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 | MRK 1 | 19.06 | 33.0289 | 18.361574 | 32.765252 | 30.564721 | 23.029207 | 128.90716196 | -29.55492804 | 249.7486 | 54111.5318171296 | 2007-01-11 12:45:49 | 54114.5836111111 | 2007-01-14 14:00:24 | 701047010 | 126.4441 | 120 | 126.4441 | 126.4441 | 0 | 126.4441 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 126.0122 | 126.0122 | 263.6237 | 2 | PROCESSED | 57637.5831944445 | 2016-09-06 13:59:48 | 54702 | 2008-08-24 00:00:00 | 54133.1552314815 | 2007-02-02 03:43:32 | 3.0.22.44 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011336 | The supermassive black holes of active galactic nuclei (AGN) are fundamentally connected to the stars of their host galaxies, but it is not clear whether this relationship is evident at X-ray energies. We will test the prediction that prolific star formation is responsible for the soft X-ray emission from a Compton thick AGN that also contains a powerful circumnuclear starburst. The AGN's deep obscuration facilitates the soft X-ray measurements, and Compton thick AGN are generally significant, both as a large fraction of the local AGN population and for their contribution to the X-ray background. Furthermore, we will use the direct measurement of the intrinsic AGN luminosity to test unified AGN models and the validity of indirect luminosity indicators. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | NANCY LEVENSON | USA | 1 | AO1 | TESTING THE STARBURST-AGN CONNECTION AND MEASURING DEEPLY OBSCURED AGN | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701047010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '701047010'
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