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 G236+38 OFF 149.4117 1.4719 148.767122 1.710754 151.004118 -10.298746 237.07053965 41.11953464 293.1755 55719.6375462963 2011-06-07 15:18:04 55721.2780092593 2011-06-09 06:40:20 506056010 70.8135 70 70.8215 70.8295 0 70.8135 2 2 0 2 1 0 0 64.4444 64.4444 141.7278 0 PROCESSED 57602.2364583333 2016-08-02 05:40:30 56127 2012-07-19 00:00:00 55757.6968518518 2011-07-15 16:43:28 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 061321 Interstellar clouds cast shadows in the soft X-ray background (SXRB). Observations of these shadows enable us to disentangle the various components of the SXRB. Unfortunately, to date, shadowing observations with XMM or Suzaku have only been published for three directions, all in the southern Galactic hemisphere. We propose two new pairs of on- and off-cloud shadowing observations, in order to sample the northern Galactic hemisphere. Our particular goal is to obtain accurate X-ray spectra of the Galactic halo, which we will compare with the predictions of models of galactic fountains and infalling extragalactic material. GALACTIC DIFFUSE EMISSION 5 B DAVID HENLEY USA 6 AO6 UNDERSTANDING THE ORIGIN OF THE GALACTIC HALO USING SHADOWING OBSERVATIONS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506056010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '506056010'

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

Go to top of this page ⏏