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 | 5 | X062228.21+375256.8 | chandra | ccd3 | 892.428 | 532.527 | 20.6598 | 4.54531 | 0.010191 | 0.00224209 | 48.6313 | 1 | 0.603651 | 0.603651 | 0 | 3.15182 | F | F | 2.01e+21 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 1 | X062230.72+375327.4 | chandra | ccd3 | 832.092 | 594.781 | 10.3397 | 3.21554 | 0.00510034 | 0.00158615 | 24.3387 | 1 | 0.75471 | 0.75471 | 0 | 3.84321 | F | F | 2.01e+21 | 6.0638e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X062231.13+375715.1 | chandra | ccd3 | 822.214 | 1057.21 | 6.56287 | 2.64576 | 0.00323727 | 0.00130507 | 15.4484 | 1 | 1.73602 | 0.622468 | 57.2521 | 6.76896 | A | F | 2e+21 | 4.08945e-14 | 1 | dx | ||||
| Report | 2 | X062223.41+375340.7 | chandra | ccd3 | 1007.5 | 621.3 | 4.95183 | 2.23607 | 0.00244259 | 0.00110298 | 11.6562 | 1 | 0.538532 | 0.492 | 65.1823 | 2.93347 | F | F | 2.01e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X062227.27+375449.3 | chandra | ccd3 | 914.75 | 760.75 | 3.94316 | 2 | 0.00194504 | 0.00098654 | 9.28185 | 0.999999 | 0.668187 | 0.492 | 78.1853 | 4.30532 | F | F | 2.01e+21 | 2.30685e-14 | 1 | dx | ||||
| Report | 1 | X062210.46+374909.9 | chandra | ccd2 | 957.167 | 1027.83 | 2.98349 | 1.73205 | 0.0014717 | 0.000854385 | 7.8685 | 0.999984 | 0.492 | 0.492 | 163.155 | 2.30805 | F | F | 2.03e+21 | 0 | 1 | d | |||||
| Report | 2 | X062209.45+374801.9 | chandra | ccd2 | 981.5 | 889.5 | 2.97642 | 1.73205 | 0.0014682 | 0.000854385 | 7.84984 | 0.999984 | 0.492 | 0.492 | 45 | 3.4476 | F | F | 2.04e+21 | 0 | 1 | d | |||||
| Report | 1 | X062219.68+375718.6 | chandra | ccd1 | 104.5 | 691 | 1.87695 | 1.41422 | 0.000925881 | 0.000697619 | 4.78987 | 0.999462 | 0.492 | 0.492 | 90 | 6.06435 | F | F | 2.01e+21 | 0 | 1 | dc | |||||
| Report | srcpi bgdpi arf | 2 | X062219.85+375717.1 | chandra | ccd1 | 100.3 | 688.1 | 4.80383 | 2.23607 | 0.00236968 | 0.00110303 | 12.2591 | 0.999999 | 1.31151 | 0.492 | 113.978 | 6.04683 | A | F | 2.01e+21 | 3.0188e-14 | 1 | dcx |
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