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 202091010 4U1746-37 267.55183 -37.05167 266.70117 -37.03771 267.98971 -13.62946 353.53098 -5.00413 97.00278 61107.58407 2026-03-08 14:01:04 61109.20699 2026-03-10 04:58:04 65.243 60.000 65.243 54.962 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 58.790 54.962 0.000 0.000 11110 313430 11310 PROCESSED 2026-03-13 08:48:06 2099-12-31 00:00:00 2026-03-14 08:48:07 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000024014 We propose to exploit the superior and unprecedented spectral capabilities of XRISM to X-ray the most energetic components of the central Galactic outflow, to securely confirm, or definitely invalidate, the tantalizing hints of up to 5 approaching and receding shells of high velocity, hot gas, tentatively seen in the Chandra-HETG spectrum of 4U 1746-37 via FeXXV-XXVI absorption. This will allow us not only to establish for the first time the existence of such high-energetic components of the Galactic outflow but also to study with unprecedented precision their physics and kinematics, one giant leap towards our understanding of the origin of the Galactic outflow, the physics at play in the Galactic center and the general problem of galaxy-SMBH co-evolution throughout the Universe lifetime. BH AND NS BINARIES 2 B FABRIZIO NICASTRO EUR 2 NOR X-RAYING THE GALACTIC OUTFLOW WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202091010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202091010'

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