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 | 1 | X004238.58+411603.5 | chandra | ccd2 | 72.8618 | 793.166 | 69.6982 | 8.58074 | 0.475262 | 0.0585109 | 49.7153 | 1 | 0.464106 | 0.464106 | 0 | 0.612734 | F | F | 1.26e+21 | 5.49219e-12 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X004222.95+411535.2 | chandra | ccd2 | 431.207 | 735.738 | 31.6383 | 5.62479 | 0.215737 | 0.0383547 | 22.5674 | 1 | 1.05387 | 0.617872 | 131.026 | 3.58879 | F | F | 1.23e+21 | 2.48931e-12 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X004213.13+411836.1 | chandra | ccd2 | 655.3 | 1103.1 | 9.92979 | 3.16228 | 0.0672646 | 0.0214213 | 7.08286 | 0.999999 | 0.892235 | 0.492 | 40.7694 | 5.90403 | A | F | 1.24e+21 | 8.34446e-13 | 1 | dx | ||||
| Report | 2 | X004231.12+411621.2 | chandra | ccd2 | 243.5 | 828.667 | 8.97962 | 3 | 0.0608281 | 0.0203221 | 6.4051 | 0.999993 | 0.492 | 0.492 | 143.13 | 2.01276 | F | F | 1.25e+21 | 0 | 1 | d | |||||
| Report | 8 | X004248.53+411521.0 | chandra | ccd3 | 781.5 | 1008.17 | 8.94532 | 3 | 0.0605958 | 0.0203221 | 41.3817 | 1 | 0.492 | 0.492 | 58.2825 | 1.51284 | F | F | 1.27e+21 | 0 | 1 | d | |||||
| Report | 1 | X004259.86+411605.5 | chandra | ccd1 | 881.875 | 151.75 | 7.98645 | 2.82843 | 0.0541004 | 0.0191598 | 43.6108 | 1 | 0.492 | 0.492 | 163.862 | 3.39687 | F | F | 1.28e+21 | 0 | 1 | d | |||||
| Report | 11 | X004232.13+411314.1 | chandra | ccd2 | 220.375 | 448.25 | 7.9795 | 2.82843 | 0.0540533 | 0.0191598 | 5.69173 | 0.99996 | 0.539488 | 0.492 | 7.33223 | 3.45675 | F | F | 1.23e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X004245.12+411621.5 | chandra | ccd3 | 859.625 | 1131.12 | 7.8472 | 2.82843 | 0.0531571 | 0.0191599 | 36.3017 | 1 | 0.492 | 0.492 | 39.0557 | 0.652024 | F | F | 1.27e+21 | 5.79059e-13 | 1 | dx | ||||
| Report | 5 | X004254.91+411603.2 | chandra | ccd1 | 995.357 | 147.072 | 6.99938 | 2.64575 | 0.0474139 | 0.0179224 | 38.2208 | 1 | 0.492 | 0.492 | 98.3496 | 2.46831 | F | F | 1.28e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X004257.95+411104.8 | chandra | ccd3 | 565.167 | 487.5 | 6.94001 | 2.64575 | 0.0470118 | 0.0179224 | 32.105 | 1 | 0.492 | 0.492 | 118.155 | 5.93455 | F | F | 1.25e+21 | 6.02767e-13 | 1 | dx | ||||
| Report | 3 | X004252.54+411854.0 | chandra | ccd1 | 1049.67 | 494.167 | 5.98479 | 2.44949 | 0.0405411 | 0.0165929 | 32.6805 | 1 | 0.492 | 0.492 | 47.1446 | 3.39102 | F | F | 1.29e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X004303.89+411804.9 | chandra | ccd1 | 789.667 | 394.667 | 5.97592 | 2.44949 | 0.040481 | 0.0165929 | 32.6321 | 1 | 0.492 | 0.492 | 100.625 | 4.5693 | F | F | 1.3e+21 | 4.88301e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X004240.66+411327.3 | chandra | ccd3 | 961.833 | 777.167 | 5.96559 | 2.44949 | 0.0404111 | 0.0165929 | 27.5973 | 1 | 0.593239 | 0.492 | 172.534 | 2.72927 | F | F | 1.24e+21 | 4.93436e-13 | 1 | dx | ||||
| Report | 8 | X004207.73+411814.6 | chandra | ccd2 | 779 | 1059.75 | 3.99798 | 2 | 0.0270824 | 0.013548 | 2.85173 | 0.984651 | 0.665846 | 0.492 | 2.7861 | 6.72341 | F | F | 1.23e+21 | 0 | 1 | d | |||||
| Report | 1 | X004247.85+411532.5 | chandra | ccd3 | 797 | 1031.5 | 3.96964 | 2 | 0.0268904 | 0.0135481 | 18.3639 | 1 | 0.492 | 0.492 | 180 | 1.30499 | F | F | 1.27e+21 | 0 | 1 | d | |||||
| Report | 1 | X004226.03+411915.7 | chandra | ccd0 | 693.75 | 241.25 | 3.96917 | 2 | 0.0268873 | 0.0135481 | 21.5694 | 1 | 0.492 | 0.492 | 45 | 4.27427 | F | F | 1.26e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X004223.19+411407.0 | chandra | ccd2 | 425.25 | 556 | 3.95761 | 2 | 0.026809 | 0.0135481 | 2.82294 | 0.984651 | 0.836546 | 0.492 | 39.4176 | 4.05622 | A | F | 1.22e+21 | 3.15919e-13 | 1 | dx | ||||
| Report | 4 | X004303.23+411528.1 | chandra | ccd1 | 804.5 | 75.8333 | 2.99171 | 1.73205 | 0.0202659 | 0.011733 | 16.3365 | 1 | 0.621484 | 0.492 | 14.3052 | 4.09177 | F | F | 1.28e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 6 | X004243.90+411630.0 | chandra | ccd3 | 887.5 | 1148.5 | 2.93572 | 1.73205 | 0.0198866 | 0.011733 | 13.5808 | 0.999984 | 0.492 | 0.492 | 45 | 0.51291 | F | F | 1.27e+21 | 2.5739e-13 | 1 | dx | ||||
| Report | 2 | X004246.97+411615.3 | chandra | ccd3 | 817.167 | 1118.5 | 2.92682 | 1.73205 | 0.0198263 | 0.011733 | 13.5397 | 0.999984 | 0.492 | 0.492 | 5.35186e-08 | 0.977542 | F | F | 1.27e+21 | 0 | 1 | d | |||||
| Report | 2 | X004231.28+411938.4 | chandra | ccd0 | 573.5 | 287.5 | 0.995303 | 1 | 0.0067422 | 0.00677402 | 5.4087 | 0.999439 | 0.492 | 0.492 | 90 | 3.98647 | F | F | 1.27e+21 | 0 | 1 | d | |||||
| Report | 3 | X004224.40+412402.8 | chandra | ccd0 | 730.5 | 825 | 3.93909 | 2 | 0.0266835 | 0.0135481 | 21.4059 | 1 | 0.982294 | 0.602219 | 158.645 | 8.52014 | A | F | 1.29e+21 | 0 | 1 | d | |||||
| Report | 4 | X004240.22+411844.5 | chandra | ccd0 | 368.9 | 177.9 | 4.98689 | 2.23607 | 0.0337813 | 0.0151472 | 27.0999 | 1 | 0.492 | 0.492 | 66.1368 | 2.58261 | F | F | 1.28e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 7 | X004245.82+411036.3 | chandra | ccd3 | 843.5 | 429.5 | 0.984687 | 1 | 0.00667029 | 0.00677403 | 4.55523 | 0.998942 | 0.492 | 0.492 | 90 | 5.62329 | F | F | 1.23e+21 | 8.23862e-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