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 SN1006 225.7268 -41.9424 224.908794 -41.746586 235.456683 -23.661429 327.58003425 14.55159393 117.0193 54521.6264351852 2008-02-25 15:02:04 54526.8613310185 2008-03-01 20:40:19 502046010 211.7373 200 211.7453 211.7373 0 211.7453 2 2 0 2 1 0 0 184.3622 184.3622 417.2759 6 PROCESSED 57541.8622337963 2016-06-02 20:41:37 54904 2009-03-14 00:00:00 54535.729375 2008-03-10 17:30:18 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020052 Thermal plasma incident SN1006 has very interesting characteristic. Suzaku PV spectrum revealed ionization parameter of the plasma is significantly low. We investigated the spatial variation of the ionization parameter, and found the outer region of SN1006 has lower ionization parameter than the inner region. However, since the center region of SN1006 is placed on the edge of FOV in the PV observation, the spectra have poor statistics, and the ionization state and the metal abundance cannot be decided with good precision. We propose to observe the center region of SN1006 deeply to decide the physical condition of the plasma of young SNR. Necessary exposure time is 150ksec. GALACTIC DIFFUSE EMISSION 5 A HIROYA YAMAGUCHI JAP 2 AO2 THE CENTER REGION OF SN1006 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502046010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '502046010'

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