All Stories

  1. First Optical Constants of Laboratory-generated Organic Refractory Materials (Tholins) Produced in the NASA Ames COSmIC Facility from the Visible to the Near Infrared (0.4–1.6 μm): Application to Titan’s Aerosols
  2. Cavity Ring-Down Spectroscopy of Anthracene, 9-Methylanthracene, and 2-Methylanthracene in Supersonic Expansion
  3. Raman Spectroscopic Study of Pyrene in Cosmic Dust Analogues: Evolution from the Gas to the Solid Phase
  4. PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars
  5. A Laboratory-driven Multiscale Investigation of X-Ray Induced Mass Loss and Photochemical Evolution in Cosmic Carbon and Silicate Dust
  6. A Cross-laboratory Comparison Study of Titan Haze Analogs: Surface Energy
  7. Families and clusters of diffuse interstellar bands: a data-driven correlation analysis
  8. The Titan Haze Simulation (THS) experiment on COSmIC. Part III. XANES study of laboratory analogs of Titan tholins
  9. Multidisciplinary investigation of benzene (C6H6) condensation in Titan’s South polar cloud system
  10. Investigating the Condensation of Benzene (C6H6) in Titan’s South Polar Cloud System with a Combination of Laboratory, Observational, and Modeling Tools
  11. Critical Laboratory Studies to Advance Planetary Science and Support Missions
  12. The Science Case for a Titan Flagship-class Orbiter with Probes
  13. New Frontiers Titan Orbiter
  14. Characterization of Cosmic Grain Analogs Formed at Low Temperature from Small Hydrocarbon Precursors in the NASA Ames COSmIC Facility
  15. New Cold-Temperature Vapor Pressure Measurements Help Constrain the Microphysical Properties of Titan’s South Pole Benzene Cloud
  16. UV/Vis+ photochemistry database: Structure, content and applications
  17. Low-temperature Formation of Carbonaceous Dust Grains from PAHs
  18. Cavity ring down spectroscopy of cold neutral phenanthrene and phenanthridine in supersonic jets
  19. The Future of Laboratory Astrophysics
  20. The Titan haze simulation experiment: Investigating Titan’s low-temperature atmospheric chemistry in a pulsed plasma jet expansion
  21. Electronic spectroscopy of PAHs and PAH derivatives in supersonic jet
  22. Low-temperature condensation of carbonaceous dust grains from PAHs
  23. C6H6 condensation on Titan’s stratospheric aerosols: An integrated laboratory, modeling and experimental approach
  24. IAU volume 15 issue 350 Cover and Front matter
  25. A Model of Titan-like Chemistry to Connect Experiments and Cassini Observations
  26. The ESO Diffuse Interstellar Bands Large Exploration Survey (EDIBLES)
  27. The Titan Haze Simulation (THS) experiment on COSmIC. Part II. Ex-situ analysis of aerosols produced at low temperature
  28. Recent Progress in Laboratory Astrophysics Achieved with NASA Ames’ COSmIC Facility
  29. Special issue on atomic and molecular data for astrophysics
  30. DIVISION B COMMISSION 14: ATOMIC AND MOLECULAR DATA
  31. FM12: A Focus Meeting on Bridging Laboratory Astrophysics and Astronomy
  32. The THS experiment: Simulating Titan's atmospheric chemistry at low temperature (200 K)
  33. Special issue on atomic & molecular data for astrophysicists
  34. First results of the ORGANIC experiment on EXPOSE-R on the ISS
  35. Organics Exposure in Orbit (OREOcube): A Next-Generation Space Exposure Platform
  36. The Titan Haze Simulation experiment on COSmIC: Probing Titan’s atmospheric chemistry at low temperature
  37. VLT/X-Shooter survey of near-infrared diffuse interstellar bands
  38. Complementary and Emerging Techniques for Astrophysical Ices Processed in the Laboratory
  39. LABORATORY INVESTIGATIONS OF POLYCYCLIC AROMATIC HYDROCARBON FORMATION AND DESTRUCTION IN THE CIRCUMSTELLAR OUTFLOWS OF CARBON STARS
  40. DIVISION XII: COMMISSION 14: ATOMIC AND MOLECULAR DATA
  41. A Critical Review of PAHs as DIB Carriers - Progress and Open Questions
  42. X-Shooter Survey of Near-Infrared DIBs
  43. The O/OREOS Mission: First Science Data from the Space Environment Viability of Organics (SEVO) Payload
  44. The impact of recent advances in laboratory astrophysics on our understanding of the cosmos
  45. The development of the Space Environment Viability of Organics (SEVO) experiment aboard the Organism/Organic Exposure to Orbital Stresses (O/OREOS) satellite
  46. COMMISSION 14: ATOMIC AND MOLECULAR DATA
  47. The ORGANIC experiment on EXPOSE-R on the ISS: Flight sample preparation and ground control spectroscopy
  48. DIVISION VI / COMMISSION 34 / WORKING GROUP ASTROCHEMISTRY
  49. Linear and circular spectropolarimetry of diffuse interstellar bands
  50. C84: A Prototype of Larger Fullerenes. Laboratory Spectroscopy and Astronomical Relevance
  51. SEARCHING FOR NAPHTHALENE CATION ABSORPTION IN THE INTERSTELLAR MEDIUM
  52. POLYCYCLIC AROMATIC HYDROCARBONS AND THE DIFFUSE INTERSTELLAR BANDS: A SURVEY
  53. ON ESTIMATING INTERSTELLAR POLYCYCLIC AROMATIC HYDROCARBON ABUNDANCES WITH CALCULATED OSCILLATOR STRENGTHS
  54. The coupling of a reflectron time-of-flight mass spectrometer with a cosmic simulation chamber: A powerful new tool for laboratory astrophysics
  55. Formation and Evolution of Circumstellar and Interstellar PAHs: A Laboratory Study
  56. COMMISSION 14: ATOMIC AND MOLECULAR DATA
  57. COMMISSION 14: ATOMIC AND MOLECULAR DATA
  58. PAHs in Astronomy - A Review
  59. Detection of diffuse interstellar bands in M 31
  60. S1(A11)←S0(A11) transition of benzo[g,h,i]perylene in supersonic jets and rare gas matrices
  61. Interstellar gas, dust and diffuse bands in the SMC
  62. The ORGANICS experiment on BIOPAN V: UV and space exposure of aromatic compounds
  63. Flow dynamics of a pulsed planar expansion
  64. Cavity ring-down spectroscopy of jet-cooled 1-pyrenecarboxyaldehyde (C17H10O) and 1-methylpyrene (C17H12) cations
  65. Modeling the influence of anode–cathode spacing in a pulsed discharge nozzle
  66. Investigation of the Ultraviolet, Visible, and Near‐Infrared Absorption Spectra of Hydrogenated Polycyclic Aromatic Hydrocarbons and Their Cations
  67. Cavity ring-down spectroscopy and vibronic activity of benzo[ghi]perylene
  68. Plasma in a pulsed discharge environment
  69. Numerical investigation of the discharge characteristics of the pulsed discharge nozzle
  70. PAH charge state distribution and DIB carriers: Implications from the line of sight toward HD 147889
  71. Cavity ring-down spectroscopy and theoretical calculations of the S1(B3u1)←S0(Ag1) transition of jet-cooled perylene
  72. The Rotational Excitation Temperature of the λ6614 Diffuse Interstellar Band Carrier
  73. Multiplex integrated cavity output spectroscopy of cold PAH cations
  74. Plasma structure in a pulsed discharge environment
  75. The Role of Polycyclic Aromatic Hydrocarbons in Ultraviolet Extinction. I. Probing Small Molecular Polycyclic Aromatic Hydrocarbons
  76. Plasma structure in a pulsed discharge environment
  77. Pulsed discharge nozzle cavity ringdown spectroscopy of cold polycyclic aromatic hydrocarbon ions
  78. Electronic Absorption Spectra of Neutral Perylene (C 20 H 12 ), Terrylene (C 30 H 16 ), and Quaterrylene (C 40 H 20 ) and Their Positive and Negative Ions:  Ne Matrix-Isolation Spectroscopy and Time-Dependent Density Functional Theory Calculations
  79. Time‐dependent Density Functional Theory Calculations of Large Compact Polycyclic Aromatic Hydrocarbon Cations: Implications for the Diffuse Interstellar Bands
  80. Detection of Diffuse Interstellar Bands in the Magellanic Clouds
  81. Spectroscopy of large PAHs
  82. D1(2B2g)→D0(2Au) fluorescence from the matrix-isolated perylene cation following laser excitation into the D5(2B3g) and D2(2B3g) electronic states
  83. Absorption and emission spectroscopy of matrix-isolated benzo[g,h,i]perylene: An experimental and theoretical study for astrochemical applications
  84. Molecular spectroscopy in astrophysics: the case of polycyclic aromatic hydrocarbons
  85. Preface
  86. Electronic Absorption Spectra of Neutral Pentacene (C 22 H 14 ) and Its Positive and Negative Ions in Ne, Ar, and Kr Matrices
  87. Polycyclic Aromatic Hydrocarbons and the Diffuse Interstellar Bands: A Survey
  88. First detection of an ultraviolet transition in an ionized polycyclic aromatic hydrocarbon
  89. Absorption and emission spectroscopy of perylene (C20H12) isolated in Ne, Ar, and N2 matrices
  90. Jet-discharge cavity ring-down spectroscopy of ionized polycyclic aromatic hydrocarbons: progress in testing the PAH hypothesis for the diffuse interstellar band problem
  91. Carbon in the Universe
  92. Matrix‐isolated Nano‐sized Carbon Grains as an Analog for the 217.5 Nanometer Feature Carrier
  93. UV Photochemistry of Ices
  94. Organics in the diffuse interstellar medium
  95. Assessment of the Polycyclic Aromatic Hydrocarbon--Diffuse Interstellar Band Proposal
  96. Neutral and Ionized PAH Spectral Properties
  97. Low temperature spectroscopy: From ground to space
  98. Neutral and ionized PAHs: contribution to the interstellar extinction
  99. Photoinduced fluorescence from the perylene cation isolated in Ne and Ar matrices
  100. Polycyclic aromatic hydrocarbon ions and the diffuse interstellar bands
  101. Absorption Spectroscopy of Neutral and Ionized PAHs. Implications for the Diffuse Interstellar Bands
  102. Visible Luminescence from PAH Cations and the Diffuse Bands in Emission
  103. Electronic absorption spectroscopy of matrix‐isolated polycyclic aromatic hydrocarbon cations. II. The phenanthrene cation (C14H10+) and its 1‐methyl derivative
  104. New Narrow Infrared Absorption Features in the Spectrum of Io between 3600 and 3100 cm-1 (2.8-3.2 μm)
  105. Is H2O Present on Io? The Detection of a New Strong Band Near 3590 cm-1 (2.79 μm)
  106. Theoretical study of the electronic spectra of a polycyclic aromatic hydrocarbon, naphthalene, and its derivatives
  107. General discussion
  108. Neutral and ionized polycyclic aromatic hydrocarbons, diffuse interstellar bands and the ultraviolet extinction curve
  109. The ultraviolet and visible spectrum of the polycyclic aromatic hydrocarbon C10H8(+) - Possible contributions to the diffuse interstellar bands and to the ultraviolet-visible extinction
  110. Is a pyrene-like molecular ion the cause of the 4,430-Å diffuse interstellar absorption band?
  111. The role of matrix material and CCl4 (electron acceptor) on the ionization mechanisms of matrix‐isolated naphthalene
  112. Electronic absorption spectroscopy of matrix‐isolated polycyclic aromatic hydrocarbon cations. I. The naphthalene cation (C10H+8)
  113. Laboratory studies of the newly discovered infrared band at 4705.2 cm−1 (2.1253 μm) in the spectrum of Io: The tentative identification of CO2
  114. A new class of absorption feature in lo's near-infrared spectrum
  115. The 2.5–5.0 μm spectra of Io: Evidence for H2S and H2O frozen in SO2
  116. Near-infrared-light-induced reaction of singlet sulfur monoxide with allene and dimethylacetylene in a rare gas matrix: infrared spectra of two novel episulfoxides
  117. Theoretical and experimental studies of the electronic states of the diatomic cation Cl 2 2 +
  118. Determination of the lowest bound ionic state threshold of Cl2 trapped in solid argon at 4.5 K using synchrotron radiation
  119. Ultraviolet photolysis and internal dynamics of molecular chlorine in an argon matrix at 4.2 K
  120. Formation and dissociation of doubly ionized methane