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 902002010 GS1354-64 209.53991 -64.73415 208.61407 -64.49075 236.1089 -48.24567 309.97731 -2.779 102.0024 61060.15144 2026-01-20 03:38:04 61063.16741 2026-01-23 04:01:04 128.637 100.000 128.637 13.468 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31300010 320000A0 107.524 0.000 0.000 13.468 11110 313430 11310 PROCESSED 2026-01-27 12:48:47 2023-09-06 00:00:00 2026-01-28 12:48:47 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000029006 A new outburst is currently taking place in the black hole X-ray binary system known as GS 1354-64. The level of its flux has reached 100 milli-Crab, and it is continuing to rise. Based on the hard X-ray data with NuSTAR, the source is supposed to be a black hole candidate that is spinning at a high rate; however, XRISM has never been observed such a kind of binaries. In order to resolve the iron line region of GS 1354-64, we request a 100 kilo-seconds XRISM observation using Resolve. This could be helpful in isolating any narrow characteristics that were not able to be resolved by the CCD-resolution data that was collected in the past, and it could also yield more accurate measurements of the black hole spin. BH AND NS BINARIES 9 A XRISM Collaboration DDT 2 DDT-TOO DDT TOO REQUEST OF GS 1354-64 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/9/902002010/ WINDOW2BURST WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '902002010'

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