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 201080010 Perseus_O3 50.03411 41.38614 49.20722 41.20582 58.63367 22.20009 150.70062 -13.33138 82.8782 60880.42366 2025-07-24 10:10:04 60882.41046 2025-07-26 09:51:04 92.411 90.000 92.411 92.536 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 92.536 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-31 12:09:49 2026-08-07 00:00:00 2025-08-01 12:09:49 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000012080 Feedback from Active Galactic Nuclei (AGN) is crucial for regulating cooling and star formation in galaxy clusters. Gas motions driven by the feedback could be important in heating the gas. We propose a multi-pointing observational program for the Perseus cluster, totaling 500 ks. We will study radial and azimuthal variations of gas kinematics and metallicity within the cluster core, mapping a transition between feedback- and mergers-dominated regions, which is crucial for distinguishing various feedback scenarios and revealing the role of turbulence in AGN feedback. We will probe gas sloshing, motions driven by rising bubbles, and turbulence association with the radio mini halo. These observations will be of legacy value, complementing large multi-wavelength data sets on Perseus. GROUPS AND CLUSTERS OF GALAXIES 2 C IRINA ZHURAVLEVA USA 1 NOR MAPPING GAS KINEMATICS IN THE X-RAY BRIGHTEST GALAXY CLUSTER processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201080010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201080010'

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