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.
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
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 3C400.2 SW 294.5545 17.147 293.991762 17.032549 300.267467 38.043132 53.47817432 -2.17482828 81.5886 56761.5284375 2014-04-14 12:40:57 56762.0730555556 2014-04-15 01:45:12 509069010 24.1528 20 24.1528 24.1528 0 24.1537 2 2 0 2 1 0 0 23.915 23.915 47.0479 3 PROCESSED 57614.2434027778 2016-08-14 05:50:30 57138 2015-04-26 00:00:00 56772.6111226852 2014-04-25 14:40:01 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 092010 Mixed morphology supernova remnants are an important, but peculiar class of supernova remnants. They have a shell-type morphology in the radio, but the X-ray emission is centrally dominated. X-ray spectroscopy of several of these supernova remnants, indicate that their central plasma is often over-ionised and have enhanced abundances. Here we propose to study a typical member of this class, which has so far not received much attention, despite being bright and only mildly absorbed: 3C400.2. The remnant can be covered with four pointings, and is bright enough for imaging spectroscopy on the scale of the Suzaku PSF. This will enable us to study spectroscopic variation, confirm the preliminary detection of an RRC and map its distribution, and study the abundances. GALACTIC DIFFUSE EMISSION 5 A JACCO VINK EUR 9 AO9 THE MIXED-MORPHOLOGY SUPERNOVA REMNANT 3C400.2 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509069010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '509069010'

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