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 | 4 | X122609.69+100518.0 | chandra | ccd6 | 176.992 | 30.3302 | 30.5826 | 5.53015 | 0.00600478 | 0.00108583 | 45.6385 | 1 | 1.26991 | 0.821623 | 19.8784 | 3.58433 | F | F | 1.94e+20 | 7.52384e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X122555.35+100109.9 | chandra | ccd7 | 585.539 | 571.987 | 23.0927 | 4.91954 | 0.00453417 | 0.000965934 | 22.3365 | 1 | 0.703444 | 0.455633 | 337.953 | 2.34252 | F | F | 1.92e+20 | 3.37387e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X122629.48+095728.0 | chandra | ccd3 | 919.604 | 338.065 | 13.1722 | 4.4377 | 0.00258632 | 0.000871326 | 5.15826 | 0.999983 | 3.5828 | 3.5828 | 0 | 9.95795 | F | F | 1.85e+20 | 3.74852e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X122642.24+095641.3 | chandra | ccd3 | 536 | 243 | 11.519 | 3.87306 | 0.0022617 | 0.000760455 | 4.51086 | 0.999947 | 0.492 | 0.492 | 45 | 12.9987 | F | F | 1.83e+20 | 3.81333e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122634.82+095826.7 | chandra | ccd3 | 758.8 | 457.1 | 7.94503 | 3.16232 | 0.00155997 | 0.000620905 | 3.11129 | 0.996956 | 2.44364 | 1.47576 | 2.30582 | 10.5387 | A | F | 1.85e+20 | 2.21384e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122614.03+100009.8 | chandra | ccd7 | 24.2144 | 449.357 | 6.69161 | 2.64576 | 0.00131386 | 0.000519482 | 6.47248 | 0.999984 | 0.778734 | 0.492 | 155.663 | 5.30116 | A | F | 1.88e+20 | 1.93997e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122602.30+100645.3 | chandra | ccd6 | 398.333 | 207.167 | 5.93695 | 2.44949 | 0.00116569 | 0.000480945 | 8.85973 | 1 | 0.492 | 0.492 | 55.278 | 3.52264 | F | F | 1.97e+20 | 1.27286e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X122556.42+100243.7 | chandra | ccd7 | 552.833 | 762.167 | 5.73004 | 2.4495 | 0.00112506 | 0.000480946 | 5.5424 | 0.999875 | 0.625789 | 0.492 | 52.3104 | 0.760056 | T | F | 1.93e+20 | 8.25426e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X122631.56+100255.7 | chandra | ccd3 | 857 | 1003.75 | 5.4229 | 2.44951 | 0.00106476 | 0.000480948 | 2.12362 | 0.965425 | 0.492 | 0.492 | 153.435 | 8.4793 | F | F | 1.88e+20 | 1.48326e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X122626.88+100838.5 | chandra | ccd2 | 1021.83 | 657.5 | 5.42263 | 2.44951 | 0.0010647 | 0.000480949 | 8.29268 | 0.999994 | 1.29737 | 0.492 | 107.143 | 8.9563 | A | F | 1.95e+20 | 1.79249e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122632.85+100922.0 | chandra | ccd2 | 842.583 | 746 | 10.35 | 3.46413 | 0.00203218 | 0.000680164 | 15.8281 | 1 | 2.40849 | 1.759 | 75.8625 | 10.5783 | F | F | 1.95e+20 | 3.01183e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X122631.12+100403.6 | chandra | ccd2 | 894.357 | 98.7856 | 11.6146 | 3.7417 | 0.00228046 | 0.000734663 | 17.7619 | 1 | 3.25253 | 1.41837 | 170.497 | 8.37417 | A | F | 1.9e+20 | 3.07758e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X122607.30+100519.4 | chandra | ccd6 | 248.25 | 32.5 | 3.95914 | 2 | 0.000777357 | 0.00039269 | 5.90824 | 0.999895 | 0.492 | 0.492 | 118.997 | 3.10699 | F | F | 1.94e+20 | 8.65781e-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