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GSFC XMM-Newton GOF Status Report #379: XMM-NEWTON NEWS #238
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- Subject: GSFC XMM-Newton GOF Status Report #379: XMM-NEWTON NEWS #238
- From: "Newsletter for users of the XMM-Newton mission via XMMNews" <xmmnews@xxx>
- Date: Thu, 10 Dec 2020 10:27:13 -0500
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News #238, 10 December 2020
CONTENTS
- New versions of the XMM-Newton Serendipitous Source Catalogues:
4XMM-DR10 and 4XMM-DR10s and a new citizen science project for
XMM-Newton data, CLAXSON
- NEW VERSION OF THE XMM-NEWTON OM CATALOGUE (XMM-OM-SUSS5.0)
- XSA V13.0 RELEASE WITH ACCESS TO 4XMM DR10, 4XMM DR10S AND
XMM-OM-SUSS5.0 CATALOGUES
- Scientific Validation Report for SAS v19.0
- HAPPY BIRTHDAY, XMM-Newton!
NEWS
New versions of the XMM-Newton Serendipitous Source Catalogues: 4XMM-DR10
and
4XMM-DR10s and a new citizen science project for XMM-Newton data, CLAXSON
To coincide with the 21st anniversary of the launch of XMM-Newton, a
new version of the XMM-Newton EPIC Serendipitous Source Catalogue,
4XMM-DR10, is being released by the XMM-Newton Survey Science Centre
(XMM-SSC) in collaboration with the SOC.
This version includes an extra year of data with respect to 4XMM-DR9.
4XMM-DR10 includes 849991 X-ray detections which relate to 575158
unique X-ray sources from 11647 observations that were public by the
31st December 2019. 4XMM-DR10 covers a total sky area, with at least 1
ks exposure, of ~1192 square degrees if overlaps are taken into
account, where some regions of the sky have been pointed as many as 74
times. Around 9% of all the detections are classified as extended, and
spectra and time series have been extracted for 36% of the detections.
The median positional uncertainty of the catalogue detections is 1.57
arcseconds (with a standard deviation of 1.44). Median sensitivities in
the catalogue are ~5.3E-15 and ~1.2E-14 erg/cm2/s in the soft (0.2-2
keV) and hard (2-12 keV) X-ray band, respectively.
With 4XMM-DR10, we also release 4XMM-DR10s, a version of the catalogue
created from overlapping observations. Stacking observations provides
longer effective exposure times, resulting in better source parameters
and higher sensitivity. 4XMM-DR10s is built from 1396 stacks (or
groups) with 7803 contributing observations. Most of the stacks are
composed of 2 observations and the largest has 352. The catalogue
contains 335812 sources, of which 256213 have several contributing
observations. 7969 good quality sources are variable on the long term.
The catalogue is described in the paper [6]Webb et al. (2020) and the
stacked catalogue is further described in [7]Traulsen et al. (2020).
Details of the catalogue, the catalogue files and full 4XMM
documentation are available on the XMM-SSC webpages at
[8]https://gcc02.safelinks.protection.outlook.com/?url=http%3A%2F%2Fxmmssc.irap.omp.eu%2FCatalogue%2F4XMM-DR10%2F4XMM_DR10.html&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519442398%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=zbYY%2FB076p9TIBjAEFlZwfzhwr8pU9hkZ%2FgGtjCD1fI%3D&reserved=0
and
[9]https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fxmmssc.aip.de%2Fcms%2Fusers-guide%2Findex.html&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519442398%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=IqGskYbVRxsIxyjl0IhMwmrAiSneKW7ehd4ruvkNoeM%3D&reserved=0
FITS files containing summary information about the observations used
in the catalogue are also provided. FITS and CSV versions of the full
4XMM catalogue and a slimline version of the FITS file are also
available for download at
[10]https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fwww.cosmos.esa.int%2Fweb%2Fxmm-newton%2Fxsa&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519442398%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=MMNlO8f2%2BhQ7ljFI8v4hdC3cEelwcsRXjxqI9QKCzP4%3D&reserved=0
The slimline version of 4XMM-DR10 has only one row per unique source
(rather than per detection as in the main catalogue) and a reduced
number of columns that essentially pertain to the unique source
quantities.
Alongside the XSA user interface, 4XMM is also distributed through:
XCATDB:
[11]https://gcc02.safelinks.protection.outlook.com/?url=http%3A%2F%2Fxcatdb.unistra.fr%2F4xmmdr10&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519442398%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=rLfQNJNs7pMngOhqlOVRs4hq34TzMGFLZVmpnzaBXdQ%3D&reserved=0
HEASARC:
[12]http://heasarc.gsfc.nasa.gov/W3Browse/xmm-newton/xmmssc.html
IRAP:
[13]https://gcc02.safelinks.protection.outlook.com/?url=http%3A%2F%2Fxmm-catalog.irap.omp.eu%2F&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519442398%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=BtYfEqsATh%2BGBFEoy4V2tCjSWcmhRnPB58tbgg036Ik%3D&reserved=0
In parallel we are releasing a citizen science project, CLAXSON, which
allows the general public to participate in the identification of the
X-ray sources in the 4XMM-DR10 catalogue. The platform can be reached
directly at
[14]https://gcc02.safelinks.protection.outlook.com/?url=http%3A%2F%2Fxmm-ssc.irap.omp.eu%2Fclaxson%2Findex.php&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519442398%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=fBgc8JbRke77pKtEvht9FZPh5sIE4YbTTzm4K7hSsNM%3D&reserved=0
and via the XMM-Newton SSC webpages.
New version of the XMM-Newton OM Catalogue (XMM-OM-SUSS5.0)
The fifth version of the XMM-Newton Optical Monitor (OM) Serendipitous
Ultraviolet Source Survey Catalogue (XMM-SUSS5) has been released.
XMM-OM-SUSS5 contains data from 10628 observations, obtained between
February 2000 and February 2020. The catalogue comprises photometric
measurements from 8.86 million detections of sources observed with one
or more optical and/or ultraviolet filters, in fields generally
observed contemporaneously with the XMM-Newton EPIC cameras. These
detections correspond to 5.97 million unique sources, of which 1.12
million have more than one detection in the catalogue, thus
facilitating the analysis of potential variability on timescales of
days to years.
The XMM-OM-SUSS5 catalogue can be accessed through the XSA search
interface. Besides, both the complete catalogue and a reduced version
can be downloaded from the XSA web page:
[15]https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fwww.cosmos.esa.int%2Fweb%2Fxmm-newton%2Fxsa&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519452358%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=eWy%2FqJaJWHehlpQnwPwEZz9JkHVqInjcT%2FM2DrBxCRw%3D&reserved=0
The catalogue fundamentals are described in [16]Page et al. (2012).
XSA V13.0 RELEASE WITH ACCESS TO 4XMM DR10, 4XMM DR10S AND XMM-OM-SUSS5.0
CATALOGUES
A new version of the XMM-Newton Science Archive (XSA v13.0) is
available at
[17]https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fwww.cosmos.esa.int%2Fweb%2Fxmm-newton%2Fxsa&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519452358%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=eWy%2FqJaJWHehlpQnwPwEZz9JkHVqInjcT%2FM2DrBxCRw%3D&reserved=0
XSA v13.0 provides access to the new versions of 4XMM DR10, 4XMM DR10S
and XMM-OM-SUSS5.0 Source Catalogue.
Scientific Validation Report for SAS v19.0
The results of the scientific validation of SAS v19.0 have been
summarised in a report available under the SAS Scientific Validation
page
[18]https://gcc02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fwww.cosmos.esa.int%2Fweb%2Fxmm-newton%2Fsas-validation&data=04%7C01%7Cmichael.arida%40nasa.gov%7Cbb6e9cfdea1d46aa17dd08d89d201bec%7C7005d45845be48ae8140d43da96dd17b%7C0%7C0%7C637432108519452358%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C1000&sdata=jnSZYVIIsnHhA9fxlAf3cfUDu3GO2owpOSef7yhGpC4%3D&reserved=0
HAPPY BIRTHDAY, XMM-Newton!
XMM-Newton [19]was launched on the 10th of December 1999 at 14:32 GMT
on an Ariane 5 from the European spaceport at Kourou, French Guiana.
Today, XMM-Newton is celebrating its 21st anniversary.
Thank you for your support and interest in the mission!
XMM-Newton Science Operations Centre at
ESA's European Space Astronomy Centre,
Villanueva de la Ca�ada, Madrid, Spain
[20]SOC Home [21]Helpdesk Web Interface [22]Contact Helpdesk
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References
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15.
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