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 rmf | 3 | X213522.94+473438.8 | chandra | ccd2 | 257.214 | 753.424 | 126.562 | 11.7056 | 0.0374375 | 0.00346256 | 39.1345 | 1 | 1.58913 | 1.24586 | 71.7624 | 6.71918 | F | F | 3.24e+21 | 6.71187e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X213418.99+474420.5 | chandra | ccd3 | 911.688 | 1113.62 | 14.8158 | 4.00002 | 0.00438253 | 0.00118321 | 30.2013 | 1 | 3.24611 | 1.49882 | 172.238 | 9.26599 | A | F | 3.29e+21 | 5.99253e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X213420.08+473800.5 | chandra | ccd3 | 891.333 | 341.333 | 7.95741 | 3.00002 | 0.00235381 | 0.000887412 | 16.2208 | 1 | 2.11973 | 1.1036 | 147.72 | 8.99869 | A | F | 3.24e+21 | 3.06832e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X213510.76+474528.0 | chandra | ccd7 | 1044.17 | 559.333 | 5.78393 | 2.4495 | 0.0017109 | 0.000724565 | 7.62719 | 0.999997 | 0.510857 | 0.492 | 128.66 | 4.43929 | F | F | 3.25e+21 | 1.61744e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X213432.14+473256.9 | chandra | ccd0 | 495 | 1182.67 | 5.40683 | 2.44951 | 0.00159935 | 0.000724569 | 11.2664 | 1 | 1.21503 | 0.492 | 79.0706 | 10.3393 | A | F | 3.23e+21 | 2.16478e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X213434.26+474337.5 | chandra | ccd3 | 598.7 | 1025.5 | 4.83304 | 2.23607 | 0.00142962 | 0.000661433 | 9.85193 | 1 | 0.779624 | 0.492 | 111.137 | 6.61576 | A | F | 3.26e+21 | 1.83563e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X213555.18+473825.7 | chandra | ccd6 | 789.7 | 510.3 | 4.67147 | 2.23608 | 0.00138183 | 0.000661436 | 9.20699 | 0.999992 | 1.35374 | 0.578844 | 5.45063 | 7.97038 | A | F | 3.26e+21 | 1.76271e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X213538.42+474342.3 | chandra | ccd7 | 477 | 345 | 3.87369 | 2 | 0.00114584 | 0.000591605 | 5.10818 | 0.999674 | 0.729085 | 0.492 | 146.599 | 5.417 | F | F | 3.26e+21 | 1.10062e-14 | 1 | dx | ||||
| Report | 4 | X213438.33+474238.0 | chandra | ccd3 | 515.5 | 904.5 | 2.97592 | 1.73205 | 0.000880282 | 0.000512344 | 6.06628 | 0.999885 | 0.492 | 0.492 | 90 | 5.63498 | F | F | 3.25e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X213528.98+474258.6 | chandra | ccd7 | 670.5 | 256 | 1.90238 | 1.41422 | 0.000562726 | 0.000418328 | 2.50864 | 0.979276 | 0.492 | 0.492 | 90 | 3.68019 | F | F | 3.25e+21 | 5.25562e-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