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 202010010 ABELL520 73.54139 2.91608 72.88741 2.83568 72.52859 -19.53051 195.80939 -24.33229 264.99739 61091.88546 2026-02-20 21:15:04 61095.91324 2026-02-24 21:55:04 187.007 200.000 187.007 179.792 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 179.792 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-03-03 11:21:10 2027-03-06 00:00:00 2026-03-04 11:21:11 03.03.015.012 gen20241115_xtd20250915_rsl20250915 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000022109 Observing shock fronts offers insights into complex intracluster medium (ICM) transport mechanisms, such as electron-ion equilibrium and thermal conduction, which remain poorly understood. A key unresolved puzzle revolves around the mechanism of electron and ion heating by these collisionless shocks. Long-standing observational discrepancies have obscured our understanding of the electron heating mechanism behind shock fronts, presenting a significant puzzle that has persisted for decades. To decisively unravel this longstanding mystery, we propose 200 ks Resolve observations of the Abell 520 galaxy cluster, our prime target for directly constraining the electron heating mechanism behind a shock front. GROUPS AND CLUSTERS OF GALAXIES 2 B ARNAB SARKAR USA 2 NOR PROBING ELECTRON HEATING MECHANISM IN ABELL 520 WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202010010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202010010'

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