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 | 8 | X091400.13+372445.2 | chandra | ccd7 | 507.017 | 720.725 | 70.5792 | 8.41337 | 0.0139474 | 0.00166259 | 68.9528 | 1 | 1.09449 | 0.566553 | 45.8116 | 4.02457 | A | F | 1.47e+20 | 1.06369e-13 | 1 | dsx | ||||
| Report | 2 | X091342.46+372603.5 | chandra | ccd7 | 934.971 | 879.61 | 67.3477 | 8.35036 | 0.0133088 | 0.00165014 | 65.7957 | 1 | 0.39154 | 0.39154 | 0 | 0.292268 | F | F | 1.48e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 4 | X091340.83+372740.9 | chandra | ccd7 | 974.47 | 1077.67 | 26.4318 | 5.28335 | 0.00522327 | 0.00104406 | 25.8227 | 1 | 0.449628 | 0.449628 | 0 | 1.60159 | F | F | 1.49e+20 | 3.92038e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X091415.28+373247.2 | chandra | ccd3 | 1106.25 | 696.375 | 25.9123 | 5.65693 | 0.0051206 | 0.00111788 | 39.937 | 1 | 3.75468 | 2.81803 | 108.235 | 9.55067 | F | F | 1.48e+20 | 7.09806e-14 | 1 | dx | ||||
| Report | 3 | X091351.42+372627.8 | chandra | ccd7 | 718.074 | 929.244 | 12.7591 | 3.57199 | 0.00252136 | 0.000705871 | 12.4651 | 1 | 0.624449 | 0.326098 | 25.1753 | 2.10442 | F | F | 1.48e+20 | 0 | 1 | ds | |||||
| Report | 2 | X091427.29+372836.8 | chandra | ccd3 | 814.786 | 187.929 | 6.65835 | 2.64576 | 0.00131577 | 0.000522835 | 10.2621 | 1 | 0.627331 | 0.492 | 168.234 | 9.53084 | F | F | 1.41e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X091307.96+372818.6 | chandra | ccd6 | 930.167 | 525.333 | 5.58323 | 2.4495 | 0.00110399 | 0.000484349 | 8.3927 | 1 | 1.41684 | 0.792961 | 147.931 | 6.92321 | A | F | 1.5e+20 | 1.3999e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X091402.52+373544.1 | chandra | ccd2 | 554.833 | 457.5 | 4.45719 | 2.44953 | 0.000881337 | 0.000484355 | 6.82889 | 0.999918 | 2.43003 | 0.755094 | 91.7071 | 10.5557 | A | F | 1.49e+20 | 1.24798e-14 | 1 | dx | ||||
| Report | 4 | X091325.34+372956.7 | chandra | ccd6 | 509.5 | 724.25 | 3.92999 | 2 | 0.000777091 | 0.000395468 | 5.90755 | 0.999902 | 0.566374 | 0.492 | 139.44 | 4.95635 | F | F | 1.5e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X091327.41+372905.9 | chandra | ccd6 | 459.5 | 621 | 3.91568 | 2 | 0.000774261 | 0.000395468 | 5.88604 | 0.999902 | 0.586634 | 0.492 | 69.6994 | 4.04499 | F | F | 1.49e+20 | 9.86771e-15 | 1 | dx | ||||
| Report | 5 | X091357.74+372730.9 | chandra | ccd7 | 564.75 | 1057 | 3.84013 | 2.00001 | 0.000758858 | 0.000395226 | 3.75164 | 0.995555 | 0.492 | 0.492 | 14.8724 | 3.61965 | F | F | 1.48e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X091338.58+372450.5 | chandra | ccd7 | 1028.5 | 730.833 | 2.87326 | 1.73205 | 0.000567792 | 0.000342276 | 2.80704 | 0.977945 | 0.492 | 0.492 | 49.7312 | 1.32915 | F | F | 1.48e+20 | 4.24612e-15 | 1 | dx | ||||
| Report | 2 | X091320.18+373108.2 | chandra | ccd6 | 634.167 | 869.833 | 2.81072 | 1.73206 | 0.000555775 | 0.000342486 | 4.22507 | 0.998875 | 0.639127 | 0.492 | 101.31 | 6.52743 | F | F | 1.5e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 6 | X091405.81+372117.8 | chandra | ccd7 | 368.5 | 298.833 | 2.14684 | 1.73207 | 0.000424243 | 0.00034228 | 2.09737 | 0.977945 | 1.00895 | 0.492 | 106.368 | 6.86985 | A | F | 1.47e+20 | 8.15764e-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