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 NGC 4151 182.6375 39.4139 182.006166 39.692011 164.091601 36.628069 155.05374688 75.05753801 112.1087 54087.8369097222 2006-12-18 20:05:09 54090.3848726852 2006-12-21 09:14:13 701034010 124.9796 125 124.9796 124.9796 0 124.9796 2 2 0 2 1 0 0 131.2741 131.2741 220.1059 3 PROCESSED 57536.4582060185 2016-05-28 10:59:49 54702 2008-08-24 00:00:00 54132.849537037 2007-02-01 20:23:20 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011327 We propose a 100 ks Suzaku observation of the brightest Seyfert Galaxy in the sky. Given the broad band-pass, and high sensitivity, the proposed observations will provide a high-quality spectrum which will allow us to search for variability in the high-ionized absorber (compared to previous observations). We will be able to obtain stringent constraints on the "Reflection Hump" and compare it to the strength of the Fe Kalpha emission line - thus providing a direct test of Reflection models. The proposed program will also complement observations of fainter and more exotic Seyferts likely to be observed during AO-1. EXTRAGALACTIC COMPACT SOURCES 7 A IAN GEORGE USA 1 AO1 DECOUPLING THE COMPONENTS IN THE BRIGHTEST SEYFERT: NGC 4151 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701034010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701034010'

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

Go to top of this page ⏏