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 | 1 | X125008.89+021523.4 | chandra | ccd7 | 486.683 | 947.891 | 25.5365 | 5.50526 | 0.00653928 | 0.00140976 | 18.1817 | 1 | 0.50325 | 0.50325 | 0 | 0.525325 | F | F | 1.73e+20 | 4.88515e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X125000.63+021401.4 | chandra | ccd7 | 738.147 | 781.06 | 20.7854 | 4.73899 | 0.00532264 | 0.00121354 | 14.7989 | 1 | 0.465239 | 0.465239 | 0 | 1.95393 | F | F | 1.73e+20 | 4.00228e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X125001.98+021356.4 | chandra | ccd7 | 697.2 | 770.928 | 15.1039 | 4.06824 | 0.00386776 | 0.00104178 | 10.7538 | 1 | 0.492031 | 0.492031 | 0 | 1.74801 | F | F | 1.73e+20 | 2.90071e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X125000.21+020840.0 | chandra | ccd7 | 750.907 | 127.811 | 17.5578 | 4.1902 | 0.00449612 | 0.00107301 | 12.5009 | 1 | 2.52192 | 1.6444 | 335.807 | 6.70528 | F | F | 1.7e+20 | 3.67214e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X125001.34+021248.7 | chandra | ccd7 | 716.167 | 632.944 | 8.87843 | 3 | 0.00227354 | 0.000768223 | 6.32133 | 0.999993 | 0.492 | 0.492 | 28.155 | 2.73496 | F | F | 1.72e+20 | 1.81131e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X125004.50+022044.1 | chandra | ccd6 | 811.833 | 560.167 | 2.6344 | 1.73206 | 0.000674601 | 0.000443537 | 5.0042 | 0.997114 | 0.7585 | 0.492 | 88.4101 | 5.62099 | A | F | 1.77e+20 | 8.49983e-15 | 1 | dbcx | ||||
| Report | srcpi bgdpi arf | 2 | X125026.08+022020.4 | chandra | ccd6 | 154.5 | 512 | 3.80899 | 2.00001 | 0.000975383 | 0.00051215 | 7.2354 | 0.999989 | 1.28497 | 0.492 | 134.349 | 7.04279 | A | F | 1.76e+20 | 1.33115e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X124959.84+022408.0 | chandra | ccd6 | 953.625 | 974.625 | 7.10039 | 2.82845 | 0.00181823 | 0.000724293 | 13.4876 | 1 | 2.56105 | 1.3582 | 78.7776 | 9.16124 | A | F | 1.8e+20 | 2.47316e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X125004.38+022039.6 | chandra | ccd6 | 815.5 | 551.039 | 12.0774 | 3.60556 | 0.0030927 | 0.000923292 | 22.9417 | 1 | 1.91836 | 0.805013 | 32.8889 | 5.55011 | A | F | 1.77e+20 | 4.13996e-14 | 1 | dcx | ||||
| Report | srcpi bgdpi arf | 5 | X125013.62+021924.3 | chandra | ccd6 | 534 | 398 | 1.95726 | 1.41422 | 0.000501203 | 0.000362144 | 3.71793 | 0.997114 | 0.58344 | 0.492 | 71.565 | 4.56381 | F | F | 1.76e+20 | 5.781e-15 | 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