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0.25deg bin images15 Monoceros30Dor OVI-Xray
30Dor log N(O VI) - Xray correlation30 Doradus5 frames
ASCC57.jpg
AchernarAirglow & Zodiacal LightAll sky
Answers to referee comments
Background information for LMCBad NUV VisitBell 2002
Bubble NebulaCD TestCSV table
C progC programCalculating flux units
Calculation of ra,decCarbon measurements in the ISMCarbon measurements in the interstellar medium
Carbon paperCelestial to eclipticChapter3: Bubble Nebula
Chi squareCole et al 1999Commands for PV Phase
Conversion of UIT fluxes to photon unitsCoordinate Converter HelpCoordinates Transformations
Correlation plots of UIT combined filter flux with all FUSE bands.Correlation plots of all UIT combined filter flux with all FUSE bands.Count Rate Limits
Create Image ModuleCreate Image TestD0880103000
D2BpaperDR1Data Archive
Data File FormatsDerivationsDetailed Registration Notes
Developer ActivitiesDevelopers removed
Diffuse UV BackgroundDimensions of Spacecraft and Solar PanelDiscussion with Israel
Distortion coeftsDocumentation of Simulation Program
Draco NebulaDraine's CalculationsDust properties from D2B data
ELAISS1 Individual CorrelationsETC HelpEclipse for Geostationary Satellite
Eclipse for Geostationary Satellite 2009Equatorial Catalog 1Estimation of FUV flux from Far-IR emission
Eta CarinaeExtension HeaderExtinction Work
Extinction mapping through broad band photometryFSSFUSE - FUSE
FUSE - FUSE CorrelationsFUSE - IR correlationsFUSE Bands
FUSE LMC paper1 figuresFUSE UIT CorrelationsFUSE files
FUSE pointings on UIT dataFUSE with IRASFUSE with UIT
FUV-NUV RATIOFUV-NUV RatioFUV and NUV correlations
Fig. 8Fig 3c &3dFigure 1
Figure 10Figure 11Figure 11.
Figure 12Figure 12.Figure 13
Figure 13.Figure 14Figure 15
Figure 16Figure 2Figure 3.
Figure 4Figure 4.Figure 5
Figure 5.Figure 6Figure 6.
Figure 7Figure 8Figure 8.
Figure 9Figure 9.Finding variable sources in TAUVEX
FirstLMCpaperFits Header ContentsFlux Calculator Documentation
Flux Calculator HelpFlux Calculator Test CasesGALEX
GALEX PIIGALEX PIIIGALEX PII PARTB
GALEX PII PaperGALEX PIVGALEX Statistics
GI1-005001GI1-TARGET 1
Geometric Distortion TestGetting started with Web ApplicationH-alpha image of the LMC showing distribution of N(OVI)
HD 148937HereHow to determine CD matrix
IAU Commission 21IR-UV correlation without ridgeIRAS
IRAS, visible and UITIRAS with UITIRIS 100 micron map
IR CheckIR Modelling of CoalsackIR and UV correlations
IR derivationISRF Variation in the RegionImage Registration Algorithm
Important relationsInput Data SimulationInstalling the Pipeline
Interstellar bubblesInterstellar medium
Issues to be discussed with ISACJM's Independent Pipeline Test
Kennicutt-Schmidt RelationKim et al 1998LMC
LMC-IILMC BarLMC NEW DATA.csv
LMC PaperLMC Paper IILMC References
LMC WestLMC missing valuesLMC paper
LSSLSS Action planLSS Points to remember
LSS RequirementsLeast SquaresLevel0 Handling
Level 0 DataLinkLink to tables containing the FUSE diffuse fraction for each individual bands
LmcLocal Interstellar MediumLog N(O VI) versus distance from the centre of 30 Doradus
Log N(O VI) versus log relative H-alpha surface brightnessLog N(O VI) versus log relative X-ray surface brightnessMain Page
Main Page/Mapping the Diffuse Ultraviolet Sky with GALEXMission Planning for the Performance Verification Phase
MissionsModelling of FUV scattering towards Eta carinae
Modelling progressModelling resultsMolecular hydrogen
More details hereN(H) with N(HI)N(HI) with FUSE
N11NHI-IRNature of Diffuse UV Background : A Study Using GALEX Observations
Newad2xy.proNon-zero interceptOLD FIGURES
OVI Absorption Profile plots of all the 70 sight linesOVI Absorption Profile plots of all the 71 sight linesObservational Details
Old tableOrigin of the UV BackgroundOther data for 30 Dor
OthersOur GALEX ArchivePII References
PII sky background imagesPV Phase-Appendix APV Phase-Appendix B
PV Phase-Appendix CPV starlistPapers in brief
Parker et al 1998Payload developmentPeople
Performance Verification for TAUVEXPerformance Verification for UVITPhotometric Zero-points
Pipeline CookbookPipeline Data Registration
Pipeline QuestionsPlots for D2B
Possibilities for Ratio IncreasePrimary HeaderProcedure
Procedure of calculation of total stellar flux for Fuse bandsPrograms for Observation PlanningQuicklook software overview
R-band image of the LMC showing Superbubbles and OVI pointingsRead Headers onlyReference
References:Carbon measurementsReporting BugsResearch notes
Running the PipelineSAGE surveySCALE FACTOR FOR FLUX CALIBRATION
SIRTFFL 00SIRTFFL 00 & SIRTFFL 01SIRTFFL 01
SIRTFFL 01 & SIRTFFL 02SIRTFFL 02SIRTFFL 03
SIRTFFL 03 & SIRTFFL 10SIRTFFL 04SIRTFFL 04, SIRTFFL 06 & SIRTFFL 09
SIRTFFL 04, SIRTFFL 09 & SIRTFFL 10SIRTFFL 04 & SIRTFFL 09SIRTFFL 05
SIRTFFL 05 & SIRTFFL 07SIRTFFL 06SIRTFFL 07
SIRTFFL 08SIRTFFL 09SIRTFFL 10
SIR 00 & SIR 01SIR 01 & SIR 02SIR 03 & SIR 10
SIR 04 & SIR 06SIR 04 & SIR 09SIR 04 & SIR 10
SIR 05 & SIR 07SIR 06 & SIR 09SIR 09 & SIR 10
SMCSMC PaperSUN RA DEC
Sandage paper 2007ScienceSee figure
Separation into different visitsShapleySimulation Tests
Simulation of UV SkySky Simulation DocSky Simulation Help
Sky Simulation TestsSoftware
Solar Activity dependence plots hereSources in FOVSpacecraft
Spectra of SMC diffuse observationsSpectra of a regionSpica
Spica Paper FiguresSpread of Sources TestStar Counts from the LMC
StepsForCombine level1StepsForIngest data
Straylight ValuesStudies of Interstellar MediumStudy of Overlap Region from different Observations
Study of Overlap RegionsSwift Diffuse LightSwift Spica observations
Swift common grid.cTAUVEXTAUVEX Action Items
TAUVEX Calibration TechniquesTAUVEX CommandsTAUVEX Data Definitions
TAUVEX Data PipelineTAUVEX Data ReceptionTAUVEX Early Ops
TAUVEX Ground CalibrationTAUVEX and UV TransientsTAUVEX bandpasses and wavelengths
TEC VariationTMCTabl1
TableTable.7Table.8
Table:1Table:2Table:3
Table 11Table 5Table 9
Table fuseTable linkTautime Configuration
Team and ProjectsTelemetry Block
Telemetry and Log FilesTempTest Results of Modules
Test of Calculation of x,y valuesTesting for Event Distribution
The Local Interstellar MediumThe steps involved in UVS ingest data and UVS combine level1 modules.htmlThese files
TogetherUIT With FUSE ObservationUVIT
UVOT CookbookUVOT Data SummaryUVS ingest data
UV observations of Active Galactic NucleiUseful ProgramsUsing CVS
Using the PipelineVNC Configuration
Visits to be checkedVoyager analysisVoyager data
WorkXyresXytest cprog
Zodiacal Light

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