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 rmf | 7 | X211347.39+022835.0 | chandra | ccd3 | 1014.23 | 426.483 | 560.429 | 25.6783 | 0.0560004 | 0.00256588 | 89.9888 | 1 | 1.59336 | 1.59336 | 0 | 6.7249 | F | F | 5.82e+20 | 1.41777e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 6 | X211358.68+022623.2 | chandra | ccd3 | 669.933 | 158.067 | 24.8459 | 5.47728 | 0.0024827 | 0.000547312 | 3.98953 | 0.999872 | 3.0243 | 1.8906 | 40.3121 | 8.96135 | A | F | 5.77e+20 | 3.57415e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X211321.17+023821.9 | chandra | ccd2 | 1137.71 | 832.416 | 32.418 | 6.16133 | 0.00323934 | 0.000615666 | 13.7682 | 1 | 3.45516 | 1.96618 | 316.887 | 8.38468 | F | F | 5.88e+20 | 4.84303e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X211311.77+023305.8 | chandra | ccd6 | 267.049 | 886.015 | 31.6035 | 7.24952 | 0.00315795 | 0.000724402 | 6.90433 | 1 | 6.11391 | 3.68721 | 131.052 | 10.3578 | F | F | 5.96e+20 | 4.48068e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X211415.33+023010.7 | chandra | ccd3 | 162.577 | 620.577 | 11.6986 | 3.60557 | 0.00116897 | 0.000360283 | 1.87845 | 0.965793 | 1.17067 | 0.639127 | 45 | 7.65405 | A | F | 5.68e+20 | 1.52685e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X211355.00+023309.7 | chandra | ccd3 | 782.274 | 984.767 | 11.2534 | 4.09042 | 0.00112448 | 0.00040873 | 1.80697 | 0.965793 | 0.655156 | 0.29126 | 90.1248 | 2.1555 | F | F | 5.76e+20 | 1.36679e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X211349.60+023536.7 | chandra | ccd2 | 271.333 | 496.167 | 11.0224 | 3.46412 | 0.0011014 | 0.000346148 | 4.6813 | 0.999931 | 0.541545 | 0.492 | 133.52 | 0.769686 | F | F | 5.78e+20 | 1.2464e-14 | 1 | dpx | ||||
| Report | srcpi bgdpi arf | 2 | X211346.42+023541.7 | chandra | ccd2 | 368.214 | 506.214 | 6.45248 | 2.64576 | 0.000644758 | 0.000264375 | 2.74043 | 0.988371 | 0.492 | 0.492 | 118.764 | 1.52699 | F | F | 5.79e+20 | 7.39185e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X211326.41+024032.0 | chandra | ccd2 | 977.625 | 1096.38 | 6.32077 | 2.82847 | 0.000631596 | 0.000282631 | 2.68449 | 0.988371 | 1.98161 | 1.37471 | 106.662 | 8.36317 | F | F | 5.85e+20 | 8.84359e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X211419.46+023237.6 | chandra | ccd1 | 830.928 | 280.072 | 6.17518 | 2.64577 | 0.000617048 | 0.000264376 | 5.44539 | 0.99994 | 1.00945 | 0.492 | 122.731 | 7.2771 | A | F | 5.64e+20 | 7.79999e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X211403.72+023557.7 | chandra | ccd1 | 1310.4 | 686.8 | 8.92289 | 3.1623 | 0.00089161 | 0.00031599 | 7.86838 | 1 | 0.714037 | 0.492 | 129.627 | 2.97392 | F | F | 5.7e+20 | 1.04472e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X211332.21+024106.0 | chandra | ccd2 | 800.833 | 1165.33 | 5.38123 | 2.44951 | 0.000537713 | 0.000244764 | 2.28545 | 0.973473 | 1.00924 | 0.492 | 145.278 | 7.72769 | A | F | 5.82e+20 | 7.26161e-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