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 SKY_53.3_-63.4 53.24 -63.4549 53.047022 -63.62196 354.144887 -74.40934 278.62179386 -45.30780651 286.1724 53797.8694444444 2006-03-03 20:52:00 53800.3342476852 2006-03-06 08:01:19 501002010 101.4752 100 101.4752 101.4752 101.4752 101.4752 2 2 2 2 1 0 0 145.4318 145.4318 212.8539 4 PROCESSED 57533.1863425926 2016-05-25 04:28:20 54401 2007-10-28 00:00:00 53906.7729282407 2006-06-20 18:33:01 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011252 We propose Suzaku XIS observations of the hot gas in the Galactic halo and Local Bubble. The spectra's bright emission lines and complexes will reveal the plasma's ionization history and thus its origins. The Local Bubble's spectrum will be garnered from an observation of a nearby opaque cloud. The halo's spectrum will be found by subtracting the Local Bubble spectrum from that of an adjacent off-cloud observation. In order to better constrain the models, we will also draw upon existing FUSE O VI emission data for these directions. With the combined O VI and soft X-ray data, we will be able to constrain the plasma's conditions and ionization history and, thus, constrain detailed models of the hot gas in the halo and Local Bubble. GALACTIC DIFFUSE EMISSION 5 A ROBIN SHELTON USA 1 AO1 SUZAKU XIS OBSERVATIONS OF THE GALACTIC HALO AND LOCAL BUBBLE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501002010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501002010'

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

Go to top of this page ⏏