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 | 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 | 332.527 | 272.655 | PX_NORMAL | N | Y | N | N | Y | Y | Y | OFF | OFF | OFF | OFF | 1 | 300000A0 | 272.655 | 0.000 | 0.000 | 0.000 | 11110 | 313430 | 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/ | WINDOW1 | 2 | Observation Log: No remarks ; Pre-pipeline Log: No remarks |
Used SQL
SELECT * FROM xrism_master_data WHERE observation_id = '300055010'
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