Table A.1.
Various details of the X-ray pulsators in the GC plus Galactic disk.
| lat | lon | ObsID | Poserr | Period (s) | PF | XMM Name | PGaia | Sig | Type | References | |
|---|---|---|---|---|---|---|---|---|---|---|---|
| arcsec | Our | Previous | 2–10 keV | > σ | |||||||
| 351.4972 | -0.3537 | 0886070601 | 0.14 | 414.5 ± 1.4 | 414.8 | 68.4 ± 1.6 | 4XMM J172511.3–361657 | 4 × 10−4 | 3 | NS HMXRB | Zurita Heras et al. (2006) |
| 353.1032 | -0.6956 | 0861171201 | 0.73 | 607.5 ± 3.7 | 45.6 ± 10.8 | 4XMM J173058.9–350812 | 1.5 × 10−2 | 3 | Likely IP | ||
| 354.7018 | 0.4782 | 0916800201 | 0.35 | 517.6 ± 3.6 | 41.3 ± 12.5 | XMMU J173029.8–330920 | 1 × 10−3 | 3 | Unknown | Mondal et al. in prep | |
| 357.1486 | -1.6563 | 0865510101 | 0.48 | 614.2 ± 1.4 | 614 | 28.2 ± 4.5 | 4XMM J174517.0–321358 | 4 × 10−3 | 3 | IP | Vermette et al. (2023) |
| 357.3792 | -2.0600 | 0743980401 | 0.57 | 4768.3 ± 151.5 | 4860 | 74.2 ± 22.4 | 4XMM J174728.9–321441 | 2.1 × 10−2 | 3 | Polar | Wevers et al. (2017) |
| 357.6116 | 0.3037 | 0886020101 | 0.79 | 5067.3 ± 260.5 | 57.9 ± 16.2 | 4XMM J173837.0–304818 | 1.2 × 10−2 | 3 | Likely Polar | ||
| 358.3043 | 0.2442 | 0886010601 | 0.48 | 432.4 ± 1.9 | 432.1 | 54.8 ± 7.7 | 4XMM J174033.8–301501 | 6.8 × 10−3 | 3 | IP | Mondal et al. (2022) |
| 359.2786 | 0.9300 | 0764191201 | 0.17 | 623.2 ± 2.6 | 626 | 37.2 ± 3.8 | 4XMM J174016.0–290337 | 1.4 × 10−3 | 3 | IP | Farrell et al. (2010) |
| 359.2882 | -1.0793 | 0152920101 | 0.65 | 2179.6 ± 18.2 | 64.1 ± 19 | 4XMM J174809.8–300616 | 2.5 × 10−2 | 3 | Unknown | ||
| 359.4941 | 1.0946 | 0764191101 | 0.6 | 725.9 ± 3.5 | 729 | 45.1 ± 6.8 | 4XMM J174009.0–284725 | 3.2 × 10−2 | 3 | IP | Kaur et al. (2010) |
| 359.8061 | -1.2096 | 0801683401 | 0.56 | 997.7 ± 7.6 | 1001.5 | 31 ± 8.9 | 4XMM J174954.6–294336 | 7.7 × 10−2 | 3 | IP | Mondal et al. (2023) |
| 0.0036 | -1.9883 | 0801682901 | 0.76 | 2917.0 ± 68.5 | 54.9 ± 12.7 | 4XMM J175327.8–295716 | 1.8 × 10−1 | 2 | Likely Polar | ||
| 0.1413 | -0.1089 | 0762250301 | 0.32 | 1737.7 ± 5.4 | 1745 | 15.8 ± 3.7 | 4XMM J174622.7–285218 | 2.5 × 10−3 | 2 | IP | Muno et al. (2009) |
| 0.1476 | -2.2564 | 0402280101 | 0.59 | 552.1 ± 1.4 | 45.1 ± 9.8 | 4XMM J175452.0–295758 | 9.9 × 10−2 | 3 | Unknown | ||
| 0.5849 | -1.5353 | 0801682801 | 0.49 | 672.5 ± 3.0 | 77.8 ± 18.9 | 4XMM J175301.3–291324 | 7.7 × 10−2 | 3 | Likely IP | ||
| 0.7407 | -0.4932 | 0801681301 | 0.44 | 1209.7 ± 11.7 | 1212.4 | 44.3 ± 8.3 | 4XMM J174917.7–283329 | 1.3 × 10−2 | 3 | IP | Mondal et al. (2023) |
| 0.7632 | -1.3587 | 0801682601 | 0.97 | 6784.4 ± 439.5 | 73 ± 20.4 | 4XMM J175244.4–285851 | 2.8 × 10−1 | 3 | Likely Polar | Bahramian et al. (2021) | |
| 0.9918 | -0.0821 | 0783160101 | 0.47 | 593.6 ± 0.7 | 593 | 41.3 ± 7.3 | 4XMM J174816.9–280750 | 6.8 × 10−2 | 3 | IP | Sidoli et al. (2006) |
| 1.3573 | 1.0522 | 0201200101 | 1.9 | 3195.8 ± 116.3 | 3200 | 28.9 ± 6.5 | 4XMM J174445.6–271344 | 6.2 × 10−1 | 3 | NS/WD ? | Lopes de Oliveira et al. (2006) |
| 1.4196 | -2.2266 | 0782770201 | 0.51 | 354.68 ± 0.7 | 47.6 ± 10.9 | 4XMM J175740.5–285105 | 9.2 × 10−1 | 3 | Likely IP | ||
| 1.5909 | 0.0633 | 0510010401 | 1.9 | 132.1 ± 0.3 | 132 | 28.9 ± 3.4 | 4XMM J174906.8–273233 | 2.0 × 10−1 | 3 | NS HMXRB | Karasev et al. (2008) |
| 2.6999 | -0.7212 | 0886081101 | 0.59 | 1.36652 ± 2 × 10−5 | 48.1 ± 12.6 | XMMU J175441.9–265919 | 7.7 × 10−3 | 3 | Likely NS XRB | ||
| 3.5626 | -0.3453 | 0886081301 | 0.53 | 1134.5 ± 12.4 | 79.1 ± 14.4 | 4XMM J175511.6–260315 | 1.7 × 10−2 | 3 | Likely IP | ||
| 3.5766 | -0.3953 | 0886081301 | 0.51 | 392.5 ± 1.5 | 28.2 ± 5 | 4XMM J175525.0–260402 | 1.5 × 10−2 | 3 | Likely NS XRB | ||
| 4.4701 | 0.6376 | 0840910501 | 0.36 | 4093.3 ± 182.3 | 34.8 ± 6.1 | 4XMM J175328.4–244627 | 8.8 × 10−2 | 3 | Likely Polar | ||
| 6.3308 | -0.4448 | 0886110501 | 0.64 | 5215.9 ± 7.5 | 61.8 ± 19.3 | XMMU J180140.3–234221 | 1.7 × 10−2 | 2 | Likely Polar | ||
Notes. The details of the X-ray pulsators, including the positional information, XMM-Newton detection ID, and the source association in the 4XMM catalog. The source XMMU J173029.8–330920, XMMU J175441.9–265919, and XMMU J180140.3–234221 are the first time detected by XMM-Newton in our ongoing Heritage survey of the Galactic disk. We also searched for Swift-XRT and Chandra counterparts of these two sources, but no counterparts were found. The PGaia represents the probability of spurious association with a Gaia source.
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