Search Publications

Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N, and TESS
DOI: 10.1093/mnras/stac199 Bibcode: 2022MNRAS.511.4551L

Guterman, P.; Alonso, R.; Deleuil, M. +115 more

We present a precise characterization of the TOI-561 planetary system obtained by combining previously published data with TESS and CHEOPS photometry, and a new set of 62 HARPS-N radial velocities (RVs). Our joint analysis confirms the presence of four transiting planets, namely TOI-561 b (P = 0.45 d, R = 1.42 R, M = 2.0 M)…

2022 Monthly Notices of the Royal Astronomical Society
CHEOPS Gaia 34
PHANGS-HST: new methods for star cluster identification in nearby galaxies
DOI: 10.1093/mnras/stab3183 Bibcode: 2022MNRAS.509.4094T

White, Richard L.; Kruijssen, J. M. Diederik; Rosolowsky, Erik +14 more

We present an innovative and widely applicable approach for the detection and classification of stellar clusters, developed for the PHANGS-HST Treasury Program, an NUV-to-I band imaging campaign of 38 spiral galaxies. Our pipeline first generates a unified master source list for stars and candidate clusters, to enable a self-consistent inventory o…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 34
Intermediate- and high-velocity clouds in the Milky Way - I. Covering factors and vertical heights
DOI: 10.1093/mnras/stac987 Bibcode: 2022MNRAS.513.3228L

Lehner, Nicolas; Howk, J. Christopher; Marasco, Antonino +1 more

Intermediate- and high-velocity clouds (IVCs, HVCs) are a potential source of fuel for star formation in the Milky Way (MW), but their origins and fates depend sensitively on their distances. We search for IVCs and HVCs in HST high-resolution ultraviolet spectra of 55 halo stars at vertical heights $|z|\gtrsim \,1$ kpc. We show that IVCs (40 ≤ |$v…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 34
Asymmetrical tidal tails of open star clusters: stars crossing their cluster's práh challenge Newtonian gravitation
DOI: 10.1093/mnras/stac2563 Bibcode: 2022MNRAS.517.3613K

Famaey, Benoit; Kroupa, Pavel; Boffin, Henri M. J. +14 more

After their birth a significant fraction of all stars pass through the tidal threshold (práh) of their cluster of origin into the classical tidal tails. The asymmetry between the number of stars in the leading and trailing tails tests gravitational theory. All five open clusters with tail data (Hyades, Praesepe, Coma Berenices, COIN-Gaia 13, NGC 7…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 34
Relentless and complex transits from a planetesimal debris disc
DOI: 10.1093/mnras/stab3475 Bibcode: 2022MNRAS.511.1647F

Mustill, A. J.; Hermes, J. J.; Gänsicke, B. T. +12 more

This article reports quasi-continuous transiting events towards WD 1054-226 at d = 36.2 pc and V = 16.0 mag, based on simultaneous, high-cadence, multiwavelength imaging photometry using ULTRACAM over 18 nights from 2019 to 2020 March. The predominant period is 25.02 h and corresponds to a circular orbit with blackbody Teq = 323 K, wher…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 33
Dwarf AGNs from Optical Variability for the Origins of Seeds (DAVOS): insights from the dark energy survey deep fields
DOI: 10.1093/mnras/stac2262 Bibcode: 2022MNRAS.516.2736B

Bacon, D.; Shen, Yue; Smith, M. +69 more

We present a sample of 706, z < 1.5 active galactic nuclei (AGNs) selected from optical photometric variability in three of the Dark Energy Survey (DES) deep fields (E2, C3, and X3) over an area of 4.64 deg2. We construct light curves using difference imaging aperture photometry for resolved sources and non-difference imaging PSF pho…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 33
The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study
DOI: 10.1093/mnras/stac1295 Bibcode: 2022MNRAS.514.1557P

Ness, J. -U.; Munari, U.; Orio, M. +12 more

On 2021 August 8, the recurrent nova RS Ophiuchi (RS Oph) erupted again, after an interval of 15.5 yr. Regular monitoring by the Neil Gehrels Swift Observatory began promptly, on August 9.9 (0.37 d after the optical peak), and continued until the source passed behind the Sun at the start of November, 86 d later. Observations then restarted on day …

2022 Monthly Notices of the Royal Astronomical Society
Exosat Gaia 33
Revisiting bright δ Scuti stars and their period-luminosity relation with TESS and Gaia DR3
DOI: 10.1093/mnras/stac2132 Bibcode: 2022MNRAS.516.2080B

Bedding, Timothy R.; Murphy, Simon J.; Hey, Daniel R. +1 more

We have used NASA's TESS mission to study catalogued δ Scuti stars. We examined TESS light curves for 434 stars, including many for which few previous observations exist. We found that 62 are not δ Scuti pulsators, with most instead showing variability from binarity. For the 372 δ Scuti stars, we provide a catalogue of the period and amplitude of …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 33
Prospects for multimessenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
DOI: 10.1093/mnras/stac1167 Bibcode: 2022MNRAS.513.4159P

Patricelli, Barbara; Bernardini, Maria Grazia; Mapelli, Michela +5 more

The joint detection of GW170817 and GRB 170817A opened the era of multimessenger astronomy with gravitational waves (GWs) and provided the first direct probe that at least some binary neutron star (BNS) mergers are progenitors of short gamma-ray bursts (S-GRBs). In the next years, we expect to have more multimessenger detections of BNS mergers, th…

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 33
Substructure detection reanalysed: dark perturber shown to be a line-of-sight halo
DOI: 10.1093/mnras/stac1967 Bibcode: 2022MNRAS.515.4391S

Dvorkin, Cora; Ostdiek, Bryan; Sengül, Atinç Çagan +1 more

Observations of structure at subgalactic scales are crucial for probing the properties of dark matter, which is the dominant source of gravity in the universe. It will become increasingly important for future surveys to distinguish between line-of-sight haloes and subhalos to avoid wrong inferences on the nature of dark matter. We reanalyse a subg…

2022 Monthly Notices of the Royal Astronomical Society
eHST 33