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Archive XMM Newton
ESA XMM-Newton Science Archive.
-
Module name:
xmm_newton -
Python class:
astroquery.esa.xmm_newton.XMMNewton - Functions: 11
Call any function below with the astroquery_execute MCP tool. Descriptions are taken from the upstream astroquery/astropy docstrings.
| Function | Summary |
|---|---|
clear_cache |
Removes all cache files. |
download_data |
Download data from XMM-Newton |
get_columns |
Get the available columns for a table in XSA TAP service |
get_epic_images |
Extracts the EPIC images from a given TAR file |
get_epic_lightcurve |
Extracts the EPIC sources light curve products from a given TAR file |
get_epic_metadata |
Downloads the European Photon Imaging Camera (EPIC) |
get_epic_spectra |
Extracts in path (when set) the EPIC sources spectral products from a |
get_postcard |
Download postcards from XSA |
get_tables |
Get the available table in XSA TAP service |
query_xsa_tap |
Launches a synchronous job to query the XSA tap |
reset_cache_location |
Resets the cache location to the default astropy cache |
Removes all cache files.
XMMNewton.clear_cache()Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="clear_cache",
params={},
)Parameters
No parameters.
Download data from XMM-Newton
XMMNewton.download_data(observation_id, *, filename=None, verbose=False, cache=True, prop=False, credentials_file=None, **kwargs)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="download_data",
params={"observation_id": "<observation_id>"},
)Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
observation_id (required)
|
string | id of the observation to be downloaded, mandatory The identifier of the observation we want to retrieve, 10 digits example: 0144090201 | |
filename |
string | None |
file name to be used to store the file |
verbose |
bool | False |
optional, default 'False' flag to display information about the process |
cache |
bool | True |
Defaults to True. If set overrides global caching behavior. See astroquery_cache. |
prop |
boolean | False |
optional, default 'False' flag to download proprietary data, the method will then ask the user to input their username and password either manually or using the credentials_file |
credentials_file |
string | None |
optional, default None path to where the users config.ini file is stored with their username and password |
**kwargs |
Returns
None if not verbose. It downloads the observation indicated —
Get the available columns for a table in XSA TAP service
XMMNewton.get_columns(table_name, *, only_names=True, verbose=False)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="get_columns",
params={"table_name": "<table_name>"},
)Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
table_name (required)
|
string, mandatory, default None | table name of which, columns will be returned | |
only_names |
bool, TAP+ only, optional, default 'True' | True |
True to load table names only |
verbose |
bool, optional, default 'False' | False |
flag to display information about the process |
Returns
A list of columns —
Extracts the EPIC images from a given TAR file
XMMNewton.get_epic_images(filename, band=[], instrument=[], get_detmask=False, get_exposure_map=False, path='', **kwargs)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="get_epic_images",
params={"filename": "<filename>"},
)This function extracts the EPIC images in a given band (or bands) and instrument (or instruments) from it
The result is a dictionary containing the paths to the extracted EPIC images with keys being the band and the instrument
If the band or the instrument are not specified this function will return all the available bands and instruments
Additionally, get_detmask and get_exposure_map can be set to True.
If so, this function will also extract the exposure maps and detector
masks within the specified bands and instruments
Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
filename (required)
|
string, mandatory | The name of the tarfile to be proccessed | |
band |
array of integers, optional, default [] | [] |
An array of intergers indicating the desired bands |
instrument |
[] |
||
get_detmask |
bool | False |
If True, also extracts the detector masks |
get_exposure_map |
bool | False |
If True, also extracts the exposure maps |
path |
string | '' |
If set, extracts the EPIC images in the indicated path |
**kwargs |
Returns
A dictionary of dictionaries with the full paths of the extracted —
Notes
The structure and the content of the extracted compressed FITS files are described in details in the Pipeline Products Description XMM-SOC-GEN-ICD-0024.
Extracts the EPIC sources light curve products from a given TAR file
XMMNewton.get_epic_lightcurve(filename, source_number, *, instrument=[], path='')Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="get_epic_lightcurve",
params={"filename": "<filename>", "source_number": "<source_number>"},
)For a given TAR file obtained with XMMNewton.download_data.
This function extracts the EPIC sources light curve products in a given instrument (or instruments) from said TAR file
The result is a dictionary containing the paths to the extracted EPIC sources light curve products with the key being the instrument
If the instrument is not specified, this function will return all available instruments
Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
filename (required)
|
string, mandatory | The name of the tarfile to be proccessed | |
source_number (required)
|
integer, mandatory | The source number, in decimal, in the observation | |
instrument |
[] |
||
path |
string | '' |
If set, extracts the EPIC images in the indicated path |
Returns
A dictionary with the full paths of the extracted EPIC sources —
Notes
The filenames will contain the source number in hexadecimal, as this is the convention used by the pipeline.
The structure and the content of the extracted compressed FITS files are described in details in the Pipeline Products Description XMM-SOC-GEN-ICD-0024.
Downloads the European Photon Imaging Camera (EPIC)
XMMNewton.get_epic_metadata(*, target_name=None, coordinates=None, radius=None)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="get_epic_metadata",
params={},
)metadata from a given target
Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
target_name |
string, optional, default None | None |
The name of the target |
coordinates |
SkyCoord, optinal, default None |
None |
The coordinates of the target in a SkyCoord object |
radius |
float, optional, default None | None |
The radius to query the target in degrees |
Returns
``Table objects — Tables containing the metadata of the target
Extracts in path (when set) the EPIC sources spectral products from a
XMMNewton.get_epic_spectra(filename, source_number, *, instrument=[], path='', verbose=False)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="get_epic_spectra",
params={"filename": "<filename>", "source_number": "<source_number>"},
)given TAR file.
This function extracts the EPIC sources spectral products in a given instrument (or instruments) from it The result is a dictionary containing the paths to the extracted EPIC sources spectral products with key being the instrument If the instrument is not specified this function will return all the available instruments
Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
filename (required)
|
string, mandatory | The name of the tarfile to be processed | |
source_number (required)
|
integer, mandatory | The source number, in decimal, in the observation | |
instrument |
[] |
||
path |
string | '' |
If set, extracts the EPIC images in the indicated path |
verbose |
bool | False |
optional, default 'False' flag to display information about the process |
Returns
A dictionary with the full paths of the extracted EPIC sources —
Notes
The filenames will contain the source number in hexadecimal, as this is the convention used by the pipeline. The structure and the content of the extracted compressed FITS files are described in details in the Pipeline Products Description [XMM-SOC-GEN-ICD-0024] (https://xmm-tools.cosmos.esa.int/external/xmm_obs_info/odf/data/docs/XMM-SOC-GEN-ICD-0024.pdf).
The RMF to be used for the spectral analysis should be generated with the same PPS version as the spectrum, background and ARF. The PPS version can be found in SASVERS keyword in the SPECTRUM file, characters [-6:-3]. Once the sas version is determined, the code should look for the proper version of RMF in the FTP tree. However, for the current PPS versions available in the archive, i.e v18.0, v19.0, v20.0 and v21.0, all RMF matrices are equal among the versions and for all instruments, so it is possible to download the last one, v21.0, available in the root FTP stored in 'rmf_ftp'. In the future, the FTP tree and/or PPS keywords will be modified to make it easier to download the appropriate RMF file for each spectrum.
Download postcards from XSA
XMMNewton.get_postcard(observation_id, *, image_type='OBS_EPIC', filename=None, verbose=False)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="get_postcard",
params={"observation_id": "<observation_id>"},
)Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
observation_id (required)
|
string | id of the observation for which download the postcard, mandatory The identifier of the observation we want to retrieve, regardless of whether it is simple or composite. | |
image_type |
string | 'OBS_EPIC' |
image type, optional, default 'OBS_EPIC' The image_type to be returned. It can be: OBS_EPIC, OBS_RGS_FLUXED, OBS_RGS_FLUXED_2, OBS_RGS_FLUXED_3, OBS_EPIC_MT, OBS_RGS_FLUXED_MT, OBS_OM_V, OBS_OM_B, OBS_OM_U, OBS_OM_L, OBS_OM_M, OBS_OM_S, OBS_OM_W |
filename |
string | None |
file name to be used to store the postcard, optional, default None |
verbose |
bool | False |
optional, default 'False' Flag to display information about the process |
Returns
None. It downloads the observation postcard indicated —
Get the available table in XSA TAP service
XMMNewton.get_tables(*, only_names=True, verbose=False)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="get_tables",
params={},
)Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
only_names |
bool, TAP+ only, optional, default 'True' | True |
True to load table names only |
verbose |
bool, optional, default 'False' | False |
flag to display information about the process |
Returns
A list of tables —
Launches a synchronous job to query the XSA tap
XMMNewton.query_xsa_tap(query, *, output_file=None, output_format='votable', verbose=False)Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="query_xsa_tap",
params={"query": "<query>"},
)Parameters
| Parameter | Type | Default | Description |
|---|---|---|---|
query (required)
|
str, mandatory | query (adql) to be executed | |
output_file |
str, optional, default None | None |
file name where the results are saved if dumpToFile is True. If this parameter is not provided, the jobid is used instead |
output_format |
str, optional, default 'votable' | 'votable' |
possible values 'votable' or 'csv' |
verbose |
bool, optional, default 'False' | False |
flag to display information about the process |
Returns
A table object —
Resets the cache location to the default astropy cache
XMMNewton.reset_cache_location()Call via MCP
astroquery_execute(
module_name="xmm_newton",
function_name="reset_cache_location",
params={},
)Parameters
No parameters.
Auto-generated from source docstrings on each release. Do not edit here — changes are overwritten.