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 201011010 IGR_J17091-3624 257.28158 -36.40766 256.4411 -36.34436 259.50383 -13.43064 349.52432 2.21243 91.34595 60724.19866 2025-02-18 04:46:04 60725.28755 2025-02-19 06:54:04 45.803 40.000 45.803 5.129 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31300010 320000A0 40.948 0.000 0.000 5.129 11110 313430 11310 PROCESSED 2025-02-27 04:43:01 2026-03-04 00:00:00 2025-02-28 04:43:01 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011083 We propose ToO observations of a Galactic transient black hole X-ray binary with a high inclination angle, during the state transition. Resolve high-resolution spectroscopy in the state where wind absorption lines have been observed enables us to obtain essential wind parameters (such as density, velocity, and the ionization stage) to determine the wind structure and launching mechanism. We also search for weak absorption and emission lines from the wind (and also jets) in the states where significant lines have rarely been observed in X-rays. Moreover, we have organized a multi-wavelength monitoring campaign simultaneously with the XRISM observations, from which we can achieve the whole picture of the evolution of the accretion disk, disk wind, and jets. BH AND NS BINARIES 2 A MEGUMI SHIDATSU JAP 1 NOR-TOO UNDERSTANDING EVOLUTION OF DISK WIND IN BLACK HOLE X-RAY BINARIES processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201011010/ WINDOW2BURST WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201011010'

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