Showing 521–540 of 2,473 results
/ Date/ Name
Feb 26, 2024The outskirts of M33: Tidally induced distortions versus signatures of gas accretionFeb 21, 2024PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field IIFeb 19, 2024Constraining the stellar populations of ultra-diffuse galaxies in the MATLAS survey using spectral energy distribution fittingFeb 19, 2024A study of the radio spectrum of Mrk 421Feb 18, 2024The boundary of cosmic filamentsFeb 17, 2024Peering into cosmic reionization: the Ly$α$ visibility evolution from galaxies at $z$ = 4.5-8.5 with JWSTFeb 15, 2024Near-infrared spectroscopic characterisation of Gaia ultra-cool dwarf candidates; Spectral types and peculiaritiesFeb 12, 2024The Firefly Sparkle: The Earliest Stages of the Assembly of A Milky Way-type Galaxy in a 600 Myr Old UniverseFeb 11, 2024SRG/ART-XC Galactic Plane Survey near Galactic Longitude $l\simeq20^\circ$: Catalog of SourcesFeb 8, 2024The Gaia-ESO Survey: The DR5 analysis of the medium-resolution GIRAFFE and high-resolution UVES spectra of FGK-type starsFeb 8, 2024UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at $z_{spec}=3.97$Feb 7, 2024Nature of the diffuse emission sources in the H I supershell in the galaxy IC 1613Feb 6, 2024JWST Observations of Young protoStars (JOYS): Linked accretion and ejection in a Class I protobinary systemFeb 6, 2024JWST observations of $^{13}$CO$_{2}$ ice: Tracing the chemical environment and thermal history of ices in protostellar envelopesFeb 5, 2024MUSE-ALMA Haloes X: The stellar masses of gas-rich absorbing galaxiesFeb 3, 2024Second Response to the critique of "Cotton Gravity''Feb 2, 2024La Silla-QUEST RR Lyrae Star Survey II: The Crater II Tidal StreamsFeb 2, 2024The first quenched galaxies, when and how?Feb 1, 2024Ordered magnetic fields around the 3C 84 central black holeJan 31, 2024Dark matter measurements combining stellar and HI kinematics: 30% $1-σ$ outliers with low dark matter content at $5R_\mathrm{e}$