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 | 4 | X115023.59+281907.3 | chandra | ccd7 | 498.742 | 876.667 | 22.5476 | 4.74843 | 0.0146518 | 0.0030856 | 55.0106 | 1 | 0.48935 | 0.48935 | 0 | 0.190301 | 14.9153 | 5 | -0.497874 | 0.313137 | F | F | 1.86e+20 | 1.09691e-13 | 1 | dsx |
| Report | 1 | X115027.97+281954.4 | chandra | ccd7 | 380.5 | 972 | 7.96445 | 2.82843 | 0.00517533 | 0.00183792 | 19.4313 | 1 | 0.492 | 0.492 | 90 | 1.27201 | F | F | 1.86e+20 | 0 | 1 | d | |||||
| Report | 2 | X115021.33+282048.9 | chandra | ccd7 | 558.833 | 1082.67 | 5.97347 | 2.44949 | 0.00388158 | 0.00159169 | 14.5738 | 1 | 0.492 | 0.492 | 14.0362 | 1.59813 | F | F | 1.86e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X115032.87+282354.1 | chandra | ccd6 | 421.25 | 444.25 | 3.94219 | 3.17945 | 0.00256165 | 0.00206602 | 16.3964 | 1 | 0.720987 | 0.492 | 79.2761 | 5.1257 | 4 | -0.0578066 | -1 | 1.14412 | F | F | 1.85e+20 | 2.92947e-14 | 1 | dx |
| Report | 3 | X115023.50+281629.5 | chandra | ccd7 | 500.5 | 555.5 | 2.98543 | 1.73205 | 0.00193994 | 0.00112549 | 7.28372 | 0.999971 | 0.492 | 0.492 | 45 | 2.76971 | F | F | 1.86e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X115034.02+281708.7 | chandra | ccd7 | 218.167 | 635.167 | 2.83061 | 2.93649 | 0.00183934 | 0.00190814 | 6.87766 | 0.99997 | 0.492 | 0.492 | 45 | 3.21786 | 2.91531 | -0.0846933 | -1 | 1.4553 | F | F | 1.86e+20 | 1.45272e-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