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 | X095502.73+170559.5 | chandra | ccd3 | 117.7 | 203.9 | 4.89135 | 2.23607 | 0.0012445 | 0.000568921 | 3.69815 | 0.997803 | 0.492 | 0.492 | 18.4349 | 0.615193 | F | F | 3.13e+20 | 1.27679e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X095439.15+170536.0 | chandra | ccd3 | 805.418 | 156.837 | 29.4444 | 5.42627 | 0.00749153 | 0.0013806 | 22.2617 | 1 | 1.90391 | 0.921526 | 94.1727 | 6.24293 | F | F | 3.14e+20 | 8.78172e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X095452.67+170604.3 | chandra | ccd3 | 410.9 | 213.7 | 4.96052 | 2.23607 | 0.0012621 | 0.00056892 | 3.75045 | 0.997803 | 0.596131 | 0.492 | 151.453 | 2.98662 | F | F | 3.13e+20 | 1.35339e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X095433.46+170639.9 | chandra | ccd3 | 970.5 | 286.333 | 5.71504 | 2.4495 | 0.00145407 | 0.000623223 | 4.32091 | 0.999533 | 1.3806 | 0.492 | 74.8123 | 7.58728 | A | F | 3.14e+20 | 1.78762e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X095504.57+170556.2 | chandra | ccd3 | 64.5545 | 197.586 | 60.6925 | 8.01195 | 0.0154419 | 0.00203847 | 45.8871 | 1 | 0.394363 | 0.394363 | 0 | 0.296815 | F | F | 3.13e+20 | 1.57532e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X095447.98+170615.0 | chandra | ccd3 | 547.5 | 235.5 | 2.98101 | 1.73205 | 0.000758454 | 0.000440684 | 2.25382 | 0.967139 | 0.492 | 0.492 | 90 | 4.10445 | F | F | 3.13e+20 | 8.39924e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X095449.50+170606.1 | chandra | ccd3 | 503.25 | 217.25 | 3.92647 | 2 | 0.000999008 | 0.000508858 | 2.96864 | 0.990881 | 0.492 | 0.492 | 45 | 3.74249 | F | F | 3.13e+20 | 1.08958e-14 | 1 | dx | ||||
| Report | 8 | X095441.37+170537.6 | chandra | ccd3 | 740.25 | 159.5 | 3.97539 | 2 | 0.00101145 | 0.000508858 | 3.00563 | 0.990881 | 0.492 | 0.492 | 180 | 5.71315 | F | F | 3.14e+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