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 201032010 TOOTHBRUSH_S 90.83052 42.20197 89.93751 42.20385 90.64976 18.76455 170.24565 9.72421 278.86915 60728.54102 2025-02-22 12:59:04 60731.55282 2025-02-25 13:16:04 166.747 100.000 166.747 137.308 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 137.308 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-03-06 14:16:20 2026-03-11 00:00:00 2025-03-07 14:16:20 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011171 At radio frequencies, the Toothbrush Cluster is a spectacular source that has been essential in revealing details of the particle acceleration generated during mergers. We propose to map the velocity field of the intracluster medium in this remarkable target with two Resolve pointings. One will probe the radio halo, where particle acceleration is driven by developed turbulence. The second will probe the region between the halo and the 2~Mpc-long radio shock, where strong gradients in the radio spectral index map indicate a transition between turbulence-driven and shock-driven acceleration. Determining and comparing the line broadening and shifts between these regions will provide key information needed to complete physical picture of cosmic ray electron acceleration on the largest scales. GROUPS AND CLUSTERS OF GALAXIES 2 A HIROKI AKAMATSU JAP 1 NOR PROBING THE PHYSICS OF TURBULENT PARTICLE ACCELERATION IN ``THE TOOTHBRUSH'' processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201032010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201032010'

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