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 3C120 68.2984 5.3555 67.633855 5.251051 67.433469 -16.402094 190.37315865 -27.39441526 237.4585 53775.1527199074 2006-02-09 03:39:55 53776.2433217593 2006-02-10 05:50:23 700001010 41.9321 160 41.9321 41.9321 41.9321 41.9321 2 2 2 2 1 0 0 34.0941 34.0941 94.2219 1 PROCESSED 57532.9769791667 2016-05-24 23:26:51 54247 2007-05-27 00:00:00 53906.2470601852 2006-06-20 05:55:46 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001003 Broad line radio galaxies (BLRGs) are rare kind of AGNs where the emission from the accretion disc is visible as well as the extended jet emission. Direct comparison of broad-band spectrum in BLRGs to those of Sy-1s provides important clue to understand the formation of relativistic jets. We propose a 160 ksec (40ksec x4) observations of the brightest BLRG 3C120 with Suzaku. Recent XMM and Beppo-SAX observations confirm remarkable spectral features including fluorescent Fe line. Our goals are three folds; (1) Monitoring the variability correlation between Fe line and the Compton reflection hump, (2) Precise measurement of total luminosity as a probe of various accretion states, and (3) Resolving excess soft components, warm absorber, and 6.9 keV line, which are still under debate. EXTRAGALACTIC COMPACT SOURCES 7 A JUN KATAOKA JAP 0 SWG BROAD-BAND MONITORING OF 3C120 IN VARIOUS ACCRETING STATES XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700001010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '700001010'

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