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
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 300055010 W49B_East 287.79356 9.09746 287.19512 9.01376 290.67235 31.26866 43.26944 -0.19979 67.99998 60423.07088 2024-04-23 01:42:04 60430.95699 2024-04-30 22:58:04 332.527 100.000 272.655 1 300000A0 272.655 0.000 0.000 0.000 11110 11310 PROCESSED 2024-09-26 05:59:21 2025-08-31 00:00:00 2024-05-15 06:53:31 03.00.013.009 gen20240315_xtd20240815_rsl20240815 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000000084 The Suzaku's discovery of recombining plasma in supernova remnants (SNRs) was a surprise because it is never expected in the fiducial Sedov model. We propose to observe the brightest recombining SNR W49B to reveal the origin of this new class of SNRs based on the high-resolution spectroscopy using XRISM/Resolve. We will identify the cooling process that formed the recombining state based on measurements of the electron temperature, ion temperature, and charge-state distribution. We will also constrain the progenitor type that regulates the SN environment, by bias-free measurements of the ejecta mass ratios of the Fe-group elements. Additionally, as an ideal goal, we will search for the signature of interaction with supra-thermal electrons and constrain the injection efficiency. SUPERNOVA REMNANTS 3 A XRISM Collaboration JAP 0 NOR TRACING A MISSING BRANCH IN THE SNR EVOLUTION: RECOMBINING PLASMA IN W49B archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/3/300055010/ Quick Look 288.00133 9.59106 287.40111 9.3513 287.64528 8.757 288.2454 8.99672 287.40518 9.5064 286.80397 9.26942 287.04525 8.67399 287.64637 8.91093 290.99331 31.72777 290.26485 31.57456 290.44675 30.95233 291.17159 31.10479 43.8019 -0.15319 43.31566 0.26103 42.89982 -0.22724 43.38671 -0.64195 WINDOW1

Used SQL

SELECT * FROM xrism_xtend_data WHERE observation_id = '300055010'

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