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 201117010 OPHIUCHUS_CLUSTER_SE 258.12864 -23.39293 257.37035 -23.33385 259.11662 -0.40103 0.56109 9.24672 94.84379 60762.93199 2025-03-28 22:22:04 60765.92782 2025-03-31 22:16:04 116.627 100.000 116.627 103.281 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 103.281 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-16 10:39:47 2026-04-16 00:00:00 2025-04-13 14:24:01 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000014021 Radio jets are powered by gas accretion onto supermassive black holes and inflate large bubbles in galaxy and cluster atmospheres. The energy input is substantial, but must be distributed and dissipated on large scales to suppress gas cooling and slow massive galaxy growth. We propose a 100ks Resolve observation of the Ophiuchus cluster to measure turbulence and bulk motion in the wake of the largest radio bubble on the sky. The bubble's wake reveals no unrelated structure and is well-matched to Resolve's field of view. By measuring the induced gas motions, we will determine the fraction of the bubble's enthalpy that is transferred to the intracluster medium (ICM), whether turbulence or bulk motion dominates and if bubbles can lift gas flows in their wakes to sustain feedback. GROUPS AND CLUSTERS OF GALAXIES 2 A HELEN RUSSELL EUR 1 NOR GAS MOTIONS IN THE WAKE OF THE LARGEST RADIO BUBBLE IN A CLUSTER CORE processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201117010/ WINDOW1 4 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201117010'

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