Hints for Searching for Data in MAST

Searching for Planets, Comets and Asteroids

Using coordinates to search MAST for moving targets such as planets and comets is not usually the most efficient way of locating such observations. The most straightforward way to search for observations of such a target is to search on the object name using the "Don't Resolve" option in the Resolver form element.

For some of the MAST missions, such as HST, the object name is designated by the original observer. For example, an observation of Jupiter might have the object name "CP1-JUP-NORTH-LIMB-A". To find all the items of interest you may want to use a wild card search using the minimum number of characters. To do this enter *JUP* in the target element of the search form. You must remember to choose the "Don't Resolve" option in the resolver form element. You can narrow the search using such items as the time of observation, instrument, filter etc. This type of search may take a little longer than a search by coordinates.

For some MAST missions, targets have been assigned a target class or category. You can utilize this to find all solar system objects. For shorter duration missions, such as HUT or UIT this might be the most efficient way of searching for planets or comets. For longer term missions such as IUE, this type of search will find many rows unless you are able to narrow the search using other criteria such as time or exposure length.

HST observations are not assigned an object class, but are given a short descriptions of the target. Every morning we generate a list of all the target descriptions currently in use. This list is linked back to the HST Science Search page, so you can read through this list (or search it with your browser's find capability) and find datasets matching the description. (see the next section for hints on searching by object class in the HST Archive).

Another way to locate observations of solar system objects is to search the abstracts of missions with a Guest Investigator program (HST, FUSE, IUE, EUVE). Entering the target of interest into these search forms will find programs that planned to observe the target. A list of the programs contains the abstract as well as links to listings of the observations associated with that program.

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Searching by Object Class in the HST Archive

There are two object category fields in the HST Archive: the "broad category" and the "target description" fields. The target description field is one of the fields explicitly on the HST search form. This is the longer description and probably the more useful search field. You may also search on the broad category utilizing the User-specified field options on the search form.

The format is NOT uniform and so you will need to utilize wild cards to search on a keyword or phrase. The words might be separated by semi-colons, spaces, or dashes so you will need to place a wild card between each word or phrase in the search criteria. For example: *GALAXY*SPIRAL*. This search will find most of the observations of interest. However, word order is important so you might need to try *SPIRAL*GALAXY* as well.

Searches on object category fields are likely to return many rows. You may wish to further qualify your search by instrument, filters etc.

Every morning we generate a list of all the target descriptions currently in use. This list is linked back to the HST Science Search page, so you can read through this list (or search it with your browser's find capability) and find datasets matching the description.

Another way to locate observations of possible interest by category is to utilize the (HST abstract search. Entering the target of interest into this search form will find programs that proposed to observe the target. A list of the programs contains the abstract as well as links to listings of the observations associated with that program.

Using the VizieR/MAST or the NED/MAST Cross-correlation tools are two addtional ways of finding classes of targets within the MAST archive. See the tutorial section VizieR/MAST Cross Correlation Search or the section MAST/NED Cross Correlation Searchfor more information. There was a tutorial published in the January 2007 Archive Newsletter (also available as a powerpoint presentation, and in the .

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Search HST catalog by Region in the Sky

The MAST "pointings" interface allows a user to search for ACS, WFPC2, STIS, FOC and NICMOS images in a powerful way. For each of these instruments we have assembled a searchable data table that allows users to look for sky regions (or pointings) which have been observed N times or more, observed with 2 or more filters, or have been observed more than twice with a time separation of more than (or less than) N days. An exposure is defined to be the file created after the shutter closes. The total number of exposures for each of the defined bands within a defined pointing were tallied. The definition of a pointing is different for each instrument. See the Search Help page for a more complete description of the methodology used to define a pointing. This page also includes descriptions of the search fields and the input and output columns.

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Searching with Ranges of Coordinates

You may search on ranges of right ascension or declination using the ".." operator. For example, you can enter 21h 51m .. 21h 52m for the right ascension, and 28 51 .. 29 51 for the declination. Comparators can also be used, i.e. ">", ">=", "<", "<=". For example,
> 85 as a declination value will return all observations with declination larger than 85 degrees. (Note when ranges of coordinates are specified the search radius will be ignored. Also, searches on ranges can be quite time consuming.)

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Searching with Ranges in Time

Searching on ranges of time is important if you wish to search on any time field. If you enter the date July 19, 2002, then midnight (00:00:00) is assumed. If you enter July 2002, then the date July 1, 2002 at midnight is assumed. If you don't know the exact time of an observation then you will need to search using a range.

To search for observations before a given date, use <, and for observations after a given date, use >. For example,
> Jul 15 2002
< Jul 15 2002

You can use the .. operator to search on a range of dates. To find all observations in July 2002 enter:
Jul 1 2002 .. Aug 1 2002
This operator is inclusive on the first date and exclusive on the second.

Finally, you can search on a list of dates or date ranges. For example,
Jul 1 2002 .. Jul 3 2002, Dec 1 2002 .. Dec 6 2002
will search for observations done within either one of these date ranges.

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Searching Across Multiple Missions

The MAST Cross Correlation Search permits searches across all the HST instruments and most MAST missions. This interface is similar to the mission search forms. For more detailed information about search options see the help page.

The top section is the same as the mission search forms and includes both the standard and file upload options. The second section permits selection of the instruments of interest. You may customize the search radius for any of the instruments. The third section gives some options such as the output format, but the options are not as extensive as the mission search pages.

The output from the search is grouped by instrument. Up to 10 rows are displayed for each instrument, but the number of available rows is displayed. The output utilizes the default output fields for each instrument/mission. The HTML version includes links to the previews, the proposal search, the references and High-Level Science Products. At the bottom of the output display is a summary listing each instrument and the number of observations found per instrument. The summary is not listed in the CSV, Excel and VOTable formats.

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Comparing observations from two different missions

Perhaps you are interested in seeing what targets (perhaps of a specific type of object) have been observed by two different missions. If you have a list of specific target then the easiest thing is to just use the Cross-correlation search described just above. But perhaps you are just interested in finding out what BL Lacertae objects have observed by both FUSE and STIS without a pre-determined list of objects. First you would need to determine the unique target names or coordinates observed by one of the instruments for that type of target. You might choose to obtain this initial list from the FUSE search, as it is easier to search by object class. Follow these steps:

After editing the file to remove any header information, you may use this file as input for an HST search. Follow these steps: