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".

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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 202055010 MR2251-178 343.52431 -17.58223 342.85788 -17.84877 338.06088 -9.76485 46.19688 -61.3255 245.63524 60997.48685 2025-11-18 11:41:04 61002.03407 2025-11-23 00:49:04 230.331 200.000 230.331 201.597 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 2 31100010 320000A0 215.637 201.597 0.000 0.000 11110 313430 11310 PROCESSED 2025-11-28 10:40:08 2026-12-03 00:00:00 2025-11-29 10:40:08 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000021275 The wind-driven feedback process by the ultra-fast outflows (UFOs) is believed to be key in the co-evolution of black holes and galaxies, transferring all their energy or momentum to the galactic outflows. However, the XRISM observation of the archetypal UFO source PDS 456 revealed the UFO's clumpy nature and its extremely large kinetic power, challenging simple feedback models. To reveal the true picture of the wind-driven feedback process, we propose a 200 ks observation of MR 2251-178, the brightest source showing both a UFO and a galactic outflow. Using Resolve's high resolution and Xtend's wide-band capabilities, we can detect the clumpy UFO feature and a broad UFO emission, allowing us to estimate the UFO's kinetic power and compare the UFO properties at different accretion rates. NON-JET-DOMINATED AGN 2 A KOUICHI HAGINO JAP 2 NOR REVEALING THE WIND-DRIVEN FEEDBACK PROCESS IN THE MODERATELY ACCRETING BLACK HOLE processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202055010/ WINDOW2 WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202055010'

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