| Lightcurve Selection | |
|---|---|
| 1.0 Navigation | |
| 1.1 Using `Back' | |
| 1.2 Help | |
| 1.3 New Search | |
| 1.4 Templates | |
| 1.5 ftp Bundle | |
| 2.0 Selected Region | |
| 3.0 Summary Table | |
| 3.1 View | |
| 3.2 Bundle | |
| 3.3 Location (J2000) | |
| 3.4 MACHO Id | |
| 3.5 Proximity | |
| 3.6 Template Magnitudes | |
The user defined region is displayed in HMS/DMS/arcsecond (J2000) notation.
The table's clickable fields initiate either:
A lightcurve browser is invoked to display the selected lightcurve. The tool provides a myriad of options such as zoom in/out, list a single observation's data, list the entire lightcurve's data, display photometry data, alter units of display.
A secondary browser window is opened for lightcurve display; it is used for all lightcurve browsing.
The lightcurve is selected for later bundling into a Unix tar file prior to ftp download.
The Macho Project identifier for the star consisting of the Macho Field, Tile, and Sequence identifiers for an individual star. Refer here for the Macho Field definitions.
Closeness to the centerpoint of the bounded region. Measured in arcseconds.
Values used as template magnitudes for the listed star. Magnitudes are measured in instrumental units.
Acknowledgement to use when referencing MACHO Project data
"This paper utilizes public domain data originally obtained by the MACHO Project,
whose work was performed under the joint auspices of
the U.S. Department of Energy, National Nuclear Security Administration by the
University of California, Lawrence Livermore National Laboratory under contract No.
W-7405-Eng-48,
the National Science Foundation through the Center for Particle Astrophysics of the
University of California under cooperative agreement AST-8809616, and
the Mount Stromlo and Siding Spring Observatory, part of the Australian National University."