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 201020010 ABELL3395_SOUTH 96.70153 -54.54647 96.4492 -54.5146 108.31294 -77.5593 263.31153 -25.26554 221.74343 60709.15838 2025-02-03 03:48:04 60714.04241 2025-02-08 01:01:04 266.408 190.000 266.408 202.825 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 202.825 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-02-13 11:49:00 2026-02-14 00:00:00 2025-02-14 11:49:00 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011129 We propose conducting high-resolution spectroscopic observations of A3391/95, the unique triple galaxy cluster at z=0.05. Despite sharing a common large-scale structure, these clusters exhibit distinct merger stages and radio emissions, as revealed by eROSITA. Utilizing XRISM, we aim to accurately constrain bulk and turbulent motions at 150 and 200 km/s levels, respectively, and distinguish between the generation processes of gas motions attributed to AGN feedback and merger activity. Comparative analysis with multi-wavelength data and simulations will provide insights into the origins of gas motion and feedback processes within the cluster cores. GROUPS AND CLUSTERS OF GALAXIES 2 C NAOMI OTA JAP 1 NOR AGN-ICM INTERACTION IN THE INTERACTING CLUSTER SYSTEM A3391/95 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201020010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201020010'

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