Introduction to the Table Access Protocol (TAP) Service

Contact authors: Leanne Guy, Melissa Graham
Last verified to run: 2024-12-17
LSST Science Pipelines version: Weekly 2024_50
Container Size: medium
Targeted learning level: beginner

Description: Explore the DP0.2 catalogs with the TAP service.

Skills: Use the TAP service. Make simple ADQL queries. Visualize retrieved datasets.

LSST Data Products: Catalog schema. Object table.

Packages: lsst.rsp

Credit: Originally developed by Leanne Guy in the context of the Rubin DP0.1.

Get Support: Find DP0-related documentation and resources at dp0.lsst.io. Questions are welcome as new topics in the Support - Data Preview 0 Category of the Rubin Community Forum. Rubin staff will respond to all questions posted there.

1. Introduction

This notebook provides a beginner-level demonstration of how to use Astronomy Data Query Language (ADQL) to access DP0.2 catalog data via Rubin's Table Access Protocol (TAP) service.

The documentation for Data Preview 0.2 includes definitions of the data products, descriptions of catalog contents, and ADQL recipes. The RSP's Portal Aspect, with its graphical user interface, is also recommended for exploring the available catalogs and for testing queries.

1.1. TAP basics

TAP provides standardized access to catalog data for discovery, search, and retrieval. Full documentation for TAP is provided by the International Virtual Observatory Alliance (IVOA).

TAP Glossary

• schema - Database terminology for the abstract design that represents the storage of data in a database.
• tap_schema - The set of tables that describe the data tables and their columns.
• table collection - A collection of tables. E.g., dp02_dc2_catalogs.
• table - A collection of related data held in a table format in a database. E.g., dp02_dc2_catalogs.Object.
• query - A string formatted in ADQL that selects data from a table, with contraints if desired.
• results - The output of the TAP service's search method when a query is passed.

1.2. ADQL basics

The documentation for ADQL includes more information about syntax, keywords, operators, functions, and so on. ADQL is similar to SQL (Structured Query Langage).

A typical ADQL statement has at least three components:

SELECT <columns> FROM <catalog> WHERE <constraints>,

where

• <columns> is a comma-separated list of the columns to return,
• <catalog> is the name of the catalog to retreive data from, and
• <constraints> imposes a restriction that only rows with column values that meet the constraints are returned.

For example, say there is a catalog called "mysurveydata" with 5 columns, "col1", "col2", and so on. The ADQL statement:

SELECT col3, col4, col5 FROM mysurveydata WHERE col1 > 0.5 AND col5 < 10

would return a table that has three columns, and as many rows as meet both of the restrictions in the WHERE statement.

As the DP0.2 catalogs are very large, the ADQL statement to return an entire table should not be used (SELECT * FROM mysurveydata).

1.3. What is not covered in this tutorial?

The following intermediate-level TAP functionalities for retrieving catalog data are not demonstrated in this tutorial, but are covered in other tutorials.

See DP0.2 tutorial notebook 02b for:

• table joins
• renaming columns
• applying mathematical functions
• converting fluxes to magnitudes
• querying and visualizing large data sets

See DP0.2 tutorial notebook 02c for ObsTAP queries for images (metadata and pixel data).

1.4. Recommendations for TAP queries

The following recommendations are all demonstrated in Section 3.

1.4.1. Use asynchronous queries

In Section 2, synchronous queries are used with results = service.search(query). This is OK for querying schema or small amounts of data, but when more data is being retrieved it is recommended to use asynchronous jobs with job = service.submit_job(query) as demonstrated in Section 3.

1.4.2. Include coordinate constraints

When possible include coordinate constraints (e.g., use a cone search). The TAP-accessible tables are sharded by coordinate (RA, Dec). ADQL query statements that include constraints by coordinate do not require a whole-catalog search, and are typically faster (and can be much faster) than ADQL query statements which only include constraints for other columns.

1.4.3. Constrain detect_isPrimary = True

As a default, it is recommended to include a constraint of detect_isPrimary = True in queries for the Object, Source, and ForcedSource catalogs. This parameter is True if a source has no children, is in the inner region of a coadd patch, is in the inner region of a coadd tract, and is not detected in a pseudo-filter. Including this constraint will remove any duplicates (i.e., will not include both a parent and its deblended children). Only remove this constraint in situations where duplicates are desired.

1.4.4. If limiting rows, use TOP

Use of TOP is preferred to maxrec because most TAP services map maxrec to SELECT TOP on the back end anyways. Using TOP ensures that queries are copy-pasteable between interfaces (e.g., into the Portal Aspect).

1.4.5. If sorting, take care with ORDER BY

Combined use of TOP and ORDER BY in ADQL queries can be dangerous: it may take an unexpectedly long time because the database is trying to first sort, and then extract the top N elements. It is best to only combine TOP and ORDER BY if the query's WHERE statements significantly cut down the number of objects that would need to be sorted.

1.5. Import packages

Import general python packages (pandas, numpy, and matplotlib), two classes from astropy, and the Rubin Science Platform (RST) TAP service.

import pandas
import numpy as np
import matplotlib.pyplot as plt
import astropy.units as u
from astropy.visualization.wcsaxes import SphericalCircle
from lsst.rsp import get_tap_service, retrieve_query

1.6. Define functions and parameters

Get an instance of the TAP service, and assert that it exists.

service = get_tap_service("tap")
assert service is not None

Set the maximum number of rows to display from pandas.

pandas.set_option('display.max_rows', 20)

2. Explore the TAP schema

This section will use ADQL queries of increasing complexity to both explore the available catalog data and to demonstrate how to use the TAP service and ADQL.

2.1. Synchronous queries

This section uses "synchronous" TAP queries. This means that the query is run and the results are retrieved at the same time. No other cells can be run while this is happening.

Since the queries in this section are very simple, and are only retrieving schemas (not data), they are very quick and synchronous queries work fine. However, when data is retrieved from catalogs, asynchronous queries should be used (Section 3).

2.2. List all catalogs (schema)

Create an ADQL query that selects all columns (*) from the tap_schema. The results of the query will be a list of available schemas (in other words, the available catalogs).

Store it in a string named query.

query = 'SELECT * FROM tap_schema.schemas'

Execute the query by passing query to the TAP service's search method, and store the output in results.

results = service.search(query)

Print the type of results.

print(type(results))

<class 'pyvo.dal.tap.TAPResults'>

TAPResults is a python class from the PyVO Data Access package. The documentation for TAPResults has more information about the class and its methods.

Typically, for convenience it is recommended to convert the results into an Astropy table.

Rerun the query, but store the results as an astropy table with the to_table() method.

results_table = service.search(query).to_table()

Print the type of results and see that it is an astropy table.

print(type(results_table))

<class 'astropy.table.table.Table'>

Display the table.

results_table

Table length=3

description	schema_index	schema_name	utype
object	int32	object	object
Data Preview 0.2 contains the image and catalog products of the Rubin Science Pipelines v23 processing of the DESC Data Challenge 2 simulation, which covered 300 square degrees of the wide-fast-deep LSST survey region over 5 years.	0	dp02_dc2_catalogs
ObsCore v1.1 attributes in ObsTAP realization	1	ivoa
A TAP-standard-mandated schema to describe tablesets in a TAP 1.1 service	100000	tap_schema

The table above shows that the DP0.2 data schema_name is dp02_dc2_catalogs.

"DC2" stands for "Data Challenge 2" and it was the name of the effort by the Dark Energy Science Collaboration to create the simulated data (The DESC DC2 Simulated Sky Survey).

Although the description says "Data Preview 0.2 contains the image and catalog products...", the dp02_dc2_catalogs contains only catalog data and image data for DP0.2 is stored in the ObsCore, with schema_name = ivoa. Accessing image data via the TAP service is covered in another tutorial.

The above table is quite short, and it is obvious from looking at it that the table collection for DP0.2 is dp02_dc2_catalogs. However, there may be times in the future when there are many more schemas available. The following demonstrates a way to search for catalogs by name.

Use a for loop to look for the presence of dp02 in the schema_name column for every row of the results table, and write the name when there is a match.

for name in results_table['schema_name']:
    if name.find('dp02') > -1:
        print(name)

dp02_dc2_catalogs

Clean up by deleting the query and its results.

del query, results, results_table

2.3. List all tables in the DP0.2 catalog

Create a query that selects all columns from tap_schema.tables for the dp02_dc2_catalogs schema. Add an ORDER BY statement to return the results sorted by table_index.

This query will return the names of all tables that are available in the dp02_dc2_catalogs.

query = "SELECT * FROM tap_schema.tables " \
        "WHERE tap_schema.tables.schema_name = 'dp02_dc2_catalogs'" \
        "ORDER BY table_index ASC"

Use a synchronous query and return the results as an astropy table.

results = service.search(query).to_table()

Display the results to see the tables in the DP0.2 schema.

results

Table length=11

description	schema_name	table_index	table_name	table_type	utype
object	object	int32	object	object	object
Properties of the astronomical objects detected and measured on the deep coadded images.	dp02_dc2_catalogs	1	dp02_dc2_catalogs.Object	table
Properties of detections on the single-epoch visit images, performed independently of the Object detections on coadded images.	dp02_dc2_catalogs	2	dp02_dc2_catalogs.Source	table
Forced-photometry measurements on individual single-epoch visit images and difference images, based on and linked to the entries in the Object table. Point-source PSF photometry is performed, based on coordinates from a reference band chosen for each Object and reported in the Object.refBand column.	dp02_dc2_catalogs	3	dp02_dc2_catalogs.ForcedSource	table
Properties of time-varying astronomical objects based on association of data from one or more spatially-related DiaSource detections on individual single-epoch difference images.	dp02_dc2_catalogs	4	dp02_dc2_catalogs.DiaObject	table
Properties of transient-object detections on the single-epoch difference images.	dp02_dc2_catalogs	5	dp02_dc2_catalogs.DiaSource	table
Point-source forced-photometry measurements on individual single-epoch visit images and difference images, based on and linked to the entries in the DiaObject table.	dp02_dc2_catalogs	6	dp02_dc2_catalogs.ForcedSourceOnDiaObject	table
Metadata about the pointings of the DC2 simulated survey, largely associated with the boresight of the entire focal plane.	dp02_dc2_catalogs	7	dp02_dc2_catalogs.Visit	table
Metadata about the 189 individual CCD images for each Visit in the DC2 simulated survey.	dp02_dc2_catalogs	8	dp02_dc2_catalogs.CcdVisit	table
Static information about the subset of tracts and patches from the standard LSST skymap that apply to coadds in these catalogs	dp02_dc2_catalogs	9	dp02_dc2_catalogs.CoaddPatches	table
Summary properties of objects from the DESC DC2 truth catalog, as described in arXiv:2101.04855. Includes the noiseless astrometric and photometric parameters.	dp02_dc2_catalogs	10	dp02_dc2_catalogs.TruthSummary	table
Match information for TruthSummary objects.	dp02_dc2_catalogs	11	dp02_dc2_catalogs.MatchesTruth	table

Clean up.

del query, results

2.4. List all columns in the Object table

For the example, use the first table: the Object table (see Section 3).

The following query selects four colums from the tap_schema.columns table, column names, data types, descriptions, and units, only for the Object table.

query = "SELECT column_name, datatype, description, unit " \
        "FROM tap_schema.columns " \
        "WHERE table_name = 'dp02_dc2_catalogs.Object'"

Run the synchronous query and store results in an astropy table.

results = service.search(query).to_table()

Display the results.

results

Table length=991

column_name	datatype	description	unit
object	object	object	object
coord_dec	double	Fiducial ICRS Declination of centroid used for database indexing	deg
coord_ra	double	Fiducial ICRS Right Ascension of centroid used for database indexing	deg
deblend_nChild	int	Number of children this object has (defaults to 0)
deblend_skipped	boolean	Deblender skipped this source
detect_fromBlend	boolean	This source is deblended from a parent with more than one child.
detect_isDeblendedModelSource	boolean	True if source has no children and is in the inner region of a coadd patch and is in the inner region of a coadd tract and is not a sky source and is a deblended child
detect_isDeblendedSource	boolean	True if source has no children and is in the inner region of a coadd patch and is in the inner region of a coadd tract and is not a sky source and is either an unblended isolated source or a deblended child from a parent with
detect_isIsolated	boolean	This source is not a part of a blend.
detect_isPatchInner	boolean	True if source is in the inner region of a coadd patch
...	...	...	...
z_pixelFlags_suspect	boolean	Source's footprint includes suspect pixels. Measured on z-band.
z_pixelFlags_suspectCenter	boolean	Source's center is close to suspect pixels. Measured on z-band.
z_psfFlux	double	Flux derived from linear least-squares fit of PSF model. Forced on z-band.	nJy
z_psfFlux_area	float	Effective area of PSF. Forced on z-band.	pixel
z_psfFlux_flag	boolean	General Failure Flag. Forced on z-band.
z_psfFlux_flag_apCorr	boolean	Set if unable to aperture correct base_PsfFlux. Forced on z-band.
z_psfFlux_flag_edge	boolean	Object was too close to the edge of the image to use the full PSF model. Forced on z-band.
z_psfFlux_flag_noGoodPixels	boolean	Not enough non-rejected pixels in data to attempt the fit. Forced on z-band.
z_psfFluxErr	double	Flux uncertainty derived from linear least-squares fit of PSF model. Forced on z-band.	nJy
z_ra	double	Position in Right Ascension. Measured on z-band.	deg

Above, notice that the table is very long (991 rows) and the display has been truncated (the '...' represents skipped rows). There are too many columns to read through.

Use a for loop to look for the presence of coord in the column_name column for every row of the results table, and write the name when there is a match.

search_string = 'coord'
for cname in results['column_name']:
    if cname.find(search_string) > -1:
        print(cname)

coord_dec
coord_ra

Repeat the above exercise, but for all columns that are related to the g-band PSF (point spread function) flux measurements. This flux measurement is appropriate to use for point-like objects, like stars.

Notice that there is a flux, and error, and several flag values. Flags indicate various warnings, e.g., if the source was close to the edge of the detector and thus might be missing some flux.

search_string = 'g_psfFlux'
for cname in results['column_name']:
    if cname.find(search_string) > -1:
        print(cname)

g_psfFlux
g_psfFlux_area
g_psfFlux_flag
g_psfFlux_flag_apCorr
g_psfFlux_flag_edge
g_psfFlux_flag_noGoodPixels
g_psfFluxErr

The datatype column has a limited set of values. Print the unique data types.

print(np.unique(results['datatype']))

datatype
--------
 boolean
    char
  double
   float
     int
    long

The units column also has a limited set of values. Print the unique set of units used in the Object table.

print(np.unique(results['unit']))

  unit  
--------
        
     deg
     nJy
   pixel
pixel**2

Clean up.

del query, results

3. Query the DP0.2 Object table

The Object table contains measurements for all objects detected in the deep coadd (stacked) images. It includes objects detected with a signal-to-noise ratio of at least five in at least one filter. Detections are deblended, e.g., overlapping galaxies (blended sources in the image), are split into individual objects (referred to as 'parent' and 'child' objects). The measurements of these objects, such as shapes, sizes, and fluxes, are made in all filters.

The Object catalog (dp02_dc2_catalogs.Object) contains sources detected in the coadded images (also called stacked or combined images).

3.1. Asynchronous queries

This section uses "asynchronous" TAP queries. This means that the query is submitted as a job to the TAP service, and it can run in the background until it completes. The results can then be retrieved right away, or at a later time. Other cells can be run while this is happening.

Since the queries in this section are more complex, and retrieving rows of data (not just schema), asynchronous queries are used.

3.2. Cone search

A cone search means a catalog query that returns all objects within a given radius of a sky coordinate. Since a given angular diameter corresponds to a larger physical diameter at larger distances, the volume queried is a cone, not a cylinder.

In ADQL, a cone search is executed with WHERE CONTAINS(POINT(), CIRCLE()) = 1.

• POINT() passes the catalog's columns for sky coordinates.
• CIRCLE() defines the center and radius of the search circle.
• CONTAINS() = 1 constrains the query to only return rows for which the statement "this circle contains this point" is "True" (=1).

In Section 2.4, the columns for sky coordinate in the Object catalog were shown to be coord_ra and coord_dec, with units of degrees. The approximate center of the DP0.2 area is RA, Dec = 62.0, -37.0 (decimal degrees). A conservative radius that ensures a quick query with a limited number of rows returned in 0.01 degrees (36 arcsec).

The following query would return the coord_ra and coord_dec columns for all rows of the Object table which are within 0.05 degrees of RA, Dec = 62.0, -37.0, and for which the detect_isPrimary column is "True" (as recommended above). The 'ICRS' stands for "International Celestial Reference System", the reference frame for the coordinates.

SELECT coord_ra, coord_dec FROM dp02_dc2_catalogs.Object 
WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.05")) = 1 
AND detect_isPrimary = 1

Define the center coordinates and the radius. TAP queries are created as strings, so define str_center_coords and str_radius as strings which can be inserted into the query string.

center_ra = 62
center_dec = -37
radius = 0.01

str_center_coords = str(center_ra) + ", " + str(center_dec)
str_radius = str(radius)

Create the query string, and print it.

query = "SELECT coord_ra, coord_dec "\
        "FROM dp02_dc2_catalogs.Object "\
        "WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), "\
        "CIRCLE('ICRS', " + str_center_coords + ", " + str_radius + ")) = 1 "\
        "AND detect_isPrimary = 1"
print(query)

SELECT coord_ra, coord_dec FROM dp02_dc2_catalogs.Object WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.01)) = 1 AND detect_isPrimary = 1

Submit the query as an asynchronous job to the TAP service.

job = service.submit_job(query)
print('Job URL is', job.url)
print('Job phase is', job.phase)

Job URL is https://data-int.lsst.cloud/api/tap/async/fu2x4xl0qv600a8v
Job phase is PENDING

Run the job.

job.run()

<pyvo.dal.tap.AsyncTAPJob at 0x7b04f1a89150>

Wait for the job status to be either "COMPLETED" or "ERROR".

This is not mandatory, but is recommended; if it is not run, there will be no other automatic notification that the job is no longer running. However, note that if this cell is executed then no other cells can be executed while the job runs in the background.

job.wait(phases=['COMPLETED', 'ERROR'])
print('Job phase is', job.phase)

Job phase is COMPLETED

Optional: If the status returned was "ERROR", uncomment and execute this cell to print the error messages.

# job.raise_if_error()

If the status returned was "COMPLETED", execute this cell to retrieve the query results as an astropy table and print the length of the table.

results = job.fetch_result().to_table()
print(len(results))

173

Optional: Uncomment and execute to display the table contents.

# results

Plot the coordinates, right ascension (RA) vs. declination (Dec).

Use the astropy class SphericalCircle to shade the query region. This class takes into account the "cos-dec" factor (for points off the celestial equator, i.e., at non-zero declination, the real distance in the right ascension axis is smaller by a factor of the cosine of the declination).

fig = plt.figure(figsize=(4, 4))

region = SphericalCircle((center_ra * u.deg, center_dec * u.deg),
                         radius * u.deg, alpha=0.2, color='blue')
plt.gca().add_patch(region)

plt.plot(results['coord_ra'], results['coord_dec'],
         'o', alpha=0.5, color='black', mew=0)

plt.xlabel('RA')
plt.ylabel('Dec')
plt.show()

Figure 1: The Right Ascension (RA) versus Declination (Dec) coordinates for Objects retrieved by the query (black dots) within the query region (blue circle).

Clean up (and save memory) by deleting the job and its results.

job.delete()
del query, results

3.3. Limit rows returned with TOP

For debugging and testing queries, it can be useful to only retrieve a subset of the rows which meet the query constraints, because this is faster.

Alter the query used above to use TOP to return only N rows.

N = 20

query = "SELECT TOP " + str(N) + " coord_ra, coord_dec "\
        "FROM dp02_dc2_catalogs.Object "\
        "WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), "\
        "CIRCLE('ICRS', " + str_center_coords + ", " + str_radius + ")) = 1 "\
        "AND detect_isPrimary = 1"
print(query)

SELECT TOP 20 coord_ra, coord_dec FROM dp02_dc2_catalogs.Object WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.01)) = 1 AND detect_isPrimary = 1

Run the job asynchronously and wait until it is finished.

job = service.submit_job(query)
job.run()
job.wait(phases=['COMPLETED', 'ERROR'])
print('Job phase is', job.phase)

Job phase is COMPLETED

results = job.fetch_result().to_table()
print(len(results))

20

fig = plt.figure(figsize=(4, 4))
region = SphericalCircle((center_ra * u.deg, center_dec * u.deg),
                         radius * u.deg, alpha=0.2, color='blue')
plt.gca().add_patch(region)
plt.plot(results['coord_ra'], results['coord_dec'],
         'o', alpha=0.5, color='black', mew=0)
plt.xlabel('RA')
plt.ylabel('Dec')
plt.show()

Figure 2: The Right Ascension (RA) versus Declination (Dec) coordinates for only the top 20 Objects retrieved by the query (black dots) within the query region (blue circle). All of the black dots are in the lower half of the blue circle.

Clean up.

job.delete()
del query, results

3.4. Use of maxrec instead of TOP

TAP queries run in the Notebook Aspect of the RSP can also use the maxrec keyword for the TAP service. Use of TOP is preferred, as described in Section 1.4.4, but they work the same way from a Jupyter Notebook.

Use the same query as above, but without TOP.

query = "SELECT coord_ra, coord_dec "\
        "FROM dp02_dc2_catalogs.Object "\
        "WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), "\
        "CIRCLE('ICRS', " + str_center_coords + ", " + str_radius + ")) = 1 "\
        "AND detect_isPrimary = 1"
print(query)

SELECT coord_ra, coord_dec FROM dp02_dc2_catalogs.Object WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.01)) = 1 AND detect_isPrimary = 1

Include maxrec as a keyword when submitting the query to the TAP service. Run the job.

job = service.submit_job(query, maxrec=N)
job.run()
job.wait(phases=['COMPLETED', 'ERROR'])
print('Job phase is', job.phase)

Job phase is COMPLETED

Retrieve the job results.

Warning: Use of maxrec might return a DALOverflowWarning when the results are retrieved. This warns the user that partial results have been returned. In this case, it is ok to ignore this warning, because the query's intent was to return partial results by using maxrec.

results = job.fetch_result().to_table()
print(len(results))

20

/opt/lsst/software/stack/conda/envs/lsst-scipipe-9.0.0/lib/python3.11/site-packages/pyvo/dal/query.py:325: DALOverflowWarning: Partial result set. Potential causes MAXREC, async storage space, etc.
  warn("Partial result set. Potential causes MAXREC, async storage space, etc.",

Plot the results.

fig = plt.figure(figsize=(4, 4))
region = SphericalCircle((center_ra * u.deg, center_dec * u.deg),
                         radius * u.deg, alpha=0.2, color='blue')
plt.gca().add_patch(region)
plt.plot(results['coord_ra'], results['coord_dec'],
         'o', alpha=0.5, color='black', mew=0)
plt.xlabel('RA')
plt.ylabel('Dec')
plt.show()

Figure 3: Identical to Figure 2.

Clean up.

job.delete()
del query, results

3.5. Sort results with ORDER BY

As described in Section 1.4.5, use ORDER BY and TOP together with caution.

The TAP service first applies WHERE constraints, then ORDER BY, and then TOP. If the query is not well constrained, i.e., if thousands or more objects meet the WHERE constraints, then they all must first be sorted before the top number are returned. This is a waste of time and compute resources.

Create the query. Add an ORDER BY statement to the TAP query to return the TOP N objects sorted by coord_ra, in ascending (ASC) order.

query = "SELECT TOP " + str(N) + " coord_ra, coord_dec "\
        "FROM dp02_dc2_catalogs.Object "\
        "WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), "\
        "CIRCLE('ICRS', " + str_center_coords + ", " + str_radius + ")) = 1 "\
        "AND detect_isPrimary = 1 "\
        "ORDER BY coord_ra ASC"
print(query)

SELECT TOP 20 coord_ra, coord_dec FROM dp02_dc2_catalogs.Object WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.01)) = 1 AND detect_isPrimary = 1 ORDER BY coord_ra ASC

Run the job.

job = service.submit_job(query)
job.run()
job.wait(phases=['COMPLETED', 'ERROR'])
print('Job phase is', job.phase)

Job phase is COMPLETED

Retrieve the results.

results = job.fetch_result().to_table()
print(len(results))

20

Plot the results.

fig = plt.figure(figsize=(4, 4))
region = SphericalCircle((center_ra * u.deg, center_dec * u.deg),
                         radius * u.deg, alpha=0.2, color='blue')
plt.gca().add_patch(region)
plt.plot(results['coord_ra'], results['coord_dec'],
         'o', alpha=0.5, color='black', mew=0)
plt.xlabel('RA')
plt.ylabel('Dec')
plt.show()

Figure 4: Similar to Figure 2, except the top 20 Objects returned (black dots) are all on the left-most edge of the blue circle, because they have the lowest RA values, and the query results were sorted by RA in ascending order before the top 20 were selected.

Clean up.

job.delete()
del query, results

3.6. Sort results with pandas

The pandas package provides high-performance, easy-to-use data structures and data analysis tools for the Python programming language. TAP query results can be converted to pandas dataframes, and then pandas functionality (such as sorting) can be applied to the dataframe.

Use the same query as above for a small, unsorted set of Objects.

query = "SELECT coord_ra, coord_dec "\
        "FROM dp02_dc2_catalogs.Object "\
        "WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), "\
        "CIRCLE('ICRS', " + str_center_coords + ", " + str_radius + ")) = 1 "\
        "AND detect_isPrimary = 1"
print(query)

SELECT coord_ra, coord_dec FROM dp02_dc2_catalogs.Object WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.01)) = 1 AND detect_isPrimary = 1

Run the job.

job = service.submit_job(query)
job.run()
job.wait(phases=['COMPLETED', 'ERROR'])
print('Job phase is', job.phase)

Job phase is COMPLETED

Retrieve the results, and use the to_pandas() method to convert results to a pandas dataframe.

results = job.fetch_result().to_table().to_pandas()
print(len(results))

173

Print the type of results and see that it is a pandas dataframe.

print(type(results))

<class 'pandas.core.frame.DataFrame'>

Display the results.

results

	coord_ra	coord_dec
0	61.989258	-37.005119
1	61.997438	-37.005796
2	62.003285	-37.006248
3	61.998238	-37.007123
4	62.003341	-37.002536
...	...	...
168	61.990251	-36.996347
169	61.989260	-36.995563
170	61.990184	-36.995566
171	61.992685	-36.998426
172	61.992210	-36.998456

173 rows × 2 columns

In general, the order of results from TAP queries cannot be assumed to be the same every time, and they will not necessarily be sorted unless ORDER BY has been used in the query statement.

Use the pandas method sort_values to sort the dataframe by coord_ra, save it as a new dataframe named sorted_results, and display the new sorted dataframe.

sorted_results = results.sort_values('coord_ra')

sorted_results

	coord_ra	coord_dec
161	61.988079	-36.999024
164	61.988408	-36.998968
154	61.988546	-36.997821
165	61.988612	-37.001517
0	61.989258	-37.005119
...	...	...
82	62.010771	-36.998845
79	62.010843	-36.999844
98	62.010987	-36.996173
97	62.011207	-36.997063
128	62.012241	-36.999059

173 rows × 2 columns

Notice that the index values did not update, and are not in the order of the sorted dataframe.

To reset the index, use the pandas method set_index to reset the index of the sorted_results dataframe.

sorted_results.set_index(np.array(range(len(sorted_results))), inplace=True)

sorted_results

	coord_ra	coord_dec
0	61.988079	-36.999024
1	61.988408	-36.998968
2	61.988546	-36.997821
3	61.988612	-37.001517
4	61.989258	-37.005119
...	...	...
168	62.010771	-36.998845
169	62.010843	-36.999844
170	62.010987	-36.996173
171	62.011207	-36.997063
172	62.012241	-36.999059

173 rows × 2 columns

Clean up.

job.delete()
del query, results, sorted_results

4. Retrieve query results with job URL

Job results are generally available from previously run queries, and can be retrieved if the URL of the job is known and if the job has not been deleted.

Do not use job.delete() if the results will be retrieved later!

First, execute the same query as used above.

query = "SELECT coord_ra, coord_dec "\
        "FROM dp02_dc2_catalogs.Object "\
        "WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), "\
        "CIRCLE('ICRS', " + str_center_coords + ", " + str_radius + ")) = 1 "\
        "AND detect_isPrimary = 1"
print(query)

job = service.submit_job(query)
job.run()
job.wait(phases=['COMPLETED', 'ERROR'])
print('Job phase is', job.phase)

SELECT coord_ra, coord_dec FROM dp02_dc2_catalogs.Object WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.01)) = 1 AND detect_isPrimary = 1
Job phase is COMPLETED

Instead of using job.fetch_result(), store the job.url as my_job_url and print it.

my_job_url = str(job.url)
print(my_job_url)

https://data-int.lsst.cloud/api/tap/async/pk5arytxjo1xedlz

This URL can be used to retrieve the query results.

The URL could be shared with another user of the Rubin TAP service, and they could retrieve the same results.

Retrieve the job by passing my_job_url to retrieve_query, then retrieve the results with fetch_result().

retrieved_job = retrieve_query(my_job_url)
retrieved_results = retrieved_job.fetch_result().to_table().to_pandas()

retrieved_results

	coord_ra	coord_dec
0	61.989258	-37.005119
1	61.997438	-37.005796
2	62.003285	-37.006248
3	61.998238	-37.007123
4	62.003341	-37.002536
...	...	...
168	61.990251	-36.996347
169	61.989260	-36.995563
170	61.990184	-36.995566
171	61.992685	-36.998426
172	61.992210	-36.998456

173 rows × 2 columns

Clean up.

job.delete()
del query, retrieved_results

4.1. Retrieve results from a Portal query

It is also possible to retrieve the results of queries executed in the Portal Aspect of the Rubin Science Platform.

4.1.1. Run an ADQL query in the Portal

In a new browser tab, go to data.lsst.cloud and enter the Portal Aspect.

Click on the tab "DP0.2 Catalogs" at the top of the screen.

Click "Edit ADQL" at upper right.

Copy-paste the following query into the ADQL box as shown in the screenshot below.

SELECT coord_ra, coord_dec FROM dp02_dc2_catalogs.Object
WHERE CONTAINS(POINT('ICRS', coord_ra, coord_dec), CIRCLE('ICRS', 62, -37, 0.01)) = 1
AND detect_isPrimary = 1

Figure 5: A screenshot of the Portal's ADQL interface, with the query statement copied in.

Click "Search" in the lower left corner of the Portal.

4.1.2. Get the job URL from the Portal

The default results view will appear as in the screenshot below.

Figure 6: A screenshot of the Portal's results view for the ADQL query in Figure 5.

The search results have been automatically saved and assigned a URL.

Click on the "Info" button (the letter i in a circle), which is in the upper right-hand corner of the table (bottom of the screen).

The pop-up window contains the URL (the Job Link).

Figure 7: A screenshot of the table information, including the Job URL.

4.1.3. Retrieve the results

Follow the instructions above to create a new URL.

Warning: Using the job URL in the screenshot above will not work, it has expired.

Copy the newly created URL into the empty quotes below to define my_portal_url.

Uncomment and execute the following cells to obtain the results of the Portal query here in the Notebook.

# my_portal_url = ''
# retrieved_job = retrieve_query(my_portal_url)
# retrieved_results = retrieved_job.fetch_result().to_table().to_pandas()

# retrieved_results

Delete the retrieved job and clean up.

# retrieved_job.delete()
# del retrieved_results