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 | RCW 38 | 134.7638 | -47.5154 | 134.339139 | -47.320051 | 162.870038 | -60.148721 | 267.93999829 | -1.06526988 | 109.8553 | 54788.5064351852 | 2008-11-18 12:09:16 | 54790.699525463 | 2008-11-20 16:47:19 | 503054010 | 81.5377 | 80 | 81.5495 | 81.5377 | 0 | 81.5415 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 60.9281 | 60.9281 | 189.4597 | 1 | PROCESSED | 57544.5092013889 | 2016-06-05 12:13:15 | 55171 | 2009-12-06 00:00:00 | 54811.741099537 | 2008-12-11 17:47:11 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030069 | We propose to make Suzaku observation of HII region RCW 38 for 80 ksec in order to study non-thermal phenomena in a massive star-forming region. The region is thought to be a site of high energy particle acceleration by interaction of strong stellar wind from high-mass stars. The main purpose is to observe extended emission from RCW 38. The high resolution spectroscopy by XIS enables us to distinguish non-thermal emission from thermal component and to obtain properties of non-thermal component. In addition, HXD will detect non-thermal radiation from RCW 38. | GALACTIC DIFFUSE EMISSION | 5 | C | HIROKAZU ODAKA | JAP | 3 | AO3 | SEARCH FOR NONTHERMAL RADIATION FROM MASSIVE STAR-FORMING REGION RCW 38 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503054010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503054010'
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