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 | 1 | X022105.50+372046.1 | chandra | ccd7 | 558.977 | 431.721 | 184.095 | 13.7211 | 0.0406899 | 0.00303273 | 127.439 | 1 | 0.427897 | 0.427897 | 0 | 0.578246 | F | F | 4.24e+20 | 0 | 1 | ds | |||||
Report | 8 | X022104.24+372015.7 | chandra | ccd7 | 589.465 | 369.991 | 17.8132 | 4.22057 | 0.0039372 | 0.000932859 | 12.3311 | 1 | 0.42884 | 0.42884 | 0 | 0.365365 | F | F | 4.24e+20 | 0 | 1 | ds | |||||
Report | 5 | X022105.43+372326.6 | chandra | ccd7 | 560.071 | 757.357 | 6.73086 | 2.64576 | 0.00148769 | 0.000584778 | 4.65941 | 0.999678 | 0.649658 | 0.492 | 31.2236 | 3.24428 | F | F | 4.25e+20 | 0 | 1 | d | |||||
Report | 6 | X022051.37+372537.8 | chandra | ccd7 | 900.643 | 1024.21 | 6.28367 | 2.64577 | 0.00138885 | 0.000584781 | 4.34984 | 0.999678 | 1.0575 | 0.748396 | 17.6362 | 6.16371 | F | T | 4.25e+20 | 0 | 1 | d | |||||
Report | 3 | X022121.81+371945.9 | chandra | ccd7 | 163 | 309 | 5.87577 | 2.44949 | 0.00129869 | 0.000541399 | 4.06748 | 0.998571 | 0.613829 | 0.492 | 162.504 | 3.16241 | F | F | 4.25e+20 | 0 | 1 | d | |||||
Report | 1 | X022026.11+372038.7 | chandra | ccd3 | 174.333 | 721 | 5.57966 | 2.4495 | 0.00123324 | 0.000541401 | 11.4178 | 1 | 1.31306 | 0.743501 | 147.207 | 7.95313 | A | F | 4.22e+20 | 0 | 1 | d | |||||
Report | 3 | X022100.24+371631.7 | chandra | ccd6 | 1051.1 | 890.1 | 4.90953 | 2.23607 | 0.00108513 | 0.000494228 | 9.77807 | 1 | 0.633074 | 0.492 | 111.766 | 3.85071 | F | F | 4.23e+20 | 0 | 1 | d | |||||
Report | 7 | X022106.00+372646.0 | chandra | ccd7 | 546.3 | 1162.7 | 4.69726 | 2.23608 | 0.00103821 | 0.000494229 | 3.25166 | 0.994328 | 1.22366 | 0.492 | 33.7742 | 6.56575 | A | F | 4.26e+20 | 0 | 1 | d | |||||
Report | 4 | X022112.96+372215.2 | chandra | ccd7 | 377.75 | 612.25 | 3.91494 | 2 | 0.000865299 | 0.000442051 | 2.7101 | 0.994328 | 0.492 | 0.492 | 125.008 | 2.46815 | F | F | 4.25e+20 | 0 | 1 | d | |||||
Report | 2 | X022101.26+372100.3 | chandra | ccd7 | 661.167 | 460.167 | 2.94945 | 1.73205 | 0.000651903 | 0.000382827 | 2.04175 | 0.980096 | 0.492 | 0.492 | 45 | 1.24714 | F | F | 4.24e+20 | 0 | 1 | d | |||||
Report | 2 | X022106.65+371242.6 | chandra | ccd6 | 895.5 | 424.5 | 1.81659 | 1.41422 | 0.000401512 | 0.000312578 | 3.61801 | 0.997787 | 0.825109 | 0.492 | 26.5651 | 7.49164 | A | F | 4.24e+20 | 0 | 1 | d | |||||
Report | 2 | X022040.59+371147.5 | chandra | ccd2 | 199.375 | 624.75 | 7.33888 | 2.82844 | 0.00162208 | 0.000625156 | 1.97167 | 0.97383 | 2.56312 | 1.65221 | 63.0032 | 9.81785 | A | F | 4.22e+20 | 0 | 1 | d | |||||
Report | 4 | X022033.50+371619.9 | chandra | ccd2 | 371.43 | 1179.16 | 28.9693 | 6.54399 | 0.006403 | 0.0014464 | 7.78292 | 1 | 2.27322 | 0.753615 | 29.0536 | 7.54328 | F | F | 4.21e+20 | 0 | 1 | ds | |||||
Report | 1 | X022110.49+371530.9 | chandra | ccd6 | 802.5 | 766.5 | 0.988854 | 1 | 0.000218561 | 0.000221025 | 1.96945 | 0.973091 | 0.492 | 0.492 | 90 | 4.76849 | F | F | 4.24e+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