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
|
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| 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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