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 G344.7-0.1 255.9588 -41.7032 255.078113 -41.633558 258.959028 -18.797881 344.67682908 -0.15577285 89.2821 54152.1890393518 2007-02-21 04:32:13 54153.2919097222 2007-02-22 07:00:21 501011010 42.1336 40 42.1336 42.1336 0 42.1336 2 2 0 2 1 0 0 34.2016 34.2016 95.28 1 PROCESSED 57537.4329050926 2016-05-29 10:23:23 54777 2008-11-07 00:00:00 54158.2352662037 2007-02-27 05:38:47 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010050 We propose an observation of a supernova remnant (SNR) G344.7-0.1 with Suzaku. In addition to emission lines from highly ionized ions (Si, S, and so on), we found a strong emission line at 6.4 keV in the spectra obtained with ASCA and XMM-Newton. This line is thought to be a K-line from the low-ionized Fe, but the origin is still unknown. Precise measurements of the line energy and the spectral parameters with the XIS will provide us with understanding the origin of the Fe-K line and the physical process in the SNR. GALACTIC DIFFUSE EMISSION 5 C SHIGEO YAMAUCHI JAP 1 AO1 SUZAKU OBSERVATION OF G344.7-0.1 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501011010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501011010'

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

Go to top of this page ⏏