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 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'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏