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 202073010 Cas_A_SW 350.83523 58.79664 350.26954 58.52208 27.34766 54.84294 111.72139 -2.14432 78.50563 61188.25560 2026-05-28 06:08:04 61192.09727 2026-06-01 02:20:04 242.424 150.000 242.424 162.170 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 162.170 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-06-05 18:06:34 2099-12-31 00:00:00 2026-06-06 18:06:34 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000021420 We propose 150 ks XRISM observation of the southwestern region of supernova remnant (SNR) Cassiopeia A (Cas A). Our goals are to observe an enhanced forbidden-to-resonance (f/r) ratio in a region where the radio observation suggested an interaction between SNR and molecular cloud (SNR/MC interaction) and to determine the f/r ratio accurately in a region where an anomalous value was observed in the PV phase. Based on the XRISM/Resolve spectra in PV observation, we have detected a narrow spectral component and discovered an enhanced f/r ratio in the western rim. These features are expected consequences of the ejecta/MC interaction. The proposed observation provides an independent test of this scenario, as the planned region includes the area of suspected SNR/MC interaction. GALACTIC DIFFUSE EMISSION AND SURVEYS 2 C HARUTO SONODA JAP 2 NOR INTERACTION BETWEEN THE SUPERNOVA REMNANT CASSIOPEIA A AND MOLECULAR CLOUD preprocessed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202073010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '202073010'

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