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 HESS J1825-137 276.5031 -13.6997 275.794781 -13.729527 276.397624 9.596588 17.87105596 -0.70261201 269.3213 54025.8175462963 2006-10-17 19:37:16 54027.1682291667 2006-10-19 04:02:15 501044010 50.293 50 50.293 50.293 50.293 50.293 2 2 2 2 1 0 0 42.9557 42.9557 116.694 1 PROCESSED 57535.8789351852 2016-05-27 21:05:40 54526 2008-03-01 00:00:00 54055.4418634259 2006-11-16 10:36:17 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010073 We propose to observe unidentified TeV gamma-ray sources. HESS surveyed the Galactic Plane and found new TeV gamma-ray sources. TeV gamma-ray emissions are direct evidence for the presence of high energy particles above TeV, but, nonetheless, many of the new extended sources are very faint in any other wavelength. In fact, we observed HESS J1616-518 in Suzaku PV phase already and found its X-ray flux is quite low compared to its TeV gamma-ray flux. It is appropriate to be called ''Dark Accelerator'' and such objects might mainly contribute to the Galactic Cosmic rays. To detect these ''Dark Accelerators'' in X-ray, we propose to observe other unidentified TeV gamma-ray sources, HESS J1614-518 and HESS J1825-137. GALACTIC DIFFUSE EMISSION 5 B HIRONORI MATSUMOTO JAP 1 AO1 SUZAKU OBSERVATIONS OF UNIDENTIFIED TEV GAMMA-RAY SOURECES XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501044010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501044010'

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

Go to top of this page ⏏