HST Science Search Help

This page describes how to use the HST Science Search form and describes the individual fields in that form.

Use the HST Science Search form to search the HST Archive Catalog by object name, position, observation date, proposal ID, wavelength, and data type. You can also mark data for retrieval using this interface.

This interface can retrieve data either to the archive staging area or directly to the destination you specify, so you can retrieve proprietary data (if you're priveleged to do so). To allow you to safely enter a destination username and password, we use the same security mechanism as many commercial sites.

Local File Name

The name of a local file containing a table or list of parameters such as coordinates, targets names, or data IDs to be uploaded to the server and used to query the database. The file must be an ASCII text file with either one entry per line (e.g., a target name, a Data ID, or a set of coordinates), or a table separated with one of the allowed delimiters, with targets, Data IDs, or RA and Dec values in the designated columns. Note in either case, only one entry per line is extracted. If, for example, a comma-separated list of target names is downloaded in one line, only the value in the designated column will be used.

The search script will perform a database search for each extracted Data ID, target, or set of coordinates, contained in the uploaded list. Target names will be resolved to coordinates. If a resolver error occurs with target names, the search will abort and the compiled results displayed. Coordinates may be given in several formats including sexigesimal and decimal degrees. If the output is requested in CSV or Excel spreadsheet format, a blank line will be used to distinguish the results of one target search from another. VOTable format incorporates separate RESOURCE tags for each database query.

Use the other form entries to specify field delimiters, RA, DEC, or Target column numbers (when the file contains a table of values), and file contents (target names or coordinates). The browse button allows users to seach local directories to locate files.

Warning: Since uploading long lists can take a while to run, uploaded files are limited to 10,000 entries.

File Contents

Specifies contents of the local file to be uploaded (e.g., coordinates, target names or Data ID's). By default, most MAST search forms assume coordinates.

Note that each target, or set of coordinates specified in the uploaded file, is treated as a separate query. The results are displayed as each query is run. If however Data ID's are entered (up to 10,000 are allowed), it is processed as a single query (e.g., select * where data_id in (did1,did2,...).

To avoid displaying column names after each target name or coordinate query, consider using the comma-separated values output format. Also keep in mind that not all target names are resolvable. For example, SIMBAD currently does not reolve most 2MASS IDs.

RA/Target/Data ID Column Number

The column number containing either the Data ID, Right Ascension (decimal degrees or sexagesimal), or target name (depending on how file_contents is set). The default is to assume the first column is to be used.

Dec Column Number

For forms allowing coordinates as input, the column number containing the Declnation (decimal degrees or sexagesimal). The default is to assume the second column contains the DEC value. If the file contents is set to Target Name or any Data ID, this parameter is ignored.

Column Delimiter

The character used to delimit table entries in the uploaded file. Allowed values include tabs( ), commas(,), vertical bar (|), or semi-colons(;). The default is to assume tabs are the delimiters. If the file contains only a single column, use tabs as the delimiter.

Target Name

The name of the astronomical object you want to search for. Examples of valid names include gam Gem, NGC 1068, JUPITER, and hd 45677. For Kepler, a sky-region limited mission, examples might be 14 Cyg, HR 7483, HD 181649, or NGC 6819. Multiple target names can be entered if separated by commas, although table sorting is turned off in these cases.

The Target Name is used in combination with the Resolver Field. If the SIMBAD, CFA (SIMBAD at CfA), NED (default) or HLA name resolver options are chosen, then coordinates returned from these services are used to perform a cone search with the specified search radius.

For most mission searches, you do NOT have to use the resolver. Choose the "Don't resolve" option to perform string searches on the object name in the database. Note Kepler catalogs do not include a generic object name field, so this option is not available for Kepler users.

When you search on the object name in the database (i.e. without using the name resolver), case will be ignored. The object name will not be wildcarded at the front and back automatically (that's so if you innocently enter IO, you don't match things like ORION). You can however wildcard the object name using * (for example, *IO*). You can also enter a comma-separated list; for example, *JUP*,*SAT* would match object names containing either JUP or SAT.

Note that most missions store some target names in a format that is not compatible with the NED or SIMBAD name resolvers. For example, most 2MASS IDs are currently not resolveable by SIMBAD.

Resolver

This field describes how target names are to be handled. If you want to resolve a target name into its coordinates (the default), this field can be used to describe which name resolver to use. You can also elect to search the database by the target name itself by choossing the "Don't resolve" option.

The two main name resolver services are SIMBAD and NED. NED is the NASA Extragalactic Database at Caltech in Pasadena, California, and SIMBAD is the Set of Identifications, Measurements, and Bibliography for Astronomical Data at the Centre de Données astronomiques in Strasbourg, France (SIMBAD at CDS). A mirror site at the Center for Astrophysics in Boston is also now available and is denoted as "SIMBAD at CFA". NED is an extragalactic database, and generally won't resolve object names within the Milky Way galaxy.

Because we occasionally have problems with network connections and web servers, we now store previously resolved target names and coordinates in our own local database and search this database before trying to access the other name resolvers using various web services. By default, If no entry is found in the local cache, the entered object names will first be sent to the NED service, and, if still not found, then CFA, CDS, and HLA in that order. You may also go directly to CFA, CDS, or HLA by changing the selected name resolver, although the local cache is always checked first.

If any error occurs, the search form will be redrawn with an error message at the top. Otherwise, the returned coordinates will then be used to search the database, along with whatever other query qualifications you have given.

We recommend that you use object name resolution to find observations of specific stationary targets. This is the most reliable way to look up observations, because the observer could have given any object name at all (for example, NGC1976 instead of M42, or PARALLEL-FIELD).

The SIMBAD and NED name resolvers can resolve only fixed objects; they cannot compute the positions of moving objects (planets, comets, etc.). To find moving objects, try selecting the appropriate category option available on most MAST search forms, or as mentioned above, enter an object name that could match what you're looking for, and select "Don't resolve" for the name resolver. Note wild cards are allowed, so for Jupiter you might enter "*JUP*".

Right Ascension, Declination

The Right Ascension and Declination values. If single values are entered, a cone search is performed using the specified search radius (default = 3 arcminutes for most missions, 0.02 arcmin. for Kepler). Values may be entered in decimal degrees or using sexagesimal notation. Although decimal hours is NOT an allowed input format, Right Ascension search results may optionally be displayed as decimal hours (see the "Output Coords" form element).

Note the examples listed below (and elsewhere) are only intended to show the format of the form entries. There is no guarantee that entering these specific values will return any search results.

You may also enter 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.)

Coordinate values may be specified using a number of formats. Examples of valid formats include:

    Decimal Degrees
       	185.63325 29.8959861111111
 
    Hours, minutes and Seconds
        12 22 31.98      29 53 45.55
        12h22m31.98s     29d53m45.55s
        12:22:31.98     +29:53:45.55
        12h22'31.98"     29d53'45.55"
        12h 22m 31.98s   29d 53m 45.55s
        12h 22' 31.98"   29d 53' 45.55"
        12h 22' 31.98"  -29d 53' 45.55"
        12h22'31".98    -29d53'45".55
        12h22m31s.98    -29o53m45s.55
        12h 22' 31".98  -29d 53' 45".55
     
    Hours/Degrees and Minutes (no seconds)
        12 22     29 53
        12h22m   +29d53m
        12h22m    29d53m
        12:22m    29:53m
        12h22'    29d53'
        12h 22m   29d 53m
        12h 22'   29d 53'
        12h 22'  -29d 53'

    The RA may be given in decimal degrees by indicating
    a D or d after the degrees:
        12d 22m   29d 53m

Spacing is not important, as long as the value is unambiguous. You can delimit the hours/degrees, minutes, and (optional) seconds with letters, colons, spaces, or any character that's not a digit or a decimal point. Like target names, multiple coordinates can be entered if separated by commas.

Radius

The radius of the search box around the RA and Dec, in floating-point arcminutes (e.g., 5.0). You should be careful about giving too restrictive a search radius since (for some missions) the coordinates of the object were given by the Guest Observer, and may not reflect the precise pointing of the instrument at the time of the observation.

The search routine computes the angular separation between each result dataset and the search center so this really is a circular radius. (Results are generally sorted on the angular separation by default.)

Equinox

The equinox of the RA and Dec you have entered, either B1900, B1950 or J2000. If B1900 or B1950 are selected, the input coordinates are precessed to year 2000, but NOT converted to FK5 or ICRS. This will add an error which (from year 1900) can range from a few arcseconds up to roughly 25" at the poles.

Note the precession is only applied to the input coordinates. The coordinates displayed in the search results will depend on the mission database and the selected output columns. (Note: all MAST missions include J2000 coordinates as default output columns.)

If you enter a target name and use either the SIMBAD or NED name resolver, the equinox will be set to J2000.

Start Time

The date of the observation. More specifically, the date and time, in GMT, on which the exposure was started. When specifying this date, you need to include a date and an optional time. The date can have any of the following formats (the month name can be spelled out or abbreviated to three letters; case is not significant):

      Jul 15 1994
      Jul 1994 15
      15 Jul 1994
      1994 Jul 15
      1994 15 Jul
      7/15/1994
      7-15-1994
      7.15.1994
    

If the day is omitted, the first day of the month is assumed. This means that a specification like "July 1994" will look for observations done on July 1 1994 00:00:00, not for observations done during July 1994. Note also that when entering a date with the month in numerical format, the American ordeing is used; i.e., the first number is the month.

If a time is omitted, then midnight (00:00:00) is assumed. Otherwise, you can specify a time in any of these formats:

      14:30
      14:30:20
      14:30:20:999
      14:30:20.9
      4am
      4 PM
      04:30:20 AM
    

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

      > Jul 15 1994
      < Jul 15 1994
    

You can use the .. operator to search on a range of dates:

     Jul 1 1994 .. Aug 1 1995
   

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 1994 .. Jul 3 1994, 
     Dec 1 1995 .. Dec 6 1995
   

will search for observations done within either one of these date ranges.

Exposure Time

The commanded exposure time in seconds. You can use operators or ranges in this field; for example,

   < 100
   > 1000.0
   100 .. 1000

You can exclude a range of exposures using a comma:

  < 100, > 1000

Observer/PI Last Name

The last name of the principal investigator of the observation. We sometimes refer to this person as the "observer".

Proposal ID

The HST proposal number under which the observation was executed. This can be a numeric ID or a comma-separated list of numeric IDs. Any characters other than digits, commas, and spaces will cause an error message to be displayed. For example, instead of searching for GO-5916, simply specify 5916. Or to search for observations from either proposal 5410 or proposal 5916, specify 5410, 5916.

Target Description

A short description of the target, supplied by the observer. like target names, these may not always be reliable- one observer's CLUSTER OF GALAXIES may be another's ELLIPTICAL- but they are generally better than nothing (especially where solar system objects are concerned; planet, asteroid, and comet names are more likely to be spelled out in the target description than in the target name).

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.

Dataset

The dataset name is the unique identifier for an HST observation. (For NICMOS and STIS, it can also represent an association of exposures.) This value can be wildcarded using a *. When you specify a dataset name, any instrument or wavelength specification will be ignored.

Apertures

Enter HST aperture(s); These examples50CCD, 50CORON, WF2-FIX, WF3-FIX are a subset of the complete list.

Filters

Enter HST filter name(s); for example F606W or F110W, F160W are a subset of the complete list.

Obset ID

The observation set within the program. This is usually the same as the visit number, though in a small number of cases it will be different. The obset ID is used as the fourth and fifth letters of a dataset name. You can enter a comma separated list here. If necessary, obset IDs will be padded with leading zeroes to two characters.

Instruments

Here you select which instruments you want data from. We've divided the instruments into Imagers, Spectrographs, and Other, but instruments that are (or were) capable of producing either images or spectra will appear in both places. These buttons will help you select only images or spectra from a particular instrument.

Users with Javascript enabled in their browsers will see two little buttons here labelled ALL and NONE. These buttons will select or deselect all of the checkboxes in the section, so you don't have to go through hitting lots of checkboxes if you only want one instrument.

Imagers

In this section, select the kind of images you want to search for by selecting the instrument.

Spectrographs

In this section, select the kind of spectra you want to search for by selecting the instrument.

Notice that some instruments are capable of producing both images and spectra. In this case, the query will be properly built to search for the selected observation type for that instrument.

Other

Here you can select data from instruments that produce neither images nor spectra: the Fine Guidance Sensors (which produce astrometric, usually interferometric, data) and the High Speed Photometer (which produced photometric data). These are not checked by default.

Release Date

Select the release date for the data, in GMT. See the observation date for the entry format. HST data has a nominal proprietary period of one year (though in special cases, this may be shortened or extended). The Release Date field gives the end of the dataset's proprietary period.

Archive Date

This is the date on which a dataset was archived. If a dataset was archived more than once (for example, if it was reprocessed by the pipeline), then this will show the latest archive date.

About 75% of all science datasets are archived within 24 hours after the end of the observation (delays longer than this are usually due to problems in pipeline calibration, or if the data stream gets backed up. Delays like this are rare, however, and are more likely to apply to the newer instruments early in their careers.)

Observations - Science or Calibration

Choose Science (default) to get only science observations in the search results. Choose Calibration to get only calibration observations in the search results. At this time, you may not choose both options at the same time.

User Specified Field n

You may use these form elements to search on any column(s) in the mission table. First, select the field you wish to search from the pulldown menu under the "User-specified field n" heading. Then, type in the qualification in the corresponding "Field Descriptions" box. Clicking on the "Field Descriptions" link, will display information on the allowed fields including the allowed range of values.

As an example, a Kepler user might select "E(B-V)" from the pulldown menu and enter "< 0.5" in the "Field Descriptions" box.

NOTE only fields which are not already included on the search form should be selected. Specifying search criteria for a field that is listed in BOTH the form and in the User Specified field, may cause either the query to fail or return unexpected results.

Output Columns

This form element allows you to choose the columns to be displayed and their order, for the search results. A set of columns that are commonly requested has been chosen as a default.

You remove output columns by highlighting the column to be removed and then clicking on the remove button to the right of the output columns list.

You may determine the order of columns by highlighting a column and then clicking the up or down buttons to the right of the list of chosen output columns.

You may also add more columns to the list, either singly or all at once. To add individual columns, select the desired column from the pull down menu beneath the list of chosen output columns, then click the add button. The column will be added to the bottom of the output column list. To add all the available columns, click the "add all" button.

Note the output column form element has its own reset button to restore the list of output columns to the values initially displayed when the page was drawn. The reset button at the top of the form is used to reset the other form elements. Clicking the "clear form" button will restore the original defaults to all isections of the form.

One warning, the amount of memory required for a search is proportional to the number of columns requested. For large requests, users may want to reduce the number of output columns to the minimum required.

Verb

Verb is an integer parameter used by the VO community for specifying the amount of output returned for a given search request. It is only available when retrieving data as a web service but works with every MAST service. Setting verb=3 in a search request is equivalent to specifying "add all" from a search form; it will return all the available columns in the output not just the standard default fields. Currently setting verb to any other value has no effect.

Sort output by:

Choose how you want the output rows sorted. You can select up to three fields to sort on. The rows will be sorted in the order of the first sort field; if two rows have the same sort field, they will be sorted in order of the second sort field, and so on. Default sort fields may be listed, but any field from the pulldown list can be used. Specifying multiple sort fields may increase executon time. If you prefer no sorting, you can specify "null" for all 3 fields. This may speed up the query, but results will be displayed in the order in which they were originally stored in the database table.

For each field, you can select that the rows be sorted in reverse order on that field by selecting the reverse checkbox. For example, you can sort the rows with the most recent observations first by selecting Observation Date for the first sort field and selecting the reverse checkbox next to it.

One word of caution: the selected sort field can change the search results when the query finds more rows than are displayed ( i.e, when the number of found rows exceeds the value of "maximum records"). For example, for a search on a particular coordinate that finds 5,000 entries, if the search is sorted on exposure time and 1,001 rows are to be displayed (the default), then the 1,001 shortest exposures from the 5,000 found entries will be displayed which may not include the entries closest to the desired position. (It is a good idea to always sort on "ang_sep" for target or coordinate searches).

Display Coordinates

Specifies the format for displaying the primary equatorial (i.e., RA and Dec) coordinates. The options include:

• Sexagesimal - The default format with Right Ascension specified as hh mm ss.sss and Declination as +/-dd mm ss.ss ( e.g., RA = 12 46 11.091, Dec = -00 30 12.08). Note an extra digit was added as of June, 2012.
• Degrees - Decimal degrees for both RA and Dec with 7 significant figures to the right of the decimal point (e.g., RA=191.5461912, Dec=-0.5033333). Note 2 extra digits were added as of June, 2012. or
• Hours - Decimal hours for RA and decimal degrees for Dec in same format as for decimal degrees (e.g., RA=12.7697512, Dec=-0.5033333). Note decimal hours = decimal degrees/15.0. (Note 2 extra digits were added as of June, 2012.)

Any other coordinate fields contained in the searched mission catalog will be displayed in their original format.

Maximum Records

This value specifies the maximum number of rows returned in a single query. For the standard mission search forms, the current default is 1,001, but values from 1 to 25,001 are allowed. For the file upload forms in which multiple targets, data ID's, or coordinates can be specified, the default is set to 20 rows per file entry, with allowed values ranging from 1 to 5,000.

Note when displayed as HTML, the latest search scripts will display 100 records per page. Links to the additional pages are shown on the results page. This paging feature however does require javascript to be turned on.

Users should be cautioned about retrieving a large number of records (i.e., > 10,000 - 15,000) in HTML format. This can cause memory problems for the browser (particulrly Safari) and prevent javascript commands from functioning. It may also cause the browser to freeze and require restarting. Using the output format options which download results in a file can reduce the problem.

Another option for large requests is to use "Casjobs". Casjobs requires requesting a user name and password, and submitting queries in SQL, but it allows users to submit large search results and save them online. For Kepler, the link ito Casjobs is http://mastweb.stsci.edu/kplrcasjobs/. For other missions, check the Search_Retrieve page in the left gutter.

When queries are submitted as a web service, the default number of rows returned is 2,000, but any value is allowed when max_rows is specified as a query parameter. (See the MAST Web services page for more information.)

Records per page

This parameter controls the number of records displayed per web page. By default, 100 rows or records are displayed per HTML page. Therefore if 400 records are returned, links to 4 pages will be displayed at the top and bottom of the results table. The paging feature however uses javascript, so if javascript is turned off, paging won't work and only the rows shown on the first page can be displayed. This is one reason why increasing the default value may be helpful. The current limit is 1000 rows per page which is recommended for large requests. Note this value is ignored when output formats other than HTML are selected.

Make Rows Distinct

Selecting this checkbox will restrict the display to only rows in which every output column value for a given row is unique. This option is primarily useful when only a small number of columns are displayed (i.e., using the "remove" button to remove default output columns) and when the selected columns have duplicate values. Including columns which already have unique values (e.g. Kepler ID or Data ID) will make the "Distinct" option ineffective.

As an example, a IUE or FUSE user might want to create a list of unique target names for a specific object class/category. He or she would specify the desired object class, select only "object Class" and "target name" for the output columns, click the "Make Rows Distinct" button, then click "Search".

Note that for some missions, columns such as RA, Dec and Magnitude were frequently defined by the observer and often have different values for the same target. If columns such as these are chosen as output columns, there will often be more than one row listed per object name.

Output Format

You may choose any of the following formats for displaying/storing search results. If you are using a browser (e.g., Firefox, etc) to submit a query from a MAST web form, the formats labelled "File: ..." offer a way to download results directly to your local computer. Choose any of the other format options if you want to display the results in the browser, or if you are submitting the request from a program (see MAST web services).

• HTML_Table (default) - results returned as a standard HTML table including various links for retrieving data, displaying previews, literature references, plotting spectra, etc.
• File: Excel_Spreadsheet - results are stored as an Excel spreadsheet file. (Note: assumes users computer/browser provides support for Excel-format files). The default file name when downloaded is "mission"_search.xls where "mission" is the mission name (e.g., fuse_search.xls).
• VOTable - an XML format adopted by the Virtual Observatory (VO) project and displayed in the user's browser. Note coordinates in VOTable format are always in decimal degrees rather than sexagesimal format. For searches returning results from more than one mission and/or target, multiple "resource" tags are created. Searches with a radius of 0 will return a VOTable file listing the output fields for that particular mission/catalog. (For more information on the XML file format, see VOTable documentation.)
• Comma-separated values - a simple ASCII array containing column headings followed by rows of comma-separated values. In file upload mode, a blank line is inserted between the search results to separate multiple target queries.
• Space-separated values - a simple ASCII array containing column headings followed by rows of space-separated values. In file upload mode, a blank line is inserted between the search results to separate multiple target queries. Note users may want to select coordinates in decimal rather than sexagesimal format to maintain the correspondence between column headings and entries although some column headings may contain blanks as well. (Semi-colons, pipes, or commas are probably safer delimiters.)
• IRAF Space-separated values with INDEFs - Like the space-separated format above except empty fields are replaced with the string "INDEF". This format is useful for IRAF-compatibility.
• Semi-colon separated values - a simple ASCII array containing column headings followed by rows of semi-colon separated values. In file upload mode, a blank line is inserted between the search results to separate multiple target queries.
• Tab-separated values - a simple ASCII array containing tabs for delimiters. May be useful for ingesting into Excel spreadsheets.
• Pipe-separated values - a simple ASCII array containing column headings followed by rows of pipe or vertical bar separated values. (Note: not offered in file upload mode.)
• Json format - Javascript Object Notation (json) is a simple machine and human-readable, name/value ASCII format supported by many programming languages. (Note: not offered in file upload mode.)
• File: comma-separated values - a simple ASCII text file containing column headings followed by rows of comma-separated values. In file upload mode, a blank line is inserted between the search results to separate multiple target queries. Rather than being displayed in the browser, the results are directly downloaded to the users computer using the file name "mission"_search.txt where "mission" is the mission name (e.g., hst_search.txt). Depending on the browser settings, the user may be prompted for a file location before the file is downloaded.
• File: Space-separated values - a simple ASCII text file containing column headings followed by rows of space-separated values. In file upload mode, a blank line is inserted between the search results to separate multiple target queries. Rather than being displayed in the browser, the results are directly downloaded to the users computer using the file name "mission"_search.txt where "mission" is the mission name (e.g., hst_search.txt). Depending on the browser settings, the user may be prompted for a file location before the file is downloaded.
• File: IRAF Space-separated values with INDEFs - Like the space-separated format above except empty fields are replaced with the string "INDEF". This file format is useful for IRAF-compatibility.
• File: Semicolon-separated values - a simple ASCII text file containing column headings followed by rows of semicolon-separated values. In file upload mode, a blank line is inserted between the search results to separate multiple target queries. Rather than being displayed in the browser, the results are directly downloaded to the users computer using the file name "mission"_search.txt where "mission" is the mission name (e.g., hst_search.txt). Depending on the browser settings, the user may be prompted for a file location before the file is downloaded.
• File: Tab-separated values - a simple ASCII file containing tabs for delimiters. May be useful for ingesting into Excel spreadsheets.
• File: Pipe-separated values - a simple ASCII text file containing column headings followed by rows of pipe-separated values. (Note: not offered in file upload mode.) Rather than being displayed in the browser, the results are directly downloaded to the users computer using the file name "mission"_search.txt where "mission" is the mission name (e.g., hst_search.txt). Depending on the browser settings, the user may be prompted for a file location before the file is downloaded.
• File: Json format - Javascript Object Notation (json) is a simple machine and human-readable, name/value ASCII format supported by many programming languages. Rather than being displayed in the browser, the results are directly downloaded to the users computer using the file name "mission"_search.txt where "mission" is the mission name (e.g., hst_search.txt). Depending on the browser settings, the user may be prompted for a file location before the file is downloaded.
• File: WGET Commands - This option is only available for certain missions. If selected, a shell script file is output which the user can execute from his own computer to download all the selected light curves or extracted spectral files with one command. The shell script file uses the "WGET" program which is available for most operating systems. Note for Kepler, two WGET options are available: "File: WGET LC commands" will create a script for downloading available light curves, "File: WGET TPF commands" will create a script for downloading target pixel files.

Note: If no entries are found for an entry a "no entries found" message is written in the selected format and the program continues. In all cases, error conditions will cause the database search to abort.