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 201042010 ABELL2029 227.73304 5.74453 227.11328 5.93287 223.53039 22.62623 6.47267 50.54594 284.99867 60873.53616 2025-07-17 12:52:04 60876.45213 2025-07-20 10:51:04 118.349 100.000 118.349 104.679 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 104.679 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-07-26 07:29:29 2026-08-01 00:00:00 2025-07-27 07:29:29 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000011220 The core region of A2029 is an excellent laboratory for estimating the Ni abundance because of a relatively hot intracluster medium (ICM) at roughly 6 keV, and constraining the contribution from Type Ia supernovae that are the monopoly manufacturer of Ni. Even though the A2029 center has two XRISM performance verification (PV) datasets, the total exposure is short (only 40 ks) and not enough to provide a strong constraint on the Ni abundance, particularly in the innermost core. Here, we suggest extending the PV observation data by doing a deep 100 ks observation of the A2029 core. This observation will reveal the Type Ia characteristics in A2029 with an accurate estimation of Ni. We will also show how AGN feedback and/or sloshing impact the dynamical evolution of the ICM. EXTRAGALACTIC DIFFUSE EMISSION AND SURVEYS 2 C KOTARO FUKUSHIMA JAP 1 NOR ESTIMATING THE SN IA ENRICHMENT AND GAS DYNAMICS IN THE CENTRAL REGION OF THE A2029 CLUSTER WITH XRISM processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201042010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201042010'

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

Go to top of this page ⏏