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 201041010 G349.7+0.2 259.50074 -37.43846 258.65087 -37.38568 261.41246 -14.31163 349.72898 0.17094 90.00147 60733.96949 2025-02-27 23:16:04 60737.47921 2025-03-03 11:30:04 206.068 300.000 206.068 185.727 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 185.776 0.046 0.000 0.000 11110 313430 11310 PROCESSED 2025-03-07 14:52:36 2026-04-05 00:00:00 2025-03-08 14:52:37 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011218 Although a textbook explanation says that stars with a mass between 8-30M_sun explodes as a standard core-collapse supernova (SN), the true mass range is still unknown: stars with masses at the lower limit of this range are believed to experience electron capture SN and such SNe is thought to eject large amount of nickel (Ni) during the explosion. Here we propose an observation of G349.7+0.2, whose Ni abundance is highest among all the SNRs. While our previous analysis has large uncertainties, XRISM has the capability to accurately determine the yields of Fe-group elements and their velocity structures, providing valuable insights into the lower mass limit for standard SNe and potentially offer the first robust evidence of electron capture SN in our Galaxy. SUPERNOVA REMNANTS 2 B HIROYUKI UCHIDA JAP 1 NOR INVESTIGATING THE NATURE OF NI-RICH SNR G349.7+0.2: SEARCHING FOR FIRST ROBUST EVIDENCE OF ELECTRON-CAPTURE EXPLOSION processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201041010/ WINDOW1 1 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201041010'

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