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 IGR J16318-4848 247.9691 -48.8061 247.034981 -48.699533 253.953463 -26.583352 335.63186461 -0.44896472 266.5948 53961.4825 2006-08-14 11:34:48 53964.3488310185 2006-08-17 08:22:19 401094010 97.2538 100 97.2698 97.2538 97.2698 97.2698 2 2 2 2 1 0 0 87.1128 87.1128 247.6059 5 PROCESSED 57535.3483564815 2016-05-27 08:21:38 54526 2008-03-01 00:00:00 54020.9181597222 2006-10-12 22:02:09 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012034 We propose a detailed study of Compton thick X-ray absorption in neutral or weakly ionized material by using 100ksec of Suzaku observations of the strongly absorbed (N_H~2E24cm2) Galactic X-ray binary IGR J16318-4848. Measuring a high signal to noise ratio broad band spectrum will allow us to determine the curvature in the >10keV continuum caused by Compton downscattering in the absorber, to deduce its ionization state from observations of the Fe Kalpha line, and to study the variability of the source and the absorber. These observations will also shed more light onto the nature of the compact object in IGR J16318-4848. GALACTIC POINT SOURCES 4 B JOERN WILMS EUR 1 AO1 OBSERVING IGR J16318-4848: PROBING COMPTON-THICK ABSORPTION XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401094010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401094010'

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

Go to top of this page ⏏