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 201006010 OPHIUCHUS_CLUSTER 258.114 -23.36865 257.35585 -23.3095 259.10124 -0.37793 0.57343 9.27166 94.84313 60765.92782 2025-03-31 22:16:04 60771.49380 2025-04-06 11:51:04 217.118 200.000 217.118 188.844 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 188.844 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-04-12 17:22:44 2026-04-16 00:00:00 2025-04-13 17:22:44 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011075 The Ophiuchus cluster, the second brightest X-ray source, provides a unique study of an exceptionally hot (9keV) cluster. Despite high temperatures indicating merger disruption, it has retained its cool core. Previous observations conflict on the internal gas velocity in the core, ranging from <100 to >2000km/s. We will use the spectral resolution of XRISM to precisely measure the velocity, resolve the discrepancy, and reveal the core destruction processes. The obtained velocity will allow the estimation of instability timescales that drive core evolution. We will also study elemental abundances to see if the population of supernovae differs from cooler clusters. This multi-pronged approach will provide insights into the formation and evolution of this extraordinary cluster. GROUPS AND CLUSTERS OF GALAXIES 2 B YUTAKA FUJITA JAP 1 NOR UNVEILING THE DYNAMICS AND CHEMICAL ENRICHMENT OF THE OPHIUCHUS GALAXY CLUSTER WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201006010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201006010'

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