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 201114010 COMA_OFFSET_N 194.94136 28.04897 194.33839 28.31829 181.45946 31.46227 59.93018 87.93793 105.84454 60689.45560 2025-01-14 10:56:04 60692.67019 2025-01-17 16:05:04 144.847 135.000 144.847 148.103 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 148.103 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-01-21 15:49:25 2026-01-23 00:00:00 2025-01-22 15:49:26 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000014004 Though crucial for cluster physics, direct measurements of the intracluster medium (ICM) velocity structure are scarce. Recent advancements have enabled ICM velocity measurements in various clusters using the XMM-Newton EPIC-pn instrument. This employs Cu Ka line for recalibration. In the Coma cluster, distinct velocities, likely linked to subgroup mergers, have been identified. To explore further, the exceptional capabilities of the XRISM instruments are vital. Hence, we propose a 135 ks observation of the Coma cluster to map its ICM velocity structure and investigate potential merging scenarios. GROUPS AND CLUSTERS OF GALAXIES 2 B EFRAIN GATUZZ EUR 1 NOR ICM VELOCITY STRUCTURE UNVEILED: THE COMA CLUSTER MERGING NATURE processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201114010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201114010'

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