Search Publications

On the Origin of the North Celestial Pole Loop
DOI: 10.3847/1538-4357/aca4d2 Bibcode: 2023ApJ...942...70M

Martin, Peter G.; Marchal, Antoine

The North Celestial Pole Loop (NCPL) provides a unique laboratory for studying the early-stage precursors of star formation. Uncovering its origin is key to understanding the dynamical mechanisms that control the evolution of its contents. In this study, we explore the 3D geometry and the dynamics of the NCPL using high-resolution dust extinction …

2023 The Astrophysical Journal
Gaia 12
Introducing the Condor Array Telescope. I. Motivation, Configuration, and Performance
DOI: 10.1088/1538-3873/acaee6 Bibcode: 2023PASP..135a5002L

Walter, Frederick M.; Shara, Michael M.; Lanzetta, Kenneth M. +4 more

The "Condor Array Telescope" or "Condor" is a high-performance "array telescope" comprised of six apochromatic refracting telescopes of objective diameter 180 mm, each equipped with a large-format, very low-read-noise (≈1.2 e-), very rapid-read-time (<1 s) CMOS camera. Condor is located at a very dark astronomical site in the southwe…

2023 Publications of the Astronomical Society of the Pacific
Gaia 12
Magnetic fluxes of solar active regions of different magneto-morphological classes - I. Cyclic variations
DOI: 10.1093/mnras/stac3338 Bibcode: 2023MNRAS.518.4746A

Abramenko, Valentina I.; Suleymanova, Regina A.; Zhukova, Anastasija V.

Data for 3046 solar active regions (ARs) observed since 1996 May 12 to 2021 December 27 were utilized to explore how the magnetic fluxes from ARs of different complexity follow the solar cycle. Magnetograms from the Michelson Doppler Imager instrument on the Solar and Heliospheric Observatory and from the Helioseismic and Magnetic Imager instrumen…

2023 Monthly Notices of the Royal Astronomical Society
SOHO 12
Gaia DR3 features of the phase spiral and its possible relation to internal perturbations
DOI: 10.1093/mnras/stad2199 Bibcode: 2023MNRAS.524.6331L

Li, Chengdong; Siebert, Arnaud; Famaey, Benoit +2 more

Disc stars from the Gaia DR3 RVS catalogue are selected to explore the phase spiral in the Galaxy. The data reveal a two-armed phase spiral pattern in the local z-vz plane inside the solar radius, which appears clearly when colour-coded by ⟨vR⟩(z, vz): this is characteristic of a breathing mode that can in principl…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 12
A brown dwarf donor and an optically thin accretion disc with a complex stream impact region in the period-bouncer candidate BW Sculptoris
DOI: 10.1093/mnras/stad1730 Bibcode: 2023MNRAS.523.6114N

Neustroev, Vitaly V.; Mäntynen, Iikka

We present an analysis of multi-epoch spectroscopic and photometric observations of the WZ Sge-type dwarf nova BW Scl, a period-bouncer candidate. We detected multiple irradiation-induced emission lines from the donor star allowing the radial velocity variations to be measured with high accuracy. Also, using the absorption lines Mg II 4481 Å and C…

2023 Monthly Notices of the Royal Astronomical Society
eHST 12
Gaia Data Release 3. Surface brightness profiles of galaxies and host galaxies of quasars
DOI: 10.1051/0004-6361/202243798 Bibcode: 2023A&A...674A..11D

Ducourant, C.; Gavras, P.; Pourbaix, D. +13 more

Context. Since July 2014, the Gaia space mission has been continuously scanning the sky and observing the extragalactic Universe with unprecedented spatial resolution in the optical domain (∼180 mas by the end of the mission). Gaia provides an opportunity to study the morphology of the galaxies of the local Universe (z < 0.45) with much higher …

2023 Astronomy and Astrophysics
Gaia 12
Characterising fast-time variations in the hard X-ray time profiles of solar flares using Solar Orbiter's STIX
DOI: 10.1051/0004-6361/202245293 Bibcode: 2023A&A...671A..79C

Krucker, Säm; Harra, Louise K.; Hayes, Laura A. +2 more


Aims: The aim of this work is to develop a method to systematically detect and characterise fast-time variations (≳1 s) in the non-thermal hard X-ray (HXR) time profiles of solar flares using high-resolution data from Solar Orbiter's Spectrometer/Telescope for Imaging X-rays (STIX).
Methods: The HXR time profiles were smoothed using Gaus…

2023 Astronomy and Astrophysics
SolarOrbiter 12
Characterization of a Set of Small Planets with TESS and CHEOPS and an Analysis of Photometric Performance
DOI: 10.3847/1538-3881/acb4e3 Bibcode: 2023AJ....165..134O

Torres, Guillermo; Bieryla, Allyson; Stassun, Keivan G. +41 more

The radius valley carries implications for how the atmospheres of small planets form and evolve, but this feature is visible only with highly precise characterizations of many small planets. We present the characterization of nine planets and one planet candidate with both NASA TESS and ESA CHEOPS observations, which adds to the overall population…

2023 The Astronomical Journal
CHEOPS Gaia 12
Properties of luminous red supergiant stars in the Magellanic Clouds
DOI: 10.1051/0004-6361/202243394 Bibcode: 2023A&A...669A..86D

Boutsia, K.; Zapartas, E.; de Wit, S. +5 more

Context. There is evidence that some red supergiants (RSGs) experience short-lived phases of extreme mass loss, producing copious amounts of dust. These episodic outburst phases help strip the hydrogen envelope from evolved massive stars, drastically affecting their evolution. However, to date, the observational data of episodic mass loss is limit…

2023 Astronomy and Astrophysics
Gaia 12
Beyond the ultradeep frontier fields and legacy observations (BUFFALO): a high-resolution strong+weak-lensing view of Abell 370
DOI: 10.1093/mnras/stad1999 Bibcode: 2023MNRAS.524.2883N

Sharon, K.; Diego, J. M.; Zitrin, A. +16 more

The HST treasury programme BUFFALO provides extended wide-field imaging of the six Hubble Frontier Fields galaxy clusters. Here we present the combined strong and weak-lensing analysis of Abell 370, a massive cluster at z = 0.375. From the reconstructed total projected mass distribution in the 6 arcmin × 6 arcmin BUFFALO field-of-view, we obtain t…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 12