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
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
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
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner5_ra
corner5_dec
corner6_ra
corner6_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner5_ra_b1950
corner5_dec_b1950
corner6_ra_b1950
corner6_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner5_ecliptic_lon
corner5_ecliptic_lat
corner6_ecliptic_lon
corner6_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
corner5_galactic_lon
corner5_galactic_lat
corner6_galactic_lon
corner6_galactic_lat
resolve_adr_mode
resolve_thr_name
resolve_shp_date
1 201050010 ABELL3667_CF_IN 303.26525 -56.88616 302.26445 -57.03687 291.71928 -35.92823 340.79538 -33.46648 250.00111 60614.74588 2024-10-31 17:54:04 60618.79241 2024-11-04 19:01:04 298.903 180.000 298.903 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 313430 11310 PROCESSED 2024-11-08 15:32:02 2025-11-13 00:00:00 2024-11-09 15:32:02 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011257 Cluster mergers are the most energetic events in the Universe since the Big Bang. A large fraction of the merger energy is dissipated in the ICM, a process that depends on a number of unknown microphysical properties of the ICM. Resolve will provide the first opportunity to detect and map the bulk and turbulent velocities in the ICM of nearby merging systems. We propose to observe a textbook example of a cold front in Abell 3667, a striking phenomenon caused by a merger. Resolve observations of this cold front would yield the bulk and turbulent velocities as a function of the distance from the interface, determining the origin of the front and providing a basis for the derivation of microphysical constraints from cold fronts, and answer a host of other interesting questions. GROUPS AND CLUSTERS OF GALAXIES 2 C YUTO ICHINOHE JAP 1 NOR GAS DYNAMICS IN THE MOST STRIKING CLUSTER COLD FRONT archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201050010/ Quick Look 303.23849 -56.91744 303.32711 -56.89985 303.30019 -56.85973 303.2856 -56.86269 303.28041 -56.85471 303.20661 -56.86925 302.23715 -57.06803 302.32637 -57.05081 302.2999 -57.01058 302.28521 -57.01348 302.2801 -57.00548 302.2058 -57.01972 291.69149 -35.95442 291.7549 -35.95053 291.75078 -35.90793 291.74032 -35.90862 291.73959 -35.90017 291.68679 -35.90332 340.75811 -33.45147 340.77841 -33.50008 340.82675 -33.48592 340.82334 -33.47791 340.83295 -33.47517 340.81612 -33.43465 HELIUM A75A 2021-12-13 00:00:00

Used SQL

SELECT * FROM xrism_resolve_data WHERE observation_id = '201050010'

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