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 | HIGH LAT. DIFFUSE B | 38.7468 | -52.2774 | 38.331334 | -52.495237 | 4.39034 | -61.411521 | 272.40280946 | -58.27300774 | 280.6379 | 53783.933900463 | 2006-02-17 22:24:49 | 53786.5211111111 | 2006-02-20 12:30:24 | 500027020 | 103.553 | 100 | 103.553 | 103.561 | 103.561 | 103.561 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 68.6094 | 68.6094 | 223.5238 | 3 | PROCESSED | 57533.0790972222 | 2016-05-25 01:53:54 | 54247 | 2007-05-27 00:00:00 | 54041.5670717593 | 2006-11-02 13:36:35 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000044 | We propose observing the diffse background at two locations where the low temperature component is particularly string. One of the these enhancement is ostensibly an extension of the local bubble, while the other it is probably due to a region of very bright emission in the halo (z> 400 pc). We can verify the thermal nature of these sources, and look for CNO abyndance ratio differences between local disk and halo gas. It is critical to make these abundance determinations before the low energy response deteriorates any further. Note that this observation should also allow a calibration of the XIS response below the carbon edge to ~20%. | GALACTIC DIFFUSE EMISSION | 5 | A | SWG | JAP | 0 | SWG | HIGH LATTITUDE DIFFUSE A & B | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500027020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '500027020'
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