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 | H2356_VICINITY_B | 359.9868 | -29.9493 | 359.345168 | -30.227755 | 347.07269 | -27.257526 | 15.89682365 | -78.35224854 | 69.5008 | 55698.0951388889 | 2011-05-17 02:17:00 | 55699.3474305556 | 2011-05-18 08:20:18 | 506029010 | 51.4072 | 50 | 51.4312 | 51.4232 | 0 | 51.4072 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 42.546 | 42.546 | 108.1559 | 1 | PROCESSED | 57602.0868402778 | 2016-08-02 02:05:03 | 56075 | 2012-05-28 00:00:00 | 55708.1035069444 | 2011-05-27 02:29:03 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060075 | We propose to observe the two vicinities of H2356-309 for 50 ks each. Absorption lines from ions at z=0 and z=0.03 has been observed with grating spectrometers in the spectrum of H2356-309. Emission analysis with Suzaku will provide independent information on the medium responsible for the absorption lines. By combining the emission surface brightness and aborption equivalent width, we will constrain the temperature and physical length of the interstellar and intergalactic medium. | GALACTIC DIFFUSE EMISSION | 5 | A | YOH TAKEI | JAP | 6 | AO6 | EMISSION/ABSORPTION COMBINATION STUDY OF GALACTIC AND INTERGALACTIC WARM-HOT GAS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506029010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506029010'
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