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  About site: http://wwwmacho.mcmaster.ca/

Title: Astronomy/Cosmology - MACHO Project Primary aim is to test the hypothesis that a significant fraction of the dark matter in the halo of the Milky Way is made up of objects like brown dwarfs or planets: these objects have come to be kn
MAP_Home_Page MAP is a MIDEX class mission, selected by NASA in 1996, to probe conditions in the early universe. MAP measures temperature differences ("anisotropy") in the cosmic microwave background radiation.

Max_Tegmark Cosmologist's personal site including discussions of movies, experiments, and data analysis efforts.

Messier_81_Internal_Motions van Maanen's astrometrically determined internal motions of the spiral nebula Messier 81.

MSAM/TopHat_High_Altitude_Scientific_Balloons A series of scientic experiments flying as balloon payloads in Texas and Antarctica, designed to measure the medium-scale anisotropy of the cosmic microwave background radiation (CMBR).

Mysteries_of_Deep_Space_-_History_of_the_Universe_Timeline From PBS Online

Ned_Wright\'s_Cosmology_Tutorial An illustrated introductory guide to the topic, attempting to summarize modern discoveries on the origin, current state, and future of our Universe.


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MACHO Project Home Page

The MACHO Project

Welcome to the MACHO Project WWW Home Page! We are maintaining two identical sites: http://wwwmacho.anu.edu.au/ (Australia)and http://wwwmacho.mcmaster.ca/ (North America) New!  Microlensing Optical DepthToward the Galactic Bulge New!  Final Catalog of Bulge Microlensing Events Novae in the LMC and SMC Cataclysmic Variables The Project Overview The MACHO Collaboration and Science Team Candidate Microlensing Events Affiliate Programme Systems MACHO Camera Systems MACHO Data System Search Fields Field Centers LMC R-band GIF showing fields [606 kb] SMC R-band GIF showing fields [649 kb] LMC R-band FITS image with WCS [1.284 Mb] SMC R-band FITS image with WCS [1.284 Mb] Original images were obtained by Greg Bothun with his "Parking Lot" camera. Versions of saoimage more recent than 1.12 will display J2000.0 coordinates if launched with: saoimage -gd 800x800 -fits R_LMC.fits MSO Great Melbourne 50-inch Telescope Publications Publication List Searchable Publication List Data New  Finder Charts for LMC 5.7 Events (0.63 sec/px, N up, W right) New  Web-based Image and Data Access New  LMC Eclipsing Cepheids from astro-ph/0201481 Binary Microlensing Events from astro-ph/9907369 LMC Microlensing Events from ApJ 486 697 (1997) SMC Microlensing Event from ApJ 491 L11 (1997) Bulge Microlensing Events from ApJ 479 119 (1997) LMC Beat RR Lyrae from ApJ 482 89 (1996)Demos Interactive Cepheid P-L RelationOther MACHO Project Web Servers Microlensing Alerts Other Dark Matter Search Links AGAPE The Direct Detection Group at the CfPA DUO EROS MOA OGLE PLANET UKDMC Acknowledgements Institute of Geophysics and Planetary Physics, Lawrence LivermoreNational Laboratory, US Department of Energy NSF-supported Center for Particle Astrophysics at the University ofCalifornia at Berkeley, Santa Barbara, and San Diego Australian National University Doug Welch Last updated: 2005 June 23
 

Primary

aim

is

to

test

the

hypothesis

that

a

significant

fraction

of

the

dark

matter

in

the

halo

of

the

Milky

Way

is

made

up

of

objects

like

brown

dwarfs

or

planets:

these

objects

have

come

to

be

kn

http://wwwmacho.mcmaster.ca/

MACHO Project 2008 December

dvd rental

dvd


Primary aim is to test the hypothesis that a significant fraction of the dark matter in the halo of the Milky Way is made up of objects like brown dwarfs or planets: these objects have come to be kn

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