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 | L106_B3 | 337.3111 | 61.2453 | 336.866796 | 60.988922 | 21.907924 | 61.425064 | 106.66847152 | 2.94694679 | 86.3781 | 55332.0617013889 | 2010-05-16 01:28:51 | 55333.5078587963 | 2010-05-17 12:11:19 | 505054010 | 59.3804 | 60 | 59.3804 | 59.3804 | 0 | 59.3804 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 54.0551 | 54.0551 | 124.908 | 3 | PROCESSED | 57551.5609259259 | 2016-06-12 13:27:44 | 55765 | 2011-07-23 00:00:00 | 55393.2646759259 | 2010-07-16 06:21:08 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050086 | We propose observarions of two fields on and near midplane (b = 0 and 3 deg.) in order to study bump-like emission peaked at 0.9 keV observed in midplane. The two fields proposed for observations has been observed by Chandra. By comparing the spectra taken by Suzaku and Chandra, we will determine the contribution of point sources (stars), and investigate posisble contribution of diffuse thermal plasma. | GALACTIC DIFFUSE EMISSION | 5 | B | YOH TAKEI | JAP | 5 | AO5 | ORIGIN OF SOFT X-RAY EMISSION IN THE MILKY-WAY DISK | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505054010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505054010'
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