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Planck 2018 results. I. Overview and the cosmological legacy of Planck
DOI: 10.1051/0004-6361/201833880 Bibcode: 2020A&A...641A...1P

Kim, J.; Miville-Deschênes, M. -A.; Boulanger, F. +192 more

The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz.…

2020 Astronomy and Astrophysics
XMM-Newton 1575
The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
DOI: 10.3847/1538-4365/aba623 Bibcode: 2020ApJS..250....8L

Brandt, W. N.; Pâris, Isabelle; Petitjean, Patrick +34 more

We present the final Sloan Digital Sky Survey IV (SDSS-IV) quasar catalog from Data Release 16 of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). This catalog comprises the largest selection of spectroscopically confirmed quasars to date. The full catalog includes two subcatalogs (the current versions are DR16Q_v4 and DR16Q_Superset_…

2020 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 408
The XMM-Newton serendipitous survey. IX. The fourth XMM-Newton serendipitous source catalogue
DOI: 10.1051/0004-6361/201937353 Bibcode: 2020A&A...641A.136W

Motch, C.; Page, M. J.; Ballet, J. +28 more

Context. Sky surveys produce enormous quantities of data on extensive regions of the sky. The easiest way to access this information is through catalogues of standardised data products. XMM-Newton has been surveying the sky in the X-ray, ultra-violet, and optical bands for 20 years.
Aims: The XMM-Newton Survey Science Centre has been producin…

2020 Astronomy and Astrophysics
AKARI Gaia XMM-Newton 297
Discovery of a 2.8 s Pulsar in a 2 Day Orbit High-mass X-Ray Binary Powering the Ultraluminous X-Ray Source ULX-7 in M51
DOI: 10.3847/1538-4357/ab8a44 Bibcode: 2020ApJ...895...60R

Salvaterra, R.; Haberl, F.; Tiengo, A. +26 more

We discovered 2.8 s pulsations in the X-ray emission of the ultraluminous X-ray source (ULX) M51 ULX-7 within the UNSEeN project, which was designed to hunt for new pulsating ULXs (PULXs) with XMM-Newton. The pulse shape is sinusoidal, and large variations of its amplitude were observed even within single exposures (pulsed fraction from less than …

2020 The Astrophysical Journal
Gaia XMM-Newton eHST 163
2SXPS: An Improved and Expanded Swift X-Ray Telescope Point-source Catalog
DOI: 10.3847/1538-4365/ab7db9 Bibcode: 2020ApJS..247...54E

Cenko, S. B.; Tagliaferri, G.; Kennea, J. A. +8 more

We present the 2SXPS (Swift-XRT Point Source) catalog, containing 206,335 point sources detected by the Swift X-ray Telescope (XRT) in the 0.3-10 keV energy range. This catalog represents a significant improvement over 1SXPS, with double the sky coverage (now 3790 deg2), and several significant developments in source detection and class…

2020 The Astrophysical Journal Supplement Series
INTEGRAL XMM-Newton 158
Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation
DOI: 10.1051/0004-6361/201936602 Bibcode: 2020A&A...636A..15M

Lovisari, L.; Pacaud, F.; Ramos-Ceja, M. E. +3 more

The isotropy of the late Universe and consequently of the X-ray galaxy cluster scaling relations is an assumption greatly used in astronomy. However, within the last decade, many studies have reported deviations from isotropy when using various cosmological probes; a definitive conclusion has yet to be made. New, effective and independent methods …

2020 Astronomy and Astrophysics
XMM-Newton 145
Quasars as standard candles. III. Validation of a new sample for cosmological studies
DOI: 10.1051/0004-6361/202038899 Bibcode: 2020A&A...642A.150L

Marconi, A.; Vignali, C.; Gilli, R. +15 more

We present a new catalogue of ∼2400 optically selected quasars with spectroscopic redshifts and X-ray observations from either Chandra or XMM-Newton. The sample can be used to investigate the non-linear relation between the ultraviolet (UV) and X-ray luminosity of quasars as well as to build a Hubble diagram up to a redshift of z ∼ 7.5. We selecte…

2020 Astronomy and Astrophysics
IUE XMM-Newton 144
X-ray quasi-periodic eruptions from the galactic nucleus of RX J1301.9+2747
DOI: 10.1051/0004-6361/202037610 Bibcode: 2020A&A...636L...2G

Miniutti, Giovanni; Giustini, Margherita; Saxton, Richard D.

Following the recent discovery of X-ray quasi-periodic eruptions (QPEs) coming from the nucleus of the galaxy GSN 069, here we report on the detection of QPEs in the active galaxy named RX J1301.9+2747. QPEs are rapid and recurrent increases of the X-ray count-rate by more than one order of magnitude with respect to a stable quiescent level. Durin…

2020 Astronomy and Astrophysics
XMM-Newton 139
The Destruction and Recreation of the X-Ray Corona in a Changing-look Active Galactic Nucleus
DOI: 10.3847/2041-8213/ab91a1 Bibcode: 2020ApJ...898L...1R

Altamirano, D.; Fabian, A. C.; Gandhi, P. +16 more

We present the drastic transformation of the X-ray properties of the active galactic nucleus (AGN) 1ES 1927+654, following a changing-look event. After the optical/ultraviolet outburst the power-law component, produced in the X-ray corona, disappeared, and the spectrum of 1ES 1927+65 instead became dominated by a blackbody component (kT ∼ 80-120 e…

2020 The Astrophysical Journal
XMM-Newton 135
The dark matter interpretation of the 3.5-keV line is inconsistent with blank-sky observations
DOI: 10.1126/science.aaw3772 Bibcode: 2020Sci...367.1465D

Safdi, Benjamin R.; Dessert, Christopher; Rodd, Nicholas L.

Observations of nearby galaxies and galaxy clusters have reported an unexpected x-ray emission line around 3.5 kilo-electron volts (keV). Proposals to explain this line include decaying dark matter—in particular, that the decay of sterile neutrinos with a mass around 7 keV could match the available data. If this interpretation is correct, the 3.5-…

2020 Science
XMM-Newton 98