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
xtend_exposure
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
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
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_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
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
xtend_data_mode1
xtend_data_mode2
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 19:01:04 298.903 180.000 243.336 1 300000A0 243.336 0.000 0.000 0.000 11110 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 302.85355 -57.3717 303.96238 -57.15165 303.55253 -56.55072 302.4578 -56.76757 301.84429 -57.5207 302.96076 -57.30519 302.55746 -56.70261 301.45543 -56.91495 291.29128 -36.33589 292.08165 -36.2871 292.01805 -35.64782 291.23304 -35.69632 340.21756 -33.23688 340.46755 -33.84069 341.19534 -33.62852 340.94053 -33.02544 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '201050010'

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