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 | NEP | 272.8227 | 66.0165 | 272.806643 | 66.002812 | 335.593486 | 88.746745 | 95.79277142 | 28.663354 | 126.3033 | 53776.2556944445 | 2006-02-10 06:08:12 | 53778.0836111111 | 2006-02-12 02:00:24 | 500026010 | 88.5082 | 80 | 88.5322 | 88.5082 | 88.5242 | 88.5322 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 83.6728 | 83.6728 | 157.902 | 0 | PROCESSED | 57532.9856481482 | 2016-05-24 23:39:20 | 54247 | 2007-05-27 00:00:00 | 54041.1403703704 | 2006-11-02 03:22:08 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000042 | We propose a second Suzaku observation of the NEP region in order to constrain the long-term and short-term valiability of OVII and OIVVV emission line intensities.Short-term variability detected in the first Suzaku observation implies existence of a charge-exchange component in oVIII linem suggesting solar wind and geo corona interaction. First purpose is to confirm this with the second observtaion.Secondly, to search a long-term variability. If it is observed, it will place a further constraints on the solar wind and interplanetary medium near the Earth. | GALACTIC DIFFUSE EMISSION | 5 | A | SWG | JAP | 0 | SWG | NEP | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500026010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '500026010'
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