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 | J081618.99+482328.4 | 124.0768 | 48.3841 | 123.174595 | 48.53824 | 114.890427 | 27.844597 | 171.01809871 | 33.69777889 | 298.4793 | 54917.0925462963 | 2009-03-27 02:13:16 | 54919.0946643518 | 2009-03-29 02:16:19 | 703042010 | 90.9224 | 90 | 90.9224 | 90.9224 | 0 | 90.9224 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 81.0739 | 81.0739 | 172.9637 | 2 | PROCESSED | 57545.9726736111 | 2016-06-06 23:20:39 | 55329 | 2010-05-13 00:00:00 | 54930.3718055556 | 2009-04-09 08:55:24 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031337 | We have discovered polar broad absorption-line quasars (BALQSOs) from their radio variabilities. We know their inclination angles. Our results derived from the archival Chandra data of one polar BALQSO indicate that the X-ray emissions are from the jet and the X-ray absorbing gas is located at tens of parsecs above the accretion disk corona. We want to confirm these results at high confidence level using better signal to noise ratio data from a big observatory, like SUZAKU. In addition, we propose to observe three more polar BALQSOs, which have wide range of radio/UV/X-ray properties. Our primary science goal of this proposal is to determine the radial distribution of the X-ray absorbing gas in 4 polar BALQSOs. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | KAJAL GHOSH | USA | 3 | AO3 | PROBING THE INNER STRUCTURE OF AGNS USING THE POLAR BALQSOS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703042010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703042010'
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