All Stories

  1. Special Section Guest Editorial: Lessons Learned from the James Webb Space Telescope Program
  2. What is the main lesson we learned from our work on designing and building the Webb Space Telescope.
  3. Constructing Highly Accurate Inflatable Parabolic Dish Reflector Antennas and Solar Concentrators
  4. Very Large-diameter, Ultralight Space Telescopes to Enable Large-scale Survey of Candidate Earth-like Planets for Signatures of Life
  5. Laser damage, a new US standard: What is in it for me?
  6. Disruptive space telescope concepts, designs, and developments: OASIS and Nautilus -INVITED
  7. Analysis of the cost, schedule, and risk for Lynx mirror assembly production
  8. Large ultra-stable telescope system study
  9. Nautilus Observatory: a space telescope array based on very large aperture ultralight diffractive optical elements
  10. The Origins Space Telescope
  11. Twenty years of Chandra operations: telescope thermal performance and application of lessons learned to the Lynx mission
  12. A Thousand Earths: A Very Large Aperture, Ultralight Space Telescope Array for Atmospheric Biosignature Surveys
  13. Lynx X-Ray Observatory: an overview
  14. Formulation of the production time and cost of the Lynx x-ray mirror assembly based on queuing theory
  15. Special Section Guest Editorial: Laser Damage IV
  16. Optics technology for large-aperture space telescopes: from fabrication to final acceptance tests
  17. The Origins Space Telescope: mission concept overview
  18. Breaking the cost curve: applying lessons learned from the James Webb space telescope development
  19. Stray light overview for the Origins Space telescope
  20. The Lynx X-ray Observatory: concept study overview and status
  21. U.S. National Committee proposed revision to the ISO Laser Damage Standard
  22. A method for the determination of defect density from standard damage frequency measurements
  23. An empirical investigation of the laser survivability curve: VIII-summary
  24. Uncertainty on areal defect density measurements
  25. SYNERGY: an Explorer mission concept for a next-generation ultraviolet survey
  26. A semi-empirical method for the prediction of molecular contaminant film accumulation (Conference Presentation)
  27. A performance budget for the x-ray surveyor telescope
  28. Status of the JWST sunshield and spacecraft
  29. Radiance from an ice contaminated surface
  30. Ensuring the enduring viability of the space science enterprise: new questions, new thinking, new paradigms
  31. End-to-end assessment of a large aperture segmented ultraviolet optical infrared (UVOIR) telescope architecture
  32. Laser damage threshold: useful idea or dangerous misconception?
  33. They never told me about this in engineering school: lessons from the front line
  34. Sensitivity test method for the characterization of laser damage behavior
  35. Statistics of Laser Damage Threshold Measurements
  36. A maximum likelihood method for the measurement of laser damage behavior
  37. An empirical investigation of the laser survivability curve: V
  38. Analysis of the laser damage characteristics of a production lot
  39. Contamination control requirements implementation for the James Webb Space Telescope (JWST), part 1: optics, instruments and thermal vacuum testing
  40. Stray light performance for the James Webb Space Telescope
  41. Determination of emissivities of key thermo-optical surfaces on the James Webb Space Telescope
  42. A new paradigm for space astrophysics mission design
  43. Lessons we learned designing and building the Chandra telescope
  44. An empirical investigation of the laser survivability curve: IV
  45. Laser damage threshold measurements via maximum likelihood estimation
  46. Direct comparision of the damage frequency method and binary search technique
  47. An empirical investigation of the laser survivability curve: III
  48. Improving laser damage threshold measurements: an explosive analogy
  49. An empirical investigation of the laser survivability curve: II
  50. S on 1 testing of AR and HR designs at 1064nm
  51. An empirical investigation of the laser survivability curve
  52. Systems engineering on the James Webb Space Telescope
  53. Life testing for laser optics: a first look
  54. Starshade scaling relations
  55. Calculation of error bars for laser damage observations
  56. The effect of pseudo-accumulation in the measurement of fatigue laser-induced damage threshold
  57. Contamination effects and requirements derivation for the James Webb Space Telescope
  58. Deployment technologies for terrestrial planet finding missions
  59. Architecting a revised optical test approach for JWST
  60. Design status of the James Webb Space Telescope
  61. New Worlds Observer system architecture
  62. Sensitivity analysis of the New Worlds starshade's shadow
  63. Toward a sustainable next generation x-ray observatory
  64. Verification, validation, and testing the New Worlds Observer: first thoughts
  65. Measurement of large cryogenic structures using a spatially phase-shifted digital speckle pattern interferometer
  66. The relationship between laser fluence profile and the cumulative probability of damage curve
  67. Effects of ice on the transmission of the James Webb Space Telescope
  68. Effects of scattered light on the performance of the New Worlds Starshade
  69. Measurement of structural damping in the backplane of the James Webb Space Telescope
  70. New Worlds Observer tolerance overview
  71. New Worlds Observer: system architecture for terrestrial planet finding
  72. Technology demonstration of large stable cryogenic composite structures for JWST
  73. External occulters for direct observation of exoplanets: an overview
  74. Optical performance of the New Worlds Occulter
  75. A mechanism for erosion of optics exposed to a laser-generated EUV plasma
  76. Architectures for space astronomical telescopes using Fresnel optics
  77. New Worlds Occulter performance: a first look
  78. The JWST backplane stability test article: a critical technology demonstration
  79. The New Worlds Observer: using occulters to directly observe planets
  80. A revised method for the fitting function in the damage frequency method
  81. Benefits from a change in the fitting function in the damage frequency method
  82. Direct comparision of the damage frequency method and binary search technique
  83. New Worlds Observer: A Novel Mission Concept for Exoplanetary Studies
  84. Towards an Optimal Observation Strategy for Direct Detection Exoplanet Searches
  85. Applications of Fresnel optics to enable new space-based astronomy
  86. Direct studies of exo-planets with the New Worlds Observer
  87. Feasibility studies of laser desorption to study surfaces of Jupiter's icy moons
  88. Image quality budget for the Generation-X Telescope
  89. SAFIR architecture concept
  90. An intermodule alignment budget for the Generation-X Telescope
  91. A 12-m Telescope Concept for SAFIR
  92. A System Feasibility Study for Satellite Based Laser Doppler Seismometry
  93. Feasibility Study of Laser Desorption to Study Surfaces of Jupiter's Icy Moons
  94. MISSE Next: In Space Testing of Optics, A Vital Engineering Research Need
  95. Calculation of the electric field magnitude at total internal reflection surfaces
  96. Interpretation of the result of a laser damage measurement
  97. Accuracy and repeatability of laser damage threshold measurements made via order statistics
  98. Calculation of electric field intensity at dielectric interfaces (Abstract Only)
  99. Characterization of particulate contamination of optics
  100. Tunable Cr:ZnSe Laser for HF Laser Diagnostics
  101. Tunable solid state laser for HF mirror metrology
  102. Calculation of relative damage thresholds for coated or contaminated total internal reflection surfaces
  103. Measurement of relative damage thresholds at total internal reflection surfaces
  104. Use of order statistics in the determination of laser damage threshold
  105. Plans for ensuring survival of SBL optics in the low earth orbit environment
  106. Uncooled resonator technology
  107. Calculation of relative damage thresholds for total internal reflection surfaces
  108. Extrapolation of the probability of survival of a large-area optic based on a small sample
  109. Error analysis of ISO 11551
  110. National round-robin test on laser induced damage at 1.064 μm: revised data reduction and correlation analysis
  111. Area budgeting in the damage frequency method
  112. Error sources in the damage frequency method
  113. Absolute calibration of the AXAF telescope effective area
  114. Comparison of the damage frequency method and the binary search technique
  115. Spatial fluence profile for certification test of laser damage resistance: call for comments
  116. Accuracy and precision of laser damage measurements made via binary search techniques
  117. Design of a certification test for laser damage resistance
  118. Uncertainty in damage-frequency threshold measurements
  119. Calculation of uncertainty in laser-damage thresholds determined by use of the damage-frequency method
  120. Determination of minimal test sample size for high-accuracy laser damage testing
  121. Monte-Carlo-based calculation of measurement quality for three variants of the damage frequency method
  122. Requirements for the detection of damage events and measurement of laser fluence for high-quality damage threshold measurements
  123. Revised damage frequency method for the determination of laser damage threshold
  124. Investigation of the accuracy and precision of the damage-frequency method of measuring laser damage threshold
  125. Motion detection system for AXAF x-ray ground testing
  126. Correlating laser damage tests
  127. Temporary laser damage threshold enhancement by laser conditioning of antireflection‐coated glass
  128. A Set of Standard Definitions for Laser Damage Parameters and Procedures
  129. Production Oriented Laser Damage Testing at Hughes Aircraft Company
  130. A Sensor for Production Oriented Damage Testing at 1.06μm
  131. On the Role of Water in the Laser Conditioning Effect
  132. Architectures for Space Astronomical Telescopes Using Fresnel Optics