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 LEDA 168563 73.0158 49.5506 72.064208 49.467096 77.740518 26.831198 157.24701812 3.42018054 86.3166 56536.8773611111 2013-09-01 21:03:24 56539.0592708333 2013-09-04 01:25:21 708017010 100.011 100 100.035 100.011 0 100.035 3 2 0 2 1 0 0 92.947 92.947 188.5018 1 PROCESSED 57612.530162037 2016-08-12 12:43:26 56383 2013-04-01 00:00:00 56608.7327893518 2013-11-12 17:35:13 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 081413 We propose to carry out Suzaku observations, a 100 ks each, of three Seyfert I nuclei 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. Especially we will test, by observing these targets, the ionized relativistic reflection (hereafter IRR). We will take advantage of Suzaku s unique capability of detecting hard X-rays beyond 10 keV by its HXD-PIN, simultaneously with X-rays in lower to medium energy bands by its XIS on board. With our proposed studies we will gain deeper understanding of accretion-powered AGN in general. Since the IRR takes place close to the black hole we will test the effects of strong gravity, such as the black hole spin. EXTRAGALACTIC COMPACT SOURCES 7 B SACHIKO TSURUTA USA 8 AO8 SPECTRAL STUDIES OF SOME HARD X-RAY SELECTED SEYFERT NUCLEI XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708017010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '708017010'

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