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 KAZ 102 270.6661 67.6374 270.701804 67.634057 77.059679 88.893324 97.62313354 29.55178422 2.066 53895.6833101852 2006-06-09 16:23:58 53896.5343055556 2006-06-10 12:49:24 701012010 41.454 40 41.454 41.462 41.47 41.47 2 2 2 2 1 0 0 40.9507 40.9507 73.5199 2 PROCESSED 57534.6269328704 2016-05-26 15:02:47 54394 2007-10-21 00:00:00 53928.2501157407 2006-07-12 06:00:10 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010112 We propose to make a detailed broad-band X-ray spectroscopic study of the radio quiet QSO (RQQ) Kaz 102. This RQQ had a power-law spectrum with a photon index ~ 1 with our ASCA observation. We also found a spectral variability over the time scale of years, from ~ 2.2 during the ROSAT All Sky Survey to ~ 1 during the Einstein / ASCA observations. From our ASCA spectra, we couldn't discriminate whether the apparently unusual hard spectrum was caused by warm absorber, Compton reflection, or a simple featureless power-law continuum. High quality and wide-band spectroscopy with Suzaku is essential to unveil the physical nature of the enigmatic hardness and spectral variability of Kaz 102. EXTRAGALACTIC COMPACT SOURCES 7 B YOSHITAKA ISHISAKI JAP 1 AO1 WHAT IS THE PHYSICAL NATURE OF KAZ 102: AN ENIGMATIC X-RAY HARD RADIO QUIET QSO? HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701012010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701012010'

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