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'
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