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 | 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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