The JPL Open Repository (JOR) replaced the JPL Technical Report Server (TRS) in 2023. It is a repository for digital copies of technical publications authored by JPL employees. It includes journal articles (the Final Accepted Version), meeting papers, presentations, and other publications cleared for external distribution from 1992 to the present. It also include research datasets from 2022 on.

Years covered: 1992 to the present.
  • 1992-2021 records were originally on the JPL Technical Report Server (TRS) on Dspace system; those records were migrated to Dataverse in 2022.
  • Records with publication date 2022 or later are native to the Dataverse.
  • Data sets: 2022 to present
  • There are a few pre-1992 records. Those were added to the system on a case-by-case request basis.

  • Persistent IDs (PIDs):
  • 1992-2021 records have Handles
  • 2022 and later records have Digital Object Identifiers (DOIs).
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    41,871 to 41,880 of 41,976 Results
    X-ray synchronization emitting Fe-rich ejecta in SNR RCW 86
    Jan 1, 2002
    Rho, J.; Dyer, K. K.; Borkowski, K. J.; Reynolds, S. P., 2002, "X-ray synchronization emitting Fe-rich ejecta in SNR RCW 86", https://hdl.handle.net/2014/9653, Astrophysical journal, JPL Open Repository
    Supernova remnants may exhibit both thermal and nonthermal X-ray emission. In a previous study with ASCA data, we found that the middle-aged supernova remnant RCW 86 showed evidence for both processes, and predicted that observations with much higher spatial resolution would dist...
    X-Ray: A potentially destructive “non-destructive evaluation” technique
    Nov 11, 2019
    Ross, Ryan; Garteiz, Gil; Zajac, Stephanie, 2019, "X-Ray: A potentially destructive “non-destructive evaluation” technique", https://hdl.handle.net/2014/51378, International Symposium for Testing and Failure Analysis (ISTFA), Portland, Oregon, November 11-13, 2019, JPL Open Repository
    No abstract provided
    X-rays and protostars in the Trifid Nebula
    Jun 3, 2001
    Rho, J.; Corcoran, M. F.; Chu, Y.-H.; Reach, W. T., 2001, "X-rays and protostars in the Trifid Nebula", https://hdl.handle.net/2014/12647, ['AAS 198th Meeting', 'Pasadena, CA, USA'], JPL Open Repository
    No abstract provided
    X-rays from Cepheus A East and West
    Jun 10, 2005
    Pravdo, Steven H.; Tsuboi, Yohko, 2005, "X-rays from Cepheus A East and West", https://hdl.handle.net/2014/39291, The Astrophysical Journal, 626:272–282, 2005 June 10, DOI: 10.1086/429988, JPL Open Repository
    We report the discovery of X-rays from both components of Cepheus A, East and West, with the XMM-Newton observatory. HH 168 joins the ranks of other energetic Herbig-Haro objects that are sources of T ≥ 10(6) K X-ray emission. The effective temperature of HH 168 is T = 5.8(-2....
    X-rays from HH 80, HH 81, and the Central Region
    Apr 1, 2004
    Maeda, Y.; Tsuboi, Y.; Pravdo, S. H., 2004, "X-rays from HH 80, HH 81, and the Central Region", https://hdl.handle.net/2014/37349, Astrophysical journal, vol.605, pp.259-271, JPL Open Repository
    We report detections of X-rays from HH 80 and HH 81 with the ACIS instrument on the Chandra X-Ray Observatory.
    X/Ka (8.4/32 GHz) celestial frame: potential for collaboration with Usuda
    Jan 24, 2018
    Jacobs, Christopher S.; Garcia-Miro, C.; Horiuchi, S.; Mercolino, M.; Snedekar, L., 2018, "X/Ka (8.4/32 GHz) celestial frame: potential for collaboration with Usuda", https://hdl.handle.net/2014/48996, XKa Collaboration, Pasadena, California, January 24, 2018, JPL Open Repository
    No abstract provided
    X/Ka (8.4/32 GHz) Celestial Frame: Roadmap to the future
    Oct 7, 2019
    Jacobs, Christopher S.; Soriano, M.; Samoska, L.; Kooi, Jacob; Bowen, James; Fung, Andy; Manthena, Raju; Lazio, J.; Firre, Daniel; Dugast, Michel; De Vicente, Javier; Murata, Yasa; Takeuchi, H., 2019, "X/Ka (8.4/32 GHz) Celestial Frame: Roadmap to the future", https://hdl.handle.net/2014/51853, Journeés 2019: Astrometry, Earth Rotation and Reference Systems in the Gaia Era, Paris, France, October 7-9, 2019, JPL Open Repository
    No abstract provided
    X/Ka component of the proposed ICRF-3: the importance of correlations
    Jun 3, 2018
    Jacobs, Christopher S.; Garcia-Miro, C.; Horiuchi, S.; Snedekar, L.; Clark, J.E.; Mercolino, M.; Sotuela, I.; White, L.A., 2018, "X/Ka component of the proposed ICRF-3: the importance of correlations", https://hdl.handle.net/2014/49853, Tenth IVS General Meeting, Longyearbyen, Norway, June 3-9, 2018, JPL Open Repository
    No abstract provided
    X/Ka Network Enhanced by Misasa, Japan’s 54-meter antenna
    Mar 15, 2021
    Jacobs, Christopher S; Murata, Y.; Takeuchi, H.; Horiuchi, S.; Firre, D.; Asmar, S.; Uchimura, T.; Numata, K., 2021, "X/Ka Network Enhanced by Misasa, Japan’s 54-meter antenna", https://hdl.handle.net/2014/54671, EVGA 2021, Pasadena, California, March 15-18, 2021, JPL Open Repository
    No abstract provided
    X/Ka-Band Dual Frequency Horn Design
    Jun 19, 1994
    Chen, Jacqueline C.; Stanton, Philip H., 1994, "X/Ka-Band Dual Frequency Horn Design", https://hdl.handle.net/2014/36302, Seattle, Washington, USA, JPL Open Repository
    The Deep Space Network has a need for a dual frequency horn for simulation dual frequency operation in a beam waveguide antenna. The dual frequency horn will receive X-band (8.4-8.5 GHz), KABLE frequency (33.6-33.8 GHz), and DSN Ka-band downlink (31.8-32.3 GHz) signals simultaneo...
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