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 GALACTIC RIDGE 281.0049 -4.0776 280.344509 -4.129178 281.602156 18.920781 28.45801897 -0.21166151 265.5297 53671.1112037037 2005-10-28 02:40:08 53673.8960069445 2005-10-30 21:30:15 500009010 93.3276 100 93.3436 93.3596 93.3436 93.3276 2 2 2 2 1 0 0 77.5364 77.5364 240.5759 0 PROCESSED 57527.7330439815 2016-05-19 17:35:35 54247 2007-05-27 00:00:00 54037.6929513889 2006-10-29 16:37:51 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001042 We propose to observe the blank Galactic plane field at (l,b)=(28.6,0.0) for 200 ksec to study energy spectra of Galactic Ridge X-ray Emission. This is a Chandra deep field where we have spent 100 ksec. We will carry out plasma diagnostics of the Galactic ridge emission using primarily iron lines, and also Kalpha and Kbeta lines of Ne, Mg, Si, and S. The 200 ksec Ridge observation by Suzaku enables us to compare Galactic center and ridge emission lines directly. We believe the Galactic Ridge X-ray emission is truely diffuse, based on our Chandra study. However, there is a claim that the ridge emission is preimaly composed of dim sources down to 10^-16 cgs in 2-10 keV. To end the controversy, we plan to carry out a 1Msec Chandra observation on this Chandra-Suzaku field. GALACTIC DIFFUSE EMISSION 5 A KEN EBISAWA JAP 0 SWG ORIGIN OF THE GALACTIC RIDGE X-RAY EMISSION N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500009010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '500009010'

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