All Stories

  1. On the Origin of Sodium in Comets
  2. Unveiling the nature of HE 0107–5240: a long period binary CEMP-no star with [Fe/H] of –5.56
  3. Alkali phenoxides in comets
  4. Explaining the 12C/13C ratio in the Galactic halo: The contribution from shell mergers in primordial massive stars
  5. Possible evidence for the 478 keV emission line from 7Be decay during the outburst phases of V1369 Cen
  6. A Sequoia stellar candidate with very high 7Li and 9Be
  7. High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds
  8. Radiocarbon Ages of a Possible Titian Painting
  9. Revisiting the multi-planetary system of the nearby star HD 20794
  10. Radiocarbon Ages of a Possible Titian’s Painting
  11. SDSS J102915.14+172927.9: Revisiting the chemical pattern
  12. A sub-Earth-mass planet orbiting Barnard’s star
  13. Extragalactic 85Rb/87Rb and 6Li/7Li ratios in the Small Magellanic Cloud
  14. Isotopic abundance of carbon in the DLA towards QSO B1331+170
  15. Three super-Earths and a possible water world from TESS and ESPRESSO
  16. The physical properties of T Pyx as measured by MUSE
  17. TESS and ESPRESSO discover a super-Earth and a mini-Neptune orbiting the K-dwarf TOI-238
  18. The compact multi-planet system GJ 9827 revisited with ESPRESSO
  19. Fundamental physics with ESPRESSO: a new determination of the D/H ratio towards PKS1937-101
  20. Probing the small-scale structure of the intergalactic medium with ESPRESSO: spectroscopy of the lensed QSO UM673
  21. Possible stellar asterisms carved on a protohistoric stone
  22. Revisiting the classics: on the evolutionary origin of the ‘Fe ii’ and ‘He/N’ spectral classes of novae
  23. The 12C/13C isotopic ratio at the dawn of chemical evolution
  24. A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO
  25. Catching a nova X-ray/UV flash in the visible? Early spectroscopy of the very slow Nova Velorum 2022 (Gaia22alz)
  26. Detection of a high-velocity sodium feature on the ultra-hot Jupiter WASP-121 b
  27. Planetary system around LTT 1445A unveiled by ESPRESSO: Multiple planets in a triple M-dwarf system
  28. Shock shaping? Nebular spectroscopy of nova V906 Carinae
  29. The pristine nature of SMSS 1605−1443 revealed by ESPRESSO
  30. ESPRESSO observations of HE 0107−5240 and other CEMP-no stars with [Fe/H] ≤ –4.5
  31. Classical novae with CUBES
  32. Detection of barium in the atmospheres of the ultra-hot gas giants WASP-76b and WASP-121b
  33. Fundamental physics with ESPRESSO: Constraining a simple parametrisation for varying α
  34. 7Be detection in the 2021 outburst of RS Oph
  35. ON THE ORIGIN OF THE KEPLERIAN TELESCOPE
  36. Fundamental physics with ESPRESSO: Constraints on Bekenstein and dark energy models from astrophysical and local probes
  37. A candidate short-period sub-Earth orbiting Proxima Centauri
  38. Fundamental physics with ESPRESSO: Precise limit on variations in the fine-structure constant towards the bright quasar HE 0515−4414
  39. Detection of 7Be ii in the Small Magellanic Cloud
  40. 7Be in the outburst of the ONe nova V6595 Sgr
  41. HD 22496 b: The first ESPRESSO stand-alone planet discovery
  42. The Rossiter–McLaughlin effect revolutions: an ultra-short period planet and a warm mini-Neptune on perpendicular orbits
  43. Into the storm: diving into the winds of the ultra-hot Jupiter WASP-76 b with HARPS and ESPRESSO
  44. Warm terrestrial planet with half the mass of Venus transiting a nearby star
  45. Six transiting planets and a chain of Laplace resonances in TOI-178
  46. A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)
  47. The atmosphere of HD 209458b seen with ESPRESSO
  48. ESPRESSO high-resolution transmission spectroscopy of WASP-76 b
  49. Fundamental physics with ESPRESSO: Towards an accurate wavelength calibration for a precision test of the fine-structure constant
  50. ESPRESSO at VLT
  51. On the Titian’s self-portrait mentioned by Vasari with technical analysis of an anonymous painting
  52. Atmospheric Rossiter–McLaughlin effect and transmission spectroscopy of WASP-121b with ESPRESSO
  53. ELT-HIRES, the high resolution spectrograph for the ELT: the Phase A study and the path to construction
  54. Broadband transmission spectroscopy of HD 209458b with ESPRESSO: evidence for Na, TiO, or both
  55. WASP-127b: a misaligned planet with a partly cloudy atmosphere and tenuous sodium signature seen by ESPRESSO
  56. The solar gravitational redshift from HARPS-LFC Moon spectra
  57. K2-111: an old system with two planets in near-resonance†
  58. A new era of fine structure constant measurements at high redshift
  59. A precise architecture characterization of theπMensae planetary system
  60. Characterization of the K2-38 planetary system
  61. Review of Particle Physics
  62. Revisiting Proxima with ESPRESSO
  63. Lithium and beryllium in the Gaia-Enceladus galaxy
  64. Direct evidence for shock-powered optical emission in a nova
  65. Search for 7Be in the outbursts of four recent novae
  66. ESPRESSO highlights the binary nature of the ultra-metal-poor giant HE 0107−5240
  67. Catalog for the ESPRESSO blind radial velocity exoplanet survey
  68. Rotational and Rotational-Vibrational Raman Spectroscopy of Air to Characterize Astronomical Spectrographs
  69. 7Li evolution in the thin and thick discs of the Milky Way
  70. Macro X-ray fluorescence imaging spectroscopy of the suggested Santi di Tito's portrait of Galileo Galilei
  71. Absorption and emission features of 7Be ii in the outburst spectra of V838 Her (Nova Her 1991)
  72. Review of Particle Physics
  73. ESPRESSO data flow in operations: results of commissioning activities
  74. Gamma-ray observations of Nova Sgr 2015 No. 2 with INTEGRAL
  75. TOPoS
  76. Cosmological evolution of the nitrogen abundance
  77. Beryllium detection in the very fast nova ASASSN-16kt (V407 Lupi)
  78. ESPRESSO on VLT: An Instrument for Exoplanet Research
  79. ESPRESSO on VLT: An Instrument for Exoplanet Research
  80. FRANCESCO FONTANA AND THE BIRTH OF THE ASTRONOMICAL TELESCOPE
  81. Thomas Harriot at the National Gallery?
  82. The GAPS Programme with HARPS-N at TNG
  83. Dark Energy Constraints from Espresso Tests of the Stability of Fundamental Couplings
  84. Dark energy constraints from ESPRESSO tests of the stability of fundamental couplings
  85. ON THE LOST PORTRAIT OF GALILEO BY THE TUSCAN PAINTER SANTI DI TITO
  86. Review of Particle Physics
  87. Highly enriched7Be in the ejecta of Nova Sagittarii 2015 No. 2 (V5668 Sgr) and the Galactic7Li origin
  88. Long-term radial-velocity variations of the Sun as a star: The HARPS view
  89. Daily variability of Ceres’ albedo detected by means of radial velocities changes of the reflected sunlight
  90. HST/STIS abundances in the uranium rich metal poor star CS 31082-001: Constraints on the r-Process
  91. The GAPS programme with HARPS-N at TNG
  92. The Earth transiting the Sun as seen from Jupiter's moons: detection of an inverse Rossiter–McLaughlin effect produced by the opposition surge of the icy Europa
  93. Lithium evolution in metal-poor stars: from pre-main sequence to the Spite plateau
  94. Lithium evolution from Pre-Main Sequence to the Spite plateau: an environmental solution to the cosmological lithium problem
  95. TOPoS
  96. The GAPS programme with HARPS-N at TNG
  97. Measurement of the radial velocity of the Sun as a star by means of a reflecting solar system body
  98. The ESO UVES Advanced Data Products Quasar Sample – IV. On the deficiency of argon in DLA systems
  99. The UVES Large Program for testing fundamental physics – III. Constraints on the fine-structure constant from three telescopes
  100. The ESO UVES advanced data products quasar sample – III. Evidence of bimodality in the [N/α] distribution
  101. ESPRESSO: the radial velocity machine for the VLT
  102. DLA abundances in the CUBES’s spectral window
  103. ESPRESSO: The next European exoplanet hunter
  104. Fundamental constants and high-resolution spectroscopy
  105. A frequency comb calibrated solar atlas
  106. X-shooter GTO: evidence for a population of extremely metal-poor, alpha-poor stars
  107. Limits on the spatial variations of the electron-to-proton mass ratio in the Galactic plane
  108. Strongly star-forming rotating disks in a complex merging system atz= 4.7 as revealed by ALMA
  109. ESPRESSO, an exo-Earths hunter for the VLT
  110. Metals in the IGM approaching the re-ionization epoch: results from X-shooter at the VLT
  111. The UVES large program for testing fundamental physics – II. Constraints on a change in μ towards quasar HE 0027−1836★
  112. The UVES Large Program for testing fundamental physics I. Bounds on a change inαtowards quasar HE 2217−2818
  113. POTASSIUM DETECTION AND LITHIUM DEPLETION IN COMETS C/2011 L4 (PANSTARRS) AND C/1965 S1 (IKEYA-SEKI)
  114. First stars
  115. Detection of the Rossiter–McLaughlin effect in the 2012 June 6 Venus transit★
  116. Edgar Allan Poe: the first man to conceive a Newtonian evolving Universe
  117. ESPRESSO: the ultimate rocky exoplanets hunter for the VLT
  118. Solar atlas revised
  119. A primordial star in the heart of the Lion
  120. Deuterium at high redshift
  121. QSO 0347-383 and the invariance ofmp/mein the course of cosmic time
  122. AMMONIA AS A TRACER OF FUNDAMENTAL CONSTANTS
  123. Possible portrait of Galileo Galilei as a young scientist
  124. First stars
  125. X-Shooter GTO: chemical analysis of a sample of EMP candidates
  126. An extremely primitive star in the Galactic halo
  127. HST-STIS abundances in the uranium-rich metal-poor star CS31082-001
  128. Lines of heavy elements and Fe ii in the UV of CS 31082-0011This article is part of a Special Issue on the 10th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas.
  129. First measurement of Mg isotope abundances at high redshifts and accurate estimate of Δα/α
  130. Optical-NIR spectra of quasars close to reionization (z ∼ 6)
  131. Extremely metal-poor stars in SDSS fields
  132. First stars
  133. First stars
  134. Robust limit on a varying proton-to-electron mass ratio from a single H2system
  135. ESO Future Facilities to Probe Fundamental Physical Constants
  136. From Varying Couplings to Fundamental Physics
  137. Robust Limit on a Varying Proton-to-Electron Mass Ratio from a Single H2 System
  138. Searching for Chameleon-Like Scalar Fields
  139. Spectrographs, Asteroids and Constants
  140. Starless Cores as Fundamental Physics Labs
  141. Ceres’ sunlight atlas
  142. Searching for chameleon-like scalar fields with the ammonia method
  143. The metal-poor end of the Spite plateau
  144. ESPRESSO: the Echelle spectrograph for rocky exoplanets and stable spectroscopic observations
  145. CODEX
  146. Searching for spatial variations ofα2/μin the Milky Way
  147. Searching for chameleon-like scalar fields with the ammonia method
  148. Calibration issues in Δα/α
  149. Cosmological observations to shed light on possible variations
  150. IAU Joint Discussion 9: Are the Fundamental Constants Varying in Space-time?
  151. Spatial and temporal variations of fundamental constants
  152. VLT and E-ELT spectrographs & fundamental-constants
  153. The metal–poor end of the Spite plateau: gravity sensitivity of the Hα wings fitting.
  154. Stringent bounds to spatial variations of the electron-to-proton mass ratio in the Milky Way
  155. Metal-rich absorbers at high redshifts: abundance patterns
  156. HST-STIS abundances in the uranium-rich very metal-poor star CS 31082-001
  157. The metal–poor end of the Spite plateau
  158. First stars XII. Abundances in extremely metal-poor turnoff stars, and comparison with the giants
  159. On the telescopes in the paintings of Jan Brueghel the Elder
  160. ESPRESSO: A High Resolution Spectrograph for the Combined Coudé Focus of the VLT
  161. The ESO Large Programme “First Stars”
  162. Bounds on the fine structure constantvariability from Fe ii absorption lines in QSO spectra
  163. CODEX: the high-resolution visual spectrograph for the E-ELT
  164. Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg
  165. Cosmic dynamics in the era of Extremely Large Telescopes
  166. Mid- and far-infrared fine-structure-line sensitivities to hypothetical variability of the fine-structure constant
  167. EUV spectral energy distribution of quasars restored from associated absorbers
  168. UVES radial velocity accuracy from asteroid observations
  169. A new approach for testing variations of fundamental constants over cosmic epochs using FIR fine-structure lines
  170. First stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876-032
  171. CS 22876–032: The Most Metal‐Poor Dwarfs. Abundances and 3D Effects
  172. The Metal‐Poor End of the Lithium Plateau
  173. First stars
  174. The isotopic6Li/7Li ratio in Centaurus X-4 and the origin of Li in X-ray binaries
  175. Variations in the lithium abundances of turn off stars in the globular cluster 47 Tucanae
  176. A new measure of $\mathsf{\Delta\alpha/\alpha}$ at redshift $\mathsf{z = 1.84}$ from very high resolution spectra of Q 1101–264
  177. First stars VII - Lithium in extremely metal poor dwarfs
  178. First stars X. The nature of three unevolved carbon-enhanced metal-poor stars
  179. Abundances in extremely metal-poor stars: comparison of the trends of abundance ratios in giants and turnoff stars
  180. First stars IX - Mixing in extremely metal-poor giants. Variation of the $ \mathsf{^{12}C/^{13}C } $, [Na/Mg] and [Al/Mg] ratios
  181. Most precise single redshift bound to $\mathsf{\Delta\alpha/\alpha}$
  182. VLT/UVES constraints on the carbon isotope ratio $^\mathsf{12}$C/$^\mathsf{13}$C at z = 1.15 toward the quasar HE 0515–4414
  183. Abundance of Heavy Elements in Extremely Metal-Poor Stars
  184. Abundance of heavy elements in extremely metal-poor stars
  185. Evidence of Mixing in Extremely Metal-Poor Giants
  186. Exploring variations in the fundamental constants with ELTs: the CODEX spectrograph on OWL
  187. CODEX: measuring the acceleration of the universe and beyond
  188. Most precise single redshift bound to the variability of the fine-structure constant
  189. Li in NGC 6752 and the formation of globular clusters
  190. Spectral energy distribution of the metagalactic ionizing radiation field from QSO absorption spectra
  191. Chemical Abundances in the Secondary Star of the Neutron Star Binary Centaurus X‐4
  192. Abundances in extremely metal-poor stars. Comparison of the trends of abundance ratios in giants and turnoff stars
  193. Lithium abundances in extremely metal-poor unevolved stars
  194. VLT/UVES constraints on the cosmological variability of the fine-structure constant
  195. VLT/UVES shows no cosmological variability of $\alpha$
  196. First stars VI – Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements
  197. Cu and Zn in the early Galaxy
  198. Galactic evolution of nitrogen
  199. First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
  200. Hints of star formation atz$\mathsf{>6}$: The chemical abundances of the DLA system in the QSO BRI 1202-0725 (z$\mathsf{_{abs}=4.383}$)
  201. Heavy elements abundances in turn-off stars and early subgiants in NGC 6752
  202. First stars IV. CS 29497–030: Evidence for operation of thes-process at very low metallicity
  203. First Stars. III. A detailed elemental abundance study of four extremely metal-poor giant stars
  204. Early stages of nitrogen enrichment in galaxies: Clues from measurements in damped Lyman αsystems
  205. The AVES adaptive optics spectrograph for the VLT: status report
  206. Extremely metal-poor Lyman limit system at $\mathsf{{\vec z}_{abs} = 2.917}$ toward the quasar HE 0940–1050
  207. A new constraint on cosmological variability of the proton-to-electron mass ratio
  208. Molecular Hydrogen, Deuterium, and Metal Abundances in the Damped Lyα System atzabs = 3.025 toward Q0347−3819
  209. The cosmic microwave background radiation temperature at $\vec{z}_\mathsf{abs} = \mathsf{3.025}$ toward QSO 0347–3819
  210. Abundances in Damped LYα Systems
  211. Commission 29: Stellar Spectra (Spectres Stellaires)
  212. Oxygen in the Very Early Galaxy
  213. A D/H measurement in the damped Lyα system at zabs = 3.025 towards QSO 0347-3819
  214. DETAILED CHEMICAL ANALYSIS OF TWO GIANTS IN THE SGR DSPH
  215. VLT/UVES OBSERVATIONS OF THE DLA AT Z=3.39 TOWARDS QSO 0000-2621
  216. An astrophysical oscillator strength for the S II 94.7-nm resonance line and S abundances in DLAs
  217. Determination of [O/Fe] in BD +23 3130 from ESO VLT-UVES observations
  218. Oxygen abundances derived in unevolved very metal-poor stars
  219. UVES observations of a damped Lyαsystem at $\mathsf{{\vec z}_{abs} = 4.466}$ towards the quasar APM BR J0307-4945
  220. Oxygen in the Very Early Galaxy
  221. The O-Na and Mg-Al anticorrelations in turn-off and early subgiants in globular clusters
  222. A new deuterium abundance measurement from a damped Lyα system at $\vec{z}_{\mathsf{abs}} =\mathsf{3.025}$
  223. UVES Observations of QSO 0000−2620: Argon and Phosphorus Abundances in the Dust‐free Damped Lyα System atzabs = 3.3901
  224. Measurement of stellar age from uranium decay
  225. Zinc as a Tracer of Metallicity Evolution of Damped Lyα Systems
  226. UVES Observations of QSO 0000−2620: Oxygen and Zinc Abundances in the Damped Lyα Galaxy atzabs = 3.3901
  227. Intrinsic colour calibration for F, G, K stars
  228. The INT Search for Metal-Poor Stars: Spectroscopic Observations and Classification via Artificial Neural Networks
  229. Design study of an adaptive optics visual echelle spectrograph and imager for the VLT
  230. Chemical Evolution of Damped Lyα Galaxies: The [S/Zn] Abundance Ratio at Redshift ≥2
  231. Abundances of metal-weak thick-disc candidates
  232. Nitrogen Abundances in Damped Lyα Galaxies
  233. Detection of the L[CLC]i[/CLC] [CSC]i[/CSC] λ6104 Transition in the Population II Star HD 140283
  234. Chemical abundances in the young galaxy at z=2.309 towards PHL 957
  235. The primordial lithium abundance
  236. The mass ratio of Nova Muscae 1991
  237. Chemical Evolution at High Redshift
  238. Neutral Nitrogen in Damped Lyman a Systems
  239. Lithium in black hole binaries: the case of X-ray Nova Muscae 1991
  240. Lithium Abundance of Halo Stars with New T eff
  241. As Metal Poor as It Could Be: the Damped System at z=3.390 Towards QSO 0000-2619
  242. Beryllium Abundances in a New Set of Halo Stars
  243. The Gunn-Peterson effect in the spectrum of the Z = 4.7 QSO 1202-0725: The intergalactic medium at very high redshifts
  244. NaI and CaII Interstellar Absorption in the Field of SN 1987A
  245. NaI and CaII interstellar absorption in the field of SN 1987A
  246. MG II observed in the local interstellar medium - The local cloud
  247. Million degree gas in the Galactic halo and the Large Magellanic Cloud. II - The line of sight to supernova 1987A
  248. NA I interstellar absorption in the direction of two LMC supergiants in the field of SN 1987A
  249. Some considerations on the non-detection of interstellar Li and B towards the SN1987a
  250. The local interstellar medium: A test-bed for the galactic ISM
  251. High-Velocity Absorption Components Toward the LMC
  252. Boron Abundance in the PopII HD 76932
  253. Lithium Abundances in a New Sample of Metal Deficient Dwarfs
  254. Lithium Abundances in a New Sample of Metal Deficient Dwarfs
  255. Distribution and kinematics of MgII in the LISM
  256. Ultraviolet interstellar lines towards nearby fast rotators: ZnII distribution and MgII/MgI ratios
  257. MgII Spectra of Late Type Stars Used to Probe the LISM
  258. Detection of Narrow C IV and Si IV Absorption Features in Spectra of Stars within 200 pc of The Sun
  259. Iue Observations of 17 Lep
  260. High-Precision Measurements of Δα/αfrom QSO Absorption Spectra
  261. From ESPRESSO to CODEX
  262. Science with a 16 m VLT: The Case for Variability of Fundamental Constants
  263. Codex
  264. Abundances in Sagittarius Stars
  265. Abundances in Damped Lyα Galaxies
  266. Scientific Objectives and Design Study of an Adaptive Optics Visual Echelle Spectrograph and Imager Coronograph (AVES-IMCO) for the NAOS Visitor Focus at the VLT
  267. A High-Redshift Damped Ly- $\alpha$ System at z abs = 4.466 Towards APM BR J0307-4945
  268. Molecular Hydrogen Abundance in the Dust-Free Damped Ly- $\alpha$ Galaxy at z = 3.4
  269. Interstellar Absorption-Line Observations of the Magellanic Clouds
  270. High-velocity absorption components toward the LMC
  271. The NaI interstellar spectrum of HVC 287.5+225+240