Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf | 6 | X115136.24+483902.2 | chandra | ccd7 | 776.878 | 45.9556 | 13.7773 | 3.71178 | 0.0030709 | 0.000827338 | 7.3423 | 1 | 0.486587 | 0.486587 | 0 | 2.70734 | F | F | 2.36e+20 | 2.39627e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X115147.33+484101.4 | chandra | ccd7 | 553.434 | 288.085 | 10.2357 | 4.8491 | 0.00228149 | 0.00108084 | 5.45489 | 0.99998 | 0.372358 | 0.372358 | 0 | 0.362814 | F | F | 2.36e+20 | 1.69645e-14 | 1 | dsx | ||||
| Report | 1 | X115153.02+483936.6 | chandra | ccd7 | 438.825 | 115.807 | 12.006 | 3.46896 | 0.00267608 | 0.000773213 | 6.39833 | 0.999999 | 0.472107 | 0.472107 | 0 | 1.3428 | F | F | 2.37e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 3 | X115140.62+484215.7 | chandra | ccd7 | 688.398 | 439.218 | 9.69309 | 3.23593 | 0.00216054 | 0.000721272 | 5.16571 | 0.99998 | 0.305159 | 0.305159 | 0 | 2.02547 | F | F | 2.36e+20 | 1.61629e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X115147.65+484426.3 | chandra | ccd7 | 546.5 | 704 | 7.772 | 2.82843 | 0.00173232 | 0.000630437 | 4.14191 | 0.999695 | 0.680541 | 0.492 | 16.845 | 3.67909 | F | F | 2.36e+20 | 1.32926e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X115212.89+483728.6 | chandra | ccd6 | 193.833 | 881.333 | 5.79845 | 2.44949 | 0.00129243 | 0.000545975 | 9.72491 | 1 | 0.708664 | 0.492 | 105.527 | 5.1533 | F | F | 2.38e+20 | 1.65367e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X115151.88+483411.9 | chandra | ccd6 | 617.167 | 481.333 | 5.60926 | 2.4495 | 0.00125026 | 0.000545976 | 9.40762 | 0.999998 | 1.1874 | 0.904342 | 69.1832 | 6.58439 | F | F | 2.37e+20 | 1.80617e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X115133.47+483210.3 | chandra | ccd6 | 988.944 | 234.278 | 7.48478 | 3.00003 | 0.0016683 | 0.000668686 | 12.5532 | 1 | 3.08881 | 1.48189 | 147.467 | 8.9617 | A | F | 2.36e+20 | 2.28414e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X115142.96+483655.1 | chandra | ccd6 | 797.125 | 813.125 | 7.81621 | 2.82843 | 0.00174218 | 0.000630437 | 13.109 | 1 | 0.999475 | 0.492 | 121.247 | 3.96692 | A | F | 2.37e+20 | 1.95413e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X115210.64+484315.4 | chandra | ccd7 | 84.1001 | 560.3 | 4.73485 | 2.23608 | 0.00105536 | 0.000498406 | 2.52333 | 0.989768 | 0.571652 | 0.492 | 161.565 | 4.37264 | F | F | 2.37e+20 | 1.38193e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X115138.97+483450.9 | chandra | ccd6 | 877.7 | 560.7 | 4.58526 | 2.23608 | 0.00102202 | 0.000498406 | 7.6902 | 0.999965 | 1.25584 | 0.610486 | 147.008 | 6.13716 | A | F | 2.37e+20 | 1.20599e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X115216.35+483643.2 | chandra | ccd6 | 124.1 | 789.3 | 4.65588 | 2.23608 | 0.00103776 | 0.000498406 | 7.80864 | 0.999998 | 0.959976 | 0.525987 | 142.84 | 6.07884 | A | F | 2.38e+20 | 1.37689e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X115132.94+483539.1 | chandra | ccd6 | 999.25 | 658.75 | 3.81755 | 2.00001 | 0.000850904 | 0.000445787 | 6.40262 | 0.999965 | 0.492 | 0.492 | 45 | 5.74961 | F | F | 2.37e+20 | 1.02947e-14 | 1 | dx |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest