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
1 3C 332 244.4239 32.3632 243.942335 32.484407 233.11322 52.57597 52.6372471 45.34839384 292.5008 55051.0341782407 2009-08-08 00:49:13 55052.4655092593 2009-08-09 11:10:20 704038010 59.8339 60 59.8339 59.8339 0 59.8339 2 2 0 2 1 0 0 46.0491 46.0491 123.652 0 PROCESSED 57548.1132407407 2016-06-09 02:43:04 55437 2010-08-29 00:00:00 55067.2557986111 2009-08-24 06:08:21 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 041413 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($L_x$) $> 45.5$~ergs~sec$^{-1}$) absorbed tyoe II QSOs in the local universe and the most ripe for study with suzaku. 3C~332 is believed to be Compton-thick as suggested by chandra observations, and 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($L_x$) $=46.5$~ergs~sec$^{-1}$. EXTRAGALACTIC COMPACT SOURCES 7 C WAYNE BAUMGARTNER USA 4 AO4 SUZAKU OBSERVATIONS OF THE MOST LUMINOUS ABSORBED TYPE II QSOS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704038010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '704038010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏