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 rmf | 1 | X101755.81+015502.8 | chandra | ccd7 | 272.476 | 314.255 | 126.249 | 11.4077 | 0.0127478 | 0.00115188 | 112.655 | 1 | 0.63122 | 0.63122 | 0 | 2.6936 | F | F | 3.93e+20 | 8.64694e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X101709.23+015420.7 | chandra | ccd2 | 226.184 | 932.202 | 50.5465 | 7.54989 | 0.00510545 | 0.000762577 | 64.6356 | 1 | 2.42341 | 2.26294 | 103.277 | 8.99853 | F | F | 3.87e+20 | 6.83506e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X101739.39+015413.3 | chandra | ccd7 | 772.671 | 213.571 | 22.4766 | 4.74095 | 0.00226955 | 0.000478713 | 20.0565 | 1 | 0.487519 | 0.487519 | 0 | 1.49069 | F | F | 3.91e+20 | 1.69845e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X101742.11+015446.6 | chandra | ccd7 | 689.945 | 281.35 | 15.6539 | 4.00684 | 0.00158064 | 0.000404588 | 13.9684 | 1 | 0.443946 | 0.443946 | 0 | 0.822815 | F | F | 3.91e+20 | 1.17169e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X101739.73+015708.8 | chandra | ccd7 | 762.48 | 570.302 | 15.0066 | 3.96752 | 0.00151528 | 0.000400617 | 13.3908 | 1 | 0.700785 | 0.302149 | 158.154 | 2.96982 | F | F | 3.9e+20 | 1.22936e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X101800.84+015647.1 | chandra | ccd7 | 119.32 | 526.285 | 28.362 | 5.3256 | 0.00286382 | 0.000537746 | 25.3082 | 1 | 1.69978 | 0.859489 | 113.826 | 4.50925 | F | F | 3.92e+20 | 2.65583e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X101746.09+014605.2 | chandra | ccd6 | 439.115 | 241.039 | 10.5649 | 3.60559 | 0.00106677 | 0.000364069 | 13.0293 | 1 | 3.10381 | 1.80927 | 143.515 | 8.43196 | A | F | 3.95e+20 | 1.28547e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 4 | X101745.60+015645.8 | chandra | ccd7 | 582.944 | 523.056 | 8.14247 | 3.00002 | 0.000822174 | 0.000302922 | 7.26575 | 0.999999 | 0.808226 | 0.492 | 80.6143 | 2.24908 | A | F | 3.91e+20 | 6.16283e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X101753.54+015256.8 | chandra | ccd7 | 341.25 | 57.5 | 3.77584 | 2.00001 | 0.00038126 | 0.000201948 | 3.36928 | 0.998119 | 0.492 | 0.492 | 90 | 2.60025 | F | F | 3.93e+20 | 2.95246e-15 | 1 | dx | ||||
| Report | 7 | X101731.80+015403.5 | chandra | ccd7 | 1003.5 | 193.167 | 2.79192 | 1.73206 | 0.00028191 | 0.000174892 | 2.4913 | 0.990703 | 0.54799 | 0.492 | 123.019 | 3.38897 | F | F | 3.91e+20 | 0 | 1 | d |
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