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 | 10 | X104106.05+144417.6 | chandra | ccd7 | 854.766 | 425.811 | 79.4812 | 9.09891 | 0.0130743 | 0.00149673 | 41.2743 | 1 | 0.414178 | 0.414178 | 0 | 0.291084 | F | F | 2.89e+20 | 9.6657e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X104101.71+144615.8 | chandra | ccd7 | 982.575 | 666.105 | 49.8841 | 7.59604 | 0.00820571 | 0.00124951 | 25.9047 | 1 | 0.462139 | 0.462139 | 0 | 2.50297 | F | F | 2.9e+20 | 6.14419e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X104110.49+144727.6 | chandra | ccd7 | 723.757 | 812.099 | 17.3122 | 4.16079 | 0.00284779 | 0.000684433 | 8.99017 | 1 | 0.669817 | 0.669817 | 0 | 3.6122 | F | F | 2.89e+20 | 2.16486e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X104046.86+143710.4 | chandra | ccd6 | 884.237 | 478.132 | 16.398 | 4.35894 | 0.00269739 | 0.000717023 | 22.3127 | 1 | 2.91676 | 2.05095 | 24.0213 | 8.27225 | F | F | 2.94e+20 | 3.26035e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X104109.47+144931.4 | chandra | ccd7 | 753.382 | 1063.15 | 14.8999 | 4.12314 | 0.00245096 | 0.000678235 | 7.73749 | 1 | 1.5563 | 1.00954 | 73.267 | 5.57754 | A | F | 2.89e+20 | 1.92882e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 9 | X104108.67+145108.8 | chandra | ccd7 | 777 | 1261.19 | 13.6024 | 4.00004 | 0.00223753 | 0.000657986 | 7.0637 | 1 | 2.10247 | 0.771871 | 42.0266 | 7.16946 | A | F | 2.9e+20 | 1.93481e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X104123.56+144839.7 | chandra | ccd7 | 338 | 958.2 | 8.86833 | 3.1623 | 0.00145879 | 0.000520182 | 4.6053 | 0.999867 | 1.06397 | 0.751351 | 80.9129 | 6.27726 | F | F | 2.87e+20 | 1.16925e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X104112.78+144011.7 | chandra | ccd6 | 119.7 | 846.5 | 4.88712 | 2.23607 | 0.000803907 | 0.000367822 | 6.64988 | 0.999978 | 0.619406 | 0.492 | 84.9377 | 4.13188 | F | F | 2.89e+20 | 9.34423e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X104045.63+144341.6 | chandra | ccd6 | 920.885 | 1273.87 | 20.6874 | 4.54834 | 0.00340298 | 0.00074818 | 28.1492 | 1 | 2.00662 | 0.570342 | 359.995 | 4.9905 | A | F | 2.93e+20 | 5.87617e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X104110.58+144418.3 | chandra | ccd7 | 720.7 | 426.7 | 4.83296 | 2.23607 | 0.000794996 | 0.000367822 | 2.50974 | 0.986119 | 0.492 | 0.492 | 95.655 | 1.11003 | F | F | 2.89e+20 | 5.91827e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X104109.31+144532.0 | chandra | ccd7 | 758.1 | 576.5 | 4.7539 | 2.23607 | 0.000781991 | 0.000367823 | 2.46868 | 0.986119 | 0.492 | 0.492 | 25.6701 | 1.70853 | F | F | 2.89e+20 | 5.8148e-15 | 1 | dx | ||||
Report | 4 | X104049.56+144135.4 | chandra | ccd6 | 804.5 | 1016.75 | 3.9237 | 2 | 0.000645429 | 0.00032899 | 5.33895 | 0.999755 | 0.492 | 0.492 | 28.9973 | 4.68329 | F | F | 2.92e+20 | 0 | 1 | d |
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