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 | 3C120 | 68.2996 | 5.3511 | 67.635075 | 5.246657 | 67.433996 | -16.406625 | 190.37800916 | -27.39591229 | 261.0003 | 55971.7483564815 | 2012-02-14 17:57:38 | 55974.8819907407 | 2012-02-17 21:10:04 | 706042020 | 118.0689 | 120 | 118.0689 | 118.0689 | 0 | 118.0689 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 103.5365 | 103.5365 | 270.7359 | 2 | PROCESSED | 57604.7019791667 | 2016-08-04 16:50:51 | 55652 | 2011-04-01 00:00:00 | 55992.3150694444 | 2012-03-06 07:33:42 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 066003 | We propose deep Suzaku observations of 6 well-known AGN with the primary aim of studying strong-gravitational physics close to these supermassive black holes (SMBH). We will conduct the first ever census of local SMBH spin, providing a new window on the growth-history of SMBHs. Suzaku's unique combination of high-throughput in the iron-K band and hard-band (>10keV) sensitivity is crucial, permitting a separation of the disk-reflection spectrum (which encodes the relativistic physics) from the effects of the warm absorber and low-velocity emission/reflection. These six datasets will be an important legacy of Suzaku, providing an important resource for AGN researchers for at least the next decade. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | CHRISTOPHER REYNOLDS | USA | 6 | AO6-KP | A SURVEY OF BLACK HOLE SPIN AND RELATIVISTIC PHYSICS IN AGN | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706042020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '706042020'
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