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 | SGR_B2 | 266.8776 | -28.4437 | 266.086356 | -28.426612 | 267.234654 | -5.032575 | 0.63615824 | -0.0985299 | 266.3663 | 55095.6093518518 | 2009-09-21 14:37:28 | 55096.0418287037 | 2009-09-22 01:00:14 | 504004010 | 10.0572 | 200 | 10.0572 | 10.0572 | 0 | 10.0572 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 9.4328 | 9.4328 | 37.3409 | 0 | PROCESSED | 57548.6152314815 | 2016-06-09 14:45:56 | 55476 | 2010-10-07 00:00:00 | 55110.2035763889 | 2009-10-06 04:53:09 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040002 | The Galactic center diffuse X-ray emission (GCDX) consists of the hot plasma, neutral iron line, and hard tail. While we have demonstrated the hot plasma truly extending, origins of the others are still under discussion. We found time variability of the neutral Fe line intensity and marginally detected neutral lines of S, Ar, and Ca from Sagittarius B2. Our purpose is to clearly detect the neutral lines of S, Ar, Ca, and time variability of the hard tail of the GCDX up to 40 keV. This observation will resolve the remaining mysteries of the GCDX. | GALACTIC DIFFUSE EMISSION | 5 | A | MASAYOSHI NOBUKAWA | JAP | 4 | AO4 | SUZAKU OBSERVATION OF SAGITTARIUS B2 -NEW APPROACH TO THE GALACTIC CENTER DIFFUSE X-RAY EMISSION- | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504004010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '504004010'
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