Monitor of All-sky X-ray Image (MAXI)
Launch Date: June 11, 2008
Extended Mission Lifetime: 2024+ (Pending JAXA Review)
End of Operations: Limited by ISS lifetime, currently 2030
Data Archive: JAXA
MAXI is a wide-field X-ray telescope designed to perform an all-sky survey. MAXI was developed by JAXA; data processing and operations are conducted by JAXA, Riken, Osaka University, Tokyo Institute of Technology, Aoyama Gakuin University, Nihon University, Kyoto University, Miyazaki University, and Chuo University.
| Instruments | Energy Range | Field of View | Localization |
|---|---|---|---|
| Solid-state Slit Camera (SSC) | 0.5 keV–10 keV | 90°x1.5° | ≤1° (statistical + systematic, 90%) |
| Gas Slit Camera (GSC) | 2 keV–30 keV | 160°x1.5° | ≤1° (statistical + systematic, 90%) |
GCN Notice Types in GCN Classic and GCN Classic Over Kafka: Detailed Descriptions and Examples
| Type | Contents | Latency |
|---|---|---|
MAXI_UNKNOWN | Signal with no catalogued source | 200 minutes |
MAXI_KNOWN | Signal with a matched catalog source | 200 minutes |
MAXI_TEST | Test notices | n/a |
JSON-Serialized GCN Notices Types in GCN Kafka:
MAXI provides Notices for both known and unknown source detections by GSC.
The known source Notice is used when the detected event is associated with a known X-ray source or cataloged object. The unknown source Notice is used when the detected event is not immediately associated with a known source and is reported as a new or unidentified transient candidate. Depending on the available localization information, an unknown source Notice may report no position uncertainty, a circular uncertainty region, an elliptical uncertainty region, or rectangular error-region corners.
Both Notice types provide basic alert metadata, event timing, sky position, flux information, and detection information.
| Type | Contents | Latency |
|---|---|---|
gcn.notices.maxi.gsc.known | Known source detections, including source/event identification, sky position, flux information, and detection information | 200 minutes |
gcn.notices.maxi.gsc.unknown | Unknown source detections or transient candidates, including sky position, flux information, detection information, and localization information when available | 200 minutes |
MAXI known source and unknown source schemas are available. Example JSON message files are available for known source Notices and for unknown source Notices with no position uncertainty, circular, elliptical, and rectangular localization information. See the Schema Browser for more information on the properties defined in the schemas. Detailed description of the properties and examples of MAXI Notices are available in the GCN Schema GitHub project.
The MAXI team maintains an archive of their JSON Notices.
Additional Notes on MAXI/GSC Notice Fields
trigger_time
The trigger_time reported in MAXI Notices is a representative time associated with the
MAXI analysis time interval for which the detection significance is highest. This time may
not always be identical to the detection time reported later in GCN Circulars or other
follow-up reports, where a different representative time may be used depending on
the event and the details of the analysis.
flux and flux_error
The flux reported in MAXI Notices is given in units of erg cm-2 s-1 to be compatible
with the core Spectral schema. It is not directly derived from spectral analysis.
Instead, it is derived from the MAXI count rate of the source or event, normalized by the count
rate measured from Crab observations, and converted to physical flux assuming a canonical
Crab spectrum. The flux_error field gives the 1-sigma statistical uncertainty on this flux.
flux_spectral_band and flux_spectral_unit
The flux_spectral_band field specifies the energy band used for the reported flux. The
flux_spectral_unit field specifies the unit of the energy band, typically keV.
detection_timescale and detection_timescale_units
The detection_timescale field gives the time scale used in the MAXI detection analysis.
The unit is specified by detection_timescale_units, which may be s for seconds, scan
for one MAXI/GSC camera scan, orbit for one ISS orbit, or d for days.
event_name
For MAXI known-source Notices, event_name gives the name of the detected known source.
For MAXI unknown-source Notices, event_name gives the transient or GRB name when available.
Localization fields
The ra and dec fields give the source position in degrees in J2000 equatorial coordinates.
The ra_dec_error field gives the statistical localization uncertainty. When the localization is circular,
this field is a single radius in degrees. When the localization is elliptical, this field is a three-element
array giving the major radius, minor radius, and position angle of the error ellipse in degrees.
The rectangular_error_corners field gives the four corners of a rectangular error box.
Each corner is represented as an [RA, Dec] pair in degrees in J2000 equatorial coordinates.
The containment_probability field gives the probability that the true source position is contained
within the reported localization region.
The systematic_included field indicates whether the reported localization uncertainty includes
systematic uncertainty.
band_flux_low, band_flux_med, and band_flux_high
For MAXI known-source Notices, these fields provide MAXI flux estimates in predefined energy bands.
Each field is a two-element array containing [flux, flux_error], where the flux is given in erg cm-2 s-1
and the error is the 1-sigma statistical uncertainty.
band_flux_low: 2-4 keV bandband_flux_med: 4-10 keV bandband_flux_high: 10-20 keV band
Common GCN Circular Types:
| Type | Latency | Example |
|---|---|---|
| Detection of a GRB | hours | GRB 210320A |
| Observation of a GW trigger | hours | LIGO/Virgo S191110af |
| Observation of a NuEM | days | NuEm-210111A |
MAXI Yearly Trigger Rates:
| Instrument | Type | Rates |
|---|---|---|
| GSC | GRB or unknown X-ray transient | 60-70 |
| Known source | 20-25 |