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| Query : 2011ATel.3611....1N |
2011ATel.3611....1N - The Astronomer's Telegram, 3611, 1 (2011/August-0)
MAXI/GSC and Swift/BAT detect a new hard X-ray transient MAXI J1836-194.
NEGORO H., NAKAJIMA M., NAKAHIRA S., MORII M., KRIMM H.A., PALMER D.M., KENNEA J.A., MIHARA T., SUGIZAKI M., SERINO M., YAMAMOTO T., SOOTOME T., MATSUOKA M., UENO S., TOMIDA H., KOHAMA M., ISHIKAWA M., KAWAI N., SUGIMORI K., USUI R., TOIZUMI T., YOSHIDA A., YAMAOKA K., TSUNEMI H., KIMURA M., KITAYAMA H., SUWA F., ASADA M., SAKAKIBARA H., UEDA Y., HIROI K., SHIDATSU M., TSUBOI Y., MATSUMURA T. and YAMAZAKI K.
Abstract (from CDS):
Swift/BAT also detects this transient source in the 15-50 keV band. The best BAT position is (RA, Dec) = (278.959, -19.385; J2000) with a 90% error radius of 3 arc minutes. The source was first detected on 2011 August 29 (MJD 55802) at a rate of 0.006 ± 0.0007 ct/s/cm^2 (∼30 mCrab). The source remained at a comparable rate on Aug. 30. It was not detectable on Aug. 28 (3-sigma upper limit of 0.0025 ct/s/cm^2). It was detected on-board Swift in a 1576-second observation starting at UT 10:14:56 on Aug. 30 at 5-sigma significance, which was below the threshold for triggering.
Follow-up target of opportunity observations of MAXI J1836-194 by Swift are currently being performed and will be reported on in a later ATEL. Follow-up observations at multi-wavelengths are strongly encouraged.
Abstract Copyright: ∼
Journal keyword(s): Binary - Black Hole - Neutron Star - Transient - Pulsar
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 | MAXI J1836-194 | XB* | 18 35 43.440 | -19 19 10.48 | ~ | 163 | 0 |
| Query : 2011ATel.3611....1N |
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| MAXI J1836-194 | [OKM2018] SWIFT J1835.7-1931 |
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References (163 between 1850 and 2026) (Total 163)
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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