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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