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 | GC CENTER #2 | 266.7693 | -28.6295 | 265.976908 | -28.611884 | 267.143281 | -5.22043 | 0.42794484 | -0.11339991 | 74.7707 | 53821.958587963 | 2006-03-27 23:00:22 | 53823.7585069444 | 2006-03-29 18:12:15 | 500005010 | 88.4247 | 100 | 88.4327 | 88.4247 | 88.4327 | 88.4327 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 64.5911 | 64.5911 | 155.5019 | 2 | PROCESSED | 57533.3630324074 | 2016-05-25 08:42:46 | 54247 | 2007-05-27 00:00:00 | 54133.0079861111 | 2007-02-02 00:11:30 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001020 | We propose to obtain high quality spectrum near the GC. The objective is to resolve 6.4, 6.7, and 6.9 keV line and determine the high energy tail and sub-structures, which may be X-ray reflection from Sgr A* (6.4 keV line + 7.1 keV edge + high energy tail), thermal plasma (6.7 + 6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. | GALACTIC DIFFUSE EMISSION | 5 | A | KATSUJI KOYAMA | JAP | 0 | SWG | SUZAKU GALACTIC CENTER OBSERVATION PROJECT: #2 SGR B1 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500005010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '500005010'
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