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 | IRAS 00182-7112 | 5.1458 | -70.9276 | 4.573856 | -71.205097 | 312.979414 | -61.496651 | 306.55074146 | -45.98323945 | 33.8687 | 56050.171087963 | 2012-05-03 04:06:22 | 56052.8759143518 | 2012-05-05 21:01:19 | 707036010 | 93.959 | 90 | 93.967 | 93.959 | 0 | 93.959 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 86.5766 | 86.5766 | 233.6819 | 1 | PROCESSED | 57605.3998263889 | 2016-08-05 09:35:45 | 56435 | 2013-05-23 00:00:00 | 56068.6299537037 | 2012-05-21 15:07:08 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 071441 | We propose to observe with the Hard X-ray Detector onboard Suzaku the two Ultraluminous Infrared Galaxies IRAS 00182-7112 and IRAS 12127-1412, both of which are known to harbour very luminous and highly obscured active galactic nuclei (AGN). An AGN reflection component arising from ionized gas is clearly identified at 2 10 keV: the detection of the direct AGN emission above 10 keV and the measure of the reflection efficiency would provide fundamental information on both the physical structure of Compton-thick AGN embedded in a nuclear starburst and their feedback on the surrounding environment. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | EMANUELE NARDINI | USA | 7 | AO7 | THE PHYSICAL STRUCTURE OF COMPTON-THICK AGN/ULIRGS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707036010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '707036010'
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