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 SBS 1301+540 196.0153 53.8063 195.478385 54.074176 163.182611 53.62856 118.79430047 63.22042238 133.9261 56991.9979976852 2014-11-30 23:57:07 56994.5141435185 2014-12-03 12:20:22 709018010 94.3176 100 94.3176 95.1576 0 95.1736 2 2 0 2 1 0 0 105.4641 105.4641 217.3498 5 PROCESSED 57617.4634143518 2016-08-17 11:07:19 57451 2016-03-04 00:00:00 57084.1361574074 2015-03-03 03:16:04 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 091411 We propose to carry out Suzaku observations, 100 ks each, of two Seyfert I nuclei, IGR J16558-5203 and SBS 1301+540, hard X-ray selected by Swift. Our goal is to distinguish between various competing models proposed for the X-ray spectra of Seyfert I nuclei. Specifically we will explore the effects of strong gravity, by testing the ionized relativistic reflection (hereafter IRR) and by measuring the spin of the black hole. We will take advantage of Suzaku s excellent capability in the broad bands from the soft through medium to hard X-ray bands. With our proposed studies we will gain deeper understanding of accretion-powered AGN in general. EXTRAGALACTIC COMPACT SOURCES 7 C SACHIKO TSURUTA USA 9 AO9 SPECTRAL STUDIES OF SOME HARD X RAY SELECTED SEYFERT NUCLEI XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/709018010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '709018010'

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