Astrophysics

Submillimeter Wave Astronomy Satellite (SWAS)

Survey Observatory · Competed · Agency-led · Launched on December 6, 1998 · Completed · LCC: $60M/$136M (2025 $)Life-cycle cost: NASA’s reported cost to build, launch, and operate a mission through its prime mission, plus documented partner contributions, in 2025 dollars. Extended missions are not included. Methods · Wikipedia

Scope Active Mission WindowActivePapers published from the first full month after science operations begin through two years after the mission ends. Citations are counted through the third calendar year after each paper appears. For SWAS, papers published February 1, 1999 to August 1, 2006. Methods LifetimeLifetimeEvery tracked publication to date, with every citation to date. For SWAS, papers published from 2000 to November 3, 2026. Methods
Tracked publicationsTracked publications: peer-reviewed papers we found that name the mission or its instruments in their titles, abstracts, or keywords. Papers that used the data without naming it are missed. Methods76
CitationsCitations: every citation these publications have drawn to date. Older missions have had longer to collect them. Methods2,992
Citation indices
h-indexh-index: the largest h such that h papers have at least h citations each. It only grows with time, so older missions score higher. Methods36
g-indexg-index: the largest g for which the g most-cited papers together hold at least g² citations. Like the h-index, but it lets the most-cited papers count for more. Methods52
m-indexm-index: a mission’s h-index divided by the years since its first peer-reviewed paper. It falls every 1 January even when nothing else changes; the figure shown is as of November 3, 2026. It also discounts the long operating life that larger missions paid for. Methods1.3
toritori (total research impact, from SciX): for every paper citing one of the mission’s papers, 1 divided by the citing paper’s reference count times the cited paper’s author count, summed, with self-citations removed. It favors citations from papers with short reference lists and from outside the mission’s own authors. Computed over the tracked citation graph, which can be slightly incomplete. Always over every tracked publication to date, whichever scope is chosen. Methods12
riqriq (research impact quotient): 1,000 times the square root of tori, divided by the years since the mission’s first paper. A rate, not a total, so it does not keep growing with age the way the h-index and tori do. Like tori, always over every tracked publication to date. Methods126

Publications and citations by year (lifetime)

Publications per yearCumulative citations

Institutional contributions (lifetime)The institutions SciX lists for each paper’s authors, as printed on the paper, located through the Research Organization Registry. A square counts a paper once, however many of its authors worked there. Methods

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Tracked publications over the lifetime (76)

All publications CSV · JSON

  1. Implications of Submillimeter Wave Astronomy Satellite Observations for Interstellar Chemistry and Star Formation

    Bergin, E. A., 2000, ApJ

    145 lifetime citations

  2. The Submillimeter Wave Astronomy Satellite: Science Objectives and Instrument Description

    Melnick, Gary J., 2000, ApJ

    144 lifetime citations

  3. Water Abundance in Molecular Cloud Cores

    Snell, R. L., 2000, ApJ

    136 lifetime citations

  4. O₂ in Interstellar Molecular Clouds

    Goldsmith, P. F., 2000, ApJ

    118 lifetime citations

  5. Gas-grain chemical models of star-forming molecular clouds as constrained by ISO and SWAS observations

    Charnley, S. B., 2001, A&A

    106 lifetime citations

  6. Low upper limits on the O₂ abundance from the Odin satellite

    Pagani, L., 2003, A&A

    95 lifetime citations

  7. The Origin of Water Vapor and Carbon Dioxide in Jupiter's Stratosphere

    Lellouch, E., 2002, Icar

    91 lifetime citations

  8. Multi-line detection of O₂ toward ρ Ophuichi A

    Liseau, R., 2012, A&A

    91 lifetime citations

  9. Water cooling of shocks in protostellar outflows. Herschel-PACS map of L1157

    Nisini, B., 2010, A&A

    87 lifetime citations

  10. Detection of Water in the Shocked Gas Associated with IC 443: Constraints on Shock Models

    Snell, R. L., 2005, ApJ

    72 lifetime citations

  11. Modeling gas-phase H₂O between 5 μ m and 540 μ m toward massive protostars

    Boonman, A. M. S., 2003, A&A

    61 lifetime citations

  12. The abundance of gaseous H₂O and O₂ in cores of dense interstellar clouds

    Roberts, H., 2002, A&A

    59 lifetime citations

  13. Submillimeter Wave Astronomy Satellite Observations of Extended Water Emission in Orion

    Snell, R. L., 2000, ApJ

    56 lifetime citations

  14. Observations of Water Vapor toward Orion BN/KL

    Melnick, G. J., 2000, ApJ

    54 lifetime citations

  15. Abundant gas-phase H₂O in absorption toward massive protostars

    Boonman, A. M. S., 2003, A&A

    53 lifetime citations

  16. Interstellar oxygen chemistry

    Viti, S., 2001, A&A

    51 lifetime citations

  17. The excitation of water in the S140 photon dominated region

    Poelman, D. R., 2005, A&A

    50 lifetime citations

  18. Large-scale ¹³CO J=5-->4 and [C I] Mapping of Orion A

    Plume, R., 2000, ApJ

    49 lifetime citations

  19. Sensitive Limits on the Water Abundance in Cold Low-Mass Molecular Cores

    Bergin, Edwin A., 2002, ApJ

    49 lifetime citations

  20. Water vapor toward starless cores: The Herschel view

    Caselli, P., 2010, A&A

    47 lifetime citations

How we found these papers

We searched NASA’s Science Explorer (SciX) for peer-reviewed articles naming SWAS in the title, abstract or keywords; standard filters drop articles that are not peer-reviewed and magazine pieces.

((=abs:"Submillimeter Wave Astronomy Satellite" OR (abs:SWAS AND abs:(observation OR submillimeter OR interstellar OR water OR oxygen) AND NOT abs:"southwestern atlantic")) AND collection:astronomy) AND property:refereed AND doctype:article AND pubdate:[1999-02 TO 2040-01] AND NOT bibstem:("A&R" OR "ACPD" OR "AIASJ" OR "AMTD" OR "AeAm" OR "AirSp" OR "AsNow" OR "AsUAI" OR "AvWST" OR "BGD" OR "C&E" OR "C&T" OR "CAPJ" OR "CliPD" OR "E&S" OR "ENews" OR "ESDD" OR "ESSDD" OR "ESuDD" OR "GID" OR "GMDD" OR "GeCAS" OR "HESSD" OR "IrAJ" OR "JCos" OR "JRASC" OR "LAstr" OR "MNSSA" OR "Met" OR "NHESD" OR "NPGD" OR "NewSc" OR "OcScD" OR "Orion" OR "PhT" OR "PhTea" OR "PhuZ" OR "PhyOJ" OR "PhyW" OR "PlR" OR "SOILD" OR "SciAm" OR "SpFl" OR "TCD" OR "ZemVs")

Open in SciX

Removed after review (3)

  1. Far-Infrared and Submillimeter Emission from Galactic and Extragalactic Photodissociation Regions General photodissociation-region model grid; names SWAS only among facilities that may use it. Decision 👨
  2. THz Instruments for Space Review of terahertz instrument technology; names SWAS only among past instruments. Decision 🤖
  3. The PhotoDissociation Region Toolbox: Software and Models for Astrophysical Analysis Software paper listing SWAS among facilities whose data it could analyze; uses no SWAS data. Decision 🤖