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 | 203008010 | OPHIUCHUS_CLUSTER_NW | 258.06221 | -23.33927 | 257.30425 | -23.27987 | 259.05144 | -0.35255 | 0.57016 | 9.32747 | 274.83997 | 61290.51810 | 2026-09-07 12:26:04 | 61291.43824 | 2026-09-08 10:31:04 | 43.576 | 100.000 | 43.576 | 44.047 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 44.047 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2026-09-18 18:27:42 | 2099-12-31 00:00:00 | 2026-09-19 18:27:43 | 03.03.015.013 | gen20241115_xtd20260315_rsl20260315 | Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 | 000031064 | Recent XRISM observations of the Ophiuchus galaxy cluster revealed a puzzling contradiction: despite morphological evidence of core disruption including cold fronts, the velocity structure is remarkably quiescent (\sigma_v ~ 115 km s^-1). Two scenarios have been proposed: (1) sloshing motion approaching a turning point with minimal velocities, or (2) core motion nearly parallel to the sky plane. We propose a 300ks XRISM observation of the western core regions, where preliminary analysis suggests elevated velocity dispersions. This will distinguish between the scenarios and offer a full understanding of the dynamics and evolution of this unique, high-temperature, cool-core cluster. | GROUPS AND CLUSTERS OF GALAXIES | 2 | B | YUTAKA FUJITA | JAP | 3 | NOR | RESOLVING THE CORE MOTION PARADOX IN THE OPHIUCHUS GALAXY CLUSTER | preprocessed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203008010/ | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '203008010'
Your request has been accepted.
The download will start soon automatically.