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 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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