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| Query : 2011ATel.3663....1P |
2011ATel.3663....1P - The Astronomer's Telegram, 3663, 1 (2011/September-0)
Swift Detection of an Intermediate Duration Burst from SAX J1712.6-3739.
PALMER D.
Abstract (from CDS):
(RA, Dec) = (258.161, -37.649) = (17h 12m 39s, -37d 38' 56") (J2000)
with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty).
Based on downlinked BAT data from T-120s to T+300s, the emission started
at T-75s, rising smoothly to a peak at T+100s, and declining to near zero at T+200s. The counts are almost all in the 15-25 keV band. Over
the time interval T-74s to T+188s the data are well-fit by OTTB (T∼4.7 keV) or Blackbody (T∼2.7 keV) models with fluence above 15 keV of ∼1.7x10^-6 erg/cm^2
The XRT began observing the field at 20:13:25.9 UT, 117.4 seconds after the BAT trigger. XRT found a bright X-ray source located at
(RA, Dec) = (258.1528, -37.6469) = (17h 12m 36.67s, Dec(J2000) = -37d 38' 48.8") (J2000)
with an uncertainty of 5.9 arcseconds (radius, 90% containment). This position is 15.6 arcseconds from the catalogued location of a known X-ray source: 1RXS J171237.1-373834 in the ROSAT RASSBSC catalogue (identified by SIMBAD with SAX J1712.6-3739 and positionally consistent
within the joint ROSAT-XRT uncertainty).
The XRT light curve shows near-constant emission until ∼T+220s, followed
by high-amplitude variation on multiple timescales for at least 7 minutes. Over T+120s to T+800s, the XRT spectrum is well fit by an absorbed black-body, kT=2.18 ± 0.07 keV and N_H = 1.69 ± 0.14 x 10^22 cm^-2. The average absorption-corrected flux is ∼2x10^-8 erg/s/cm^2.
This timescale indicates that event is an intermediate duration burst (typical timescale ∼30 minutes), not a superburst (typical timescale ∼10
hours), and not an ordinary Type I burst (typical timescale ∼10 seconds). (See Cumming et al. 2006, ApJ 646, 429.)
The history of this source includes an ordinary Type I burst seen by BAT in July 2010 (ATel #2717; Strohmeyer & Baumgartner, 2010) and an intermediate duration burst in 1999 found in RXTE/ASM archival data (ATEL #2141; Kuulkers, 2009).
Abstract Copyright: ∼
Journal keyword(s): Gamma Ray - Neutron 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 | [KRL2007b] 228 | LXB | 17 12 37.0 | -37 38 42 | 12.25 | ~ | 81 | 0 |
| Query : 2011ATel.3663....1P |
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| INTEGRAL1 47 |
1RXS J171237.1-373834
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SWIFT J1712.8-3737 | [KRL2007b] 228 |
| INTREF 758 | SAX J1712.6-3739 | SWIFT J1712.6-3736 | |
| PBC J1712.6-3737 | SRGA J171237.0-373843 | XMMSL1 J171236.3-373841 |
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References (81 between 1850 and 2026) (Total 81)
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
Data at NED - NASA/IPAC Extragalactic Database : [KRL2007b] 228
Link by name to the catalogue in VizieR :
| 1RXS J171237.1-373834 |
Search by coordinates in Vizier (radius: 5 arcsec)
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