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Gas flows in the central region of the Seyfert galaxy NGC 4593 with MUSE
DOI: 10.1051/0004-6361/202450076 Bibcode: 2024A&A...690A.277M

Knapen, J. H.; Comerón, S.; Pereira-Santaella, M. +4 more

Context. Understanding how gas flows into galactic centres, fuels the active galactic nucleus (AGN), and is in turn expelled back through feedback processes is of great importance to appreciate the role AGN play in the growth and evolution of galaxies. Aims. We use Multi Unit Spectroscopic Explorer-adaptive optics (MUSE-AO) optical spectra of the …

2024 Astronomy and Astrophysics
eHST 1
Detection of Close Kuiper Belt Binaries with HST WFC3
DOI: 10.3847/PSJ/ad3f19 Bibcode: 2024PSJ.....5..143P

Porter, Simon B.; Verbiscer, Anne J.; Noll, Keith S. +3 more

Binaries in the Kuiper Belt are common. Here we present our analysis of the Solar System Origins Legacy Survey (SSOLS) to show that using a point-spread function (PSF)-fitting method can roughly double the number of binaries identified in that data set. Out of 198 Kuiper Belt objects (KBOs) observed by SSOLS, we find 23 to be visually separated bi…

2024 The Planetary Science Journal
Gaia eHST 1
A Star-based Method for the Precise Flux Calibration of the Chinese Space Station Telescope Slitless Spectroscopic Survey
DOI: 10.3847/1538-4365/ad2207 Bibcode: 2024ApJS..271...37Y

Huang, Bowen; Yuan, Haibo; Xiao, Kai +5 more

The upcoming Chinese Space Station Telescope (CSST) slitless spectroscopic survey poses a challenge of flux calibration, which requires a large number of flux-standard stars. In this work, we design an uncertainty-aware residual attention network, the UaRA-net, to derive the CSST spectral energy distributions (SEDs) with a resolution of R = 200 ov…

2024 The Astrophysical Journal Supplement Series
Gaia eHST 1
Chandra and HST studies of the X-ray sources in the globular cluster NGC 362
DOI: 10.1093/mnras/stae865 Bibcode: 2024MNRAS.530...82K

Heinke, Craig O.; Cohn, Haldan N.; Lugger, Phyllis M. +1 more

We analyse a Chandra observation of the rich globular cluster NGC 362, finding 33 X-ray sources within 1 arcmin (1.2 half-mass radii) of the cluster centre. Spectral analysis of the brightest source (X1) shows blackbody-like emission, indicating it is likely a quiescent low-mass X-ray binary; we find a possible counterpart that falls in the sub-su…

2024 Monthly Notices of the Royal Astronomical Society
Gaia eHST 1
Hubble Space Telescope proper motions of Large Magellanic Cloud star clusters: I. Catalogues and results for NGC 1850
DOI: 10.1051/0004-6361/202450255 Bibcode: 2024A&A...689A.162N

Martocchia, S.; Cabrera-Ziri, I.; Bastian, N. +11 more

We present proper motion (PM) measurements for a sample of 23 massive star clusters within the Large Magellanic Cloud using multi-epoch data from the Hubble Space Telescope (HST). We combined archival data from the ACS/WFC and WFC3/UVIS instruments with observations from a dedicated HST programme, resulting in time baselines between 4.7 and 18.2 y…

2024 Astronomy and Astrophysics
Gaia 1
The Lockman-SpReSO project. Main properties of infrared-selected star-forming galaxies
DOI: 10.1051/0004-6361/202449238 Bibcode: 2024A&A...687A..19G

Krongold, Yair; Sánchez-Portal, Miguel; Bongiovanni, Ángel +18 more


Aims: In this work, we carry out a comprehensive study using galaxy data from the Lockman Spectroscopic Redshift Survey using Osiris (Lockman-SpReSO) project, a far-infrared (FIR) selected sample of galaxies observed using optical spectroscopy. We analyse a sub-sample of star-forming galaxies (SFGs) with secure spectroscopic redshifts, mostly…

2024 Astronomy and Astrophysics
XMM-Newton 1
Searching the SN 1987A SETI Ellipsoid with TESS
DOI: 10.3847/1538-3881/ad2064 Bibcode: 2024AJ....167..101C

Davenport, James R. A.; Siemion, Andrew P. V.; Cody, Ann Marie +4 more

The SETI Ellipsoid is a strategy for technosignature candidate selection that assumes that extraterrestrial civilizations who have observed a galactic-scale event—such as supernova 1987A—may use it as a Schelling point to broadcast synchronized signals indicating their presence. Continuous wide-field surveys of the sky offer a powerful new opportu…

2024 The Astronomical Journal
Gaia 1
Ultra-long-period Cepheids as Standard Candles from Gaia to Rubin-LSST
DOI: 10.3847/1538-4365/ad863c Bibcode: 2024ApJS..275...26M

Di Criscienzo, M.; Ripepi, V.; Molinaro, R. +10 more

An analysis of the properties of ultra-long-period Cepheids (ULPs) could significantly contribute to understanding the Hubble constant tension, e.g., the current discrepancy between determinations based on local distance indicators and those relying on cosmic microwave background measurements. These highly luminous variables are observable beyond …

2024 The Astrophysical Journal Supplement Series
Gaia 1
Large Glacier-Like Forms on Mars: Insights From Crater Morphologies and Crater Retention Ages
DOI: 10.1029/2023JE008207 Bibcode: 2024JGRE..12908207D

El-Maarry, M. R.; Driver, G.; Hubbard, B. +1 more

Glacier-Like Forms (GLFs) are a subset of ice-rich landforms known as Viscous Flow Features that populate Mars' mid-latitudes. GLFs are morphologically similar to terrestrial valley glaciers and are thought to result from the redistribution of water ice from the Martian poles during periods of high obliquity throughout the Amazonian period. Their …

2024 Journal of Geophysical Research (Planets)
MEx 1
A comprehensive study of five candidate δ Scuti-type pulsators in detached eclipsing binaries
DOI: 10.1051/0004-6361/202451126 Bibcode: 2024A&A...691A.101P

Hełminiak, K. G.; Konacki, M.; Moharana, A. +4 more

Context. Pulsating stars in eclipsing binaries (EBs) provide an excellent opportunity to obtain precise, model-independent stellar parameters for studying these oscillations in detail. One of the most common classes of pulsators found in such EBs exhibits δ Scuti-type oscillations. Characterising these pulsators using the precise stellar parameter…

2024 Astronomy and Astrophysics
Gaia 1