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 201092010 A2034 227.5489 33.51047 227.04412 33.69924 211.49775 48.69869 53.57168 59.53069 321.39531 60843.47782 2025-06-17 11:28:04 60846.38894 2025-06-20 09:20:04 126.838 120.000 126.838 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 313430 11310 PROCESSED 2025-07-15 01:43:09 2026-07-04 00:00:00 2025-06-26 07:48:18 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012133 Velocity power spectra (PS) of the ICM are necessary for testing multi-scale physics in numerical simulations and measuring turbulent dissipation/plasma properties. XRISM allows direct studies of ICM kinematics, but the large PSF makes it challenging to extract PS. However, by combining high-resolution imaging and spectroscopic missions, one can calibrate indirect methods of measuring PS. We aim to test the relation between turbulent Mach numbers measured with XRISM and ICM density fluctuations probed with Chandra by observing two clusters, A2034/A1914, with 120/100 ks exposures. These clusters have dissimilar fluctuations measured over a wide scale range, which is ideal for our goal. This calibration will provide a robust method to measure velocity PS and probe ICM transport properties. GROUPS AND CLUSTERS OF GALAXIES 2 B IRINA ZHURAVLEVA USA 1 NOR COMBINING XRISM AND CHANDRA FOR ROBUST VELOCITY POWER SPECTRA MEASUREMENTS IN THE ICM archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201092010/ Quick Look 227.50775 33.51433 227.54625 33.47408 227.58624 33.50079 227.57984 33.50741 227.58782 33.51265 227.55584 33.54624 227.0029 33.70324 227.04127 33.66286 227.08149 33.68942 227.07511 33.69607 227.08314 33.70127 227.05126 33.73498 211.44789 48.68825 211.5171 48.66455 211.54681 48.70251 211.53534 48.70639 211.54133 48.71388 211.4837 48.73372 53.58248 59.56478 53.50019 59.53459 53.54975 59.50005 53.56327 59.50507 53.57297 59.49817 53.64158 59.52321 HELIUM A75A 2021-12-13 00:00:00

Used SQL

SELECT * FROM xrism_resolve_data WHERE observation_id = '201092010'

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