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 | SWIFT J0505.7-2348 | 76.4285 | -23.9055 | 75.907939 | -23.972083 | 71.84647 | -46.496539 | 225.00444872 | -33.15769393 | 284.9903 | 53826.9254166667 | 2006-04-01 22:12:36 | 53829.1216898148 | 2006-04-04 02:55:14 | 701014010 | 78.5544 | 80 | 78.5544 | 78.5544 | 78.5544 | 78.5544 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 53.4937 | 53.4937 | 189.6979 | 1 | PROCESSED | 57533.4023726852 | 2016-05-25 09:39:25 | 54439 | 2007-12-05 00:00:00 | 53945.2822569444 | 2006-07-29 06:46:27 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 010122 | The number of Compton thick AGNs is the biggest issue in the origin of the X-ray background and AGN evolution. According to the latetest population synthesis model, its estimate is strongly coupled with the broad band spectral shape of type-2 AGNs, which is only poorly understood. Recently, Swift/BAT has provided the first unbiased AGN sample above 15 keV, which includes many new type-2 AGNs that can be best followed-up with Suzaku. Here we propose to observe two of them to measure the amount of reflection component with unpreceded accuracy, a key parameter to determine the total contribution of Compton thick AGNs to the X-ray background. This proposal is complementary to our separate proposal entitled "direct determination of the fraction of Compton-thick AGNs in the local universe". | EXTRAGALACTIC COMPACT SOURCES | 7 | A | YOSHIHIRO UEDA | JAP | 1 | AO1 | BROAD BAND SPECTRA OF NEW SWIFT/BAT AGNS AND THE ORIGIN OF THE X-RAY BACKGROUND | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701014010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '701014010'
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