Retrieving Exoplanet Archive Data With Table Access Protocol
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Synchronous and Asynchronous QueriesConstructing Synchronous TAP Queries
Using Spatial Constraints in Queries
Retrieving Table Schema
Best Practices
More Examples
The NASA Exoplanet Archive's TAP service allows users to programmatically access and retrieve data from some of its data tables as an alternative to the interactive web interface.
If you use any of the following data sets for your research, please cite the archive's DOI for the data.
The Exoplanet Archive's TAP service is connected to the following tables:
More archive tables will be transitioned to TAP in the coming months. To programmatically retrieve data from archive tables not currently supported by TAP, such as the Mission Stars table, please use the archive's existing application programming interface (API).
About Table Access Protocol
Table Access Protocol (TAP) is a recommended standard developed by the Virtual Astronomy community and now maintained by the International Virtual Observatory Alliance (IVOA). The TAP technical specification is on the IVOA website (http://www.ivoa.net/documents/TAP).
The archive's TAP service uses Structured Query Language (SQL), and the output can be formatted in VOTable (votable), comma-separated values (csv), tab-separated values (tsv), or JavaScript Object Notation (JSON). You may also select output columns and perform functions on the results.
Synchronous and Asynchronous Queries
In a nutshell, a synchronous query runs until it completes, and then streams the results back. An asynchronous query runs in the background and gives you a place to check whether your job is done, rather than streaming results back directly.
The archive's TAP service supports both synchronous and asynchronous queries, but the two tables currently supported are small enough so synchronous queries should be adequate. However, we do recommend using a TAP client when downloading large data sets (e.g., the entire Planetary Systems table) in the default VOTable format because some web browsers may struggle to display all of the data.
Constructing Synchronous TAP Queries
TAP is a URL-based HTTP web service, so the query can be entered directly into a web browser. TAP-compatible clients and software like TOPCAT and PyVO, and TAP+ all work with the Exoplanet Archive TAP service. A list of valid queries are given at the end of this document.
SELECT <column list> FROM <table> WHERE <constraints>To construct a synchronous TAP query:
(Required) Step 1: Start with the base service URL.
- For web browsers:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query= - For clients such as TOPCAT and pyVO:
https://exoplanetarchive.ipac.caltech.edu/TAP
(Required) Step 2: Next, add the query argument using the required select and from ADQL statements (in this order).
selectspecifies which columns to return. An asterisk (*) tells the system to return all columns.fromspecifies the database table.
In the following example, the entire Planetary Systems table is returned in VOTable format:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+*+from+ps
Alternatively, you can name specific columns (separated with commas, no spaces) to return if you don't want the entire table. Here is a revised example that returns only data in the Planet Name (pl_name), Planet Mass (pl_masse), Right Ascension (ra) and Declination (dec) columns:.
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+pl_name,pl_masse,ra,dec+from+ps
Note that for encoding purposes, all spaces in the SQL should be replaced with a plus (+) symbol.
(Optional) Step 3: Add more constraints using the where clause.
The where clause, though optional, allows you to include more complex constraints in your query by using AND, OR, and parentheses.
Here are some examples:
| Enter this... | To specify this... |
|---|---|
dec > 0. |
Planets that have a declination greater than 0 degrees |
pl_masse between 0.5 and 2.0 |
Planets that have a mass between 0.5 and 2.0 Earth masses |
discoverymethod = 'Radial Velocity' |
Planets that were discovered by the radial velocity method |
|
All planets listed as confirmed in lower-case in the soltype column of the database table All planets listed as confirmed in upper-case in the soltype column of the database table |
default_flag=1 |
Show only the default solution |
pl_rade < = 2 |
Planets with Earth radii less than or equal to 2 Rearth |
pl_orbper > = 1000 |
Planets with orbital periods greater than or equal to 1000 days |
So, our example query that returns the planet names, masses, and coordinates for all confirmed planets of about Earth size would read:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=+where+upper(soltype)+like+'%25CONF%25'+and+pl_masse+between+0.5+and+2.0
select+pl_name,pl_masse,ra,dec+from+ps
(Optional) Step 4 : Specify the output file format.
Unless otherwise specified, query results are automatically returned as a VOTable. Other supported formats:
| Format Name | Parameter |
| JSON | json |
| TSV | tsv |
| CSV | csv |
| VOTable | votable |
So, returning to our example from Step 3, we append the query to specify CSV format:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+pl_name,pl_masse,ra,dec+from+ps&format=csv
+where+upper(soltype)+like+'%25CONF%25'+and+pl_masse+between+0.5+and+2.0
Using Spatial Constraints In Queries
TAP also allows you to include ADQL-style spatial constraints using custom functions in the WHERE clause to define a circle, box, or polygon region.
In the following example, the query directs TAP to find and return all records in the Planetary Systems table where the point defined by the ra and dec columns in the database table for a circle, box, and polygon area based on the coordinates of Proxima Centauri (217.42896,-62.67947).
| For this shape... | Define the area as... | Using this query... |
|---|---|---|
| Circle | Inside a 0.1-degree circle | https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+*+from+ps+where+contains(point('icrs',ra,dec),circle('icrs',217.42896,-62.67947,0.1))=1 |
| Box | Same center as a circle, and a size of 0.1 x 0.1 degrees |
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+pl_name,ra,dec+from+ps+where+contains(point('icrs',ra,dec),box('icrs',217.42896,-62.67947,0.1,0.1))=1 |
| Polygon | Give the coordinates of four corners, rather than the center |
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+pl_name,ra,dec+from+ps+where+contains(point('icrs',ra,dec),polygon('icrs',217.,-62.,218.,-62.,218.,-63.,217.,-63))=1 |
The spatial constraints act like any other other constraint (e.g.,
dec > 0.) in that they can appear mixed in with the regular relational
constraints and inside AND/OR and parenthesis constructs. For more information about ADQL geometric constraints, see the IVOA document.
Retrieving Table Schema
The TAP service provides information about the tables being served, including table names, column names, and data types. To compose a query, you need to know the table names, column names, and types. The TAP_SCHEMA can be queried like the other tables in order to return information about the data tables.
Some examples:
| Use This Query... | To Return This... |
|---|---|
| https://exoplanetarchive.ipac.caltech.edu/TAP/tables | A comprehensive XML document of all tables, column names, and metadata available through the archive's TAP service. |
|
Lists of available schemas (sets of tables) through TAP |
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=
select+schema_name,table_name+from+TAP_SCHEMA.tables |
A list of available tables |
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=
select+*+from+TAP_SCHEMA.columns+%20where+table_name+like+
%27ps%27 |
Returns basic information on the Planetary Systems table, such as column names, column type, width, format, etc.
Note: The PS and PSCompPars Table Data Column Definitions Document also provides this information. |
More information about the TAP_SCHEMA specification is in this IVOA document.
Best Practices
-
Always specify a table, i.e.,
select+*+from+psorselect+*+from+pscomppars -
Encode special characters in web queries, including plus signs (+) as
%2B,%27for a single quotation mark ( ' ),%20for a space, and%25for letters (especially if the first two letters are A-F, which are used for different unicode characters). Note that most web browsers will automatically encode queries entered into their search field and some utility programs, such as wget (but not curl), will do so as well. -
Queries must be on a single line. Line breaks in the examples given in this document are for display purposes only.
-
Be aware of case-sensitivity: ADQL and Oracle table and column names are not case-sensitive. However, values like CONFIRMED or CANDIDATE are case-sensitive, as well as object names (e.g., "eps CrB b"). Query the TAP schema to verify capitalization, or use the
upper()andlower()functions and wildcards (%25) if you're unsure about capitalization. - Use a TAP client when returning large data sets. If you're downloading the entire PS or PSCompPars tables in VOTable format, your web browser may struggle to display all of the results. Try using a client like TOPCAT, pyVO, or TAP+.
More Examples
Count the total number of confirmed planets, from PS table
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+count(pl_name)+from+ps+where+default_flag=1&format=csv
All confirmed planets found by TESS, from PS Table:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+*+from+ps+where+disc_facility+=+'Transiting Exoplanet Survey Satellite (TESS)'
Confirmed planets, listed alphabetically, that have been detected by transit method, from PS Table:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+distinct(pl_name)+from+ps+where+tran_flag+=+1+order+by+pl_name+desc+&format=csv
All Earth-sized planets (R<=1.8 Rearth) that have a mass measurement (pl_masse > 0.) from PS Table:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+hostname,pl_name,pl_rade,pl_masse+from+ps+where+pl_rade+<+=+1.8+and+pl_masse+>+0
All confirmed planets with the best mass (as identified by the archive) and their reference, and with an orbital period with semi-major axis and their references, and with more than one star in the system, and the best planet mass is less than or equal to 13, listed in order of best mass in descending order, from PSCompPars Table:
https://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+pl_name,pl_bmassj,pl_bmassj_reflink,pl_orbsmax,pl_orbsmax_reflink,sy_snum +from+pscomppars+where+sy_snum+>+1+and+pl_bmassj+<=+13+order+by+pl_bmassj+desc
Last updated: 7 October 2024
