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Copy file name to clipboardExpand all lines: docs/esa/euclid/euclid.rst
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@@ -12,7 +12,7 @@ out to redshifts ~2, or equivalently to a look-back time of 10 billion years. It
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expanded and how structure has formed over cosmic history, revealing more about the role of gravity and the nature of
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dark energy and dark matter.
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This package allows the access to the European Space Agency Euclid Archive (https://eas.esac.esa.int/).
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This package allows access to the European Space Agency Euclid Archive (https://eas.esac.esa.int/).
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The Euclid Survey is done in a 'step-and-stare' mode, where the telescope points to a position on the sky and then
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imaging and spectroscopic measurements are performed on an area of ~0.48 deg\ :sup:`2` around this position. The telescope
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each take a 560s exposure, consisting of a direct visible image and a red grism exposure. This is followed by further
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NISP exposures in the Y, J, and H band filters (87 seconds each). The telescope is then dithered, and the sequence is
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repeated starting with a different grism position angle. There are actually two operational grisms oriented 180 degrees
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from each other. Each grism which will be used twice in this sequence, but with slight angular offsets (+/- 4 degrees),
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from each other. Each grism will be used twice in this sequence, but with slight angular offsets (+/- 4 degrees),
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effectively creating the four different grism angles (Scaramella et al. 2022, A&A 662, A112).
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This standard four-dithers operating mode sequence is called a single observation and all the individual exposures
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TAP provides two operation modes: Synchronous and Asynchronous:
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* Synchronous: the response to the request will be generated as soon as the request received by the server.
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(Do not use this method for queries that generate a big amount of results.)
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(Do not use this method for queries that generate a large amount of results.)
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* Asynchronous: the server starts a job that will execute the request.
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The first response to the request is the required information (a link) to obtain the job status.
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Once the job is finished, the results can be retrieved.
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ESA EUCLID TAP+ server provides two access mode: public and authenticated:
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ESA EUCLID TAP+ server provides two access modes: public and authenticated:
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* Public: this is the standard TAP access.
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A user can execute ADQL queries and upload tables to be used in a query 'on-the-fly' (these tables will be removed
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once the query is executed). The results are available to any other user and they will remain in the server for a
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once the query is executed). The results are available to any other user, and they will remain in the server for a
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limited space of time.
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* Authenticated: some functionalities are restricted to authenticated users only.
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The results are saved in a private user space and they will remain in the server for ever (they can be removed by the
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The results are saved in a private user space and they will remain in the server forever (they can be removed by the
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user).
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* ADQL queries and results are saved in a user private area.
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The Euclid Science Archive has several environments serving different purposes for the Euclid Consortium members.
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1. The OTF ("on-the-fly") environment of the Euclid science archive, first started at the start of science operation exposed data as processed as processed by
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1. The OTF ("on-the-fly") environment of the Euclid science archive, first started at the start of science operation exposed data as processed by
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the SGS (Science Ground Segment) soon after acquisition to provide an access as soon as possible. In this environment
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the data will not be reprocessed and the processing is therefore heterogeneous.
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2. The REG (for non-regression testing) environment of the Euclid science archive, where a large area in the sky is processed with the same version for
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all data products. The first campaign was run in September 2024, for area of about 500 square degrees (~1000
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observation), the next campaign shall be run in March-April 2025.
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observations), the next campaign shall be run in March-April 2025.
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3. The IDR (Internal Data Release) environment of the Euclid science archive holds the data that will then become public. The first release Q1
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opened on the 6th of November 2024, with a first pass on the three Euclid deep fields (EDFN, EDFS and EDFF) as well as
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>>> from astroquery.esa.euclid import EuclidClass
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>>> euclid = EuclidClass(environment='IDR')
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The parameter *environment* can take only the following values: *IDR*, *OTF*, *PDR* or *REG*.
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The parameter *environment* is limited to *IDR*, *OTF*, *PDR* or *REG*.
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1. Non authenticated access
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1.1. Getting public tables metadata
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^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
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Table and columns metadata are specified by IVOA TAP_ recommendation (to access to the actual data, an ADQL query must be executed).
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Table and column metadata are specified by IVOA TAP_ recommendation (to access to the actual data, an ADQL query must be executed).
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To load only table names metadata (TAP+ capability):
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@@ -179,8 +178,7 @@ To load only table names metadata (TAP+ capability):
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...
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To load all tables metadata (TAP compatible):
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To load all table metadata (TAP compatible):
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.. doctest-remote-data::
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WARNING: This method implements the ADQL BOX function that is deprecated in the latest version of the standard
The following example searches for all the sources contained in an squared region of side = 0.1 degrees around an specific point in ra/dec coordinates. The results are sorted by distance (``dist``) in ascending order.
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The following example searches for all the sources contained in an squared region of side = 0.1 degrees around a specific point in ra/dec coordinates. The results are sorted by distance (``dist``) in ascending order.
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The method returns the job results as astropy.table
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@@ -371,9 +369,9 @@ The previous query can be executed as an asynchronous version:
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^^^^^^^^^^^^^^^^^^^^^^
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The results of a synchronous query are stored at the user side (i.e., they are not saved in the server). These queries
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can only used when the amount of data to be retrieved (number of rows) is small, otherwise, a timeout error can be raised.
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can only be used when the amount of data to be retrieved (number of rows) is small, otherwise, a timeout error can be raised.
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The output of the synchronous queries is limited to 2000 rows. If you need more than that, you must use asynchronous queries.
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The results of asynchronous queries can be saved in memory (default) or in a file but is also stored on the server/archive
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The results of asynchronous queries can be saved in memory (default) or in a file but are also stored on the server/archive
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so you can access the results by logging in on the archive website too.
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Query without saving results in a file:
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The method returns a Job object.
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Query saving results in a file (you may use 'output_format' to specified the results data format, available formats are:
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Query saving results in a file (you may use 'output_format' to specify the results' data format. Available formats are:
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'votable', 'votable_plain', 'fits', 'csv' and 'json', default is 'votable'):
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.. Skipping authentication requiring examples
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