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 201054010 RCW86_SW 220.22387 -62.67192 219.2403 -62.45774 240.72966 -44.19932 315.12495 -2.42043 114.99726 60743.60838 2025-03-09 14:36:04 60750.66741 2025-03-16 16:01:04 431.262 280.000 431.262 409.239 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 1 300000A0 409.239 0.000 0.000 0.000 11110 313430 11310 PROCESSED 2025-03-29 23:39:38 2026-04-05 00:00:00 2025-03-30 23:39:38 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000015001 Collisionless shocks are one of the most attracting phenomena in the universe, as the sites where the shock kinetic energy is transformed into thermal and non-thermal energies. They are important research targets in both physical and astronomical aspects. One of the ideal and most well-studied collisionless shocks are seen in supernova remnants. We propose a 280 ks XRISM observation of the southwestern region of RCW 86, where the Fe-K emission is brightest over the remnant. We will 1) determine Fe-Ka and Kb centroids, flux ratio and broadening, and robustly estimating the efficiency of the collisionless electron heating and reverse shock velocity, and 2) locating the reverse shock surface based on the spatial distribution of the Fe-Kb flux. SUPERNOVA REMNANTS 2 A HIROMASA SUZUKI JACCO VINK JEU 1 NOR COLLISIONLESS ELECTRON HEATING AT A REVERSE SHOCK IN THE SUPERNOVA REMNANT RCW 86 processed https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201054010/ WINDOW1 2 Observation Log: No remarks ; Pre-pipeline Log: No remarks

Used SQL

SELECT * FROM xrism_master_data WHERE observation_id = '201054010'

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