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 RCW 86 221.2555 -62.3618 220.269135 -62.150858 241.140538 -43.714444 315.68741681 -2.33681001 278.3377 53959.4574652778 2006-08-12 10:58:45 53961.1294907407 2006-08-14 03:06:28 501037010 59.8054 60 59.8294 59.8054 59.8294 59.8214 2 2 2 2 1 0 0 54.405 54.405 144.42 1 PROCESSED 57535.2984259259 2016-05-27 07:09:44 54394 2007-10-21 00:00:00 54021.0740972222 2006-10-13 01:46:42 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010054 We propose an observation of the Northwest region of RCW 86, one of Galactic supernova remnants (SNRs). Hard X-ray continuum of RCW 86 is accompanied by Fe K line emission at 6.4keV. There is strong possibility that the origin of this line is electrons and protons accelerated in the shell of the SNR. In PV phase, the Southeast region of RCW 86 will be observed, and the density of this region is much larger than that of the Northwest region. Therefore we must compare the fluxes of Fe line and hard continuum of both regions, and discuss the correlation between the flux and the density of emitting region. Such comparative study is very useful for understanding the particle acceleration in the shell-like SNRs. GALACTIC DIFFUSE EMISSION 5 B HIROYA YAMAGUCHI JAP 1 AO1 RCW 86:PECULIAR SNR WITH NEUTRAL FE K LINE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501037010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501037010'

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

Go to top of this page ⏏