DARTS/Astro Query System - SQL Search -

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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 300013030 3C397 286.91107 7.12972 286.30349 7.05014 289.3559 29.43974 41.12055 -0.33236 103.00106 60405.30352 2024-04-05 07:17:04 60407.70491 2024-04-07 16:55:04 103.517 100.000 103.517 94.405 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 94.405 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2024-09-24 19:00:04 2025-08-31 00:00:00 2024-04-23 16:23:06 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000031 Yield of Fe-peak elements (Cr, Mn, Fe, Ni) and Ti in Type Ia supernovae is the critical information for understanding their explosion mechanism. Especially in single degenerate systems where the progenitor mass is near the Chandrasekhar mass limit, mass ratios among Fe-peak elements and Ti are greatly sensitive to the central density of the progenitor. Here we propose a XRISM observation of 3C 397, a remnant of single degenerate Type Ia supernova. Utilizing the extremely high energy resolution of Resolve, we put strong constraint of {Cr,Mn,Ni}/Fe and Ti/Fe. We will observationally probe the central density of the progenitor for the first time. SUPERNOVA REMNANTS 3 C XRISM Collaboration JAP 0 NOR PROBING CENTRAL DENSITY OF TYPE IA SUPERNOVA PROGENITOR IN SINGLE DEGENERATE SYSTEM BY AN OBSERVATION OF 3C 397 archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300013030/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '300013030'

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