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 | 1 | X174025.94+100005.9 | chandra | ccd7 | 705.156 | 430.115 | 173.869 | 13.651 | 0.034202 | 0.0026853 | 85.247 | 1 | 0.382314 | 0.382314 | 0 | 0.582407 | F | F | 8.23e+20 | 2.23134e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 1 | X173948.31+100416.4 | chandra | ccd3 | 567.84 | 303.463 | 169.448 | 13.7945 | 0.0333323 | 0.00271353 | 37.1184 | 1 | 4.84253 | 4.00429 | 349.179 | 10.1244 | F | F | 8.22e+20 | 4.16738e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X174034.73+095418.4 | chandra | ccd6 | 94.1434 | 693.924 | 99.3477 | 9.96733 | 0.0195428 | 0.00196069 | 142.838 | 1 | 2.26998 | 1.68985 | 51.5494 | 5.80826 | F | F | 8.22e+20 | 2.08738e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X173953.08+100324.8 | chandra | ccd3 | 424.036 | 198.143 | 24.6649 | 5.29154 | 0.00485185 | 0.0010409 | 5.40297 | 0.999999 | 2.60533 | 1.67009 | 163.689 | 8.68487 | A | F | 8.22e+20 | 5.94822e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X174011.32+095121.9 | chandra | ccd6 | 796.833 | 334.69 | 18.4433 | 4.58261 | 0.003628 | 0.000901449 | 26.517 | 1 | 3.14877 | 1.85859 | 29.0194 | 8.86856 | A | F | 8.19e+20 | 3.87768e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X174025.06+095843.1 | chandra | ccd7 | 731.625 | 261.783 | 12.7447 | 3.56997 | 0.00250702 | 0.000702252 | 6.24865 | 0.999998 | 0.401599 | 0.401599 | 0 | 0.878219 | F | F | 8.22e+20 | 1.64327e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X174016.46+100318.1 | chandra | ccd7 | 989.798 | 820.735 | 12.0661 | 3.47363 | 0.00237354 | 0.000683302 | 5.91594 | 0.999998 | 1.37556 | 0.475604 | 131.987 | 4.23404 | F | F | 8.23e+20 | 1.72472e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X173944.40+100052.8 | chandra | ccd2 | 366.519 | 887.777 | 19.4337 | 5.05577 | 0.00382283 | 0.000994529 | 7.85103 | 1 | 5.26478 | 4.09694 | 88.4437 | 10.0267 | F | F | 8.19e+20 | 4.7075e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X173949.00+095910.2 | chandra | ccd2 | 228 | 678.594 | 27.1688 | 5.65691 | 0.00534439 | 0.00111278 | 10.9759 | 1 | 2.96045 | 2.79122 | 81.4843 | 8.81688 | F | F | 8.18e+20 | 6.49349e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X174017.01+100617.3 | chandra | ccd7 | 972.833 | 1184.61 | 8.06973 | 3.00002 | 0.0015874 | 0.000590137 | 3.95654 | 0.999606 | 1.42486 | 0.989328 | 68.5366 | 6.96308 | F | F | 8.26e+20 | 1.31559e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X174030.40+100308.7 | chandra | ccd7 | 570.875 | 801.125 | 7.69502 | 2.82843 | 0.00151369 | 0.000556384 | 3.77282 | 0.998731 | 0.684773 | 0.492 | 71.8953 | 3.81278 | F | F | 8.25e+20 | 1.03517e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X174019.20+095826.0 | chandra | ccd7 | 907.071 | 226.643 | 6.83615 | 2.64576 | 0.00134475 | 0.000520449 | 3.35173 | 0.996206 | 0.492 | 0.492 | 143.677 | 1.79456 | F | F | 8.21e+20 | 8.89029e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X174008.41+095257.2 | chandra | ccd6 | 884.167 | 528.333 | 5.2991 | 2.44951 | 0.00104239 | 0.000481845 | 7.61881 | 0.999988 | 1.42093 | 0.785608 | 159.414 | 7.76538 | A | F | 8.19e+20 | 1.09515e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X174027.29+095527.2 | chandra | ccd6 | 317.1 | 833.1 | 4.9018 | 2.23607 | 0.000964238 | 0.000439859 | 7.0476 | 0.999988 | 0.555758 | 0.492 | 6.74787 | 4.1867 | F | F | 8.21e+20 | 9.34625e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X174040.88+100152.4 | chandra | ccd7 | 256.1 | 646.1 | 4.82104 | 2.23607 | 0.000948351 | 0.00043986 | 2.36373 | 0.973485 | 0.611129 | 0.492 | 53.9394 | 4.57659 | F | F | 8.26e+20 | 6.73011e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X174028.39+095645.1 | chandra | ccd6 | 284.25 | 991.5 | 3.93926 | 2 | 0.000774896 | 0.000393422 | 5.6637 | 0.999852 | 0.492 | 0.492 | 27.7457 | 2.97795 | F | F | 8.21e+20 | 7.40678e-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