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'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏