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 IRAS 09104+4109 138.3378 40.9513 137.53478 41.157946 128.03448 23.67766 180.99146588 43.55010524 90.0004 55883.9878356482 2011-11-18 23:42:29 55885.7675694444 2011-11-20 18:25:18 706038010 81.3276 80 81.3356 81.3276 0 81.3356 2 2 0 2 1 0 0 76.5883 76.5883 153.73 2 PROCESSED 57603.9341203704 2016-08-03 22:25:08 56264 2012-12-03 00:00:00 55895.209849537 2011-11-30 05:02:11 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 062009 We propose to observe IRAS 09104+4109 for 80 ks with Suzaku in order to confirm the ~3 sigma BeppoSAX PDS detection of the source and increase the detection significance with the HXD/PIN to 10 sigma in the 10--80 keV band, allowing the detailed spectral shape to be determined. IRAS 09104+4109 is a hyperluminous Type 2 quasar embedded in a central cluster galaxy at redshift 0.442. It is likely to be the hard-X-ray-brightest such object observed with Suzaku and could well be the prototype Compton-thick Type 2 quasar. The Suzaku observation, especially above 10 keV will most likely reveal one of the most luminous Compton--thick Type 2 QSO to date. EXTRAGALACTIC COMPACT SOURCES 7 C CHIA-YING CHIANG EUR 6 AO6 THE TYPE 2 HYPERLUMINOUS QUASAR IRAS 09104+4109 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706038010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '706038010'

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