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 201098010 ABELL2163_CENTER 243.93879 -6.14531 243.27146 -6.02155 243.12818 14.89586 6.76383 30.47109 292.00046 60884.27296 2025-07-28 06:33:04 60889.74241 2025-08-02 17:49:04 223.164 200.000 223.164 205.202 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 205.202 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-08-06 11:02:21 2026-08-09 00:00:00 2025-08-07 11:02:22 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012147 Abell 2163 is the hottest, most massive low redshift cluster in the universe. It is actively merging along the line-of-sight, with a Bullet-like cool core driving a turbulence-generating shock front ahead of it that has accelerated one of the most powerful radio halos known--a property known to correlate with higher turbulent velocity dispersion. With a single pointing of the center, we aim to measure turbulent line broadening, velocity offsets, and ion temperatures from the lines in the 6.7 keV and 7 keV Fe complexes with Resolve in two regions: one covering the reheated cool core and the other likely dominated by gas moving in the opposite direction. We will also constrain the larger-scale thermodynamic structure of the cluster with Xtend and NuSTAR. EXTRAGALACTIC DIFFUSE EMISSION AND SURVEYS 2 B DANIEL WIK USA 1 NOR GAS DYNAMICS IN THE LINE-OF-SIGHT MERGER ABELL 2163 WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201098010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201098010'

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