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 | 202039010 | ABELL2256_P1 | 256.06685 | 78.63996 | 256.77676 | 78.70528 | 102.46376 | 77.30502 | 111.00004 | 31.74038 | 229.98506 | 60975.25769 | 2025-10-27 06:11:04 | 60978.58269 | 2025-10-30 13:59:04 | 181.636 | 150.000 | 181.636 | 167.797 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 167.797 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2025-11-07 11:57:44 | 2026-11-13 00:00:00 | 2025-11-08 11:57:45 | 03.03.015.012 | gen20241115_xtd20250915_rsl20250915 | Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 | 000022190 | XRISM PV results on merging galaxy clusters show low velocity dispersion, at the lower end of cosmological simulation predictions. This raises questions on turbulence development timescales, implemented physics in the simulations, and whether the PV sample favors more relaxed clusters. To address this, we propose three Resolve pointings (510 ks total) of A2256 - a complex merger with disturbed X-ray morphology and striking radio structures. We will map gas kinematics and, supported by simulations of the A2256 analog, interpret its complexity, reconstruct merger geometry and energy partition. Correlating peculiar radio emission variations with gas motions will test cosmic ray re-acceleration models. We will constrain the velocity power spectrum, building on the first such attempt in Coma. | GROUPS AND CLUSTERS OF GALAXIES | 2 | B | IRINA ZHURAVLEVA | USA | 2 | NOR | ICM TURBULENCE IN THE MERGING CHAOS OF ABELL 2256 | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202039010/ | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '202039010'
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