Archive for February, 2010

Thank you, Soichi!

Friday, February 26th, 2010

Soichi Noguchi, the Japanese astronaut currently onboard the ISS, installed a new data converter for MAXI.   MAXI has two channels for the data telemetry. One is the “low speed line”, or, if you are familiar with the space flight tech, MIL-STD-1553B, which is robust and reliable, but the bandpath is limited.   The other is called “medium speed line”, which is in fact a wired ethernet similar to what you find in your office, and should be able to transmit  mega bits per second.   GSC can transmit the essential science data over the low speed line, but SSC relies heavily on the medium speed line.  Due to a misunderstanding in a network protocol, combined with the design feature of MAXI data processor, the transmission over the ethernet was never smooth.  We had to modify the header in the ethernet packets, and had to filter out broken or illegal ethernet frames which can occur in a crowded LAN.  Since a few months after the launch, we used a laptop computer already present in JEM as a filtering bridge, but it was not stable either.  Several times we had to reboot MAXI to recover the communication over the medium speed line.

With the latest shuttle flight, a new device “Armadillo” specifically designed for this job was transported from the ground, and Soichi installed it in the network.  Now MAXI seems to be happily sending out data in the medium speed line.

Mrk 421 in Flare!

Thursday, February 18th, 2010

Latest X-ray light curve of Mrk 421

Latest X-ray light curve of Mrk 421 in 1-day biniing

Markarian 421, a BL Lac object, is currently undergoing a bright X-ray flare. We have reported the news to Astronomers Telegram #2444. Following is the posted text.

MAXI/GSC has detected a bright X-ray flare from a BL Lac object Mrk 421. Its X-ray flux increased to 156 +- 11 mCrab (1.5 – 10 keV) on 2010 February 16 (mid MJD = 55243.5) from <30 mCrab on 2010 February 14. The current flux is higher than that in the recent bright X-ray flare reported by MAXI on 2010 January 01 (116 +- 10 mCrab, ATEL #2368). Multiwavelength observations of this source are encouraged.

The latest light curve and image of this source are available at the following URL:  http://maxi.riken.jp/sourcelist.html.

Sudden drop of the flux in GX 339-4

Thursday, February 18th, 2010

MAXI light curves of GX 339-4 show a sudden drop of the flux on Feb 15, 2010. This is probably due to the shade by the solar paddles of the ISS, and not real. Some data on Feb 16 show that the source having a hard spectrum seems to be brighter.

Observational condition near the Galactic center including GX 339-4 has been wrong since the beginning of this month. The method of corrections for the shade of the paddles and a space shuttle are still under development.

Pulsation of Crab was detected.

Wednesday, February 10th, 2010

The 33ms pulsation of  Crab pulsar was detected by MAXI/GSC. The timing information of X-ray photons were verified to be correct. The figure  shows data from Jan. 1 to Jan. 7, 2010.  Pulse profile of Crab

MAXI/GSC detection of a short X-ray transient

Thursday, February 4th, 2010

scan_2-10kev_weblc_2-20

The MAXI team reported a detection of a transient X-ray source to GCN (#10359) and Atel (#2415). The pictures above show the error box of the position and the light curve (in 2-20 keV) of the transient.