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 | 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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