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| Query : 2011ATel.3218....1C |
2011ATel.3218....1C - The Astronomer's Telegram, 3218, 1 (2011/March-0)
Chandra localization of SAX J1806.5-2215.
CHAKRABARTY D., JONKER P. and MARKWARDT C.B.
Abstract (from CDS):
The source was detected with a measured source intensity of 1.61(4) count/s or 0.64(4) count/frame, uncorrected for pileup. We estimate a pileup fraction of less than 30 percent. The best-fit X-ray source position is:
RA(J2000) = 18h 06m 32.177s
Dec(J2000) = -22d 14' 17.20"
with an uncertainty radius of 0.6 arcsec (90% confidence). We note that this is somewhat outside the recently reported 2.0 arcsec (90% confidence) Swift X-ray error circle (ATEL #3202), lying 5.4 arcsec from its center. No other sources were detected in the 1x8 arcmin ACIS subarray field. Our measured source position is not consistent with any of the sources detected in a 2001 archival Chandra image taken during the quiescent state of SAX J1806.5-2215 (Cornelisse et al. 2002, A&A, 392, 931).
Abstract Copyright: ∼
Journal keyword(s): Star - Transient
Simbad objects: 1
| Number of rows : 1 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | [OKM2018] SWIFT J1806.5-2223 | LXB | 18 06 34 | -22 15.1 | ~ | 58 | 0 |
| Query : 2011ATel.3218....1C |
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| SAX J1806.5-2215 | [OKM2018] SWIFT J1806.5-2223 |
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References (58 between 1850 and 2026) (Total 58)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center
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