activity
20122026
most citedThe XXL Survey XX: The 365 cluster catalogue

131 citations · 220 across the 13 of their papers we have counts for

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Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2026

Dissecting ultra-diffuse galaxies in the field

A. Vanzanella, K. Malek, Junais +16

Context. Ultra-diffuse galaxies (UDGs) in the field are faint, diffuse systems that remain poorly represented in the literature due to the need for spectroscopic confirmation and t…

astro-ph.GA2026

From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies

Hareesh Thuruthipilly, Krzysztof Lisiecki, Junais +19

Low-surface-brightness galaxies (LSBGs) are vital for understanding galaxy formation, but their diffuse nature makes them challenging to detect. Upcoming large-scale surveys are ex…

astro-ph.GA2025★ 2 cited

Characterizing the outer disk of eXtended-UV galaxies in the optical domain with deep surveys

E. Bernaud, S. Boissier, Junais +3

Aims : Extended-UV (XUV) galaxies are galaxies presenting an extended outer ultraviolet disks. Although some Giant Low Surface Brightness (GLSB) galaxies are also XUV, their relati…

astro-ph.GA2025★ 4 cited

DES to HSC: Detecting low surface brightness galaxies in the Abell 194 cluster using transfer learning

H. Thuruthipilly, Junais, J. Koda +7

Low surface brightness galaxies (LSBGs) are important for understanding galaxy evolution and cosmological models. The upcoming large-scale surveys are expected to uncover a large n…

astro-ph.GA2024★ 18 cited

Effects of galaxy environment on merger fraction

W. J. Pearson, D. J. D. Santos, T. Goto +13

Aims. In this work, we intend to examine how environment influences the merger fraction, from the low density field environment to higher density groups and clusters. We also aim t…

astro-ph.GA2024

Attenuation proxy hidden in surface brightness-colour diagrams. A new strategy for the LSST era

K. Małek, Junais, A. Pollo +22

Large future sky surveys, such as the LSST, will provide optical photometry for billions of objects. This paper aims to construct a proxy for the far ultraviolet attenuation (AFUVp…

astro-ph.GA2023

A comparative study of the fundamental metallicity relation: the impact of methodology on its observed evolution

F. Pistis, A. Pollo, M. Figueira +10

We used 5487 star-forming galaxies at redshift z~0.63 extracted from the VIPERS and 143774 comparison galaxies in the local Universe from the GSWLC catalog. We employed two familie…

astro-ph.GA2023★ 11 cited

Shedding Light on Low Surface Brightness Galaxies in Dark Energy Survey with Transformers

H. Thuruthipilly, Junais, A. Pollo +5

Low surface brightness galaxies (LSBGs) which are defined as galaxies that are fainter than the night sky, play a crucial role in understanding galaxy evolution and cosmological mo…

astro-ph.GA2023★ 14 cited

MUSE observations of the giant low surface brightness galaxy Malin 1: Numerous HII regions, star formation rate, metallicity, and dust attenuation

Junais, P. M. Weilbacher, B. Epinat +6

Giant low-surface brightness (GLSB) galaxies are an extreme class of objects with very faint and extended gas-rich disks. Malin 1 is the largest GLSB galaxy known to date, but its…

astro-ph.GA2023★ 16 cited

X-ray luminosity-star formation rate scaling relation: Constraints from the eROSITA Final Equatorial Depth Survey (eFEDS)

G. Riccio, G. Yang, Małek +7

We present measurements of the relation between X-ray luminosity and star formation activity for a sample of normal galaxies spanning the redshift range between 0 and 0.25. We use…

astro-ph.GA2023★ 8 cited

Decoding the IRX-β dust attenuation relation in star-forming galaxies at intermediate redshift

M. Hamed, F. Pistis, M. Figueira +11

We aim to understand what drives the IRX-βdust attenuation relation at intermediate redshift (0.5 < z < 0.8) in star-forming galaxies. We investigate the role of various galaxy pro…