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 202060010 IRAS_F05189-2524 80.25601 -25.36233 79.74555 -25.4107 76.69511 -48.35257 227.8888 -30.29253 269.99929 61111.26255 2026-03-12 06:18:04 61119.55213 2026-03-20 13:15:04 341.958 300.000 341.958 313.924 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 313.924 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-03-26 15:33:51 2027-04-10 00:00:00 2026-03-27 15:33:51 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000021348 Ultrafast outflows (UFOs) launched near supermassive black holes (SMBHs) are key to understanding AGN feedback, which is crucial to the co-evolution of galaxies and their central SMBHs. However, the acceleration mechanism remains unclear and is a major open question. During the XRISM PV phase, we observed the AGN-starburst composite system IRAS 05189 2524 and identified at least three UFO components with distinct bulk velocities and velocity widths. In AO2, we propose a 300 ksec follow-up observation to probe variability in each UFO component and investigate correlations with X-ray luminosity. This will provide new insights into the acceleration mechanism and enable robust estimates of outflow properties, which are essential for quantifying AGN feedback and its impact on galaxy evolution. NON-JET-DOMINATED AGN 2 A HIROFUMI NODA JAP 2 NOR XRISM STUDY OF THE VARIABILITY OF ULTRA-FAST OUTFLOWS WITH MULTIPLE VELOCITIES & VELOCITY WIDTHS IN IRAS 05189-2524 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202060010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202060010'

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