Data file acquisition is the result of a 3 step process:
(1) user specifies the record selection criteria using the query input form;
(2) user reviews, and optionally edits, the logical query generated from
the input form;
(3) on display of the selected record summaries, the user selects
The database search returns all records which satisfy the logical expression built from the user's input. The generated search query is composed of the form's fields separated by AND. Each field may be a composite of subfields. In that case, the generated field is composed of the subfields separated by OR. If no value is entered for a field and no default provided, it is not included. An example of the generated search query is: ObsId_input AND ObsDate_input AND Exposure_input AND Airmass_input .
The syntax of the field is defined by the record data. Refer to the descriptions below to determine if a field
Numeric subfields may be either
For example, an ObsId subfield defined thusly:
"20, >500, 100:200, 10>"
results in the logical sub-expression:
"((ObsId=20) OR (ObsId>500) OR (ObsId=100:200) OR (ObsId<10))" .
Refer here for
detailed information on the generated expressions.
The form's search fields are:
Right Ascension of the center point in bounding box defined by the RA/Dec/radius parameters.
Declination of the center point in bounding box defined by the RA/Dec/radius parameters.
Radius of the bounding box defined by the RA/Dec/radius parameters.
Select the equinox in which the RA/Dec are expressed.
Identifier for a Field centered on a MACHO Project predetermined RA/Dec. Refer here for the Macho Field definitions.
Identifier for the set of Fields comprising a MACHO Project predetermined Domain. Refer here for the Macho Domain definitions.
Position of the telecope camera relative to its supporting pier.
Identifier assigned to an observation.
Date of observation.
Image exposure time.
Photometry type of reduced data.
Average width of the point spread function calculated by SoDoPhot.
Mass column of atmosphere along the line of sight relative to the mass column at zenith.
Brightness of the sky over the entire image. It's calculated as a simple average of all subimages' average-sky-value. The latter was calculated during SoDoPhot photometry reduction.
Select the Reset button to return the form to default values.
Select the Submit button to initiate input field validation and the subsequent creation of the database search expression.
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."
and