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 3C 326 238.0402 20.0989 237.485976 20.247377 230.081092 39.212111 33.27596058 48.22956027 119.5805 54484.6775 2008-01-19 16:15:36 54486.215462963 2008-01-21 05:10:16 702006010 61.7381 60 61.7381 61.7381 0 61.7381 2 2 0 2 1 0 0 53.4126 53.4126 132.8598 1 PROCESSED 57541.3565162037 2016-06-02 08:33:23 54888 2009-02-26 00:00:00 54515.0338078704 2008-02-19 00:48:41 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020014 Suzaku observations of two giant radio galaxies, 3C 326 and 3C 35, are proposed. In 60 ks exposure on the individual targets, inverse Component X-ray emission from their lobes is detected with high signal statistics. As a result, the energy densities of electrons and magnetic fields in these lobesare precisely deteremined. The size of these radio galaxies are significantly larger than that of the previous sample. Therefore, the size dependence of energetics in the lobes will be investigated. EXTRAGALACTIC COMPACT SOURCES 7 C NAOKI ISOBE JAP 2 AO2 SUZAKU OBSERVATIONS OF LOBES OF GIANT RADIO GALAXIES, 3C 326 AND 3C 35 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702006010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702006010'

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