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 | IRASF11223-1244 | 171.2239 | -12.9662 | 170.593283 | -12.69128 | 177.194404 | -15.365769 | 272.54538498 | 44.73919633 | 107.3062 | 54064.7275347222 | 2006-11-25 17:27:39 | 54065.5709953704 | 2006-11-26 13:42:14 | 701008010 | 40.9415 | 40 | 41.1015 | 40.9415 | 0 | 41.1095 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 37.6804 | 37.6804 | 72.8639 | 1 | PROCESSED | 57536.1775925926 | 2016-05-28 04:15:44 | 54735 | 2008-09-26 00:00:00 | 54088.8556828704 | 2006-12-19 20:32:11 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 010038 | The source of huge energy output from ultraluminous infrared galaxies (ULIRGs) is still under debate. We propose to search for a hidden QSO as the energy source by observing ULIRGs with high luminosity optical emission lines classified as a Seyfert 2. The data will be used to constrain the power of the central AGN and to study the nature of infrared selected type 2 QSOs. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | YUICHI TERASHIMA | JAP | 1 | AO1 | A SEARCH FOR HIDDEN QSO IN ULTRALUMINOUS INFRARED GALAXIES | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701008010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '701008010'
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