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
|
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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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