33 31 Light-curve classification in massive variability surveys - II. Transients towards the Large Magellanic Cloud. BELOKUROV V., EVANS N.W. and DU Y.L.
2005ApJ...631..301B 33 19 Photometric confirmation of MACHO Large Magellanic Cloud microlensing events. BENNETT D.P., BECKER A.C. and TOMANEY A.
2005ApJ...633..906B 28 38 Large Magellanic Cloud microlensing optical depth with imperfect event selection. BENNETT D.P.
2005MNRAS.359..464G 7 13 Contamination in the MACHO data set and the puzzle of Large Magellanic Cloud microlensing. GRIEST K. and THOMAS C.L.
2006A&A...459..407C 10 23 Microlensing towards the Large Magellanic Cloud: a study of the LMC halo contribution. CALCHI NOVATI S., DE LUCA F., JETZER P., et al.
2007MNRAS.374..365E 6 8 The microlensing optical depth towards the Large Magellanic Cloud: is there a puzzle? EVANS N.W. and BELOKUROV V.
2011MNRAS.413..493W 77           X         2 19 52 The OGLE view of microlensing towards the Magellanic clouds – III. Ruling out subsolar MACHOs with the OGLE-III LMC data. WYRZYKOWSKI L., KOZLOWSKI S., SKOWRON J., et al.
2024ApJS..273....4M 90           X         2 30 ~ Microlensing Optical Depth and Event Rate toward the Large Magellanic Cloud Based on 20 yr of OGLE Observations. MROZ P., UDALSKI A., SZYMANSKI M.K., et al.
2024ApJ...977L..37M 63       D     X         2 11 ~ Millinovae: A New Class of Transient Supersoft X-Ray Sources without a Classical Nova Eruption. MROZ P., KROL K., SZEGEDI H., et al.

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