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 | NORTH POLAR SPUR | 260.5905 | 4.7489 | 259.972652 | 4.795886 | 259.371969 | 27.842624 | 26.83412197 | 21.95376599 | 264.1143 | 53646.4785763889 | 2005-10-03 11:29:09 | 53647.4515277778 | 2005-10-04 10:50:12 | 100038010 | 43.0689 | 50 | 43.1489 | 44.2129 | 43.0689 | 43.2929 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 40.7715 | 40.7715 | 84.0019 | 0 | PROCESSED | 57527.5342824074 | 2016-05-19 12:49:22 | 54247 | 2007-05-27 00:00:00 | 54035.8928009259 | 2006-10-27 21:25:38 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000038 | We propose to observe the North Polar Spur for 100 ksec. The main objectives are below (1) Search for emission lines of N and C that originates from low kT emission (2) Precisely determine the abundance of the NPS The measurement of N and C lines will be the first for XIS. This is also the first for extended sources. The first trial to measure the emission from the C-band (below 0.3keV) by using BI. This will be a guide line how to use the C-band data. Since the C-band intensity is already known, this will be the first calibration of the BI at low energy. The scientific objectives are already given in the mail distributed in the swg. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | North Polar Spur | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100038010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100038010'
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