Search Publications

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 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
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
Relation of X-ray activity and rotation in M dwarfs and predicted time-evolution of the X-ray luminosity
DOI: 10.1051/0004-6361/201937408 Bibcode: 2020A&A...638A..20M

Scholz, A.; Stelzer, B.; Covey, K. R. +3 more

The relation of activity to rotation in M dwarfs is of high astrophysical interest because it provides observational evidence of the stellar dynamo, which is poorly understood for low-mass stars, especially in the fully convective regime. Previous studies have shown that the relation of X-ray activity to rotation consists of two different regimes:…

2020 Astronomy and Astrophysics
XMM-Newton 73
Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A
DOI: 10.1051/0004-6361/201936718 Bibcode: 2020A&A...636A..22O

Miceli, M.; Bocchino, F.; Orlando, S. +8 more

Context. Massive stars end their lives in catastrophic supernova (SN) explosions. Key information on the explosion processes and on the progenitor stars can be extracted from observations of supernova remnants (SNRs), which are the outcome of SNe. Deciphering these observations, however, is challenging because of the complex morphology of SNRs.

2020 Astronomy and Astrophysics
XMM-Newton 64
First detection of stacked X-ray emission from cosmic web filaments
DOI: 10.1051/0004-6361/202038521 Bibcode: 2020A&A...643L...2T

Aghanim, N.; Douspis, M.; Malavasi, N. +2 more

We report the first statistical detection of X-ray emission from cosmic web filaments in ROSAT data. We selected 15 165 filaments at 0.2 < z < 0.6 ranging from 30 Mpc to 100 Mpc in length, identified in the Sloan Digital Sky Survey survey. We stacked the X-ray count-rate maps from ROSAT around the filaments, excluding resolved galaxy groups …

2020 Astronomy and Astrophysics
XMM-Newton 58
Collimated synchrotron threads linking the radio lobes of ESO 137-006
DOI: 10.1051/0004-6361/202037800 Bibcode: 2020A&A...636L...1R

Govoni, F.; Ramaila, A. J. T.; Serra, P. +14 more

We present MeerKAT 1000 MHz and 1400 MHz observations of a bright radio galaxy in the southern hemisphere, ESO 137-006. The galaxy lies at the centre of the massive and merging Norma galaxy cluster. The MeerKAT continuum images (rms ∼0.02 mJy beam-1 at ∼10″ resolution) reveal new features that have never been seen in a radio galaxy befo…

2020 Astronomy and Astrophysics
XMM-Newton 56
The XMM-Newton serendipitous survey. X. The second source catalogue from overlapping XMM-Newton observations and its long-term variable content
DOI: 10.1051/0004-6361/202037706 Bibcode: 2020A&A...641A.137T

Motch, C.; Page, M. J.; Ballet, J. +12 more

Context. The XMM-Newton Survey Science Centre Consortium (SSC) develops software in close collaboration with the Science Operations Centre to perform a pipeline analysis of all XMM-Newton observations. In celebration of the twentieth anniversary of the XMM-Newton launch, the SSC has compiled the fourth generation of serendipitous source catalogues…

2020 Astronomy and Astrophysics
Gaia XMM-Newton 52