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 | 201062010 | G344.7-0.1 | 255.95821 | -41.71689 | 255.0774 | -41.64725 | 258.9695 | -18.81379 | 344.66569 | -0.16375 | 269.99717 | 60914.75769 | 2025-08-27 18:11:04 | 60917.54241 | 2025-08-30 13:01:04 | 121.753 | 100.000 | 121.753 | 108.405 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 108.405 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 11310 | PROCESSED | 2025-09-04 17:07:06 | 2026-09-12 00:00:00 | 2025-09-05 17:07:09 | 03.02.014.010 | gen20241115_xtd20241115_rsl20241115 | Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 | 000011333 | Although Type Ia SNe have attracted a great deal of interest, the explosion mechanism is still controversial. So far, two possible scenarios have been put forward: explosion of a white dwarf close to the Chandrasekhar limit (near-Ch) or smaller than the limit (sub-Ch). According to the latest theories, abudances and velocity structures significantly differ between the near-/sub-Ch models. Here we propose a XRISM observation of G344.7-0.1, which is one of the brightest Type Ia SNR. While previous studies suggest detections of Cr and Mn, the measurement is still uncertain and better precision measurements are required. This observation will reveal abundances of rare elements and their velocity structures, both of which are critical to elucidate the explosion mechanism of Type Ia SNe. | SUPERNOVA REMNANTS | 2 | C | MOE ANAZAWA | JAP | 1 | NOR | UNVEILING EXPLOSION MECHANISM OF TYPE IA SNR G344.7-0.1 BY MEASURING RARE ELEMENTS AND VELOCITY STRUCTURES WITH XRISM | processed | https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201062010/ | WINDOW1 | 1 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '201062010'
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