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 | 3C382 | 278.7516 | 32.7087 | 278.287499 | 32.667445 | 283.134608 | 55.751017 | 61.3132426 | 17.46021716 | 69.589 | 54217.9621412037 | 2007-04-27 23:05:29 | 54220.8119097222 | 2007-04-30 19:29:09 | 702125010 | 130.58 | 120 | 130.588 | 130.58 | 0 | 130.588 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 122.4707 | 122.4707 | 246.1958 | 2 | PROCESSED | 57538.5400694444 | 2016-05-30 12:57:42 | 54777 | 2008-11-07 00:00:00 | 54228.2765740741 | 2007-05-08 06:38:16 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 024353 | We propose Suzaku observations of the X-ray bright Broad-Line Radio Galaxy 3C382 to study its complex broad-band X-ray spectrum and its variability on longer timescales. To this end, we ask for 3 separate observations of 40 ks each, to be scheduled randomly but not less than a couple of days apart. We aim at probing the origin of the reflection features and strong soft excess in 3C382, ultimately determining the structure and ionization state of the accretion flow. The addition of 3C382 to the Suzaku program (already including 3C120 and 3C390.3) will allow us to explore BLRGs central engines over a wide range of accretion/jet parameters. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | RITA SAMBRUNA | Jun Kataoka | USJ | 2 | AO2 | THE HIGH-ENERGY SPECTRA OF BROAD-LINE RADIO GALAXIES | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702125010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702125010'
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