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 GC SOUTH BGD 266.1893 -28.9082 265.395265 -28.887768 266.639666 -5.511508 359.92534776 0.17564926 265.0003 54007.8931365741 2006-09-29 21:26:07 54009.2884143518 2006-10-01 06:55:19 501009010 51.19 50 51.198 51.206 51.19 51.198 2 2 2 2 1 0 0 47.7157 47.7157 120.5479 0 PROCESSED 57535.7087847222 2016-05-27 17:00:39 54735 2008-09-26 00:00:00 54020.9371064815 2006-10-12 22:29:26 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010044 Past X-ray observations have discovered diffuse X-rays extended within a hundred parsec of the Galactic center (GC) region. Moreover, Suzaku PV observation indicates that the diffuse X-rays can well be explained by a thermal emission from hot(8 keV) plasma. The most plausible energy injection sources are the multiple SNe. The huge thermal energy (10^47 J) and short timescale (10^5 yr) of the hot plasma suggest that the GC region harbors at least 10 young SNRs. To confirm the scenario, we propose to observe two SNR candidates at the south of the GC with a single pointing. One exhibits a non-thermal shell-like X-ray SNR feature, and the other shows a thin-thermal SNR feature. We also propose to observe the symmetric position with respect to the Galactic plane for the background estimation. GALACTIC DIFFUSE EMISSION 5 A KATSUJI KOYAMA JAP 1 AO1 SUZAKU OBSERVATIONS OF G359.79-0.26 AND G359.92-0.09: THERMAL AND NONTHERMAL SUPERNOVA REMNANTS NEAR THE GALACTIC CENTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501009010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501009010'

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

Go to top of this page ⏏