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 202034010 AWM7_P2 43.55685 41.60485 42.74777 41.40179 53.6692 23.84376 146.28442 -15.6323 269.99929 61055.37991 2026-01-15 09:07:04 61060.15144 2026-01-20 03:38:04 218.122 200.000 218.122 209.941 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 209.941 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-01-24 10:32:18 2027-01-29 00:00:00 2026-01-25 10:32:18 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000022156 AGN feedback regulates gas cooling in galaxy clusters, but the precise role of AGN-driven turbulence remains unclear. We propose three XRISM observations of the cool-core cluster AWM 7 to map its ICM velocity dispersion and directly compare with Perseus Cluster PV studies. Unlike Perseus, AWM 7 shows no signs of active AGN feedback, but shares similar redshift and sloshing signatures. By matching radial and line-of-sight scales, these observations test whether small-scale gas motions found in Perseus arise from AGN feedback. Our goals include measuring turbulence, non-thermal pressure support, chemical abundance profiles, and resonant scattering. AWM 7, as a bright feedback-free cluster, provides a unique opportunity to isolate the kinematic role of AGN feedback in cluster cores. GROUPS AND CLUSTERS OF GALAXIES 2 B HANNAH MCCALL USA 2 NOR A TALE OF TWO DRIVERS: UNDERSTANDING THE KINEMATIC ROLE OF AGN FEEDBACK processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202034010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202034010'

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