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 203014010 PUPPIS_A_BEK 126.04575 -42.97174 125.61488 -42.80874 147.75078 -59.39725 260.5872 -3.11992 58.00506 61298.15005 2026-09-15 03:36:04 61302.97852 2026-09-19 23:29:04 210.063 200.000 210.063 182.358 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 182.358 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2026-09-25 21:10:27 2027-10-03 00:00:00 2026-09-26 21:10:28 03.03.015.013 gen20241115_xtd20260315_rsl20260315 Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 000031081 We propose to observe the Galactic middle-aged supernova remnant Puppis A with an exposure time of 200 ks. This observation is motivated by recent findings by a XRISM observation of this remnant: 1) Resolve possibly detected stronger-than-expected line emission from low-ionized ions, and 2) Xtend detected hard X-ray emission localized in the northeastern area. Low-ionized ions may originate from dust grains destroyed by thermal sputtering, whose X-ray signature has been long-awaited but still uncovered in hot dusty plasmas. To find solid evidence for eroding dust, we propose to observe the bright eastern knot. Xtend's large field of view can cover the hard X-ray emitting region, allowing us to map the distribution of the hard X-ray emission. SUPERNOVA REMNANTS 2 B SATORU KATSUDA JAP 3 NOR FIRST DETECTION OF X-RAY SIGNATURES OF ERODING DUST AND CONFIRMATION OF POSSIBLE HARD X-RAY EMISSION IN PUPPIS~A SNR processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/203014010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '203014010'

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