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 | X045950.07-710118.6 | chandra | ccd6 | 165.812 | 400.533 | 33.7892 | 7.81053 | 0.0098932 | 0.00228686 | 68.912 | 1 | 6.97829 | 4.36223 | 93.7901 | 15.9551 | A | F | 1.43e+21 | 1.40496e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X050130.79-704306.4 | chandra | ccd1 | 714.395 | 418.457 | 24.8203 | 4.982 | 0.00726725 | 0.0014587 | 52.1334 | 1 | 0.924492 | 0.408835 | 70.6361 | 4.55668 | F | F | 1.33e+21 | 8.80664e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X050135.80-704822.3 | chandra | ccd3 | 544.5 | 820.722 | 8.88465 | 3 | 0.00260135 | 0.000878376 | 18.8371 | 1 | 0.73193 | 0.492 | 107.177 | 4.45705 | F | F | 1.35e+21 | 3.13454e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X050158.94-703823.5 | chandra | ccd1 | 427.75 | 992 | 7.80879 | 3.00003 | 0.00228635 | 0.000878383 | 16.4019 | 1 | 0.788935 | 0.504101 | 110.157 | 9.62967 | A | F | 1.31e+21 | 2.96008e-14 | 1 | dx | ||||
| Report | 2 | X050024.70-704945.4 | chandra | ccd2 | 200.9 | 488.5 | 4.98144 | 2.23607 | 0.00145852 | 0.000654702 | 10.9999 | 1 | 0.603419 | 0.492 | 151.512 | 4.16868 | F | F | 1.38e+21 | 0 | 1 | d | |||||
| Report | 1 | X045942.08-704618.6 | chandra | ccd2 | 629.5 | 907.5 | 3.96923 | 2 | 0.00116216 | 0.000585584 | 8.76481 | 0.999997 | 0.541235 | 0.492 | 163.155 | 5.52697 | F | F | 1.38e+21 | 0 | 1 | d | |||||
| Report | 5 | X045942.26-705014.3 | chandra | ccd2 | 625.5 | 428.25 | 3.85043 | 2.00001 | 0.00112737 | 0.000585585 | 8.50247 | 0.999997 | 0.543417 | 0.492 | 57.3118 | 6.88025 | F | F | 1.4e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X045931.44-703623.3 | chandra | ccd0 | 889.735 | 1076.74 | 12.9809 | 4.12319 | 0.0038007 | 0.00120724 | 2.0623 | 0.975784 | 4.20743 | 3.54377 | 13.1276 | 11.6481 | F | F | 1.32e+21 | 5.35968e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf rmf | 5 | X050046.09-704436.1 | chandra | ccd0 | 134.378 | 77.8127 | 576.462 | 24.821 | 0.168785 | 0.00726745 | 91.5836 | 1 | 0.568247 | 0.450569 | 98.2635 | 1.52442 | F | F | 1.35e+21 | 3.96318e-12 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X050148.45-705242.6 | chandra | ccd3 | 419.833 | 291.167 | 2.86699 | 1.73206 | 0.000839429 | 0.000507132 | 6.07853 | 0.999915 | 0.492 | 0.492 | 45 | 8.20673 | F | F | 1.37e+21 | 1.1382e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X050157.18-704012.0 | chandra | ccd1 | 446.5 | 771.5 | 2.80876 | 1.73206 | 0.00082238 | 0.000507132 | 5.89961 | 0.999908 | 0.673699 | 0.492 | 116.565 | 8.14869 | F | F | 1.32e+21 | 1.03696e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X045938.61-704600.0 | chandra | ccd2 | 664.5 | 945 | 1.9595 | 1.41422 | 0.000573725 | 0.00041407 | 4.32694 | 0.998766 | 0.492 | 0.492 | 26.5651 | 5.8104 | F | F | 1.38e+21 | 6.98641e-15 | 1 | dx | ||||
| Report | 3 | X045944.43-705234.5 | chandra | ccd2 | 602.5 | 143.5 | 0.894419 | 1 | 0.000261878 | 0.000292793 | 1.97504 | 0.981636 | 0.492 | 0.492 | 90 | 8.37385 | F | F | 1.41e+21 | 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