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 | 5 | X204726.89+295951.7 | chandra | ccd3 | 170.699 | 591.128 | 104.256 | 11.5278 | 0.010724 | 0.00118578 | 23.9049 | 1 | 1.35692 | 1.35692 | 0 | 6.38158 | F | F | 1.63e+21 | 7.32314e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 6 | X204651.84+300715.7 | chandra | ccd2 | 631.487 | 566.903 | 54.4585 | 9.15328 | 0.00560358 | 0.00094184 | 13.4983 | 1 | 0.974106 | 0.974106 | 0 | 5.19339 | F | F | 1.71e+21 | 6.48747e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X204639.16+301102.7 | chandra | ccd2 | 964.815 | 1028.17 | 36.2584 | 9.74719 | 0.00373086 | 0.00100295 | 8.98717 | 1 | 2.29894 | 2.16774 | 169.053 | 9.3788 | F | F | 1.75e+21 | 4.55842e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X204714.35+295925.3 | chandra | ccd3 | 501.78 | 537.467 | 14.7119 | 5.4179 | 0.0015133 | 0.000557297 | 3.3733 | 0.998772 | 1.03194 | 0.445588 | -0 | 6.23481 | F | F | 1.65e+21 | 1.66742e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X204720.82+300248.7 | chandra | ccd3 | 331.09 | 950.903 | 17.7658 | 5.61706 | 0.00182744 | 0.000577786 | 4.07352 | 0.999833 | 0.435608 | 0.435608 | 0 | 3.15468 | F | F | 1.66e+21 | 2.00397e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X204731.55+300210.1 | chandra | ccd1 | 964.96 | 421.616 | 23.9578 | 7.96711 | 0.00246436 | 0.000819517 | 2.25446 | 0.984693 | 0.925049 | 0.925049 | 0 | 5.05442 | F | F | 1.64e+21 | 2.58741e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X204753.35+300823.1 | chandra | ccd1 | 390.67 | 1180.31 | 58.2478 | 16.4703 | 0.00599152 | 0.00169418 | 5.4812 | 1 | 3.42089 | 3.42089 | 0 | 8.76718 | F | F | 1.65e+21 | 7.42208e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X204703.59+300756.4 | chandra | ccd2 | 321.585 | 649.36 | 18.5629 | 5.91894 | 0.00191006 | 0.000609039 | 4.60108 | 0.999962 | 0.622525 | 0.622525 | 0 | 3.3068 | F | F | 1.71e+21 | 1.9769e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X204657.43+300017.4 | chandra | ccd3 | 948.091 | 643 | 17.9194 | 4.69047 | 0.00184324 | 0.000482473 | 4.10875 | 0.999833 | 2.30576 | 0.969313 | 38.1364 | 6.55156 | A | F | 1.67e+21 | 2.30122e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X204654.04+300726.5 | chandra | ccd2 | 572.869 | 588.237 | 14.5296 | 4.35896 | 0.00149504 | 0.000448521 | 3.60136 | 0.999256 | 0.761483 | 0.516265 | 62.6486 | 4.80691 | F | F | 1.71e+21 | 1.65846e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X204653.64+300802.6 | chandra | ccd2 | 583.954 | 662.158 | 10.931 | 5.31736 | 0.00112476 | 0.000547137 | 2.7094 | 0.994873 | 0.67968 | 0.59999 | 60.9718 | 5.14369 | F | F | 1.71e+21 | 1.27521e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X204641.41+300711.8 | chandra | ccd2 | 906.585 | 559.29 | 65.4036 | 9.18397 | 0.0067298 | 0.000944998 | 16.2112 | 1 | 4.79992 | 4.79992 | 0 | 7.35604 | T | F | 1.72e+21 | 7.79043e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 6 | X204734.78+300105.1 | chandra | ccd1 | 879.679 | 289.62 | 829.438 | 30.2603 | 0.0853182 | 0.00311266 | 78.0512 | 1 | 2.04029 | 1.19843 | 0.0190752 | 6.31479 | A | F | 1.63e+21 | 1.71392e-12 | 1 | dsxf |
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