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 201123010 ABELL2142 239.57587 27.23704 239.05874 27.37907 229.18665 46.4587 44.23416 48.69612 318.00176 60889.74241 2025-08-02 17:49:04 60892.33824 2025-08-05 08:07:04 111.817 100.000 111.817 105.876 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 105.876 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-08-09 12:54:01 2026-08-15 00:00:00 2025-08-10 12:54:02 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000014047 We propose to observe the core of Abell 2142 with XRISM for 100 ks to map turbulence and bulk motions with the exquisite spectral resolution of RESOLVE. XRISM will costrain the level of turbulence in the core of the brightest and nearest clusters and it is thus important to map a variety of dynamical states. A2142 stands up for (1) its high flux in the 2-10 keV band, ideal for a gate-valve closed observation; (2) its intermediate state between a relaxed cool core and a violent merger, mirrored by an unusual radio emission; (3) its rich variety of motions suggested by its extreme sloshing and a close pair of BCGs with extreme difference in velocity along the line of sight. Therefore, A2142 is an ideal target for an AO1 XRISM observation. GROUPS AND CLUSTERS OF GALAXIES 2 C FABIO GASTALDELLO EUR 1 NOR AN ATLAS OF MOTIONS IN A2142 AT HIGH SPECTRAL RESOLUTION WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201123010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201123010'

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