Search Publications

The first simultaneous X-ray broadband view of Mrk 110 with XMM-Newton and NuSTAR
DOI: 10.1051/0004-6361/202141577 Bibcode: 2021A&A...654A..89P

Grosso, N.; Porquet, D.; Reeves, J. N. +2 more

Context. Soft and hard X-ray excesses, compared to the continuum power-law shape between ∼2−10 keV, are common features observed in the spectra of active galactic nuclei (AGN) and are associated with the accretion disc-corona system around the supermassive black hole. However, the dominant process at work is still highly debated and has been propo…

2021 Astronomy and Astrophysics
XMM-Newton 25
New Evidence for Extended He I> Reionization at z ≳ 3.5 from He II Lyman Alpha and Beta Transmission Spikes
DOI: 10.3847/1538-4357/abee17 Bibcode: 2021ApJ...912...38M

Richter, Philipp; Hennawi, Joseph F.; Worseck, Gábor +3 more

We present new high-resolution (R = λ/Δλ ∼ 14,000) spectra of the two brightest He II-transparent quasars in the far-UV at zem > 3.5, HE2QS J2311-1417 (zem = 3.70) and HE2QS J1630+0435 (zem = 3.81), obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope. In the predominantly saturated He II …

2021 The Astrophysical Journal
eHST 25
Metallicity Estimation of RR Lyrae Stars From Their I-Band Light Curves
DOI: 10.3847/1538-4357/ac106f Bibcode: 2021ApJ...920...33D

Grebel, Eva K.; Pojmański, Grzegorz; Dékány, István

We have revisited the problem of metallicity prediction of RR Lyrae stars from their near-infrared light curves in the Cousins I wave band. Our study is based on high-quality time series photometry and state-of-the-art high-resolution spectroscopic abundance measurements of 80 fundamental-mode (RRab) and 24 first-overtone (RRc) stars, spanning ~[-…

2021 The Astrophysical Journal
Gaia 25
The Nature of the Milky Way's Stellar Halo Revealed by the Three Integrals of Motion
DOI: 10.3847/1538-4357/abd7a4 Bibcode: 2021ApJ...908..191C

Carollo, Daniela; Chiba, Masashi

We developed a new selection method of halo stars in the phase-space distribution defined by the three integrals of motion in an axisymmetric Galactic potential (E, Lz, I3), where I3 is the third integral of motion. The method is used to explore the general chemodynamical structure of the halo based on stellar samp…

2021 The Astrophysical Journal
Gaia 25
ALMA Lensing Cluster Survey: a strongly lensed multiply imaged dusty system at z ≥ 6
DOI: 10.1093/mnras/stab191 Bibcode: 2021MNRAS.505.4838L

Wang, T.; Laporte, N.; Bauer, F. E. +20 more

We report the discovery of an intrinsically faint, quintuply-imaged, dusty galaxy MACS0600-z6 at a redshift z = 6.07 viewed through the cluster MACSJ0600.1-2008 (z = 0.46). A ≃ 4σ dust detection is seen at 1.2mm as part of the ALMA Lensing Cluster Survey (ALCS), an on-going ALMA Large programme, and the redshift is secured via [C II] 158 µm …

2021 Monthly Notices of the Royal Astronomical Society
Herschel eHST 24
The VMC survey - XLI. Stellar proper motions within the Small Magellanic Cloud
DOI: 10.1093/mnras/stab206 Bibcode: 2021MNRAS.502.2859N

Sun, Ning-Chen; de Grijs, Richard; Ripepi, Vincenzo +13 more

We used data from the near-infrared Visible and Infrared Telescope for Astronomy (VISTA) survey of the Magellanic Cloud system (VMC) to measure proper motions (PMs) of stars within the Small Magellanic Cloud (SMC). The data analysed in this study comprise 26 VMC tiles, covering a total contiguous area on the sky of ∼40 deg2. Using multi…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
Exemplary Merging Clusters: Weak-lensing and X-Ray Analysis of the Double Radio Relic, Merging Galaxy Clusters MACS J1752.0+4440 and ZWCL 1856.8+6616
DOI: 10.3847/1538-4357/ac0d00 Bibcode: 2021ApJ...918...72F

Dawson, William A.; Jones, Christine; Forman, William R. +8 more

The investigation of merging galaxy clusters that exhibit radio relics is strengthening our understanding of the formation and evolution of galaxy clusters, the nature of dark matter, the intracluster medium, and astrophysical particle acceleration. Each merging cluster provides only a single view of the cluster formation process, and the variety …

2021 The Astrophysical Journal
XMM-Newton eHST 24
A Spatially Resolved Survey of Distant Quasar Host Galaxies. I. Dynamics of Galactic Outflows
DOI: 10.3847/1538-4357/ac0f56 Bibcode: 2021ApJ...919..122V

Armus, Lee; Larkin, James E.; Wright, Shelley A. +6 more

We present observations of ionized gas outflows in 11 z = 1.39-2.59 radio-loud quasar host galaxies. Data were taken with the integral field spectrograph OSIRIS and the adaptive optics system at the W.M. Keck Observatory targeting nebular emission lines (Hβ, [O III], Hα, [N II], and [S II]) redshifted into the near-infrared (1-2.4 µm). Outfl…

2021 The Astrophysical Journal
Gaia 24
Solar Orbiter's first Venus flyby: Observations from the Radio and Plasma Wave instrument
DOI: 10.1051/0004-6361/202140934 Bibcode: 2021A&A...656A..18H

Maksimovic, M.; Bale, S. D.; Chust, T. +41 more

Context. On December 27, 2020, Solar Orbiter completed its first gravity assist manoeuvre of Venus (VGAM1). While this flyby was performed to provide the spacecraft with sufficient velocity to get closer to the Sun and observe its poles from progressively higher inclinations, the Radio and Plasma Wave (RPW) consortium, along with other operational…

2021 Astronomy and Astrophysics
SolarOrbiter 24
Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
DOI: 10.1051/0004-6361/202140876 Bibcode: 2021A&A...654A..80S

Feltre, A.; Kollatschny, W.; Mahler, G. +17 more

Rest-frame ultraviolet (UV) emission lines probe electron densities, gas-phase abundances, metallicities, and ionization parameters of the emitting star-forming galaxies and their environments. The strongest main UV emission line, Lyα, has been instrumental in advancing the general knowledge of galaxy formation in the early universe. However, obse…

2021 Astronomy and Astrophysics
eHST 24