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 | X143004.24+354445.0 | chandra | ccd2 | 464.401 | 1030.69 | 19.3549 | 4.39942 | 0.00428899 | 0.000974899 | 31.2599 | 1 | 1.13706 | 1.13706 | 0 | 4.86081 | F | F | 1.18e+20 | 5.79581e-14 | 1 | dsx | ||||
| Report | 1 | X143027.08+354306.4 | chandra | ccd1 | 1386.01 | 657.182 | 14.9131 | 3.86175 | 0.00330244 | 0.000855167 | 23.3736 | 1 | 0.506373 | 0.506373 | 0 | 1.15055 | F | F | 1.17e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 1 | X143011.09+354909.4 | chandra | ccd0 | 987.9 | 742.4 | 8.9714 | 3.1623 | 0.00198666 | 0.000700272 | 14.4998 | 1 | 1.88543 | 0.721423 | 24.6199 | 7.54735 | A | F | 1.17e+20 | 2.57185e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X143004.08+353916.8 | chandra | ccd2 | 468.389 | 363.056 | 8.89996 | 3 | 0.0019722 | 0.000664788 | 14.3742 | 1 | 0.906977 | 0.492 | 49.0825 | 4.98576 | A | F | 1.18e+20 | 2.4453e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X143036.70+353743.6 | chandra | ccd3 | 482.167 | 814.5 | 8.86256 | 3 | 0.00196256 | 0.000664332 | 13.977 | 1 | 0.718705 | 0.492 | 4.06505 | 5.04662 | F | F | 1.18e+20 | 2.31222e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X142957.28+354813.6 | chandra | ccd0 | 1329.5 | 629.375 | 7.72872 | 2.82843 | 0.00171148 | 0.000626339 | 12.4913 | 1 | 1.31179 | 0.549974 | 116.187 | 8.22236 | A | F | 1.17e+20 | 2.49864e-14 | 1 | dx | ||||
| Report | 2 | X143017.78+354015.3 | chandra | ccd3 | 950.929 | 1122.79 | 6.9585 | 2.64575 | 0.00154092 | 0.000585886 | 10.9741 | 1 | 0.492 | 0.492 | 137.199 | 2.27456 | F | F | 1.18e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X143025.76+354008.0 | chandra | ccd3 | 753.214 | 1107.93 | 6.93943 | 2.64575 | 0.00153669 | 0.000585886 | 10.9441 | 1 | 0.492 | 0.492 | 93.5625 | 1.99034 | F | F | 1.18e+20 | 1.70242e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X143017.35+353959.1 | chandra | ccd3 | 961.643 | 1089.93 | 6.92848 | 2.64575 | 0.00153427 | 0.000585886 | 10.9268 | 1 | 0.492 | 0.492 | 95.004 | 2.54605 | F | F | 1.18e+20 | 2.08385e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X143018.76+354220.2 | chandra | ccd2 | 104.5 | 735.643 | 6.87511 | 2.64575 | 0.0015235 | 0.000586289 | 11.1039 | 1 | 0.557652 | 0.492 | 57.9533 | 1.1517 | F | F | 1.17e+20 | 1.85672e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X142955.53+353707.6 | chandra | ccd2 | 680.5 | 100.786 | 6.54038 | 2.64576 | 0.00144932 | 0.00058629 | 10.5633 | 1 | 1.12172 | 0.492 | 71.8078 | 7.67731 | A | F | 1.18e+20 | 1.927e-14 | 1 | dx | ||||
| Report | 6 | X143001.23+354248.5 | chandra | ccd2 | 538.5 | 793.5 | 5.86412 | 2.44949 | 0.00129946 | 0.000542798 | 9.47107 | 1 | 0.492 | 0.492 | 144.217 | 4.73967 | F | F | 1.18e+20 | 0 | 1 | d | |||||
| Report | 3 | X143025.10+354337.6 | chandra | ccd0 | 641.7 | 68.1001 | 4.9682 | 2.23607 | 0.00110018 | 0.000495164 | 8.02972 | 0.999997 | 0.590718 | 0.492 | 1.97259 | 1.53421 | F | F | 1.17e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X143037.55+353831.3 | chandra | ccd3 | 461.167 | 911.5 | 2.942 | 1.73205 | 0.000651488 | 0.000383553 | 4.63978 | 0.999209 | 0.492 | 0.492 | 180 | 4.47638 | F | F | 1.17e+20 | 7.53515e-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