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 227 146.9365 7.4245 146.275614 7.656926 146.610705 -5.546093 228.57888407 42.2858038 108.3139 56237.0794675926 2012-11-06 01:54:26 56239.0279513889 2012-11-08 00:40:15 707004010 82.5325 80 82.5405 82.5325 0 82.5405 2 2 0 2 1 0 0 71.4299 71.4299 168.3338 0 PROCESSED 57608.0036342593 2016-08-08 00:05:14 56631 2013-12-05 00:00:00 56264.6488773148 2012-12-03 15:34:23 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070012 Radio galaxies are a key class to understand the origin and effects of AGN feedback to the surroundings. However, the fundamental question, how the structure of the nucleus is different between AGNs with and without jets, is not resolved yet. A key parameter to understand the accretion flow is the Eddington ratio. BLRGs of 4C 50.55 and 3C 120 are rare objects having high Eddington ratio (L_bol/L_Edd~0.4) compared with Seyferts and typical BLRGs (< 0.1). Though the accretion disks in many BLRGs are known to be truncated and/or inner parts covered by corona, unified picture of accretion flows over a wide range of accretion rate is far from established. Therefore we propose observing a BLRG of 3C 227, which has the highest Eddington ratio in the hard X-ray luminous BLRGs. EXTRAGALACTIC COMPACT SOURCES 7 C FUMIE TAZAKI JAP 7 AO7 STUDY OF NUCLEAR STRUCTURE OF BLRGS WITH HIGH ACCRETION RATE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707004010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '707004010'

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