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 | 202049010 | SN1987A | 83.86802 | -69.2701 | 83.95966 | -69.29965 | 307.58252 | -86.44576 | 279.70377 | -31.93657 | 301.00728 | 61143.72227 | 2026-04-13 17:20:04 | 61151.93199 | 2026-04-21 22:22:04 | 505.580 | 300.000 | 505.580 | 414.114 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 414.114 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2026-05-02 15:04:09 | 2027-05-12 00:00:00 | 2026-05-03 15:04:10 | 03.03.015.013 | gen20241115_xtd20260315_rsl20260315 | Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003 | 000021197 | SN1987A is the unique SN in which human beings can see the evolution from SN to SNR. Now 37 years post-explosion, the predominant X-ray emissions are transitioning from the shocked CSM to ejecta. Resolve spectra in PV (2024) are well described by NEI model from 'non-metal rich' ejecta, which aligns with the outer low-metallicity envelope of ejecta (XRISM collaboration 2025). Therefore, the reverse shock has not yet reached the inner pure ejecta. The line Doppler widths in PV reflect bulk motion of ejecta; AO-2 (2026) observation will examine 10^{9-10} km inner part of ejecta. Per 3D MHD simulations (Orlando et al 2025), AO-2 and future observations will highlight 'pure ejecta' emissions, which grow mostly during AO-2. Such new features are crucial for understanding SN to SNR evolution. | SUPERNOVA REMNANTS | 2 | B | YUKIKATSU TERADA | JAP | 2 | NOR | XRISM VIEW OF SN TO SNR EVOLUTION OF SN1987A | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/202049010/ | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '202049010'
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