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
xtend_exposure
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
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
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
xtend_data_mode1
xtend_data_mode2
1 201061010 3C397 286.88076 7.14565 286.27326 7.06622 289.32409 29.45953 41.12086 -0.29832 282.99838 60595.50907 2024-10-12 12:13:04 60600.03963 2024-10-17 00:57:04 186.504 150.000 157.670 1 300000A0 157.670 0.000 0.000 0.000 11110 11310 PROCESSED 2024-10-26 13:15:39 2025-10-31 00:00:00 2024-10-27 13:15:40 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011331 Thermonuclear explosions of carbon-oxygen white dwarfs (WDs), or Type Ia supernovae (SNe Ia), are important astrophysical phenomena but their exact nature still remains uncertain. Here we propose an XRISM observation of 3C 397, an ``outlier'' of Type Ia supernova remnant likely originating from a near-Chandrasekhar mass WD with an exceptionally high central density (Ohshiro et al. 2021). Thanks to the high spectral resolution of Resolve, we can measure the abundance ratios of Fe-peak elements with unprecedented accuracy. In combination with the performance verification phase observation, this SNR is fully covered by Resolve FoV, enabling us to investigate the spatial distribution of heavy elements. SUPERNOVA REMNANTS 2 B YUKEN OHSHIRO JAP 1 NOR THE SUPERNOVA REMNANT 3C 397: A PROBE FOR TYPE IA SUPERNOVAE ORIGINATING FROM EXCEPTIONALLY HIGH-DENSITY WHITE DWARFS archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201061010/ Quick Look 286.42654 6.85855 287.05344 6.71541 287.19867 7.34036 286.57015 7.48381 285.81777 6.78123 286.44388 6.63517 286.59203 7.25944 285.96431 7.40582 288.76826 29.23384 289.45321 29.0103 289.71328 29.61022 289.02395 29.83531 40.65862 -0.02997 40.81782 -0.64856 41.43893 -0.48859 41.27944 0.13077 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '201061010'

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