Kim Griest

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Kim Griest

Kim Griest

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Limits vary<br />

according to<br />

Milky Way halo<br />

model

What is different about LINER Galaxies

Stephen Murray - Astronomy and Astrophysics - University of ...

UCSC Astronomy & Astrophysics Orientation Guide last update ...

Astronomy 1: Introduction to the Cosmos, Winter 2013, UCSC

Light, Optics and Telescopes Trip to Lick Observatory

Frank van den Bosch

Jason X. Prochaska

Leo Blitz

Kathryn Johnston

Risa Wechsler - Astronomy and Astrophysics

Stéphane Courteau

Ofer Lahav

Michael Strauss

Laurence Tresse

Combined MACHO and EROS limits on short duration = small mass objects

Limits vary according to Milky Way halo model

Page 1 and 2: Microlensing and Dark Matter August
Page 4 and 5: Executive Summary • Basic Result:
Page 7: LMC in neutral H looks like a face-
Page 10: •Masses 0.1 - 1.0 Msun preferred
Page 13 and 14: The number of non-Macho events is p
Page 15 and 16: LMC-23
Page 17 and 18: Much written on LMC self lensing si
Page 19 and 20: Contamination? • Contamination wa
Page 21 and 22: What do to? Other experiments!
Page 26 and 27: LMC Limits on Macho Dark Matter •
Page 28 and 29: MEGA: M31 Microlensing Found 4 even
Page 30 and 31: Other M31 results • WeCAPP (Wende
Page 32 and 33: BULGE Microlensing: three collabora
Page 35 and 36: 34 candidate events probably from t
Page 37: Conclusion • The mystery of LMC/M