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 | 6 | X145214.93+443210.7 | chandra | ccd7 | 179.829 | 377.893 | 77.8379 | 8.82258 | 0.00821811 | 0.000931486 | 49.1858 | 1 | 0.682485 | 0.682485 | 0 | 2.68655 | F | F | 1.92e+20 | 6.36338e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X145147.97+442151.4 | chandra | ccd6 | 635.566 | 138.08 | 60.618 | 7.78576 | 0.00640009 | 0.000822026 | 76.7714 | 1 | 5.36229 | 5.36229 | 0 | 9.52408 | F | F | 1.94e+20 | 7.98731e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X145124.94+443635.2 | chandra | ccd3 | 46.6777 | 422.589 | 40.3367 | 6.70826 | 0.00425879 | 0.000708266 | 46.6084 | 1 | 2.30808 | 1.53393 | 175.51 | 8.47016 | A | F | 1.91e+20 | 8.29362e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X145157.67+442855.3 | chandra | ccd6 | 423.849 | 999.638 | 28.6614 | 5.43555 | 0.00302609 | 0.000573889 | 36.299 | 1 | 0.657374 | 0.657374 | 0 | 2.2582 | F | F | 1.93e+20 | 3.2338e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X145148.00+443332.0 | chandra | ccd7 | 764.81 | 543.169 | 15.8464 | 4.27279 | 0.00167307 | 0.000451122 | 10.0133 | 1 | 0.555631 | 0.555631 | 0 | 3.38499 | F | F | 1.92e+20 | 1.32126e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X145153.26+443620.7 | chandra | ccd7 | 650.563 | 885.967 | 16.3523 | 4.0438 | 0.00172647 | 0.000426943 | 10.333 | 1 | 1.5 | 1.23315 | 95.0209 | 5.44451 | F | F | 1.91e+20 | 1.3682e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X145048.87+443015.1 | chandra | ccd2 | 698.389 | 687.278 | 11.8867 | 4.24275 | 0.00125502 | 0.000447956 | 13.8674 | 1 | 4.31631 | 2.68636 | 168.39 | 12.9113 | A | F | 1.93e+20 | 1.78692e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X145210.07+443306.0 | chandra | ccd7 | 285.528 | 490.181 | 9.50497 | 3.10148 | 0.00100353 | 0.000327453 | 6.00619 | 0.999998 | 0.479882 | 0.129619 | 88.8421 | 2.56111 | A | F | 1.92e+20 | 7.63364e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X145201.75+443632.0 | chandra | ccd7 | 465.7 | 908.4 | 9.20119 | 3.16229 | 0.00097146 | 0.000333874 | 5.81423 | 0.999987 | 0.961692 | 0.492 | 56.9863 | 5.44097 | A | F | 1.91e+20 | 7.65811e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X145145.73+442816.2 | chandra | ccd6 | 683.214 | 919.786 | 6.79186 | 2.64576 | 0.000717089 | 0.000279341 | 8.60174 | 1 | 0.61493 | 0.492 | 178.467 | 3.93986 | F | F | 1.93e+20 | 7.97362e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X145112.34+443417.8 | chandra | ccd3 | 320.875 | 144 | 6.79015 | 2.82845 | 0.000716912 | 0.000298632 | 7.84592 | 0.999999 | 2.19435 | 0.568135 | 3.59112 | 9.26636 | A | F | 1.93e+20 | 1.03658e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X145217.42+443444.3 | chandra | ccd7 | 125.333 | 689.5 | 5.73565 | 2.4495 | 0.000605569 | 0.000258617 | 3.62436 | 0.998846 | 0.536505 | 0.492 | 71.1266 | 4.65786 | F | F | 1.91e+20 | 4.82534e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X145202.60+442747.1 | chandra | ccd6 | 316.1 | 860.5 | 4.83811 | 2.23607 | 0.000510811 | 0.000236086 | 6.12736 | 0.999952 | 0.492 | 0.492 | 155.457 | 3.31902 | F | F | 1.93e+20 | 5.58238e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X145142.66+442554.3 | chandra | ccd6 | 750.3 | 631.3 | 4.49793 | 2.23608 | 0.000474895 | 0.000236087 | 5.69653 | 0.999952 | 0.799298 | 0.574968 | 28.9973 | 6.14811 | F | F | 1.94e+20 | 5.57946e-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