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 | MCG0208 | 43.0963 | -8.5129 | 42.484335 | -8.717227 | 37.842662 | -23.868775 | 185.55840319 | -55.88722126 | 57.4541 | 55016.0987037037 | 2009-07-04 02:22:08 | 55017.2134722222 | 2009-07-05 05:07:24 | 704045010 | 42.9115 | 40 | 42.9435 | 42.9115 | 0 | 42.9195 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 36.7878 | 36.7878 | 96.286 | 5 | PROCESSED | 57547.7724768518 | 2016-06-08 18:32:22 | 55395 | 2010-07-18 00:00:00 | 55027.1160532407 | 2009-07-15 02:47:07 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 041414 | We propose to use Suzaku to measure the amount of absorption, the intensity of Compton reflection component and other spectral components for a sample of 5 AGN selected from our ultra-deep, 3 Msec, INTEGRAL survey. These observations are ~3x deeper than the INTEGRAL and Swift/BAT all-sky surveys. Both the absorption distribution and the intensity of the Compton reflection component are fundamental parameters in understanding the AGN population. In fact, the uncertainty in the latter quantity is the main reason why the X-ray background can not be used to constrain the number of Compton Thick AGN. We have supporting multi-wavelength observations for all sources, critical to measure other source parameters like bolometric luminosity, re-radiated emission, black hole mass, etc. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | EZEQUIEL TREISTER | USA | 4 | AO4 | THE NATURE OF THE FAINTEST HARD X-RAY SELECTED AGN | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704045010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '704045010'
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