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 300073010 COMA_CENTER 194.94363 27.94653 194.3405 28.21584 181.51561 31.37171 57.29432 87.97895 285.8439 60500.30352 2024-07-09 07:17:04 60509.20699 2024-07-18 04:58:04 402.101 200.000 356.832 1 300000A0 356.832 0.000 0.000 0.000 11110 11310 PROCESSED 2024-09-21 10:35:08 2025-08-31 00:00:00 2024-07-28 19:44:44 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000102 We propose the first direct measurement of the power spectrum of turbulence in the intracluster medium. The spectrum determines the flow of kinetic energy down the turbulent cascade and the amount that dissipates into heat and feeds cosmic ray acceleration and magnetic field amplification. The nearby Coma cluster is the best system for such a measurement, as it does not have a cool core or a powerful AGN, thus all gas motions should be merger-generated and the turbulence should develop in an isotropic, textbook fashion. Our full mosaic of 5 pointings will yield a measurement of the power spectrum normalization and injection scale, a combination that determines the energy flow. Our minimum case is the first detection of turbulence in a merging cluster using the central pointing. GROUPS AND CLUSTERS OF GALAXIES 3 A XRISM Collaboration JAP 0 NOR FIRST DIRECT MEASUREMENT OF THE POWER SPECTRUM OF INTERGALACTIC TURBULENCE archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300073010/ Quick Look 194.41892 27.68139 195.11267 27.50823 195.31167 28.12496 194.61337 28.29927 193.81407 27.95134 194.50927 27.77734 194.70976 28.39382 194.00996 28.56898 181.17054 30.92622 181.90211 31.04733 181.76156 31.67735 181.02436 31.55522 55.06831 88.50917 44.19517 87.96239 58.14084 87.60974 70.36038 88.05528 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '300073010'

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