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 | 3C 390.3 | 280.629 | 79.7686 | 281.497615 | 79.715169 | 81.957835 | 76.491681 | 111.4356997 | 27.05756334 | 197.286 | 54083.1426851852 | 2006-12-14 03:25:28 | 54085.1384722222 | 2006-12-16 03:19:24 | 701060010 | 0.024 | 100 | 99.3678 | 99.3678 | 0.024 | 99.3678 | 2 | 2 | 1 | 2 | 1 | 0 | 0 | 97.8813 | 97.8813 | 172.4199 | 3 | PROCESSED | 57536.3784722222 | 2016-05-28 09:05:00 | 54702 | 2008-08-24 00:00:00 | 54132.9968055556 | 2007-02-01 23:55:24 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011363 | We propose Suzaku observations of the X-ray bright Broad-Line Radio Galaxies 3C382 and 3C390.3 to study their complex broad-band X-ray spectra. The HXD will constrain the continuum above 10 keV, discriminating between competing physically-different models, while at the same time the XIS will determine the parameters of the FeKalpha line and the shape of the soft X-rays. The proposed observations will allow us to shed light on the origin of reflection features in radio-loud AGN, ultimately determining the structure and ionization state of the accretion flow in these objects. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | RITA SAMBRUNA | USA | 1 | AO1 | THE BROAD-BAND X-RAY SPECTRUM OF BROAD-LINE RADIO GALAXIES | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701060010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '701060010'
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