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 | 1 | X111814.65+570542.7 | chandra | ccd3 | 1006.44 | 520.734 | 47.3497 | 6.89057 | 0.0100561 | 0.00146342 | 81.3305 | 1 | 0.683207 | 0.409871 | 151.593 | 3.45398 | F | F | 7.22e+19 | 0 | 1 | ds | |||||
| Report | 1 | X111714.23+570818.9 | chandra | ccd1 | 973.447 | 748.447 | 16.5487 | 4.35893 | 0.0035146 | 0.000925746 | 28.4806 | 1 | 3.37657 | 1.34107 | 12.8216 | 10.0045 | A | F | 7.12e+19 | 0 | 1 | d | |||||
| Report | 4 | X111812.35+565854.7 | chandra | ccd2 | 961 | 723.9 | 9.90362 | 3.16228 | 0.00210332 | 0.000671602 | 16.8694 | 1 | 0.647629 | 0.492 | 82.3392 | 3.35543 | F | F | 7.23e+19 | 0 | 1 | d | |||||
| Report | 3 | X111811.56+570316.0 | chandra | ccd3 | 1057.21 | 222.071 | 6.94806 | 2.64575 | 0.00147562 | 0.000561902 | 11.9344 | 1 | 0.492 | 0.492 | 151.512 | 1.01742 | F | F | 7.21e+19 | 0 | 1 | d | |||||
| Report | 1 | X111739.94+570033.9 | chandra | ccd0 | 440.071 | 823.214 | 6.84643 | 2.64575 | 0.00145404 | 0.000561903 | 12.051 | 1 | 0.697893 | 0.523771 | 54.9276 | 4.79575 | F | F | 7.2e+19 | 0 | 1 | d | |||||
| Report | 2 | X111752.15+570353.5 | chandra | ccd1 | 346.9 | 207.5 | 4.94034 | 2.23607 | 0.00104922 | 0.000474894 | 8.50241 | 0.999998 | 0.492 | 0.492 | 36.6504 | 3.25602 | F | F | 7.19e+19 | 0 | 1 | d | |||||
| Report | 1 | X111854.57+565818.6 | chandra | ccd2 | 259.5 | 651.5 | 4.70458 | 2.23608 | 0.000999154 | 0.000474896 | 8.01356 | 0.999998 | 0.974413 | 0.492 | 113.863 | 6.91624 | A | F | 7.27e+19 | 0 | 1 | d | |||||
| Report | 4 | X111740.02+570336.3 | chandra | ccd1 | 548 | 172.75 | 3.94402 | 2 | 0.000837626 | 0.000424758 | 6.78772 | 0.999972 | 0.492 | 0.492 | 17.6088 | 4.66636 | F | F | 7.18e+19 | 0 | 1 | d | |||||
| Report | 2 | X111742.51+565812.9 | chandra | ccd0 | 398 | 536.5 | 3.93422 | 2 | 0.000835546 | 0.000424758 | 6.92495 | 0.999978 | 0.492 | 0.492 | 16.845 | 5.78996 | F | F | 7.21e+19 | 0 | 1 | d | |||||
| Report | 3 | X111833.66+570129.0 | chandra | ccd2 | 607.5 | 1037.75 | 3.9181 | 2 | 0.000832121 | 0.000424758 | 6.67389 | 0.99997 | 0.492 | 0.492 | 90 | 2.93089 | F | F | 7.25e+19 | 0 | 1 | d | |||||
| Report | 3 | X111804.65+565955.7 | chandra | ccd0 | 30 | 745 | 3.91743 | 2 | 0.000831979 | 0.000424759 | 6.89539 | 0.999978 | 0.492 | 0.492 | 2.35031e-08 | 2.59299 | F | F | 7.22e+19 | 0 | 1 | d | |||||
| Report | 4 | X111759.73+565852.5 | chandra | ccd0 | 111.75 | 616.5 | 3.94573 | 2 | 0.00083799 | 0.000424758 | 6.94521 | 0.999978 | 0.492 | 0.492 | 90 | 3.83593 | F | F | 7.22e+19 | 0 | 1 | d | |||||
| Report | 2 | X111850.89+565835.4 | chandra | ccd2 | 320.75 | 685.5 | 3.86711 | 2 | 0.000821293 | 0.000424759 | 6.58705 | 0.99997 | 0.50335 | 0.492 | 34.722 | 6.34498 | F | F | 7.27e+19 | 0 | 1 | d | |||||
| Report | 2 | X111843.37+570333.5 | chandra | ccd3 | 529.833 | 258.167 | 2.95299 | 1.73205 | 0.000627153 | 0.000367851 | 5.07222 | 0.99958 | 0.771213 | 0.492 | 79.3747 | 4.34066 | A | F | 7.27e+19 | 0 | 1 | d | |||||
| Report | 3 | X111741.46+570507.5 | chandra | ccd1 | 523.833 | 358.167 | 2.94665 | 1.73205 | 0.000625806 | 0.000367851 | 5.07123 | 0.999586 | 0.492 | 0.492 | 4.73116 | 5.14176 | F | F | 7.18e+19 | 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