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 Database: CHANNSGPSC
   Chandra Nearby Spiral Galaxies Point Source Catalog
Database Index | Basic Search | Advanced Search
 Name Resolver
Name:

 Search Co-ordinates
Co-ords:

Co-ordinate system:
Equatorial Ecliptic Galactic
Equinox: 1950 2000

 Search Type
Cone search, radius: arcmin.
Square search, width: arcmin.
Rectangle search, size: arcmin
 Output Options
 Output coordinates in:
Decimal  Sexagesimal
 Output system:
Equatorial   Ecliptic   Galactic
 Output epoch:
J2000   B1950
 Output format:
Filter Search  
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Parameter
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Definition
 
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<- Sort by distance from search centre (default)
 GALAXY_NAME 
Galaxy Designation
 NAME 
Source identification
 RA 
Right Ascension
 DECL 
Declination
 LII 
Galactic Longitude
 BII 
Galactic Latitude
 SB_COUNTS_1 
First Observation 0.3-1.0 keV Counts
 SB_COUNTS_1_ERROR 
Error in First Observation 0.3-1.0 keV Counts
 SB_COUNTS_1_FLAG 
Flag on First Observation 0.3-1.0 keV Counts
 MB_COUNTS_1 
First Observation 1.0-2.0 keV Counts
 MB_COUNTS_1_ERROR 
Error in First Observation 1.0-2.0 keV Counts
 MB_COUNTS_1_FLAG 
Flag on First Observation 1.0-2.0 keV Counts
 HB_COUNTS_1 
First Observation 2.0-8.0 keV Counts
 HB_COUNTS_1_ERROR 
Error in First Observation 2.0-8.0 keV Counts
 HB_COUNTS_1_FLAG 
Flag on First Observation 2.0-8.0 keV Counts
 FB_COUNTS_1 
First Observation 0.3-8.0 keV Counts
 FB_COUNTS_1_ERROR 
Error in First Observation 0.3-8.0 keV Counts
 FB_COUNTS_1_FLAG 
Flag on First Observation 0.3-8.0 keV Counts
 SB_COUNTS_2 
Second Observation 0.3-1.0 keV Counts
 SB_COUNTS_2_ERROR 
Error in Second Observation 0.3-1.0 keV Counts
 SB_COUNTS_2_FLAG 
Flag on Second Observation 0.3-1.0 keV Counts
 MB_COUNTS_2 
Second Observation 1.0-2.0 keV Counts
 MB_COUNTS_2_ERROR 
Error in Second Observation 1.0-2.0 keV Counts
 MB_COUNTS_2_FLAG 
Flag on Second Observation 1.0-2.0 keV Counts
 HB_COUNTS_2 
Second Observation 2.0-8.0 keV Counts
 HB_COUNTS_2_ERROR 
Error in Second Observation 2.0-8.0 keV Counts
 HB_COUNTS_2_FLAG 
Flag on Second Observation 2.0-8.0 keV Counts
 FB_COUNTS_2 
Second Observation 0.3-8.0 keV Counts
 FB_COUNTS_2_ERROR 
Error in Second Observation 0.3-8.0 keV Counts
 FB_COUNTS_2_FLAG 
Flag on Second Observation 0.3-8.0 keV Counts
 SOFT_COLOR_1 
First Observation Soft Color
 SOFT_COLOR_1_POS_ERR 
Upper Limit Error for First Observation Soft Color
 SOFT_COLOR_1_NEG_ERR 
Lower Limit Error for First Observation Soft Color
 HARD_COLOR_1 
First Observation Hard Color
 HARD_COLOR_1_POS_ERR 
Upper Limit Error for First Observation Hard Color
 HARD_COLOR_1_NEG_ERR 
Lower Limit Error for First Observation Hard Color
 SOFT_COLOR_2 
Second Observation Soft Color
 SOFT_COLOR_2_POS_ERR 
Upper Limit Error for Second Observation Soft Color
 SOFT_COLOR_2_NEG_ERR 
Lower Limit Error for Second Observation Soft Color
 HARD_COLOR_2 
Second Observation Hard Color
 HARD_COLOR_2_POS_ERR 
Upper Limit Error for Second Observation Hard Color
 HARD_COLOR_2_NEG_ERR 
Lower Limit Error for Second Observation Hard Color
 FLUX_1 
First Observation 0.3-8.0 keV Power Law Flux (erg/s/cm^2)
 FLUX_1_ERROR 
Error in First Observation 0.3-8.0 keV Power Law Flux (erg/s/cm^2)
 FLUX_1_FLAG 
Flag on First Observation 0.3-8.0 keV Power Law Flux
 LX_1 
First Observation 0.3-8.0 keV Power Law Luminosity (erg/s)
 LX_1_ERROR 
Error in First Observation 0.3-8.0 keV Power Law Luminosity (erg/s)
 LX_1_FLAG 
Flag on First Observation 0.3-8.0 keV Power Law Luminosity
 FLUX_2 
Second Observation 0.3-8.0 keV Power Law Flux (erg/s/cm^2)
 FLUX_2_ERROR 
Error in Second Observation 0.3-8.0 keV Power Law Flux (erg/s/cm^2)
 FLUX_2_FLAG 
Flag for Second Observation 0.3-8.0 keV Power Law Flux
 LX_2 
Second Observation 0.3-8.0 keV Power Law Luminosity (erg/s)
 LX_2_ERROR 
Error in Second Observation 0.3-8.0 keV Power Law Luminosity (erg/s)
 LX_2_FLAG 
Flag for Second Observation 0.3-8.0 keV Power Law Luminosity
 VARIABILITY_FLAG 
Flag Indicates Variability
 NOTES 
Additional Notes Alternate Source Names from Literature CCD (If Not S3)

 Output number of lines:  
If you have any problems, please consult the help page or mail ledas-help@star.le.ac.uk
 
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