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 | ESP 39607 | 11.5922 | -40.0968 | 10.997666 | -40.369881 | 351.254657 | -40.701682 | 307.24150307 | -76.98900447 | 243.1952 | 55549.7680208333 | 2010-12-19 18:25:57 | 55551.3175810185 | 2010-12-21 07:37:19 | 705048010 | 60.6687 | 60 | 60.6927 | 60.6687 | 0 | 60.6847 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 48.9555 | 48.9555 | 133.8399 | 3 | PROCESSED | 57554.5018402778 | 2016-06-15 12:02:39 | 55960 | 2012-02-03 00:00:00 | 55593.2278472222 | 2011-02-01 05:28:06 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051443 | We propose to observe the five most luminous type II AGN detected in the Swift BAT all sky hard X-ray survey (14-195 keV). Because BAT's detection efficiency for absorbed sources in the high energy band is very high, these sources are the most luminous (log(L_x) > 45.5 erg/sec) absorbed type II QSOs in the local universe and the most ripe for study with Suzaku. The newly discovered source SWIFT J2344.6-4233 at a redshift of z=0.6 is the most luminous object in the BAT sample with log(L_x) = 46.5 erg/sec. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | WAYNE BAUMGARTNER | USA | 5 | AO5 | SUZAKU OBSERVATIONS OF THE MOST LUMINOUS ABSORBED TYPE II QSOS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705048010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705048010'
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