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 MKN 841 225.9811 10.3761 225.377197 10.570593 220.178092 26.525473 11.09749436 54.61837916 292.433 54304.6970949074 2007-07-23 16:43:49 54306.218912037 2007-07-25 05:15:14 701084020 50.9253 50 50.9253 50.9333 0 50.9333 2 2 0 2 1 0 0 47.6556 47.6556 131.4738 2 PROCESSED 57539.3432060185 2016-05-31 08:14:13 54800 2008-11-30 00:00:00 54339.5240277778 2007-08-27 12:34:36 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012028 We propose to perform two 50 ks Suzaku observations of Mkn 841, at an interval of a few months, in order to elucidate the origin of its different X-ray components. Strong soft excess and complex iron line profile are known to be present in this source and recent XMM observations reveal their extreme and puzzling spectral and temporal behaviors. Nevertheless, while the XMM observations help to better constrain their natures, their physical interpretation strongly suffer from the lack of data above 10 keV. Two dedicated Suzaku observations will provide crucial information for our understanding of these components, allowing 1) to obtain high S/N and striclty simultaneous broad band X-ray spectra from the soft X-ray up to the reflection bump and 2) to study their spectral variability behaviors EXTRAGALACTIC COMPACT SOURCES 7 B PIERRE-OLIVIER PETRUCCI EUR 1 AO1 PROBING THE ORIGIN OF THE STRONG SOFT EXCESS AND PUZZLING REFLECTION COMPONENTS IN MKN 841 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701084020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701084020'

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

Go to top of this page ⏏