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 203085010 MKW4 181.11302 1.89646 180.4725 2.17482 180.26652 2.18264 276.90822 62.37023 293.80105 61201.88755 2026-06-10 21:18:04 61204.23338 2026-06-13 05:36:04 100.029 85.000 100.029 95.788 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 95.788 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-06-18 07:52:50 2099-12-31 00:00:00 2026-06-19 07:52:50 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000032059 Galaxy groups have historically received less attention than larger clusters due to their lower X-ray luminosities, resulting in their relatively understudied nature. However, they encompass a significant portion of the Universe's baryons and are crucial for understanding structure formation. Recent Hitomi observations of the Perseus cluster have demonstrated the potential for precise measurements of metal abundances with micro-calorimeters, indicating new possibilities for studying chemical enrichment processes in galaxy groups. Therefore, we propose an 85 ks observation of the MKW4 galaxy group using Resolve to capitalize on this opportunity and achieve unprecedented detail in measuring chemical enrichment at the group scale. GROUPS AND CLUSTERS OF GALAXIES 2 B ARNAB SARKAR USA 3 NOR CHEMICAL ENRICHMENT IN COOL-CORE GALAXY GROUP, MKW4 preprocessed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203085010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '203085010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏