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
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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