DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
| No. |
observation_id
|
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
exposure
|
awarded_exposure
|
resolve_exposure
|
xtend_exposure
|
resolve_data_mode
|
resolve_with_filter_be
|
resolve_with_filter_fe55
|
resolve_with_filter_nd
|
resolve_with_filter_poly
|
resolve_with_filter_open
|
resolve_with_filter_undef
|
is_resolve_gatevalve_closed
|
is_resolve_mxs1
|
is_resolve_mxs2
|
is_resolve_mxs3
|
is_resolve_mxs4
|
xtend_number_modes
|
xtend_dataclass_file1
|
xtend_dataclass_file2
|
xtend_window1_exposure
|
xtend_window2_exposure
|
xtend_window1_burst_exposure
|
xtend_window2_burst_exposure
|
xtend_code
|
resolve_code
|
gen_code
|
processing_status
|
processing_date
|
public_date
|
distribution_date
|
processing_version
|
caldb_version
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
proposal_type
|
proposal_title
|
observation_status
|
data_access_url
|
xtend_data_mode1
|
xtend_data_mode2
|
processing_count
|
remarks
|
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 202000010 | GX339-4 | 255.70535 | -48.79084 | 254.75751 | -48.71984 | 259.58491 | -25.86707 | 338.93811 | -4.32691 | 81.15424 | 61077.18824 | 2026-02-06 04:31:04 | 61078.01394 | 2026-02-07 00:20:04 | 41.262 | 30.000 | 41.262 | 35.749 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 2 | 31100010 | 320000A0 | 38.238 | 35.749 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2026-02-12 03:58:02 | 2027-02-19 00:00:00 | 2026-02-13 03:58:02 | 03.03.015.012 | gen20241115_xtd20250915_rsl20250915 | Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 | 000022002 | The evolution of accretion disks as a function of the Eddington-scaled mass accretion rate is at the heart of black hole fueling and ejection. A central prediction is that the inner disk should be truncated below a threshold in M-dot because cooling becomes inefficient. This is the basis for radiatively- inefficient accretion flow models (RIAFs), and may the key to jet production. Yet, even in stellar-mass black holes, observations offer little clear evidence of disk truncation at accessible fluxes. In the recurrent transient GX 339-4, however, there is enough continuum and Fe K-a line flux at an Eddington fraction of 0.001 to obtain definitive, positive evidence of disk truncation in a 30 ks XRISM exposure. We request a TOO observation of GX 339-4 in Cycle 2. | BH AND NS BINARIES | 2 | A | JON MILLER | USA | 2 | NOR-TOO | A DEFINITIVE MEASUREMENT OF DISK TRUNCATION WITH XRISM | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202000010/ | WINDOW2 | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '202000010'
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