Search Publications

Exploiting NIKA2/XMM-Newton imaging synergy for intermediate-mass high-z galaxy clusters within the NIKA2 SZ large program. Observations of ACT-CL J0215.4+0030 at z ∼ 0.9
DOI: 10.1051/0004-6361/202038933 Bibcode: 2020A&A...644A..93K

Berta, S.; Aussel, H.; Adam, R. +40 more

High-resolution mapping of the intracluster medium (ICM) up to high redshift and down to low masses is crucial to derive accurate mass estimates of the galaxy cluster and to understand the systematic effects affecting cosmological studies based on galaxy clusters. We present a spatially resolved Sunyaev-Zel'dovich (SZ)/X-ray analysis of ACT-CL J02…

2020 Astronomy and Astrophysics
Herschel XMM-Newton 19
Deep XMM-Newton observations of the northern disc of M31. II. Tracing the hot interstellar medium
DOI: 10.1051/0004-6361/201937008 Bibcode: 2020A&A...637A..12K

Williams, Benjamin F.; Sasaki, Manami; Haberl, Frank +10 more


Aims: We use new deep XMM-Newton observations of the northern disc of M31 to trace the hot interstellar medium (ISM) in unprecedented detail and to characterise the physical properties of the X-ray emitting plasmas.
Methods: We used all XMM-Newton data up to and including our new observations to produce the most detailed image yet of the…

2020 Astronomy and Astrophysics
XMM-Newton eHST 19
The Pristine survey XI: the FORS2 sample
DOI: 10.1093/mnras/staa589 Bibcode: 2020MNRAS.493.4677C

Bonifacio, P.; Caffau, E.; Jablonka, P. +11 more

Extremely metal-poor (EMP) stars are old objects that mostly formed very early after the big bang. They are rare and, to select them, we have to rely on low-resolution spectroscopic or photometric surveys; specifically the combination of narrow- and broad-band photometry provides a powerful and time efficient way to select MP stars. The Pristine p…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 19
The MAVERIC survey: a hidden pulsar and a black hole candidate in ATCA radio imaging of the globular cluster NGC 6397
DOI: 10.1093/mnras/staa631 Bibcode: 2020MNRAS.493.6033Z

Gelfand, Joseph D.; Strader, Jay; Bahramian, Arash +9 more

Using a 16.2-h radio observation by the Australia Telescope Compact Array and archival Chandra data, we found >5σ radio counterparts to four known and three new X-ray sources within the half-light radius (rh) of the Galactic globular cluster NGC 6397. The previously suggested millisecond pulsar (MSP) candidate, U18, is a steep-spectr…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 19
Testing the CIBER cosmic infrared background measurements and axionlike particles with observations of TeV blazars
DOI: 10.1103/PhysRevD.101.063004 Bibcode: 2020PhRvD.101f3004L

Tam, P. H. T.; Zhu, W. S.; Long, G. B. +1 more

The first measurements from the CIBER experiment of extragalactic background light (EBL) in near-infrared (NIR) band exhibit a higher intensity than those inferred through γ -ray observations. Recent theoretical-EBL intensities are typically consistent with the very high energy (VHE) γ -ray observations. Yet, it is possible that the excess NIR rad…

2020 Physical Review D
AKARI 19
The TOI-763 system: sub-Neptunes orbiting a Sun-like star
DOI: 10.1093/mnras/staa2502 Bibcode: 2020MNRAS.498.4503F

Fridlund, M.; Pätzold, M.; Rauer, H. +51 more

We report the discovery of a planetary system orbiting TOI-763(aka CD-39 7945), a V = 10.2, high proper motion G-type dwarf star that was photometrically monitored by the TESS space mission in Sector 10. We obtain and model the stellar spectrum and find an object slightly smaller than the Sun, and somewhat older, but with a similar metallicity. Tw…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 19
Temporal and Spectral Studies by XMM-Newton of Jupiter's X-ray Auroras During a Compression Event
DOI: 10.1029/2019JA027676 Bibcode: 2020JGRA..12527676W

Coates, A. J.; Jackman, C. M.; Branduardi-Raymont, G. +16 more

We report the temporal and spectral results of the first XMM-Newton observation of Jupiter's X-ray auroras during a clear magnetospheric compression event on June 2017 as confirmed by data from the Jovian Auroral Distributions Experiment (JADE) instrument onboard Juno. The northern and southern auroras were visible twice and thrice respectively as…

2020 Journal of Geophysical Research (Space Physics)
XMM-Newton eHST 19
OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk
DOI: 10.3847/1538-3881/ab9ac3 Bibcode: 2020AJ....160...74H

Soszyński, I.; Szymański, M. K.; Pietrukowicz, P. +100 more

We report the discovery and analysis of the planetary microlensing event OGLE-2017-BLG-0406, which was observed both from the ground and by the Spitzer satellite in a solar orbit. At high magnification, the anomaly in the light curve was densely observed by ground-based-survey and follow-up groups, and it was found to be explained by a planetary l…

2020 The Astronomical Journal
Gaia 19
First in situ detection of the CN radical in comets and evidence for a distributed source
DOI: 10.1093/mnras/staa2387 Bibcode: 2020MNRAS.498.2239H

Altwegg, Kathrin; Hänni, Nora; Rubin, Martin +4 more

Although the debate regarding the origin of the cyano (CN) radical in comets has been ongoing for many decades, it has yielded no definitive answer to date. CN could previously only be studied remotely, strongly hampering efforts to constrain its origin because of very limited spatial information. Thanks to the European Space Agency's Rosetta spac…

2020 Monthly Notices of the Royal Astronomical Society
Rosetta 19
Hot Subdwarf Stars Identified in Gaia DR2 with Spectra of LAMOST DR6 and DR7. II.Kinematics
DOI: 10.3847/1538-4357/ab98f3 Bibcode: 2020ApJ...898...64L

Luo, Yangping; Németh, Péter; Li, Qida

Combining LAMOST radial velocities with Gaia parallaxes and proper motions, we present 3D Galactic space motions and the orbits of 182 single-lined hot subdwarf stars. These stars were identified by Lei et al. in Gaia DR2 with LAMOST DR6 and DR7 spectra. He-rich hot subdwarf stars with $\mathrm{log}(y)\geqslant 0$ show the largest standard deviati…

2020 The Astrophysical Journal
Gaia 19